Angle: Difference between revisions

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search
imported>Mathnerd314159
restore edits reverted by User:ZergTwo - no reply on talk, appears to be drive-by revert
 
imported>Alexander Lozovsky
Combining angle pairs: Fixed: consecutive angles of a parallelogram are supplementary, not complementary
 
(2 intermediate revisions by 2 users not shown)
Line 2: Line 2:
{{Distinguish|Angel}}
{{Distinguish|Angel}}
{{About|angles in geometry}}
{{About|angles in geometry}}
[[File:Angle.svg|alt=two line bent at a point|thumb|upright=1.25|A green angle formed by two red [[Ray (geometry)|rays]] on the [[Cartesian coordinate system]]]]
{{CS1 config|mode=cs2}}
{{Use dmy dates|cs1-dates=sy|date=September 2025}}
[[File:Angle.svg|class=skin-invert-image|alt=two line bent at a point|thumb|upright=1.25|A green angle formed by two red [[Ray (geometry)|rays]] on the [[Cartesian coordinate system]]]]


In [[Euclidean geometry]], an '''angle''' can refer to a number of concepts relating to the intersection of two straight [[Line (geometry)|lines]] at a point. Formally, an angle is a figure lying in a [[Euclidean plane|plane]] formed by two [[Ray (geometry)|rays]], called the ''[[Side (plane geometry)|sides]]'' of the angle, sharing a common endpoint, called the ''[[vertex (geometry)|vertex]]'' of the angle.<ref>{{Cite book |last=Hilbert |first=David |url=https://math.berkeley.edu/~wodzicki/160/Hilbert.pdf |title=The Foundations of Geometry |pages=9}}</ref><ref>{{harvnb|Sidorov|2001|ignore-err=yes}}</ref> More generally angles are also formed wherever two lines, rays or [[Line segment|line segments]] come together, such as at the corners of triangles and other polygons. An angle can be considered as the region of the plane bounded by the sides.<ref>{{Cite book |last=Evgrafov |first=M. A. |url=https://books.google.com/books?id=N8-wDwAAQBAJ&dq=angle+and+%2522angular+sector%2522+domain&pg=PA126 |title=Analytic Functions |date=2019-09-18 |publisher=Courier Dover Publications |isbn=978-0-486-84366-7 |language=en}}</ref><ref>{{Cite book |last=Papadopoulos |first=Athanase |url=https://books.google.com/books?id=f6yZeVMqhNEC&dq=angle+and+%2522angular+sector%2522+region&pg=PA12 |title=Strasbourg Master Class on Geometry |date=2012 |publisher=European Mathematical Society |isbn=978-3-03719-105-7 |language=en}}</ref>{{efn|An angular sector can be constructed by the combination of two rotated [[half-plane]]s, either their intersection or union (in the case of acute or obtuse angles, respectively).<ref>{{Cite book |last=D'Andrea |first=Francesco |url=https://books.google.com/books?id=BszREAAAQBAJ&dq=angle+and+%2522angular+sector%2522&pg=PA68 |title=A Guide to Penrose Tilings |date=2023-08-19 |publisher=Springer Nature |isbn=978-3-031-28428-1 |language=en}}</ref><ref>{{Cite book |last1=Bulboacǎ |first1=Teodor |url=https://books.google.com/books?id=r0miDwAAQBAJ&dq=angle+and+%2522angular+sector%2522+half-planes&pg=PT22 |title=Complex Analysis: Theory and Applications |last2=Joshi |first2=Santosh B. |last3=Goswami |first3=Pranay |date=2019-07-08 |publisher=Walter de Gruyter GmbH & Co KG |isbn=978-3-11-065803-3 |language=en}}</ref> It corresponds to a [[circular sector]] of infinite radius and a flat [[pencil of half-lines]].<ref>{{Cite book |last=Redei |first=L. |url=https://books.google.com/books?id=XMTSBQAAQBAJ&dq=half-pencil+of+lines&pg=PA45 |title=Foundation of Euclidean and Non-Euclidean Geometries according to F. Klein |date=2014-07-15 |publisher=Elsevier |isbn=978-1-4832-8270-1 |language=en}}</ref>}} Angles can also be formed by the intersection of two planes or by two intersecting [[curve]]s, in which case the rays lying [[tangent]] to each curve at the point of intersection define the angle.
In [[geometry]], an '''angle''' is formed by two [[Line (geometry)|lines]] that meet at a point.<ref>{{cite book |last1=Heath |first1=Thomas Little |last2=Heiberg |first2=J. L. (Johan Ludvig) |title=The thirteen books of Euclid's Elements |date=1908 |publisher=Cambridge, The University Press |page=176 |url=https://archive.org/details/thirteenbookseu02heibgoog/page/n196/mode/2up|quote=A plane angle is the inclination to one another of two lines in a plane which meet one another and do not lie in a straight line.}}</ref> Each line is called a ''[[Side (plane geometry)|side]]'' of the angle, and the point they share is called the ''[[vertex (geometry)|vertex]]'' of the angle.<ref name=":0">{{cite book |last=Hilbert |first=David |url=https://math.berkeley.edu/~wodzicki/160/Hilbert.pdf |title=The Foundations of Geometry |pages=9}}</ref><ref>{{harvnb|Sidorov|2001|ignore-err=yes}}</ref> The term ''angle'' is used to denote both geometric figures and their size or [[magnitude (mathematics)|magnitude]]. '''Angular measure''' or '''measure of angle''' are sometimes used to distinguish between the measurement and figure itself. The measurement of angles is intrinsically linked with circles and rotation, and this is often visualized or defined using the [[Arc (geometry)|arc]] of a [[circle]] centered at the vertex and lying between the sides.


The term ''angle'' is also used for the size, [[magnitude (mathematics)|magnitude]] or [[Physical quantity|quantity]] of these types of geometric figures and in this context an angle consists of a number and unit of measurement. '''Angular measure''' or '''measure of angle''' are sometimes used to distinguish between the measurement and figure itself. The measurement of angles is intrinsically linked with circles and rotation. For an ordinary angle, this is often visualized or defined using the [[Arc (geometry)|arc]] of a [[circle]] centered at the vertex and lying between the sides.
== Fundamentals ==


==Fundamentals==
There is no universally agreed definition of an angle.<ref>{{Cite book |last=Saxon |first=John, H |title=Algebra I An Incremental Development}}</ref> Angles can be conceived of and used in a variety of ways and while valid definitions may be given for specific contexts, it is difficult to give a single formal definition that is completely satisfactory in capturing all aspects of the general concept of ''angle''.<ref>{{Cite book |last=Henderson |title=Experiencing Geometry- Euclildian and non-Euclidian With History |publisher=Pearson Prentice Hall |year=2020 |isbn=978-1-4297-9985-0}}</ref>
An angle is a figure lying in a plane formed by two distinct rays (half-lines emanating indefinitely from an endpoint in one direction), which share a common endpoint. The rays are called the sides or arms of the angle, and the common endpoint is called the vertex. The sides divide the plane into two regions: the ''interior of the angle'' and the ''exterior of the angle.''


=== Notation ===
One standard definition is that an angle is a ''figure'' consisting of two rays which lie in a plane and share a common endpoint. Alternatively, given such a figure, an angle might be defined as: the ''opening'' between the rays; the ''area of the plane'' that lies between the rays; or the ''amount of rotation'' about the vertex of one ray to the other.
[[File:Angle diagram.svg|thumb|300x300px|<math>\angle BAC</math> is formed by rays <math>\vec{AB}</math> and '''<math>\vec{AC}</math>'''.  '''<math>\theta</math>''' is the conventional measure of <math>\angle BAC</math> and '''<math>\beta</math>''' is an alternative measure.]]
In geometric figures and [[Expression (mathematics)|mathematical expressions]], it is common to use [[Greek letter]]s (<var>α</var>, <var>β</var>, <var>γ</var>, <var>θ</var>, <var>φ</var>,&nbsp;.&nbsp;.&nbsp;.&nbsp;) or lower case Roman letters (''a'',&nbsp;''b'',&nbsp;''c'',&nbsp;.&nbsp;.&nbsp;.&nbsp;) as [[Variable (mathematics)|variables]] denoting the size of an angle.{{sfn|Aboughantous|2010|p=18}} The Greek letter {{math|[[Pi (letter)|π]]}} is typically not used for this purpose to avoid confusion with the [[Pi|circle constant]].


An angle symbol (<math>\angle</math> or <math>\widehat{ \quad }</math>) with three defining points may also identify angles in geometric figures. For example, <math>\angle BAC</math> or <math>\widehat{BAC}</math> denotes the angle with vertex A formed by the [[ray (geometry)|rays]] AB and AC. Where there is no risk of confusion, the angle may sometimes be referred to by a single vertex alone (in this case, "angle A").
More generally, angles are also formed wherever two [[line segment]]s come together, such as at the corners of triangles and other polygons,<ref name=":0" /> or at the intersection of two planes or [[curve]]s, in which case the rays lying [[tangent]] to each curve at the point of intersection define the angle.{{sfn|Chisholm|1911}}


Conventionally, angle size is measured "between" the sides through the interior of the angle and given as a [[Magnitude (mathematics)|magnitude]] or [[Scalar (physics)|scalar quantity]] without direction. At other times it might be a measure through the exterior of the angle or indicate a direction of measurement (see ''{{section link|#Signed angles}}'').
It is common to consider that the sides of the angle divide the plane into two regions called the ''interior of the angle'' and the ''exterior of the angle''. The interior of the angle is also referred to as an '''angular sector'''.<ref>{{cite book |last=Evgrafov |first=M. A. |url=https://books.google.com/books?id=N8-wDwAAQBAJ&dq=angle+and+%2522angular+sector%2522+domain&pg=PA126 |title=Analytic Functions |date=1966 |publisher=W. B. Saunders }}</ref><ref>{{cite book |last=Papadopoulos |first=Athanase |url=https://books.google.com/books?id=f6yZeVMqhNEC&dq=angle+and+%2522angular+sector%2522+region&pg=PA12 |title=Strasbourg Master Class on Geometry |date=2012 |publisher=European Mathematical Society |isbn=978-3-03719-105-7 }}</ref>{{efn|An angular sector can be constructed by the combination of two rotated [[half-plane]]s, either their intersection or union (in the case of acute or obtuse angles, respectively).<ref>{{cite book |last=D'Andrea |first=Francesco |url=https://books.google.com/books?id=BszREAAAQBAJ&dq=angle+and+%2522angular+sector%2522&pg=PA68 |title=A Guide to Penrose Tilings |date=2023 |publisher=Springer |isbn=978-3-031-28428-1 }}</ref><ref>{{cite book |last1=Bulboacǎ |first1=Teodor |url=https://books.google.com/books?id=r0miDwAAQBAJ&dq=angle+and+%2522angular+sector%2522+half-planes&pg=PT22 |title=Complex Analysis: Theory and Applications |last2=Joshi |first2=Santosh B. |last3=Goswami |first3=Pranay |date=2019 |publisher=Walter de Gruyter GmbH & Co KG |isbn=978-3-11-065803-3 }}</ref> It corresponds to a [[circular sector]] of infinite radius and a flat [[pencil of half-lines]].<ref>{{cite book |last=Redei |first=L. |url=https://books.google.com/books?id=XMTSBQAAQBAJ&dq=half-pencil+of+lines&pg=PA45 |title=Foundation of Euclidean and Non-Euclidean Geometries according to F. Klein |date=2014 |publisher=Elsevier |isbn=978-1-4832-8270-1 }}</ref>}}


=== Common angles and units of measurement ===
=== Notation and measurement ===
{{Multiple image
[[File:Angle diagram.svg|thumb|class=skin-invert-image|<math>\angle \text{BAC}</math> is formed by rays <math>\vec{\text{AB}}</math> and <math>\vec{\text{AC}}</math>. <math>\theta</math> is the conventional measure of <math>\angle \text{BAC}</math> and <math>\beta</math> is an alternative measure.]]
|perrow = 2/3
An angle symbol (<math>\angle</math> or <math>\widehat{ \quad }</math>, read as "angle") together with one or three defining points is used to identify angles in geometric figures. For example, the angle with vertex A formed by the [[ray (geometry)|rays]] <math>\vec{\text{AB}}</math> and <math>\vec{\text{AC}}</math> is denoted as <math>\angle \text{A}</math> (using the vertex alone) or <math>\angle \text{BAC}</math> (with the vertex always named in the middle). The size or measure of the angle is denoted <math>m\angle \text{A}</math> or <math>m\angle \text{BAC}</math>.
|align=right
|direction=horizontal
|image1=Angle obtuse acute straight.svg
|width1=200
|caption1=Acute (<var>a</var>), obtuse (<var>b</var>), and straight (<var>c</var>) angles. All acute and obtuse angles are also oblique angles.


|image2=Zero angle.svg
In geometric figures and [[Expression (mathematics)|mathematical expressions]], it is also common to use [[Greek letter]]s (''α'', ''β'', ''γ'', ''θ'', ''φ'',&nbsp;...) or lower case Roman letters (''a'',&nbsp;''b'',&nbsp;''c'',&nbsp;...) as [[Variable (mathematics)|variables]] to represent the size of an angle.{{sfn|Aboughantous|2010|p=18}} Angular measure is commonly a [[Scalar (physics)|scalar quantity]],<ref>{{cite web |title=NIST Guide to the SI, Chapter 7: Rules and Style Conventions for Expressing Values of Quantities |url=https://www.nist.gov/pml/special-publication-811/nist-guide-si-chapter-7-rules-and-style-conventions-expressing-values#7.2 |website=NIST |access-date=8 August 2025 |date=2016 |quote=α is a quantity symbol for plane angle.}}</ref> although in physics and some fields of mathematics, [[Sign (mathematics)|signed]] angles are used by convention to indicate a direction of rotation: positive for anti-clockwise; negative for clockwise.<ref>{{cite journal |last1=De |first1=Villiers |title=The Value of using Signed Quantities in Geometry |journal=Learning and Teaching Mathematics |date=2020 |volume=29 |issue=2020 |pages=30–34 |hdl=10520/ejc-amesal_n29_a8.pdf-v29-n2020-a8 |url=https://www.amesa.org.za/amesal_n29_a8.pdf |access-date=8 August 2025}}</ref>
|width2=81
|caption2=Zero angle


|image3=Right angle.svg
=== Units of measurement ===
|width3=111
|caption3=[[Right angle]]


|image4=Reflex angle.svg
Angles are measured in various units, the most common being the [[Degree (angle)|degree]] (denoted by the symbol '''°'''), [[radian]] (denoted by the symbol '''rad''') and [[Turn (angle)|turn]]. These units differ in the way they divide up a ''full angle'', an angle where one ray, initially congruent to the other, performs a compete rotation about the vertex to return back to its starting position.<ref>{{cite web |last=Weisstein |first=Eric W. |title=Angle |url=https://mathworld.wolfram.com/Angle.html |access-date=2025-06-13 |website=mathworld.wolfram.com }}</ref>
|width4=81
|caption4=Reflex angle


|image5=Full angle.svg
Degrees and turns are defined directly with reference to a full angle, which measures 1 turn or 360°.<ref>{{cite web |last=Weisstein |first=Eric W. |title=Degree |url=https://mathworld.wolfram.com/Degree.html |access-date=2025-06-14 |website=mathworld.wolfram.com }}</ref> A measure in turns gives an angle's size as a proportion of a full angle and a degree can be considered as a subdivision of a turn. Radians are not defined directly in relation to a full angle (see ''{{Section link|#Measuring angles}}''), but in such a way that its measure is 2{{math|π}}&nbsp;rad, approximately 6.28&nbsp;rad.<ref>{{cite web |last=Weisstein |first=Eric W. |title=Radian |url=https://mathworld.wolfram.com/Radian.html |access-date=2025-06-14 |website=mathworld.wolfram.com }}</ref>
|width5=81
 
|caption5=Full angle
=== Addition and subtraction ===
}}
{{anchor|Angle addition postulate}}
Angles are measured in various units, the most common being the [[Degree (angle)|degree]] (denoted by the symbol '''°'''), [[radian]] (denoted by symbol '''rad''') and [[Turn (angle)|turn]]. These units differ in the way they divide up a ''full angle'', an angle where one ray, initially congruent to the other, performs a compete rotation about the vertex to return back to its starting position.
[[File:Angle addition.svg|thumb|class=skin-invert-image|The angle addition postulate defines addition and subtraction of angles: {{nowrap|1=''θ'' + ''α'' = ''φ''}}; {{nowrap|1=''φ'' − ''α'' = ''θ''}}.]]
The '''angle addition postulate''' states that if D is a point lying in the interior of <math>\angle \text{BAC}</math> then:<ref name=":1">{{cite book |last=Moise |first=Edwin E. |url=https://www.ime.usp.br/~toscano/disc/2021/Moise.pdf |title=Elementary geometry from an advanced standpoint |publisher=Addison-Wesley Publishing Company |year=1990 |edition=3rd |pages=}}</ref> <math display="block"> m\angle \text{BAC} = m\angle \text{BAD} + m\angle \text{DAC}.</math> This relationship ''defines'' what it means to add any two angles: their vertices are placed together while sharing a side to create a new larger angle. The measure of the new larger angle is the sum of the measures of the two angles. Subtraction follows from rearrangement of the formula.<ref name=":1" />


Degrees and turns are defined directly with reference to a full angle, which measures 1 turn or 360'''°'''. A measure in turns gives an angle's size as a proportion of a full angle and a degree can be considered as a subdivision of a turn. Radians are not defined directly in relation to a full angle (see {{Section link|2=Measuring angles|nopage=Y}}), but in such a way that its measure is <math>2\pi</math> rad, approximately 6.28 rad.
== Types<span class="anchor" id="Types of angles"></span> ==<!--8 redirects target previous header #Types_of_angles-->
{{redirect|Oblique angle|the cinematographic technique|Dutch angle}}


There is some common terminology for angles, whose conventional measure is always non-negative (see ''{{section link|#Signed angles}}''):
=== Common angles ===
[[File:Angle types.svg|thumb|class=skin-invert-image|Common types of angles|alt=Diagram visualizing common angles: zero, acute, right, obtuse, straight, reflex, full]]
* An angle equal to 0° or not turned is called a ''zero angle''.{{sfn|Moser|1971|p=41}}
* An angle equal to 0° or not turned is called a ''zero angle''.{{sfn|Moser|1971|p=41}}
* An angle smaller than a right angle (less than 90°) is called an ''acute angle''{{sfn|Godfrey|Siddons|1919|p=9}} ("acute" meaning "[[Sharpness (visual)|sharp]]").
* An angle smaller than a right angle (less than 90°) is called an ''acute angle''.{{sfn|Godfrey|Siddons|1919|p=9}}
* An angle equal to {{sfrac|4}}&nbsp;[[Turn (angle)|turn]] (90° or {{sfrac|{{math|π}}|2}} [[radian]]s) is called a ''[[right angle]]''. Two lines that form a right angle are said to be ''[[normal (geometry)|normal]]'', ''[[orthogonality|orthogonal]]'', or ''[[perpendicular]]''.{{sfn|Moser|1971|p=71}}
* An angle equal to {{sfrac|4}}&nbsp;[[Turn (angle)|turn]] (90° or {{sfrac|{{math|π}}|2}}&nbsp;rad) is called a ''[[right angle]]''. Two lines that form a right angle are said to be ''[[normal (geometry)|normal]]'', ''[[orthogonality|orthogonal]]'', or ''[[perpendicular]]''.{{sfn|Moser|1971|p=71}}
* An angle larger than a right angle and smaller than a straight angle (between 90° and 180°) is called an ''obtuse angle''{{sfn|Godfrey|Siddons|1919|p=9}} ("obtuse" meaning "blunt").
* An angle larger than a right angle and smaller than a straight angle (between 90° and 180°) is called an ''obtuse angle''{{sfn|Godfrey|Siddons|1919|p=9}} ("obtuse" meaning "blunt").
* An angle equal to {{sfrac|2}}&nbsp;turn (180° or {{math|π}} radians) is called a ''straight angle''.{{sfn|Moser|1971|p=41}}
* An angle equal to {{sfrac|2}}&nbsp;turn (180° or {{math|π}}&nbsp;rad) is called a ''straight angle''.{{sfn|Moser|1971|p=41}}
* An angle larger than a straight angle but less than 1&nbsp;turn (between 180° and 360°) is called a ''reflex angle''.
* An angle larger than a straight angle but less than 1&nbsp;turn (between 180° and 360°) is called a ''reflex angle''.
* An angle equal to 1 turn (360° or 2{{math|π}} radians) is called a ''full angle'', ''complete angle'', ''round angle'' or ''perigon''.
* An angle equal to 1 turn (360° or 2{{math|π}}&nbsp;rad) is called a ''full angle'', ''complete angle'', ''round angle'' or ''perigon''.
* An angle that is not a multiple of a right angle is called an ''oblique angle''.
* An angle that is not a multiple of a right angle is called an ''oblique angle''.


The names, intervals, and measuring units are shown in the table below:
=== Adjacent and vertical angles<span class="anchor" id="adjacent"></span> ===<!--4 redirects target #adjacent-->
{{redirect-distinguish|Vertical angle|Zenith angle}}
{{Gallery|align=right
|File:Adjacentangles.svg|Angles A and B are adjacent.
|class1=skin-invert-image
|File:Vertical Angles.svg|Angles A and B, and pair C and D are two pairs of vertical angles. [[Hatch_mark#Congruency_notation|Hatch marks]] indicate equality between pairs.
|class2=skin-invert-image
}}
'''''Adjacent angles''''' (abbreviated ''adj. ∠s''), are angles that share a common vertex and edge but do not share any interior points. In other words, they are angles side by side or adjacent, sharing an "arm".


{|class = wikitable style="text-align:center;"
'''''Vertical angles''''' are formed when two straight lines intersect at a point producing four angles. A pair of angles opposite each other are called ''vertical angles'', ''opposite angles'' or ''vertically opposite angles'' (abbreviated ''vert. opp. ∠s''),<ref name="tb">{{harvnb|Wong|Wong|2009|pp=161–163}}</ref> where "vertical" refers to the sharing of a vertex, rather than an up-down orientation. A theorem states that vertical angles are always congruent or equal to each other.{{sfn|Shute| Shirk|Porter|1960|pp=25–27}}
|style = "background:#f2f2f2; text-align:center;" | Name&nbsp;&nbsp;
A [[Transversal (geometry)|''transversal'']] is a line that intersects a pair of (often parallel) lines and is associated with ''exterior angles'', ''interior angles'', ''alternate exterior angles'', ''alternate interior angles'', ''corresponding angles'', and ''consecutive interior angles''.{{sfn|Jacobs|1974|p=255}}
|style = "width:3em;" | zero angle
|style = "width:3em;" | acute angle
|style = "width:3em;" | right angle
|style = "width:3em;" | obtuse angle
|style = "width:3em;" | straight angle
|style = "width:3em;" | reflex angle
|style = "width:3em;" | full angle
|-
! Unit !! colspan=10 | [[Interval (mathematics)|Interval]]
|-
|style = "background:#f2f2f2; text-align:center;" | [[Turn (geometry)|turn]]&nbsp;&nbsp;
|style = "width:3em;" | {{nowrap|0 turn}}
|style = "width:3em;" | {{nowrap|(0, {{sfrac|1|4}}) turn}}
|style = "width:3em;" | {{nowrap|{{sfrac|1|4}} turn}}
|style = "width:3em;" | {{nowrap|({{sfrac|1|4}}, {{sfrac|1|2}}) turn}}
|style = "width:3em;" | {{nowrap|{{sfrac|1|2}} turn}}
|style = "width:3em;" | {{nowrap|({{sfrac|1|2}}, 1) turn}}
|style = "width:3em;" | {{nowrap|1 turn}}
|-
|style = "background:#f2f2f2; text-align:center;" | [[radian]]
| {{nowrap|0 rad}}
| {{nowrap|(0, {{sfrac|1|2}}''{{pi}}'') rad}}
| {{nowrap|{{sfrac|1|2}}''{{pi}}'' rad}}
| {{nowrap|({{sfrac|1|2}}''{{pi}}'', ''{{pi}}'') rad}}
| {{nowrap|''{{pi}}'' rad}}
| {{nowrap|(''{{pi}}'', 2''{{pi}}'') rad}}
| {{nowrap|2''{{pi}}'' rad}}
|-
|style = "background:#f2f2f2; text-align:center;" | [[Degree (angle)|degree]]&nbsp;&nbsp;
|style = "width:3em;" | 0°
|style = "width:3em;" | (0,&nbsp;90)°
|style = "width:3em;" | 90°
|style = "width:3em;" | (90,&nbsp;180)°
|style = "width:3em;" | 180°
|style = "width:3em;" | (180,&nbsp;360)°
|style = "width:3em;" | 360°
|-
|style = "background:#f2f2f2; text-align:center;" | [[Gradian|gon]]&nbsp;&nbsp;
|style = "width:3em;" | 0<sup>g</sup>
|style = "width:3em;" | (0,&nbsp;100)<sup>g</sup>
|style = "width:3em;" | 100<sup>g</sup>
|style = "width:3em;" | (100,&nbsp;200)<sup>g</sup>
|style = "width:3em;" | 200<sup>g</sup>
|style = "width:3em;" | (200,&nbsp;400)<sup>g</sup>
|style = "width:3em;" | 400<sup>g</sup>
|-
|}


==Types{{anchor|Types of angles}}==
=== Combining angle pairs ===
{{Redirect|Oblique angle|the cinematographic technique|Dutch angle}}
When summing two angles (either adjacent or separated in space), three special cases are named ''complementary'', ''supplementary'', and ''explementary'' angles.


===Vertical and {{vanchor|adjacent}} angle pairs===
<span class="anchor" id="Complementary angle"></span>'''''Complementary angles''''' are angle pairs whose measures sum to a right angle ({{sfrac|4}} turn, 90°, or {{sfrac|{{math|π}}|2}} rad). If the two complementary angles are adjacent, their non-shared sides form a right angle. In a [[Right triangle|right-angle triangle]] the two acute angles are complementary as the sum of the internal angles of a [[triangle]] is 180°. The difference between an angle and a right angle is termed the ''complement'' of the angle.{{sfn|Chisholm|1911}}
[[File:Vertical Angles.svg|thumb|150px|right|Angles A and B are a pair of vertical angles; angles C and D are a pair of vertical angles. [[Hatch_mark#Congruency_notation|Hatch marks]] are used here to show angle equality.]]
{{redirect-distinguish|Vertical angle|Zenith angle}}


When two straight lines intersect at a point, four angles are formed. Pairwise, these angles are named according to their location relative to each other.
<span class="anchor" id="Supplementary angle"></span>'''''Supplementary angles''''' sum to a straight angle ({{sfrac|2}} turn, 180°, or {{math|π}} rad). If the two supplementary angles are [[Angle#adjacent|adjacent]], their non-shared sides form a straight angle or [[Line (geometry)|straight line]] and are called a ''linear pair of angles''.{{sfn|Jacobs|1974|p=97}} The difference between an angle and a straight angle is termed the ''supplement'' of the angle.<ref>{{cite book |last1=Rhoad |first1=Richard |url=http://archive.org/details/geometryforenjoy00geor |title=Geometry for enjoyment and challenge |last2=Milauskas |first2=George |last3=Whipple |first3=Robert |last4=McDougal Littell |date=1991 |publisher=Evanston, Ill. : McDougal, Littell |others=Internet Archive |isbn=978-0-86609-965-3 |page=67}}</ref>
{{bulleted list
| A pair of angles opposite each other, formed by two intersecting straight lines that form an "X"-like shape, are called ''vertical angles'' or ''opposite angles'' or ''vertically opposite angles''. They are abbreviated as ''vert. opp. ∠s''.<ref name="tb">{{harvnb|Wong|Wong|2009|pp=161–163}}</ref>
{{pb}}
The equality of vertically opposite angles is called the ''vertical angle theorem''. [[Eudemus of Rhodes]] attributed the proof to [[Thales|Thales of Miletus]].<ref>{{cite book|author=Euclid|author-link=Euclid|title=The Elements|title-link=Euclid's Elements}} Proposition I:13.</ref>{{sfn|Shute| Shirk|Porter|1960|pp=25–27}} The proposition showed that since both of a pair of vertical angles are supplementary to both of the adjacent angles, the vertical angles are equal in measure. According to a historical note,{{sfn|Shute| Shirk|Porter|1960|pp=25–27}} when Thales visited Egypt, he observed that whenever the Egyptians drew two intersecting lines, they would measure the vertical angles to make sure that they were equal. Thales concluded that one could prove that all vertical angles are equal if one accepted some general notions such as:
* All straight angles are equal.
* Equals added to equals are equal.
* Equals subtracted from equals are equal.


When two adjacent angles form a straight line, they are supplementary. Therefore, if we assume that the measure of angle ''A'' equals ''x'', the measure of angle ''C'' would be {{nowrap|180° − ''x''}}. Similarly, the measure of angle ''D'' would be {{nowrap|180° − ''x''}}. Both angle ''C'' and angle ''D'' have measures equal to {{nowrap|180° − ''x''}} and are congruent. Since angle ''B'' is supplementary to both angles ''C'' and ''D'', either of these angle measures may be used to determine the measure of Angle ''B''. Using the measure of either angle ''C'' or angle ''D'', we find the measure of angle ''B'' to be {{nowrap|1=180° − (180° − ''x'') = 180° − 180° + ''x'' = ''x''}}. Therefore, both angle ''A'' and angle ''B'' have measures equal to ''x'' and are equal in measure.
<span class="anchor" id="Explementary angle"></span>'''''Explementary angles''''' or '''''conjugate angles''''' sum to a full angle (1 turn, 360°, or 2{{math|π}} radians).<ref>{{cite book |last=Willis |first=Clarence Addison |url=https://archive.org/details/planegeometryexp00willrich/page/8/ |title=Plane Geometry |publisher=Blakiston's Son |year=1922 |page=8}}</ref> The difference between an angle and a full angle is termed the ''explement'' or ''conjugate'' of the angle.<ref>{{cite book |last1=Halsted |first1=George Bruce |title=Elementary Synthetic Geometry |date=1899 |publisher=Wiley |page=7 |url=https://books.google.com/books?id=UaJXAAAAYAAJ&dq=explement&pg=PA7 }}</ref><ref>{{cite thesis |last1=Linton |first1=John Alexander |title=Phase and amplitude variation of Chandler wobble |date=1973 |publisher=University of British Columbia |doi=10.14288/1.0052929 |url=https://open.library.ubc.ca/soa/cIRcle/collections/ubctheses/831/items/1.0052929 |quote=The latitude of a point on earth is defined as the conjugate of the angle between the point where the rotation axis pierces the celestial sphere (celestial pole) and the point where the local vertical pierces the same sphere (zenith).}}</ref>


[[File:Adjacentangles.svg|right|thumb|225px|Angles ''A'' and ''B'' are adjacent.]]
Examples of non-adjacent supplementary angles include the consecutive angles of a [[parallelogram]] and opposite angles of a [[cyclic quadrilateral]]. For a circle with center O, and [[Tangent lines to circles|tangent lines]] from an exterior point P touching the circle at points T and Q, the resulting angles ∠TPQ and ∠TOQ are supplementary.
| ''Adjacent angles'', often abbreviated as ''adj. ∠s'', are angles that share a common vertex and edge but do not share any interior points. In other words, they are angles side by side or adjacent, sharing an "arm". Adjacent angles which sum to a right angle, straight angle, or full angle are special and are respectively called ''complementary'', ''supplementary'', and ''explementary'' angles (see ''{{section link|#Combining angle pairs}}'' below).
}}
A [[Transversal (geometry)|transversal]] is a line that intersects a pair of (often parallel) lines and is associated with ''exterior angles'', ''interior angles'', ''alternate exterior angles'', ''alternate interior angles'', ''corresponding angles'', and ''consecutive interior angles''.{{sfn|Jacobs|1974|p=255}}


===Combining angle pairs===
<gallery class="skin-invert-image center">
{{anchor|Angle addition postulate}}The '''angle addition postulate''' states that if B is in the interior of angle AOC, then
File:Complement angle.svg|Angles <code>a</code> and <code>b</code> are ''complementary'' angles
File:Angle obtuse acute straight.svg|Angles <code>a</code> and <code>b</code> are ''supplementary'' angles
File:Conjugate_Angles.svg|Angles <code>AOB</code> and <code>COD</code> are ''explementary'' ''or conjugate'' angles
</gallery>


<math display="block"> m\angle \mathrm{AOC} = m\angle \mathrm{AOB} + m\angle \mathrm{BOC} </math>
=== Polygon-related angles ===
[[File:ExternalAngles.svg|thumb|class=skin-invert-image|Internal and external angles]]
* An angle that is part of a [[simple polygon]] is called an ''[[interior angle]]'' if it lies on the inside of that simple polygon. A simple [[concave polygon]] has at least one interior angle, that is, a reflex angle. {{pb}}<!--pb


I.e., the measure of the angle AOC is the sum of the measure of angle AOB and the measure of angle BOC.
--> In [[Euclidean geometry]], the measures of the interior angles of a [[triangle]] add up to {{math|π}} radians, 180°, or {{sfrac|2}} turn; the measures of the interior angles of a simple [[convex polygon|convex]] [[quadrilateral]] add up to 2{{math|π}} radians, 360°, or 1 turn. In general, the measures of the interior angles of a simple convex [[polygon]] with ''n'' sides add up to (''n''&nbsp;−&nbsp;2){{math|π}}&nbsp;radians, or (''n''&nbsp;−&nbsp;2)180&nbsp;degrees, (''n''&nbsp;−&nbsp;2)2 right angles, or (''n''&nbsp;−&nbsp;2){{sfrac|1|2}}&nbsp;turn.
* The supplement of an interior angle is called an ''[[exterior angle]]''; that is, an interior angle and an exterior angle form a [[#Linear pair of angles|linear pair of angles]]. There are two exterior angles at each vertex of the polygon, each determined by extending one of the two sides of the polygon that meet at the vertex; these two angles are vertical and hence are equal. An exterior angle measures the amount of rotation one must make at a vertex to trace the polygon.{{sfn|Henderson|Taimina|2005|p=104}} If the corresponding interior angle is a reflex angle, the exterior angle should be considered [[Negative number|negative]]. Even in a non-simple polygon, it may be possible to define the exterior angle. Still, one will have to pick an [[orientation (space)|orientation]] of the [[plane (mathematics)|plane]] (or [[surface (mathematics)|surface]]) to decide the sign of the exterior angle measure. {{pb}} <!--pb


Three special angle pairs involve the summation of angles:
{{anchor|complementary angle}}
[[File:Complement angle.svg|thumb|150px|The ''complementary'' angles <var>a</var> and <var>b</var> (<var>b</var> is the ''complement'' of <var>a</var>, and <var>a</var> is the complement of <var>b</var>.)]]
{{bulleted list
| ''Complementary angles'' are angle pairs whose measures sum to one right angle ({{sfrac|4}} turn, 90°, or {{sfrac|{{math|π}}|2}} radians).<ref>{{Cite web|title=Complementary Angles|url=https://www.mathsisfun.com/geometry/complementary-angles.html|access-date=2020-08-17 | website=www.mathsisfun.com}}</ref> If the two complementary angles are adjacent, their non-shared sides form a right angle. In Euclidean geometry, the two acute angles in a right triangle are complementary because the sum of internal angles of a [[triangle]] is 180 degrees, and the right angle accounts for 90 degrees.
{{pb}}
The adjective complementary is from the Latin ''complementum'', associated with the verb ''complere'', "to fill up". An acute angle is "filled up" by its complement to form a right angle.
{{pb}}
The difference between an angle and a right angle is termed the ''complement'' of the angle.<ref name="Chisholm 1911">{{harvnb|Chisholm|1911}}</ref>
{{pb}}
If angles ''A'' and ''B'' are complementary, the following relationships hold: <math display="block">
\begin{align}
& \sin^2A + \sin^2B = 1 & & \cos^2A + \cos^2B = 1 \\[3pt]
& \tan A = \cot B  & & \sec A = \csc B
\end{align}</math>
{{pb}}
(The [[tangent]] of an angle equals the [[cotangent]] of its complement, and its secant equals the [[cosecant]] of its complement.)
{{pb}}
The [[prefix]] "[[co (function prefix)|co-]]" in the names of some trigonometric ratios refers to the word "complementary".
{{clear|right}}
[[File:Angle obtuse acute straight.svg|thumb|right|300px|The angles <var>a</var> and <var>b</var> are ''supplementary'' angles.]]
| {{anchor|Linear pair of angles|Supplementary angle}}Two angles that sum to a straight angle ({{sfrac|2}} turn, 180°, or {{math|π}} radians) are called ''supplementary angles''.<ref>{{Cite web|title=Supplementary Angles|url=https://www.mathsisfun.com/geometry/supplementary-angles.html|access-date=2020-08-17 | website=www.mathsisfun.com}}</ref>
{{pb}}
If the two supplementary angles are [[#adjacent|adjacent]] (i.e., have a common [[vertex (geometry)|vertex]] and share just one side), their non-shared sides form a [[line (geometry)|straight line]]. Such angles are called a ''linear pair of angles''.{{sfn|Jacobs|1974|p=97}} However, supplementary angles do not have to be on the same line and can be separated in space. For example, adjacent angles of a [[parallelogram]] are supplementary, and opposite angles of a [[cyclic quadrilateral]] (one whose vertices all fall on a single circle) are supplementary.
{{pb}}
If a point P is exterior to a circle with center O, and if the [[tangent lines to circles|tangent lines]] from P touch the circle at points T and Q, then ∠TPQ and ∠TOQ are supplementary.
{{pb}}
The sines of supplementary angles are equal. Their cosines and tangents (unless undefined) are equal in magnitude but have opposite signs.
{{pb}}
In Euclidean geometry, any sum of two angles in a triangle is supplementary to the third because the sum of the internal angles of a triangle is a straight angle.
{{clear|right}}
{{anchor|explementary angle}}
[[File:Conjugate Angles.svg|thumb|Angles AOB and COD are conjugate as they form a complete angle. Considering magnitudes, 45° + 315° = 360°.]]
| Two angles that sum to a complete angle (1 turn, 360°, or 2{{math|π}} radians) are called ''explementary angles'' or ''conjugate angles''.<ref>{{cite book |last=Willis |first=Clarence Addison |year=1922 |publisher=Blakiston's Son |title=Plane Geometry |page=8 |url=https://archive.org/details/planegeometryexp00willrich/page/8/ }}</ref>
{{pb}}
The difference between an angle and a complete angle is termed the ''explement'' of the angle or ''conjugate'' of an angle.
{{clear|right}}
}}
===Polygon-related angles===
[[File:ExternalAngles.svg|thumb|300px|right|Internal and external angles]]
* An angle that is part of a [[simple polygon]] is called an ''[[interior angle]]'' if it lies on the inside of that simple polygon. A simple [[concave polygon]] has at least one interior angle, that is, a reflex angle. {{pb}} <!-- --> In [[Euclidean geometry]], the measures of the interior angles of a [[triangle]] add up to {{math|π}} radians, 180°, or {{sfrac|2}} turn; the measures of the interior angles of a simple [[convex polygon|convex]] [[quadrilateral]] add up to 2{{math|π}} radians, 360°, or 1 turn. In general, the measures of the interior angles of a simple convex [[polygon]] with ''n'' sides add up to (''n''&nbsp;−&nbsp;2){{math|π}}&nbsp;radians, or (''n''&nbsp;−&nbsp;2)180&nbsp;degrees, (''n''&nbsp;−&nbsp;2)2 right angles, or (''n''&nbsp;−&nbsp;2){{sfrac|1|2}}&nbsp;turn.
* The supplement of an interior angle is called an ''[[exterior angle]]''; that is, an interior angle and an exterior angle form a [[#Linear pair of angles|linear pair of angles]]. There are two exterior angles at each vertex of the polygon, each determined by extending one of the two sides of the polygon that meet at the vertex; these two angles are vertical and hence are equal. An exterior angle measures the amount of rotation one must make at a vertex to trace the polygon.{{sfn|Henderson|Taimina|2005|p=104}} If the corresponding interior angle is a reflex angle, the exterior angle should be considered [[Negative number|negative]]. Even in a non-simple polygon, it may be possible to define the exterior angle. Still, one will have to pick an [[orientation (space)|orientation]] of the [[plane (mathematics)|plane]] (or [[surface (mathematics)|surface]]) to decide the sign of the exterior angle measure. {{pb}} <!--
--> In Euclidean geometry, the sum of the exterior angles of a simple convex polygon, if only one of the two exterior angles is assumed at each vertex, will be one full turn (360°). The exterior angle here could be called a ''supplementary exterior angle''. Exterior angles are commonly used in [[Logo (programming language)|Logo Turtle programs]] when drawing regular polygons.
--> In Euclidean geometry, the sum of the exterior angles of a simple convex polygon, if only one of the two exterior angles is assumed at each vertex, will be one full turn (360°). The exterior angle here could be called a ''supplementary exterior angle''. Exterior angles are commonly used in [[Logo (programming language)|Logo Turtle programs]] when drawing regular polygons.
* In a [[triangle]], the [[bisection|bisectors]] of two exterior angles and the bisector of the other interior angle are [[concurrent lines|concurrent]] (meet at a single point).<ref name=Johnson>Johnson, Roger A. ''Advanced Euclidean Geometry'', Dover Publications, 2007.</ref>{{rp|p=149}}
* In a [[triangle]], the [[bisection|bisectors]] of two exterior angles and the bisector of the other interior angle are [[concurrent lines|concurrent]] (meet at a single point).<ref name=Johnson>Johnson, Roger A. ''Advanced Euclidean Geometry'', Dover Publications, 2007.</ref>{{rp|p=149}}
* In a triangle, three intersection points, each of an external angle bisector with the opposite [[extended side]], are [[collinearity|collinear]].<ref name=Johnson/>{{rp|p=149}}
* In a triangle, three intersection points, each of an external angle bisector with the opposite [[extended side]], are [[collinearity|collinear]].<ref name=Johnson/>{{rp|p=149}}
* In a triangle, three intersection points, two between an interior angle bisector and the opposite side, and the third between the other exterior angle bisector and the opposite side extended are collinear.<ref name=Johnson/>{{rp|p=149}}
* In a triangle, three intersection points, two between an interior angle bisector and the opposite side, and the third between the other exterior angle bisector and the opposite side extended are collinear.<ref name=Johnson/>{{rp|p=149}}
* Some authors use the name ''exterior angle'' of a simple polygon to mean the ''explement exterior angle'' (''not'' supplement!) of the interior angle.<ref>{{citation|editor=D. Zwillinger|title=CRC Standard Mathematical Tables and Formulae|place=Boca Raton, FL|publisher=CRC Press | year=1995 | page= 270}} as cited in {{MathWorld |urlname=ExteriorAngle |title=Exterior Angle}}</ref> This conflicts with the above usage.
* Some authors use the name ''exterior angle'' of a simple polygon to mean the ''explement exterior angle'' (''not'' supplement!) of the interior angle.<ref>{{citation |editor=D. Zwillinger |title=CRC Standard Mathematical Tables and Formulae |place=Boca Raton, FL |publisher=CRC Press | year=1995 | page= 270}} as cited in {{MathWorld |urlname=ExteriorAngle |title=Exterior Angle}}</ref> This conflicts with the above usage.


===Plane-related angles===
=== Plane-related angles ===
* The angle between two [[Plane (mathematics)|planes]] (such as two adjacent faces of a [[polyhedron]]) is called a ''[[dihedral angle]]''.<ref name="Chisholm 1911"/> It may be defined as the acute angle between two lines [[Normal (geometry)|normal]] to the planes.
* The angle between two [[Plane (mathematics)|planes]] (such as two adjacent faces of a [[polyhedron]]) is called a ''[[dihedral angle]]''.{{sfn|Chisholm|1911}} It may be defined as the acute angle between two lines [[Normal (geometry)|normal]] to the planes.
* The angle between a plane and an intersecting straight line is complementary to the angle between the intersecting line and the [[normal (geometry)|normal]] to the plane.
* The angle between a plane and an intersecting straight line is complementary to the angle between the intersecting line and the [[normal (geometry)|normal]] to the plane.


==Measuring angles{{anchor|Measurement}}==<!-- linked from [[Degree (angle)]] -->
== Measuring angles <span class="anchor" id="Measurement"></span> ==
{{see also|Angle measuring instrument}}
<!-- linked from [[Degree (angle)]] -->
[[File:Basic angle in circle.svg|thumb|300x300px|The angle size <math>\theta</math> can be measured as s/r radians or s/C turns]]
{{see also|List of measuring instruments#Angle}}
Measurement of angles is intrinsically linked with circles and rotation. An angle is measured by placing it within a circle of any size, with the vertex at the circle's centre and the sides intersecting the perimeter.  
Angle measurement encompasses both direct physical measurement using a measuring instrument such as a [[protractor]], as well as the theoretical calculation of angle size from other known quantities. While the measurement of angles is intrinsically linked with rotation and circles, there are various perspectives as to exactly ''what'' is being measured, including amongst others: the amount of rotation about the vertex of one ray to the other;<ref>{{Cite book |last=Serra |first=Michael |url=http://archive.org/details/Discovering_Geometry_An_Investigative_Approach_by_Michael_Serra |title=Discovering geometry : an investigative approach |date=2008 |publisher=Emeryville, CA : Key Curriculum Press |isbn=978-1-55953-882-4}}</ref> the amount of opening between the rays;<ref>{{Cite book |last=Alexander |first=Daniel C. |url=http://archive.org/details/elementarygeomet0000alex_o5k5_4ed |title=Elementary geometry for college students |date=2006 |publisher=Boston, MA : Houghton Mifflin |others=Internet Archive |isbn=978-0-618-64525-1}}</ref> or the length of the arc that subtends the angle at the centre of a unit circle.<ref name="SIBrochure9thEd" />


An [[circular arc|arc]] <var>s</var> is formed as the shortest distance on the perimeter between the two points of intersection, which is said to be the arc [[Subtended angle|subtended]] by the angle.  
The measurement of angles is inherently different from the measurement of other physical quantities such as length.<ref>{{Cite journal |last1=Grötschel |first1=Martin |last2=Hanche-Olsen |first2=Harald |last3=Holden |first3=Helge |last4=Krystek |first4=Michael P. |date=2022 |title=On Angular Measures in Axiomatic Euclidean Planar Geometry |url=https://sciendo.com/article/10.2478/msr-2022-0019 |journal=Measurement Science Review |volume=22 |issue=4 |pages=152–159 |doi=10.2478/msr-2022-0019 |bibcode=<!-- useless bibcode: 2022MeScR..22..152G --> |hdl=11250/3033842 }}</ref> Angles of special significance (such as the right angle) inform the systems and units of angular measurement, which is not the case for length where the units of measurement (metres, feet) are arbitrary.


The length of ''s'' can be used to measure the angle's size <math>\theta</math>, however as ''s'' is dependent on the size of the circle chosen, it must be adjusted so that any arbitrary circle will give the same measure of angle. This can be done in two ways: by taking the ratio to either the radius ''r'' or circumference ''C'' of the circle.
Broadly there are two approaches to measuring angles: relative to a reference angle (such as a right angle); and circular measurement.


The ratio of the length <var>s</var> by the radius <var>r</var> is the number of [[radian]]s in the angle, while the ratio of length <var>s</var> by the circumference <var>C</var> is the number of [[Turn (angle)|turns]]:<ref name="SIBrochure9thEd">{{citation |author=International Bureau of Weights and Measures |title=The International System of Units (SI) |date=20 May 2019 |url=https://www.bipm.org/utils/common/pdf/si-brochure/SI-Brochure-9.pdf |archive-url=https://web.archive.org/web/20211018184555/https://www.bipm.org/documents/20126/41483022/SI-Brochure-9.pdf/fcf090b2-04e6-88cc-1149-c3e029ad8232 |archive-date=18 October 2021 |url-status=live |edition=9th |isbn=978-92-822-2272-0 |author-link=New SI}}</ref>
=== Reference angle ===
<math display="block"> \theta = \frac{s}{r} \, \mathrm{rad}. </math><math display="block"> \theta = \frac{s}{ C} \ = \frac{s}{2\pi r} \, \mathrm{turns} </math>
A chosen reference angle (right angle, straight angle or full angle) can be divided into equal parts, and the size of one part used as a unit for measurement of other angles.


[[File:Angle measure.svg|right|thumb|The measure of angle {{math|''θ''}} is {{nowrap|{{sfrac|''s''|''r''}} radians}}.]]
In the most common method of practical angular measurement a right angle is divided into 90 equal parts called [[Degree (angle)|degrees]], while in the rarely used ''centesimal'' system, a right angle is divided into 100 equal parts called [[gradian]]s.<ref>{{cite book |last=Loney |first=Sidney Luxton |title=Plane trigonometry |date=1893 |page=1}}</ref><ref name=":2" />


The value of {{math|''θ''}} thus defined is independent of the size of the circle: if the length of the radius is changed, then both the circumference and the arc length change in the same proportion, so the ratios <math>\frac{s}{r}</math>and <math>\frac{s}{C}</math> are unaltered.{{refn|group="nb"|This approach requires, however, an additional proof that the measure of the angle does not change with changing radius {{math|''r''}}, in addition to the issue of "measurement units chosen". A smoother approach is to measure the angle by the length of the corresponding unit circle arc. Here "unit" can be chosen to be dimensionless in the sense that it is the real number 1 associated with the unit segment on the real line. See Radoslav M. Dimitrić, for instance.<ref name="Dimitric_2012"/>}}
=== Circular measurement ===
[[File:Basic angle in circle.svg|thumb|class=skin-invert-image|The angle size <math>\theta</math> can be measured as ''s''/''r'' radians or ''s''/''C'' turns]]
With circular measurement an angle is placed within a circle of any size, with the vertex at the circle's centre and the sides intersecting the perimeter.


Angles of the same size are said to be ''equal'' ''congruent'' or ''equal in measure''.
An [[circular arc|arc]] with length <var>s</var> is formed as the perimeter between the two points of intersection, which is said to [[Subtended angle|subtend]] the angle. The length ''s'' can be used to measure the angle's size ''θ'', however as ''s'' is dependent on the size of the circle chosen, the measure must be scaled. This can be done by taking the ratio of ''s'' to either the radius ''r'' or circumference ''C'' of the circle.


=== Units ===
The ratio of the length <var>s</var> by the radius <var>r</var> is the number of [[radian]]s in the angle,<ref name="SIBrochure9thEd">{{citation |author=International Bureau of Weights and Measures |title=The International System of Units (SI) |date=2019 |url=https://www.bipm.org/utils/common/pdf/si-brochure/SI-Brochure-9.pdf |archive-url=https://web.archive.org/web/20211018184555/https://www.bipm.org/documents/20126/41483022/SI-Brochure-9.pdf/fcf090b2-04e6-88cc-1149-c3e029ad8232 |archive-date=18 October 2021 |url-status=live |edition=9th |isbn=978-92-822-2272-0 |author-link=New SI}}</ref> while the ratio of length <var>s</var> by the circumference <var>C</var> is the number of [[Turn (angle)|turns]]:
In addition to the radian and turn, other angular units exist, typically based on subdivisions of the turn, including the [[degree (angle)|degree]] ( ° ) and the [[gradian]] (grad), though many others have been used throughout [[History of Mathematics|history]].<ref>{{Cite web |title=angular unit |url=https://www.thefreedictionary.com/angular+unit |access-date=2020-08-31 |website=TheFreeDictionary.com}}</ref>  
<math display="block">\theta = \frac{s}{r} \, \mathrm{rad} = \frac{s}{C} \, \mathrm{turn} = \frac{s}{2\pi r} \, \mathrm{turn}</math>
[[File:Radian measurement.svg|thumb|class=skin-invert-image|The radian measure of {{math|''θ''}}<math display="block">\theta = \frac{s}{r} = \frac{s}{s_N}</math>]]
The value of {{math|''θ''}} thus defined is independent of the size of the circle: if the length of the radius is changed, then both the circumference and the arc length change in the same proportion, so the ratios {{sfrac|''s''|''r''}} and {{sfrac|''s''|''C''}} are unaltered.{{refn|group="nb"|This approach requires, however, an additional proof that the measure of the angle does not change with changing radius {{math|''r''}}, in addition to the issue of "measurement units chosen". A smoother approach is to measure the angle by the length of the corresponding unit circle arc. Here "unit" can be chosen to be dimensionless in the sense that it is the real number 1 associated with the unit segment on the real line. See {{harvtxt|Dimitrić|2012}}, for instance.}}


Conversion between units may be obtained by multiplying the anglular measure in one unit by a conversion constant of the form <math>\frac{k_a}{k_b}</math> where <math>{k_a}</math> and <math>{k_b}</math> are the measures of a complete turn expressed in units a and b. For example, {{nowrap|1= ''k'' = 360°}} for [[degree (angle)|degrees]] or 400 grad for [[gradian]]s):<math display="block"> \theta_\deg = \frac{360}{2\pi} \cdot \theta </math>The following table lists some units used to represent angles.
The ratio {{sfrac|''s''|''r''}} is called the "radian measure"<ref name=":1" /> or "circular measure"<ref name=":3">{{cite book |last=Loney |first=Sidney Luxton |url=https://name.umdl.umich.edu/abn7298.0001.001 |title=Plane trigonometry |date=1893 |page=5}}</ref><ref name=":2">{{cite book |last=Todhunter |first=Isaac |url=https://books.google.com/books?id=bo5FAAAAcAAJ&pg=PA10 |title=Plane Trigonometry: For the Use of Colleges and Schools. With Numerous Examples |date=1864 |publisher=MacMillan and Company }}</ref><ref>{{cite web |title=Earliest Known Uses of Some of the Words of Mathematics (R) |url=https://mathshistory.st-andrews.ac.uk/Miller/mathword/r/ |access-date=2025-08-01 |website=Maths History }}</ref> of an angle, but is also used to define a [[unit of measurement]] called a radian, which is defined as an angle for which the ratio {{sfrac|''s''|''r''}} = 1.<ref name=":3" /> Thus, the measurement of an angle given by {{sfrac|''s''|''r''}} can be thought of in two ways: firstly as a measure in terms of the angle's own proportions (ratio of arc length to radius), or secondly as the quantity of units in the angle (ratio of arc length of measured angle to arc length of unit angle).<ref>{{cite journal |last1=Quincey |first1=Paul |title=Angles are inherently neither length ratios nor dimensionless |date=2019 |arxiv=1909.08389 |last2=Mohr |first2=Peter J. |last3=Phillips |first3=William D. |journal=Metrologia |volume=56 |issue=4 |page=043001 |doi=10.1088/1681-7575/ab27d7 |bibcode=<!-- useless bibcode: 2019Metro..56d3001Q --> }}</ref><ref name=":2" />


=== Units ===
The following table lists some notable units used to represent angles.
{|class = "wikitable"
{|class = "wikitable"
!Name !!Number in one turn!!In degrees !!Description
!Name (symbol) !! Number in one turn !! 1 unit in degrees !! Description
|-
|[[radian]]||{{math|2''π''}}||≈57°17′45″||The ''radian'' is determined by the circumference of a circle that is equal in length to the radius of the circle (''n''&nbsp;=&nbsp;2{{pi}}&nbsp;=&nbsp;6.283...). It is the angle subtended by an arc of a circle that has the same length as the circle's radius. The symbol for radian is ''rad''. One turn is 2{{math|π}}&nbsp;radians, and one radian is {{sfrac|180°|{{pi}}}}, or about 57.2958 degrees. Often, particularly in mathematical texts, one radian is assumed to equal one, resulting in the unit ''rad'' being omitted. The radian is used in virtually all mathematical work beyond simple, practical geometry due, for example, to the pleasing and "natural" properties that the [[trigonometric function]]s display when their arguments are in radians. The radian is the (derived) unit of angular measurement in the [[SI]].
|-
|[[degree (angle)|degree]] ||360 ||1°|| The ''degree'', denoted by a small superscript circle (°), is 1/360 of a turn, so one ''turn'' is 360°. One advantage of this old [[sexagesimal]] subunit is that many angles common in simple geometry are measured as a whole number of degrees. Fractions of a degree may be written in normal decimal notation (e.g., 3.5° for three and a half degrees), but the [[Minute and second of arc|"minute" and "second"]] sexagesimal subunits of the "degree–minute–second" system (discussed next) are also in use, especially for [[Geographic coordinate system|geographical coordinates]] and in [[astronomy]] and [[ballistics]] (''n''&nbsp;=&nbsp;360)
|-
| [[arcminute]]||21,600 ||0°1′|| The ''minute of arc'' (or ''MOA'', ''arcminute'', or just ''minute'') is {{sfrac|60}} of a degree = {{sfrac|21,600}} turn. It is denoted by a single prime (&nbsp;′&nbsp;). For example, 3°&nbsp;30′ is equal to 3&nbsp;×&nbsp;60&nbsp;+&nbsp;30&nbsp;=&nbsp;210 minutes or 3&nbsp;+&nbsp;{{sfrac|30|60}} = 3.5 degrees. A mixed format with decimal fractions is sometimes used, e.g., 3°&nbsp;5.72′ = 3&nbsp;+&nbsp;{{sfrac|5.72|60}} degrees. A [[nautical mile]] was historically defined as an arcminute along a [[great circle]] of the Earth. (''n''&nbsp;=&nbsp;21,600). 
|-
| [[arcsecond]]||1,296,000 ||0°0′1″||The ''second of arc'' (or ''arcsecond'', or just ''second'') is {{sfrac|60}} of a minute of arc and {{sfrac|3600}} of a degree (''n''&nbsp;=&nbsp;1,296,000). It is denoted by a double prime (&nbsp;″&nbsp;). For example, 3°&nbsp;7′&nbsp;30″ is equal to 3 + {{sfrac|7|60}} + {{sfrac|30|3600}} degrees, or 3.125&nbsp;degrees. The arcsecond is the angle used to measure a [[parsec]]
|-
| [[grad (angle)|grad]]||400 ||0°54′ || The ''grad'', also called ''grade'', ''[[gradian]]'', or ''gon''. It is a decimal subunit of the quadrant. A right angle is 100 grads. A [[kilometre]] was historically defined as a [[centi]]-grad of arc along a [[meridian (geography)|meridian]] of the Earth, so the kilometer is the decimal analog to the [[sexagesimal]] [[nautical mile]] (''n''&nbsp;=&nbsp;400). The grad is used mostly in [[triangulation (surveying)|triangulation]] and continental [[surveying]].
|-
|[[turn (geometry)|turn]]||1||360° || The ''turn'' is the angle subtended by the circumference of a circle at its centre. A turn is equal to 2{{pi}} or [[Turn_(angle)#Proposals_for_a_single_letter_to_represent_2π|{{tau}} (tau)]] radians.
|-
| [[hour angle]] || 24 || 15° || The astronomical ''hour angle'' is {{sfrac|24}}&nbsp;turn. As this system is amenable to measuring objects that cycle once per day (such as the relative position of stars), the sexagesimal subunits are called ''minute of time'' and ''second of time''. These are distinct from, and 15 times larger than, minutes and seconds of arc. 1&nbsp;hour = 15° = {{sfrac|{{pi}}|12}}&nbsp;rad = {{sfrac|6}}&nbsp;quad = {{sfrac|24}}&nbsp;turn = {{sfrac|16|2|3}}&nbsp;grad.
|-
| [[Points of the compass|(compass) point]] || 32 || 11°15′ || The ''point'' or ''wind'', used in [[navigation]], is {{sfrac|32}} of a turn. 1&nbsp;point = {{sfrac|8}} of a right angle = 11.25° = 12.5&nbsp;grad. Each point is subdivided into four quarter points, so one turn equals 128.
|-
| [[milliradian]] || {{math|2000''π''}} || ≈0.057° || The true milliradian is defined as a thousandth of a radian, which means that a rotation of one [[Turn (geometry)|turn]] would equal exactly 2000π&nbsp;mrad (or approximately 6283.185&nbsp;mrad). Almost all [[Telescopic sight|scope sights]] for [[firearm]]s are calibrated to this definition. In addition, three other related definitions are used for artillery and navigation, often called a 'mil', which are ''approximately'' equal to a milliradian. Under these three other definitions, one turn makes up for exactly 6000, 6300, or 6400 mils, spanning the range from 0.05625 to 0.06 degrees (3.375 to 3.6 minutes). In comparison, the milliradian is approximately 0.05729578 degrees (3.43775 minutes). One "[[NATO]] mil" is defined as {{sfrac|6400}} of a turn. Just like with the milliradian, each of the other definitions approximates the milliradian's useful property of subtensions, i.e. that the value of one milliradian approximately equals the angle subtended by a width of 1 meter as seen from 1&nbsp;km away ({{sfrac|2{{pi}}|6400}} = 0.0009817... ≈ {{sfrac|1000}}).
|-
|[[Binary angular measurement|binary degree]] ||256||1°33′45″  || The ''binary degree'', also known as the ''[[binary radian]]'' or ''brad'' or ''binary angular measurement (BAM)''.<ref name="ooPIC"/> The binary degree is used in computing so that an angle can be efficiently represented in a single [[byte]] (albeit to limited precision). Other measures of the angle used in computing may be based on dividing one whole turn into 2<sup>''n''</sup> equal parts for other values of ''n''.
<ref name="Hargreaves_2010"/> It is {{sfrac|256}} of a turn.<ref name="ooPIC"/>
|-
|-
|{{anchor|Multiples of π}}{{pi}} radian||2||180° || The ''multiples of {{pi}} radians'' (MUL{{pi}}) unit is implemented in the [[Reverse Polish Notation|RPN]] scientific calculator [[WP&nbsp;43S]].<ref name="Bonin_2016"/> See also: [[IEEE 754 recommended operations]]
| [[turn (geometry)|turn]] || 1 || 360° || The ''turn'' is the angle subtended by the circumference of a circle at its centre. A turn is equal to 2{{pi}} or [[Tau (mathematics)|{{tau}}]] radians.
|-
|-
|[[circular sector|quadrant]]||4||90°||One ''quadrant'' is a {{sfrac|4}}&nbsp;turn and also known as a ''[[right angle]]''. The quadrant is the unit in [[Euclid's Elements]]. In German, the symbol <sup>∟</sup> has been used to denote a quadrant. 1 quad = 90° = {{sfrac|{{pi}}|2}}&nbsp;rad = {{sfrac|4}} turn = 100&nbsp;grad.
| [[degree (angle)|degree]] (&nbsp;°&nbsp;)
| 360 || || The ''degree'' may be defined such that one ''turn'' is equal to 360 degrees.
|-
|-
|[[circular sector|sextant]]||6||60°||The ''sextant'' was the unit used by the [[Babylonians]],<ref name="Jeans_1947"/><ref name="Murnaghan_1946"/> The degree, minute of arc and second of arc are [[sexagesimal]] subunits of the Babylonian unit. It is straightforward to construct with ruler and compasses. It is the ''angle of the [[equilateral triangle]]'' or is {{sfrac|6}}&nbsp;turn. 1 Babylonian unit = 60° = {{pi}}/3&nbsp;rad ≈ 1.047197551&nbsp;rad.
| [[radian]] (rad)
| {{math|2''π''}} || {{val|57.2957|end=...|u=°}} || The ''radian'' is the angle subtended by an arc of a circle that has the same length as the circle's radius.
|-
|-
| hexacontade||60 ||||The ''hexacontade'' is a unit used by [[Eratosthenes]]. It equals 6°, so a whole turn was divided into 60 hexacontades.
| [[grad (angle)|grad]] (gon)
| 400 || 0.9° || The ''grad'', also called ''grade'', ''[[gradian]]'', or ''gon'', is defined such that a right angle is equal to as 100 gradians. The grad is used mostly in [[triangulation (surveying)|triangulation]] and continental [[surveying]].
|-
|-
| [[pechus]]|| 144 to 180 || 2° to 2°30′ || The ''pechus'' was a [[Babylonian mathematics|Babylonian]] unit equal to about 2° or {{sfrac|2|1|2}}°.
| [[arcminute]] (&nbsp;′&nbsp;)
| {{val|21600}} || {{sfrac|1|60}}° || The ''minute of arc'' (or ''arcminute'', or just ''minute'') is a sexagesimal subunit of a degree.
|-
|-
| diameter part || ≈376.991 || ≈0.95493° || The ''diameter part'' (occasionally used in Islamic mathematics) is {{sfrac|60}} radian. One "diameter part" is approximately 0.95493°. There are about 376.991 diameter parts per turn.
| [[arcsecond]] (&nbsp;″&nbsp;)
| {{val|1296000}} || {{sfrac|1|3600}}° ||The ''second of arc'' (or ''arcsecond'', or just ''second'') is a sexagesimal subunit of a minute of arc.
|-
|-
| zam || 224 || ≈1.607° || In old Arabia, a [[Turn (geometry)|turn]] was subdivided into 32 Akhnam, and each akhnam was subdivided into 7 zam so that a [[Turn (geometry)|turn]] is 224 zam.
| [[milliradian]] (mrad)
| {{math|2000{{px2}}''π''}} || {{val|0.05729|end=...|u=°}} || The milliradian is a thousandth of a radian. For artillery and navigation a unit is used, often called a 'mil', which are ''approximately'' equal to a milliradian. One turn is exactly 6000, 6300, or 6400 mils, depending on which definition is used.
|}
|}


===Dimensional analysis===
=== Dimensional analysis ===
{{Further|Radian#Dimensional analysis}}
{{Further|Radian#Dimensional analysis}}
In mathematics and the [[International System of Quantities]], an angle is defined as a dimensionless quantity, and in particular, the [[radian]] unit is dimensionless. This convention impacts how angles are treated in [[dimensional analysis]]. For example, when one measures an angle in radians by dividing the arc length by the radius, one is essentially dividing a length by another length, and the units of length cancel each other out. Therefore the result—the angle—doesn't have a physical "dimension" like meters or seconds. This holds true with all angle units, such as radians, degrees, or turns—they all represent a pure number quantifying how much something has turned. This is why, in many equations, angle units seem to "disappear" during calculations, which can sometimes be a bit confusing.
In mathematics and the [[International System of Quantities]], an angle is defined as a dimensionless quantity,<ref>{{cite web |title=ISO 80000-3:2006 Quantities and Units - Space and Time |date=2017 |url=https://www.iso.org/standard/31888.html}}</ref> and in particular, the [[radian]] is defined as dimensionless in the [[International System of Units]].<ref>{{SIbrochure9th|page=137}}</ref> This convention prevents angles providing information for [[dimensional analysis]]. For example, when one measures an angle in radians by dividing the arc length by the radius, one is essentially dividing a length by another length, and the units of length cancel each other out. Therefore the result—the angle—doesn't have a physical "dimension" like meters or seconds.<ref>{{cite book |last1=Leonard |first1=William J. |url=https://books.google.com/books?id=ShcCF5Gb408C&pg=PA262 |title=Minds-on Physics: Advanced topics in mechanics |date=1999 |publisher=Kendall Hunt |isbn=978-0-7872-5412-4 |page=262 }}</ref> This holds true with all angle units, such as radians, degrees, or turns—they all represent a pure number quantifying how much something has turned.<ref>{{cite journal |last1=French |first1=Anthony P. |date=1992 |title=What happens to the 'radians'? (comment) |journal=The Physics Teacher |volume=30 |issue=5 |pages=260–261 |doi=10.1119/1.2343535}}</ref> This is why, in many equations, angle units seem to "disappear" during calculations, which feels inconsistent and can lead to mixing up angle units.<ref>{{cite journal |last1=Prando |first1=Giacomo |date=2020 |title=A spectral unit |journal=Nature Physics |volume=16 |issue=8 |pages=888 |bibcode=<!-- useless bibcode: 2020NatPh..16..888P --> |doi=10.1038/s41567-020-0997-3 |doi-access=free }}</ref><ref>{{cite journal |last1=Oberhofer |first1=E. S. |date=1992 |title=What happens to the 'radians'? |journal=The Physics Teacher |volume=30 |issue=3 |pages=170–171 |bibcode=<!-- useless bibcode: 1992PhTea..30..170O --> |doi=10.1119/1.2343500}}</ref>


This disappearing act, while mathematically convenient, has led to significant discussion among scientists and teachers, as it can be tricky to explain and feels inconsistent. To address this, some scientists have suggested treating the angle as having its own fundamental dimension, similar to length or time. This would mean that angle units like radians would always be explicitly present in calculations, making the dimensional analysis more straightforward. However, this approach would also require changing many well-known mathematical and physics formulas, making them longer and perhaps a bit less familiar. For now, the established practice is to consider angles dimensionless, understanding that while units like radians are important for expressing the angle's magnitude, they don't carry a physical dimension in the same way that meters or kilograms do.
This has led to significant discussion among scientists and educators. Some scientists have suggested treating the angle as having its own fundamental dimension, similar to length or time.<ref name="Quincey">{{cite journal |last1=Quincey |first1=Paul |last2=Brown |first2=Richard J C |date=2016 |title=Implications of adopting plane angle as a base quantity in the SI |journal=Metrologia |volume=53 |issue=3 |pages=998–1002 |arxiv=1604.02373 |bibcode=<!-- useless bibcode: 2016Metro..53..998Q --> |doi=10.1088/0026-1394/53/3/998 }}</ref> This would mean that angle units like radians would always be explicitly present in calculations, facilitating dimensional analysis. However, this approach would also require changing many well-known mathematical and physics formulas, making them longer and perhaps a bit less familiar.<ref>{{cite journal |last1=Quincey |first1=Paul |title=Angles in the SI: a detailed proposal for solving the problem |journal=Metrologia |date=2021 |volume=58 |issue=5 |pages=053002 |doi=10.1088/1681-7575/ac023f |arxiv=2108.05704 |bibcode=<!-- useless bibcode: 2021Metro..58e3002Q --> }}</ref> For now, the established practice is to write angle units where appropriate but consider them dimensionless, understanding that these units are important but behave differently from meters or kilograms.<ref>{{cite journal |last1=Aubrecht |first1=Gordon J. |last2=French |first2=Anthony P. |last3=Iona |first3=Mario |last4=Welch |first4=Daniel W. |date=1993 |title=The radian—That troublesome unit |journal=The Physics Teacher |volume=31 |issue=2 |pages=84–87 |bibcode=<!-- useless bibcode: 1993PhTea..31...84A --> |doi=10.1119/1.2343667}}</ref>


===Signed angles ===
=== Signed angles ===
{{main|Angle of rotation}}
{{main|Angle of rotation}}
{{see also|Sign (mathematics)#Angles|Euclidean space#Angle}}
{{see also|Sign (mathematics)#Angles|Euclidean space#Angle}}
[[File:Angles on the unit circle.svg|right|thumb|Measuring from the [[x-axis]], angles on the [[unit circle]] count as positive in the [[counterclockwise]] direction, and negative in the [[clockwise]] direction.]]
[[File:Angles on the unit circle.svg|right|thumb|class=skin-invert-image|Measuring from the [[x-axis]], angles on the [[unit circle]] count as positive in the [[counterclockwise]] direction, and negative in the [[clockwise]] direction.]]


An angle denoted as {{math|∠BAC}} might refer to any of four angles: the clockwise angle from B to C about A, the anticlockwise angle from B to C about A, the clockwise angle from C to B about A, or the anticlockwise angle from C to B about A, It is therefore frequently helpful to impose a convention that allows positive and negative angular values to represent [[Orientation (geometry)|orientations]] and/or [[Rotation (mathematics)|rotations]] in opposite directions or "sense" relative to some reference.
An angle denoted as {{math|∠BAC}} might refer to any of four angles: the clockwise angle from B to C about A, the anticlockwise angle from B to C about A, the clockwise angle from C to B about A, or the anticlockwise angle from C to B about A, It is therefore frequently helpful to impose a convention that allows positive and negative angular values to represent [[Orientation (geometry)|orientations]] and/or [[Rotation (mathematics)|rotations]] in opposite directions or "sense" relative to some reference.
Line 270: Line 164:
In a two-dimensional [[Cartesian coordinate system]], an angle is typically defined by its two sides, with its vertex at the origin. The ''initial side'' is on the positive [[x-axis]], while the other side or ''terminal side'' is defined by the measure from the initial side in radians, degrees, or turns, with ''positive angles'' representing rotations toward the positive [[y-axis]] and ''negative angles'' representing rotations toward the negative ''y''-axis. When Cartesian coordinates are represented by ''standard position'', defined by the ''x''-axis rightward and the ''y''-axis upward, positive rotations are [[anticlockwise]], and negative cycles are [[clockwise]].
In a two-dimensional [[Cartesian coordinate system]], an angle is typically defined by its two sides, with its vertex at the origin. The ''initial side'' is on the positive [[x-axis]], while the other side or ''terminal side'' is defined by the measure from the initial side in radians, degrees, or turns, with ''positive angles'' representing rotations toward the positive [[y-axis]] and ''negative angles'' representing rotations toward the negative ''y''-axis. When Cartesian coordinates are represented by ''standard position'', defined by the ''x''-axis rightward and the ''y''-axis upward, positive rotations are [[anticlockwise]], and negative cycles are [[clockwise]].


In many contexts, an angle of −''θ'' is effectively equivalent to an angle of "one full turn minus ''θ''". For example, an orientation represented as −45° is effectively equal to an orientation defined as 360°&nbsp;&nbsp;45° or 315°. Although the final position is the same, a physical rotation (movement) of −45° is not the same as a rotation of 315° (for example, the rotation of a person holding a broom resting on a dusty floor would leave visually different traces of swept regions on the floor).
In many contexts, an angle of −''θ'' is effectively equivalent to an angle of "one full turn minus ''θ''". For example, an orientation represented as −45° is effectively equal to an orientation defined as {{nowrap|360° − 45°}} or 315°. Although the final position is the same, a physical rotation (movement) of −45° is not the same as a rotation of 315° (for example, the rotation of a person holding a broom resting on a dusty floor would leave visually different traces of swept regions on the floor).


In three-dimensional geometry, "clockwise" and "anticlockwise" have no absolute meaning, so the direction of positive and negative angles must be defined in terms of an [[Orientability|orientation]], which is typically determined by a [[Normal (geometry)|normal vector]] passing through the angle's vertex and perpendicular to the plane in which the rays of the angle lie.
In three-dimensional geometry, "clockwise" and "anticlockwise" have no absolute meaning, so the direction of positive and negative angles must be defined in terms of an [[Orientability|orientation]], which is typically determined by a [[Normal (geometry)|normal vector]] passing through the angle's vertex and perpendicular to the plane in which the rays of the angle lie.
Line 276: Line 170:
In [[navigation]], [[bearing (navigation)|bearings]] or [[azimuth]] are measured relative to north. By convention, viewed from above, bearing angles are positive clockwise, so a bearing of 45° corresponds to a north-east orientation. Negative bearings are not used in navigation, so a north-west orientation corresponds to a bearing of 315°.
In [[navigation]], [[bearing (navigation)|bearings]] or [[azimuth]] are measured relative to north. By convention, viewed from above, bearing angles are positive clockwise, so a bearing of 45° corresponds to a north-east orientation. Negative bearings are not used in navigation, so a north-west orientation corresponds to a bearing of 315°.


===Equivalent angles===
=== Equivalent angles ===
* Angles that have the same measure (i.e., the same magnitude) are said to be ''equal'' or ''[[Congruence (geometry)|congruent]]''. An angle is defined by its measure and is not dependent upon the lengths of the sides of the angle (e.g., all ''right angles'' are equal in measure).
* Angles that have the same measure (i.e., the same magnitude) are said to be ''equal'' or ''[[Congruence (geometry)|congruent]]''. An angle is defined by its measure and is not dependent upon the lengths of the sides of the angle (e.g., all ''right angles'' are equal in measure).
* Two angles that share terminal sides, but differ in size by an integer multiple of a turn, are called ''coterminal angles''.
* Two angles that share terminal sides, but differ in size by an integer multiple of a turn, are called ''coterminal angles''.
* The ''reference angle'' (sometimes called ''related angle'') for any angle ''θ'' in standard position is the positive acute angle between the terminal side of ''θ'' and the x-axis (positive or negative).<ref>{{cite web|url=http://www.mathwords.com/r/reference_angle.htm|title=Mathwords: Reference Angle|website=www.mathwords.com|access-date=26 April 2018|url-status=live|archive-url=https://web.archive.org/web/20171023035017/http://www.mathwords.com/r/reference_angle.htm|archive-date=23 October 2017}}</ref><ref>{{cite book |last1=McKeague |first1=Charles P. |title=Trigonometry |date=2008 |publisher=Thomson Brooks/Cole |location=Belmont, CA |isbn=978-0495382607 |page=110 |edition=6th}}</ref> Procedurally, the magnitude of the reference angle for a given angle may determined by taking the angle's magnitude [[modulo]] {{sfrac|2}} turn, 180°, or {{math|π}} radians, then stopping if the angle is acute, otherwise taking the supplementary angle, 180° minus the reduced magnitude. For example, an angle of 30 degrees is already a reference angle, and an angle of 150 degrees also has a reference angle of 30 degrees (180° − 150°). Angles of 210° and 510° correspond to a reference angle of 30 degrees as well (210° mod 180° = 30°, 510° mod 180° = 150° whose supplementary angle is 30°).
* The ''reference angle'' (sometimes called ''related angle'') for any angle ''θ'' in standard position is the positive acute angle between the terminal side of ''θ'' and the x-axis (positive or negative).<ref>{{cite book |last1=McKeague |first1=Charles P. |title=Trigonometry |date=2008 |publisher=Thomson Brooks/Cole |location=Belmont, CA |isbn=978-0495382607 |page=110 |edition=6th}}</ref> Procedurally, the magnitude of the reference angle for a given angle may determined by taking the angle's magnitude [[modulo]] {{sfrac|2}} turn, 180°, or {{math|π}} radians, then stopping if the angle is acute, otherwise taking the supplementary angle, 180° minus the reduced magnitude. For example, an angle of 30 degrees is already a reference angle, and an angle of 150 degrees also has a reference angle of 30 degrees ({{nowrap|180° − 150°}}). Angles of 210° and 510° correspond to a reference angle of 30 degrees as well ({{nowrap|1=210° mod 180° = 30°}}, {{nowrap|1=510° mod 180° = 150°}} whose supplementary angle is 30°).


===Related quantities===
=== Related quantities ===
For an angular unit, it is definitional that the [[angle addition postulate]] holds. Some quantities related to angles where the angle addition postulate does not hold include:
For an angular unit, it is definitional that the [[angle addition postulate]] holds, however some measurements or quantities related to angles are in use that do not satisfy this postulate:
* The ''[[slope]]'' or ''gradient'' is equal to the [[tangent (trigonometric function)|tangent]] of the angle; a gradient is often expressed as a percentage. For very small values (less than 5%), the slope of a line is approximately the measure in radians of its angle with the horizontal direction.
* The ''[[slope]]'' or ''gradient'' is equal to the [[tangent (trigonometric function)|tangent]] of the angle and is often expressed as a percentage ("rise" over "run"). For very small values (less than 5%), the slope of a line is approximately the measure in radians of its angle with the horizontal direction. An [[Grade (slope)|elevation grade]] is a slope used to indicate the steepness of roads, paths and railway lines.
* The ''[[spread (rational trigonometry)|spread]]'' between two lines is defined in [[rational geometry]] as the square of the sine of the angle between the lines. As the sine of an angle and the sine of its supplementary angle are the same, any angle of rotation that maps one of the lines into the other leads to the same value for the spread between the lines.
* The ''[[spread (rational trigonometry)|spread]]'' between two lines is defined in [[rational geometry]] as the square of the sine of the angle between the lines. As the sine of an angle and the sine of its supplementary angle are the same, any angle of rotation that maps one of the lines into the other leads to the same value for the spread between the lines.
* Although done rarely, one can report the direct results of [[trigonometric functions]], such as the [[sine]] of the angle.
* Although done rarely, one can report the direct results of [[trigonometric functions]], such as the [[sine]] of the angle.


==Angles between curves==
== Angles between curves ==
[[File:Curve angles.svg|thumb|right|The angle between the two curves at ''P'' is defined as the angle between the tangents <var>A</var> and <var>B</var> at <var>P</var>.]]
[[File:Curve angles.svg|thumb|right|class=skin-invert-image|The angle between the two curves at P is defined as the angle between the tangents <var>A</var> and <var>B</var> at <var>P</var>.]]
The angle between a line and a [[curve]] (mixed angle) or between two intersecting curves (curvilinear angle) is defined to be the angle between the [[tangent]]s at the point of intersection. Various names (now rarely, if ever, used) have been given to particular cases:—''amphicyrtic'' (Gr. {{lang|grc|ἀμφί}}, on both sides, κυρτός, convex) or ''cissoidal'' (Gr. κισσός, ivy), biconvex; ''xystroidal'' or ''sistroidal'' (Gr. ξυστρίς, a tool for scraping), concavo-convex; ''amphicoelic'' (Gr. κοίλη, a hollow) or ''angulus lunularis'', biconcave.<ref>{{harvnb|Chisholm|1911}}; {{harvnb|Heiberg|1908|p=178}}</ref><!-- Again, most of this paragraph is from EB1911, with Heath as its source. -->
The angle between a line and a [[curve]] (mixed angle) or between two intersecting curves (curvilinear angle) is defined to be the angle between the [[tangent]]s at the point of intersection. Various names (now rarely, if ever, used) have been given to particular cases:—''amphicyrtic'' (Gr. {{lang|grc|ἀμφί}}, on both sides, κυρτός, convex) or ''cissoidal'' (Gr. κισσός, ivy), biconvex; ''xystroidal'' or ''sistroidal'' (Gr. ξυστρίς, a tool for scraping), concavo-convex; ''amphicoelic'' (Gr. κοίλη, a hollow) or ''angulus lunularis'', biconcave.<ref>{{harvnb|Chisholm|1911}}; {{harvnb|Heiberg|1908|p=178}}</ref><!-- Again, most of this paragraph is from EB1911, with Heath as its source. -->


==Bisecting and trisecting angles==
== Bisecting and trisecting angles ==
{{Main article|Bisection#Angle bisector|Angle trisection}}
{{Main|Bisection#Angle bisector|Angle trisection}}


The [[Greek mathematics|ancient Greek mathematicians]] knew how to bisect an angle (divide it into two angles of equal measure) using only a [[compass and straightedge]] but could only trisect certain angles. In 1837, [[Pierre Wantzel]] showed that this construction could not be performed for most angles.
The [[Greek mathematics|ancient Greek mathematicians]] knew how to bisect an angle (divide it into two angles of equal measure) using only a [[compass and straightedge]] but could only trisect certain angles. In 1837, [[Pierre Wantzel]] showed that this construction could not be performed for most angles.


==Dot product and generalisations{{anchor|Dot product}}==
== Dot product and generalisations <span class="anchor" id="Dot product"></span> ==
In the [[Euclidean space]], the angle ''θ'' between two [[Euclidean vector]]s '''u''' and '''v''' is related to their [[dot product]] and their lengths by the formula
In the [[Euclidean space]], the angle ''θ'' between two [[Euclidean vector]]s '''u''' and '''v''' is related to their [[dot product]] and their lengths by the formula
<math display="block"> \mathbf{u} \cdot \mathbf{v} = \cos(\theta) \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>
<math display="block"> \mathbf{u} \cdot \mathbf{v} = \cos(\theta) \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>


This formula supplies an easy method to find the angle between two planes (or curved surfaces) from their [[normal vector]]s and between [[skew lines]] from their vector equations.
This formula supplies an easy method to find the angle between two planes (or curved surfaces) from their [[normal vector]]s and between [[skew lines]] from their vector equations.


===Inner product===
=== Inner product ===
To define angles in an abstract real [[inner product space]], we replace the Euclidean dot product ( '''·''' ) by the inner product <math> \langle \cdot , \cdot \rangle </math>, i.e.
To define angles in an abstract real [[inner product space]], we replace the Euclidean dot product ( '''·''' ) by the inner product <math> \langle \cdot , \cdot \rangle </math>, i.e.
<math display="block"> \langle \mathbf{u} , \mathbf{v} \rangle = \cos(\theta)\ \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>
<math display="block"> \langle \mathbf{u} , \mathbf{v} \rangle = \cos(\theta)\ \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>


In a complex [[inner product space]], the expression for the cosine above may give non-real values, so it is replaced with
In a complex [[inner product space]], the expression for the cosine above may give non-real values, so it is replaced with
<math display="block"> \operatorname{Re} \left( \langle \mathbf{u} , \mathbf{v} \rangle \right) = \cos(\theta) \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>
<math display="block"> \operatorname{Re} \left( \langle \mathbf{u} , \mathbf{v} \rangle \right) = \cos(\theta) \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>
or, more commonly, using the absolute value, with
or, more commonly, using the absolute value, with
<math display="block"> \left| \langle \mathbf{u} , \mathbf{v} \rangle \right| = \left| \cos(\theta) \right| \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>
<math display="block"> \left| \langle \mathbf{u} , \mathbf{v} \rangle \right| = \left| \cos(\theta) \right| \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| .</math>


The latter definition ignores the direction of the vectors. It thus describes the angle between one-dimensional subspaces <math>\operatorname{span}(\mathbf{u})</math> and <math>\operatorname{span}(\mathbf{v})</math> spanned by the vectors <math>\mathbf{u}</math> and <math>\mathbf{v}</math> correspondingly.
The latter definition ignores the direction of the vectors. It thus describes the angle between one-dimensional subspaces <math>\operatorname{span}(\mathbf{u})</math> and <math>\operatorname{span}(\mathbf{v})</math> spanned by the vectors <math>\mathbf{u}</math> and <math>\mathbf{v}</math> correspondingly.


===Angles between subspaces===
=== Angles between subspaces ===
The definition of the angle between one-dimensional subspaces <math>\operatorname{span}(\mathbf{u})</math> and <math>\operatorname{span}(\mathbf{v})</math> given by
The definition of the angle between one-dimensional subspaces <math>\operatorname{span}(\mathbf{u})</math> and <math>\operatorname{span}(\mathbf{v})</math> given by
<math display="block"> \left| \langle \mathbf{u} , \mathbf{v} \rangle \right| = \left| \cos(\theta) \right| \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| </math>
<math display="block"> \left| \langle \mathbf{u} , \mathbf{v} \rangle \right| = \left| \cos(\theta) \right| \left\| \mathbf{u} \right\| \left\| \mathbf{v} \right\| </math>
in a [[Hilbert space]] can be extended to subspaces of finite number of dimensions. Given two subspaces <math> \mathcal{U} </math>, <math> \mathcal{W} </math> with <math> \dim ( \mathcal{U}) := k \leq \dim ( \mathcal{W}) := l </math>, this leads to a definition of <math>k</math> angles called canonical or [[principal angles]] between subspaces.


in a [[Hilbert space]] can be extended to subspaces of finite dimensions. Given two subspaces <math> \mathcal{U} </math>, <math> \mathcal{W} </math> with <math> \dim ( \mathcal{U}) := k \leq \dim ( \mathcal{W}) := l </math>, this leads to a definition of <math>k</math> angles called canonical or [[principal angles]] between subspaces.
=== Angles in Riemannian geometry ===
 
===Angles in Riemannian geometry===
In [[Riemannian geometry]], the [[metric tensor]] is used to define the angle between two [[tangent]]s. Where ''U'' and ''V'' are tangent vectors and ''g''<sub>''ij''</sub> are the components of the metric tensor ''G'',
In [[Riemannian geometry]], the [[metric tensor]] is used to define the angle between two [[tangent]]s. Where ''U'' and ''V'' are tangent vectors and ''g''<sub>''ij''</sub> are the components of the metric tensor ''G'',
<math display="block">
<math display="block">
\cos \theta = \frac{g_{ij} U^i V^j}{\sqrt{ \left| g_{ij} U^i U^j \right| \left| g_{ij} V^i V^j \right|}}.
\cos \theta = \frac{g_{ij} U^i V^j}{\sqrt{ \left| g_{ij} U^i U^j \right| \left| g_{ij} V^i V^j \right|}}.
</math>
</math>


===Hyperbolic angle===
=== Hyperbolic angle ===
[[File:Hyperbolic_rotation.gif|thumb|right|200px|A constant hyperbolic angle (0.2), under [[hyperbolic rotation]], corresponds to a variable circular angle.]]
A [[hyperbolic angle]] is an [[argument of a function|argument]] of a [[hyperbolic function]] just as the ''circular angle'' is the argument of a [[circular function]]. The comparison can be visualized as the size of the openings of a [[hyperbolic sector]] and a [[circular sector]] since the [[area]]s of these sectors correspond to the angle magnitudes in each case.<ref>[[Robert Baldwin Hayward]] (1892) [https://archive.org/details/algebraofcoplana00haywiala/page/n5/mode/2up ''The Algebra of Coplanar Vectors and Trigonometry''], chapter six</ref> Unlike the circular angle, the hyperbolic angle is unbounded. When the circular and hyperbolic functions are viewed as [[infinite series]] in their angle argument, the circular ones are just [[alternating series]] forms of the hyperbolic functions. This comparison of the two series corresponding to functions of angles was described by [[Leonhard Euler]] in ''[[Introduction to the Analysis of the Infinite]]'' (1748).
A [[hyperbolic angle]] is an [[argument of a function|argument]] of a [[hyperbolic function]] just as the ''circular angle'' is the argument of a [[circular function]]. The comparison can be visualized as the size of the openings of a [[hyperbolic sector]] and a [[circular sector]] since the [[area]]s of these sectors correspond to the angle magnitudes in each case.<ref>[[Robert Baldwin Hayward]] (1892) [https://archive.org/details/algebraofcoplana00haywiala/page/n5/mode/2up ''The Algebra of Coplanar Vectors and Trigonometry''], chapter six</ref> Unlike the circular angle, the hyperbolic angle is unbounded. When the circular and hyperbolic functions are viewed as [[infinite series]] in their angle argument, the circular ones are just [[alternating series]] forms of the hyperbolic functions. This comparison of the two series corresponding to functions of angles was described by [[Leonhard Euler]] in ''[[Introduction to the Analysis of the Infinite]]'' (1748).


==History and etymology==
== History and etymology ==
The word ''angle'' comes from the [[Latin]] word {{Lang|la|angulus}}, meaning "corner". [[Cognate]] words include the [[Greek language|Greek]] {{lang|grc|ἀγκύλος}} ({{Lang|grc-la|ankylοs}}) meaning "crooked, curved" and the [[English language|English]] word "[[ankle]]". Both are connected with the [[Proto-Indo-European language|Proto-Indo-European]] root ''*ank-'', meaning "to bend" or "bow".<ref>{{harvnb|Slocum|2007}}</ref>
The word ''angle'' comes from the [[Latin]] word {{Lang|la|angulus}}, meaning "corner". [[Cognate]] words include the [[Greek language|Greek]] {{lang|grc|ἀγκύλος}} ({{Lang|grc-la|ankylοs}}) meaning "crooked, curved" and the [[English language|English]] word "[[ankle]]". Both are connected with the [[Proto-Indo-European language|Proto-Indo-European]] root ''*ank-'', meaning "to bend" or "bow".<ref>{{harvnb|Slocum|2007}}</ref>
<!--Note: ἀγκύλος rather than ἀνκύλος is correct; the γκ is a digraph pronounced [ŋk].-->
<!--Note: ἀγκύλος rather than ἀνκύλος is correct; the γκ is a digraph pronounced [ŋk].-->


[[Euclid]] defines a plane angle as the inclination to each other, in a plane, of two lines that meet each other and do not lie straight with respect to each other. According to the Neoplatonic metaphysician [[Proclus]], an angle must be either a quality, a quantity, or a relationship. The first concept, angle as quality, was used by [[Eudemus of Rhodes]], who regarded an angle as a deviation from a [[straight line]]; the second, angle as quantity, by [[Carpus of Antioch]], who regarded it as the interval or space between the intersecting lines; Euclid adopted the third: angle as a relationship.<ref>{{harvnb|Chisholm|1911}}; {{harvnb|Heiberg|1908|pp=177–178}}</ref><!-- This paragraph is quoted from EB1911, but its source seems to be Heath.-->
Philosophers have debated the nature of angles for millennia, with some arguing that angles are a measure (quantity), and others saying they are a kind of shape defined by the lines that bound it (qualitative relation), and still others saying an angle is both.<ref>{{cite book |last1=Morrow |first1=Glenn Raymond |title=A commentary on the first book of Euclid's Elements |date=1992 |pages=98–104 |quote=the angle as such is none of the things mentioned but exists as a combination of all these categories |orig-date=1970}}</ref> Pedagogically, the accepted answer is that angles are defined as figures, and the measure of an angle is defined as the number of congruent non-overlapping copies of a unit angle necessary to cover the angle and its interior. Angles are said to be equal in measure and [[Similarity (geometry)|similar]] or [[Congruence (geometry)|congruent]] in shape.<ref>{{cite journal |last1=Jackson |first1=Stanley B. |date=1967 |title=Congruence and measurement |url=https://files.eric.ed.gov/fulltext/ED046716.pdf#page=68 |journal=The Arithmetic Teacher |volume=14 |issue=2 |pages=94–102 |doi=10.5951/AT.14.2.0094 |access-date=8 August 2025}}</ref>
 
[[Euclid]] defines a plane angle as the inclination to each other, in a plane, of two lines that meet each other and do not lie straight with respect to each other. According to the Neoplatonic metaphysician [[Proclus]], an angle must be either a quality, a quantity, or a relationship. The first concept, angle as quality, was used by [[Eudemus of Rhodes]], who regarded an angle as a deviation from a [[straight line]]; the second, angle as quantity, by [[Carpus of Antioch]], who regarded it as the interval or space between the intersecting lines; Euclid adopted the third: angle as a relationship.<ref>{{harvnb|Chisholm|1911}}; {{harvnb|Heiberg|1908|pp=177–178}}</ref>


==Angles in geography and astronomy==
=== Vertical angle theorem ===
The equality of vertically opposite angles is called the ''vertical angle theorem''. [[Eudemus of Rhodes]] attributed the proof to [[Thales|Thales of Miletus]].<ref>{{cite book |author=Euclid |author-link=Euclid |title=The Elements |title-link=Euclid's Elements}} Proposition I:13.</ref>{{sfn|Shute|Shirk|Porter|1960|pp=25–27}} The proposition showed that since both of a pair of vertical angles are supplementary to both of the adjacent angles, the vertical angles are equal in measure. According to a historical note,{{sfn|Shute|Shirk|Porter|1960|pp=25–27}} when Thales visited Egypt, he observed that whenever the Egyptians drew two intersecting lines, they would measure the vertical angles to make sure that they were equal. Thales concluded that one could prove that all vertical angles are equal if one accepted some general notions such as:
* All straight angles are equal.
* Equals added to equals are equal.
* Equals subtracted from equals are equal.
 
When two adjacent angles form a straight line, they are supplementary. Therefore, if we assume that the measure of angle ''A'' equals ''x'', the measure of angle ''C'' would be {{nowrap|180° − ''x''}}. Similarly, the measure of angle ''D'' would be {{nowrap|180° − ''x''}}. Both angle ''C'' and angle ''D'' have measures equal to {{nowrap|180° − ''x''}} and are congruent. Since angle ''B'' is supplementary to both angles ''C'' and ''D'', either of these angle measures may be used to determine the measure of Angle ''B''. Using the measure of either angle ''C'' or angle ''D'', we find the measure of angle ''B'' to be {{nowrap|1=180° − (180° − ''x'') = ''x''}}. Therefore, both angle ''A'' and angle ''B'' have measures equal to ''x'' and are equal in measure.
 
== Angles in geography and astronomy ==
In [[geography]], the location of any point on the Earth can be identified using a ''[[geographic coordinate system]]''. This system specifies the [[latitude]] and [[longitude]] of any location in terms of angles subtended at the center of the Earth, using the [[equator]] and (usually) the [[Greenwich meridian]] as references.
In [[geography]], the location of any point on the Earth can be identified using a ''[[geographic coordinate system]]''. This system specifies the [[latitude]] and [[longitude]] of any location in terms of angles subtended at the center of the Earth, using the [[equator]] and (usually) the [[Greenwich meridian]] as references.


In [[astronomy]], a given point on the [[celestial sphere]] (that is, the apparent position of an astronomical object) can be identified using any of several ''[[astronomical coordinate systems]]'', where the references vary according to the particular system. Astronomers measure the ''[[angular separation]]'' of two [[star]]s by imagining two lines through the center of the [[Earth]], each intersecting one of the stars. The angle between those lines and the angular separation between the two stars can be measured.
In [[astronomy]], a given point on the [[celestial sphere]] (that is, the apparent position of an astronomical object) can be identified using any of several ''[[astronomical coordinate systems]]'', where the references vary according to the particular system. Astronomers measure the ''[[angular separation]]'' of two [[star]]s by imagining two lines through the center of the [[Earth]], each intersecting one of the stars. The angle between those lines and the angular separation between the two stars can be measured.


In both geography and astronomy, a sighting direction can be specified in terms of a [[vertical angle]] such as [[altitude angle|altitude]] /[[elevation angle|elevation]] with respect to the [[horizon]] as well as the [[azimuth]] with respect to [[north]].
In both geography and astronomy, a sighting direction can be specified in terms of a [[vertical angle]] such as [[altitude angle]] or [[elevation angle|elevation]] with respect to the [[horizon]] as well as the [[azimuth]] with respect to [[north]].


Astronomers also measure objects' ''apparent size'' as an [[angular diameter]]. For example, the [[full moon]] has an angular diameter of approximately 0.5° when viewed from Earth. One could say, "The Moon's diameter subtends an angle of half a degree." The [[small-angle formula]] can convert such an angular measurement into a distance/size ratio.
Astronomers also measure objects' ''apparent size'' as an [[angular diameter]]. For example, the [[full moon]] has an angular diameter of approximately 0.5° when viewed from Earth. One could say, "The Moon's diameter subtends an angle of half a degree." The [[small-angle formula]] can convert such an angular measurement into a distance/size ratio.


Other astronomical approximations include:
Other astronomical approximations include:
* 0.5° is the approximate diameter of the [[Sun]] and of the [[Moon]] as viewed from Earth.
* 0.5° is the approximate angular diameter of the [[Sun]] and of the [[Moon]] as viewed from Earth.
* 1° is the approximate width of the [[little finger]] at arm's length.
* 1° is the approximate angular width of the [[little finger]] at arm's length.
* 10° is the approximate width of a closed fist at arm's length.
* 10° is the approximate angular width of a closed fist at arm's length.
* 20° is the approximate width of a handspan at arm's length.
* 20° is the approximate angular width of a handspan at arm's length.
These measurements depend on the individual subject, and the above should be treated as rough [[rule of thumb]] approximations only.
These measurements depend on the individual subject, and the above should be treated as rough [[rule of thumb]] approximations only.


In astronomy, [[right ascension]] and [[declination]] are usually measured in angular units, expressed in terms of time, based on a 24-hour day.
In astronomy, [[right ascension]] is usually measured in angular units that are expressed in terms of time based on a 24-hour day.<ref>{{cite book |last1=Snell |first1=Ronald Lee |last2=Kurtz |first2=Stanley E. |last3=Marr |first3=Jonathan M. |title=Fundamentals of radio astronomy: astrophysics |date=2019 |publisher=CRC Press, Taylor & Francis Group |location=Boca Raton, FL |isbn=9781498725798 |chapter=Introductory Material}}</ref>
{|class="wikitable"  
{|class="wikitable"  
|-
|-
! Unit !! [[Sexagesimal|Symbol]] !! Degrees !! Radians !! Turns !! Other
! Unit !! Symbol !! Degrees !! Radians !! Turns !! Other
|-
|-
! Hour
! Hour
Line 366: Line 263:
|-
|-
! Minute
! Minute
| m || 0°15′ || {{frac|{{pi}}|720}} rad ||{{frac|1|1,440}} turn || {{frac|1|60}} hour  
| m || 0°15′ || {{frac|{{pi}}|720}} rad ||{{frac|1|{{val|1440}}}} turn || {{frac|1|60}} hour  
|-
|-
! Second
! Second
| s || 0°0′15″ || {{frac|{{pi}}|43200}} rad || {{frac|1|86,400}} turn || {{frac|1|60}} minute
| s || 0°0′15″ || {{frac|{{pi}}|{{val|43200}}}} rad || {{frac|1|{{val|86400}}}} turn || {{frac|1|60}} minute
|}
|}


==See also==
== See also ==
{{div col |colwidth=22em}}
{{div col |colwidth=22em}}
* [[Angle measuring instrument]]
* [[Angle measuring instrument]]
Line 404: Line 301:
{{div col end}}
{{div col end}}


==Notes==
== Notes ==
{{Reflist|group="nb"}}
{{reflist|group="nb"}}
{{notelist}}
{{notelist}}


==References==
== References ==
{{Reflist|refs=
{{reflist}}
<ref name="Jeans_1947">{{cite book |author-first=James Hopwood |author-last=Jeans |author-link=James Hopwood Jeans |date=1947 |title=The Growth of Physical Science |publisher=CUP Archive |page=[https://archive.org/details/in.ernet.dli.2015.210060/page/n25 7] |url=https://archive.org/details/in.ernet.dli.2015.210060}}</ref>
<ref name="Murnaghan_1946">{{cite book |author-first=Francis Dominic |author-last=Murnaghan |author-link=Francis Dominic Murnaghan (mathematician) |date=1946 |title=Analytic Geometry |page=2}}</ref>
<ref name="Dimitric_2012">{{cite journal |title=On Angles and Angle Measurements |author-first=Radoslav M. |author-last=Dimitrić |journal=The Teaching of Mathematics |date=2012 |volume=XV |number=2 |pages=133–140 |url=http://elib.mi.sanu.ac.rs/files/journals/tm/29/tm1525.pdf |access-date=2019-08-06 |url-status=live |archive-url=https://web.archive.org/web/20190117195213/http://elib.mi.sanu.ac.rs/files/journals/tm/29/tm1525.pdf |archive-date=2019-01-17}}</ref>
<ref name="ooPIC">{{cite web |title=ooPIC Programmer's Guide - Chapter 15: URCP |work=[[ooPIC]] Manual & Technical Specifications - ooPIC Compiler Ver 6.0 |orig-year=1997 |date=2007 |publisher=Savage Innovations, LLC |url=http://www.oopic.com/pgchap15.htm |access-date=2019-08-05 |url-status=dead |archive-url=https://web.archive.org/web/20080628051746/http://www.oopic.com/pgchap15.htm |archive-date=2008-06-28}}</ref>
<ref name="Hargreaves_2010">{{cite web |title=Angles, integers, and modulo arithmetic |author-first=Shawn |author-last=Hargreaves |author-link=:pl:Shawn Hargreaves |publisher=blogs.msdn.com |url=http://blogs.msdn.com/shawnhar/archive/2010/01/04/angles-integers-and-modulo-arithmetic.aspx |access-date=2019-08-05 |url-status=live |archive-url=https://web.archive.org/web/20190630223817/http://www.shawnhargreaves.com/blogindex.html |archive-date=2019-06-30}}</ref>
<ref name="Bonin_2016">{{cite web |title=RE: WP-32S in 2016? |date=2016-01-11 |author-first=Walter |author-last=Bonin |work=HP Museum |url=https://www.hpmuseum.org/forum/thread-5427-post-48957.html#pid48957 |access-date=2019-08-05 |url-status=live |archive-url=https://web.archive.org/web/20190806141349/https://www.hpmuseum.org/forum/thread-5427-post-48957.html |archive-date=2019-08-06}}</ref>
}}


== Bibliography ==
== Bibliography ==
{{refbegin|30em}}
* {{citation
* {{citation
  | last = Aboughantous | first = Charles H.  
  | last = Aboughantous | first = Charles H.  
Line 427: Line 318:
  | isbn = 978-1-59942-822-2
  | isbn = 978-1-59942-822-2
}}
}}
* {{cite journal |last1=Brinsmade |first1=J. B. |title=Plane and Solid Angles. Their Pedagogic Value When Introduced Explicitly |journal=American Journal of Physics |date=December 1936 |volume=4 |issue=4 |pages=175–179 |doi=10.1119/1.1999110 |bibcode=1936AmJPh...4..175B}}
* {{cite journal |title=On Angles and Angle Measurements |author-first=Radoslav M. |author-last=Dimitrić |journal=The Teaching of Mathematics |date=2012 |volume=XV |number=2 |pages=133–140 |url=http://elib.mi.sanu.ac.rs/files/journals/tm/29/tm1525.pdf |access-date=2019-08-06 |url-status=live |archive-url=https://web.archive.org/web/20190117195213/http://elib.mi.sanu.ac.rs/files/journals/tm/29/tm1525.pdf |archive-date=2019-01-17}}
* {{cite journal |last1=Brownstein |first1=K. R. |title=Angles—Let's treat them squarely |journal=American Journal of Physics |date=July 1997 |volume=65 |issue=7 |pages=605–614 |doi=10.1119/1.18616 |bibcode=1997AmJPh..65..605B |doi-access=free}}
* {{cite journal |last1=Eder |first1=W E |title=A Viewpoint on the Quantity "Plane Angle" |journal=Metrologia |date=January 1982 |volume=18 |issue=1 |pages=1–12 |doi=10.1088/0026-1394/18/1/002 |bibcode=1982Metro..18....1E |s2cid=250750831}}
* {{cite journal |last1=Foster |first1=Marcus P |title=The next 50 years of the SI: a review of the opportunities for the e-Science age |journal=Metrologia |date=1 December 2010 |volume=47 |issue=6 |pages=R41–R51 |doi=10.1088/0026-1394/47/6/R01 |s2cid=117711734 |url=https://publications.csiro.au/rpr/download?pid=csiro:EP11794&dsid=DS4}}
* {{citation
* {{citation
  | last1 = Godfrey | first1 = Charles
  | last1 = Godfrey | first1 = Charles
Line 443: Line 331:
* {{citation |last=Heiberg |first=Johan Ludvig |year=1908 |title=Euclid |editor-first=T. L. |editor-last=Heath |editor-link=T. L. Heath |series=The Thirteen Books of Euclid's Elements |volume=1 |publisher=Cambridge University Press |location=[[Cambridge, England|Cambridge]] |url=https://books.google.com/books?id=UhgPAAAAIAAJ }}.
* {{citation |last=Heiberg |first=Johan Ludvig |year=1908 |title=Euclid |editor-first=T. L. |editor-last=Heath |editor-link=T. L. Heath |series=The Thirteen Books of Euclid's Elements |volume=1 |publisher=Cambridge University Press |location=[[Cambridge, England|Cambridge]] |url=https://books.google.com/books?id=UhgPAAAAIAAJ }}.
* {{citation |last=Jacobs |first=Harold R. |date=1974 |title=Geometry|publisher=W. H. Freeman|isbn=978-0-7167-0456-0|pages=97, 255}}
* {{citation |last=Jacobs |first=Harold R. |date=1974 |title=Geometry|publisher=W. H. Freeman|isbn=978-0-7167-0456-0|pages=97, 255}}
* {{cite journal |last1=Leonard |first1=B P |title=Proposal for the dimensionally consistent treatment of angle and solid angle by the International System of Units (SI) |journal=Metrologia |date=1 October 2021 |volume=58 |issue=5 |pages=052001 |doi=10.1088/1681-7575/abe0fc |bibcode=2021Metro..58e2001L |s2cid=234036217}}
* {{cite journal |last1=Lévy-Leblond |first1=Jean-Marc |title=Dimensional angles and universal constants |journal=American Journal of Physics |date=September 1998 |volume=66 |issue=9 |pages=814–815 |doi=10.1119/1.18964 |bibcode=1998AmJPh..66..814L |url=https://www.researchgate.net/publication/253371022}}
* {{cite journal |last1=Mills |first1=Ian |title=On the units radian and cycle for the quantity plane angle |journal=Metrologia |date=1 June 2016 |volume=53 |issue=3 |pages=991–997 |doi=10.1088/0026-1394/53/3/991 |bibcode=2016Metro..53..991M |s2cid=126032642}}
* {{cite journal |last1=Mohr |first1=Peter J |last2=Phillips |first2=William D |title=Dimensionless units in the SI |journal=Metrologia |date=1 February 2015 |volume=52 |issue=1 |pages=40–47 |doi=10.1088/0026-1394/52/1/40 |arxiv=1409.2794 |bibcode=2015Metro..52...40M |doi-access=free}}
* {{cite journal |last1=Mohr |first1=Peter J |last2=Shirley |first2=Eric L |last3=Phillips |first3=William D |last4=Trott |first4=Michael |title=On the dimension of angles and their units |journal=Metrologia |date=23 June 2022 |volume=59 |issue=5 |page=053001 |doi=10.1088/1681-7575/ac7bc2 |doi-access=free |arxiv=2203.12392 |bibcode=2022Metro..59e3001M}}
* {{citation
* {{citation
  | last = Moser | first = James M.
  | last = Moser | first = James M.
Line 455: Line 338:
  | url = https://archive.org/details/modernelementary0000mose/page/41/mode/2up
  | url = https://archive.org/details/modernelementary0000mose/page/41/mode/2up
}}
}}
* {{cite journal |last1=Quincey |first1=Paul |title=The range of options for handling plane angle and solid angle within a system of units |journal=Metrologia |date=1 April 2016 |volume=53 |issue=2 |pages=840–845 |doi=10.1088/0026-1394/53/2/840 |bibcode=2016Metro..53..840Q |s2cid=125438811}}
* {{SpringerEOM |last=Sidorov |first=L. A. |date=2001 |id=Angle&oldid=13323 |title=Angle}}
* {{cite journal |last1=Quincey |first1=Paul |title=Angles in the SI: a detailed proposal for solving the problem |journal=Metrologia |date=1 October 2021 |volume=58 |issue=5 |pages=053002 |doi=10.1088/1681-7575/ac023f |arxiv=2108.05704 |bibcode=2021Metro..58e3002Q |s2cid=236547235}}
* {{citation |last=Slocum |first=Jonathan |date=2007 |url=http://www.utexas.edu/cola/centers/lrc/ielex/X/P0089.html |title=Preliminary Indo-European lexicon&nbsp;— Pokorny PIE data |access-date=2 Feb 2010 |publisher=[[Linguistics Research Center at UT Austin|University of Texas research department: linguistics research center]] |archive-date=27 June 2010 |archive-url=https://web.archive.org/web/20100627012240/http://www.utexas.edu/cola/centers/lrc/ielex/X/P0089.html |url-status=dead}}
* {{cite journal |last1=Romain |first1=Jacques E. |title=Angle as a fourth fundamental quantity |journal=Journal of Research of the National Bureau of Standards Section B |date=July 1962 |volume=66B |issue=3 |pages=97 |doi=10.6028/jres.066B.012 |doi-access=free}}
* {{citation |last1=Shute |first1=William G. |last2=Shirk |first2=William W. |last3=Porter |first3=George F. |date=1960 |title=Plane and Solid Geometry |publisher=American Book Company |pages=25–27}}
* {{SpringerEOM|mode=cs2 |last=Sidorov |first=L. A. |date=2001 |id=Angle&oldid=13323 |title=Angle}}
* {{citation |last1=Wong |first1=Tak-wah |last2=Wong |first2=Ming-sim |date=2009 |chapter=Angles in Intersecting and Parallel Lines |title=New Century Mathematics |location=Hong Kong |publisher=Oxford University Press |edition=1 |volume=1B |pages=161–163 |isbn=978-0-19-800177-5}}
* {{citation|last=Slocum|first=Jonathan|date=2007|url=http://www.utexas.edu/cola/centers/lrc/ielex/X/P0089.html|title=Preliminary Indo-European lexicon&nbsp;— Pokorny PIE data|access-date=2 Feb 2010|publisher=[[Linguistics Research Center at UT Austin|University of Texas research department: linguistics research center]]|archive-date=27 June 2010|archive-url=https://web.archive.org/web/20100627012240/http://www.utexas.edu/cola/centers/lrc/ielex/X/P0089.html|url-status=dead}}
{{EB1911 |wstitle=Angle |volume=2 |page=14 }}
* {{citation |last1=Shute |first1=William G. |last2=Shirk |first2=William W. |last3=Porter |first3=George F. |date=1960 |title=Plane and Solid Geometry |publisher=American Book Company |pages=25–27}}
{{refend}}
* {{cite journal |last1=Torrens |first1=A B |title=On Angles and Angular Quantities |journal=Metrologia |date=1 January 1986 |volume=22 |issue=1 |pages=1–7 |doi=10.1088/0026-1394/22/1/002 |bibcode=1986Metro..22....1T |s2cid=250801509}}
 
* {{citation |last1=Wong |first1=Tak-wah |last2=Wong |first2=Ming-sim |date=2009 |chapter=Angles in Intersecting and Parallel Lines |title=New Century Mathematics |location=Hong Kong |publisher=Oxford University Press |edition=1 |volume=1B |pages=161–163  |isbn=978-0-19-800177-5}}
== Further reading ==
{{EB1911 |wstitle=Angle |volume=2 |page=14 |mode=cs2}}
{{refbegin|30em}}
* {{cite journal |last1=Brinsmade |first1=J. B. |title=Plane and Solid Angles. Their Pedagogic Value When Introduced Explicitly |journal=American Journal of Physics |date=1936 |volume=4 |issue=4 |pages=175–179 |doi=10.1119/1.1999110 |bibcode=<!-- useless bibcode: 1936AmJPh...4..175B -->}}
* {{cite journal |last1=Brownstein |first1=K. R. |title=Angles—Let's treat them squarely |journal=American Journal of Physics |date=1997 |volume=65 |issue=7 |pages=605–614 |doi=10.1119/1.18616 |bibcode=<!-- useless bibcode: 1997AmJPh..65..605B --> |doi-access=free}}
* {{cite journal |last1=Eder |first1=W E |title=A Viewpoint on the Quantity "Plane Angle" |journal=Metrologia |date=1982 |volume=18 |issue=1 |pages=1–12 |doi=10.1088/0026-1394/18/1/002 |bibcode=<!-- useless bibcode: 1982Metro..18....1E --> }}
* {{cite journal |last1=Foster |first1=Marcus P. |title=The next 50 years of the SI: a review of the opportunities for the e-Science age |journal=Metrologia |date=2010 |volume=47 |issue=6 |pages=R41–R51 |doi=10.1088/0026-1394/47/6/R01  |url=https://publications.csiro.au/rpr/download?pid=csiro:EP11794&dsid=DS4}}
* {{cite journal |last1=Leonard |first1=B. P. |title=Proposal for the dimensionally consistent treatment of angle and solid angle by the International System of Units (SI) |journal=Metrologia |date=2021 |volume=58 |issue=5 |pages=052001 |doi=10.1088/1681-7575/abe0fc |bibcode=<!-- useless bibcode: 2021Metro..58e2001L --> }}
* {{cite journal |last1=Lévy-Leblond |first1=Jean-Marc |title=Dimensional angles and universal constants |journal=American Journal of Physics |date=1998 |volume=66 |issue=9 |pages=814–815 |doi=10.1119/1.18964 |bibcode=<!-- useless bibcode: 1998AmJPh..66..814L --> |id={{ResearchGatePub|253371022}}}}
* {{cite journal |last1=Mills |first1=Ian |title=On the units radian and cycle for the quantity plane angle |journal=Metrologia |date=2016 |volume=53 |issue=3 |pages=991–997 |doi=10.1088/0026-1394/53/3/991 |bibcode=<!-- useless bibcode: 2016Metro..53..991M --> }}
* {{cite journal |last1=Mohr |first1=Peter J. |last2=Phillips |first2=William D. |title=Dimensionless units in the SI |journal=Metrologia |date=2015 |volume=52 |issue=1 |pages=40–47 |doi=10.1088/0026-1394/52/1/40 |arxiv=1409.2794 |bibcode=<!-- useless bibcode: 2015Metro..52...40M --> |doi-access=free}}
* {{cite journal |last1=Mohr |first1=Peter J. |last2=Shirley |first2=Eric L. |last3=Phillips |first3=William D. |last4=Trott |first4=Michael |title=On the dimension of angles and their units |journal=Metrologia |date=2022 |volume=59 |issue=5 |page=053001 |doi=10.1088/1681-7575/ac7bc2 |doi-access=free |arxiv=2203.12392 |bibcode=<!-- useless bibcode: 2022Metro..59e3001M -->}}
* {{cite journal |last1=Quincey |first1=Paul |title=The range of options for handling plane angle and solid angle within a system of units |journal=Metrologia |date=2016 |volume=53 |issue=2 |pages=840–845 |doi=10.1088/0026-1394/53/2/840 |bibcode=<!-- useless bibcode: 2016Metro..53..840Q --> }}
* {{cite journal |last1=Romain |first1=Jacques E. |title=Angle as a fourth fundamental quantity |journal=Journal of Research of the National Bureau of Standards Section B |date=1962 |volume=66B |issue=3 |pages=97 |doi=10.6028/jres.066B.012 |doi-access=free}}
* {{cite journal |last1=Torrens |first1=A. B. |title=On Angles and Angular Quantities |journal=Metrologia |date=1986 |volume=22 |issue=1 |pages=1–7 |doi=10.1088/0026-1394/22/1/002 |bibcode=<!-- useless bibcode: 1986Metro..22....1T --> }}
{{refend}}


==External links==
== External links ==
{{Commons category|Angles (geometry)}}
{{Commons category|Angles (geometry)}}
{{Wikibooks|Geometry|Unified Angles}}  
{{Wikibooks|Geometry|Unified Angles}}  
* {{cite EB9 |wstitle=Angle |volume=2 |pages=29–30 |mode=cs2|short=x }}
* {{cite EB9 |wstitle=Angle |volume=2 |pages=29–30 |short=x }}


{{Authority control}}
{{Authority control}}


[[Category:Angle| ]]
[[Category:Angle| ]]

Latest revision as of 07:16, 17 November 2025

Template:Short description Script error: No such module "Distinguish". Script error: No such module "about". Template:CS1 config Template:Use dmy dates

two line bent at a point
A green angle formed by two red rays on the Cartesian coordinate system

In geometry, an angle is formed by two lines that meet at a point.[1] Each line is called a side of the angle, and the point they share is called the vertex of the angle.[2][3] The term angle is used to denote both geometric figures and their size or magnitude. Angular measure or measure of angle are sometimes used to distinguish between the measurement and figure itself. The measurement of angles is intrinsically linked with circles and rotation, and this is often visualized or defined using the arc of a circle centered at the vertex and lying between the sides.

Fundamentals

There is no universally agreed definition of an angle.[4] Angles can be conceived of and used in a variety of ways and while valid definitions may be given for specific contexts, it is difficult to give a single formal definition that is completely satisfactory in capturing all aspects of the general concept of angle.[5]

One standard definition is that an angle is a figure consisting of two rays which lie in a plane and share a common endpoint. Alternatively, given such a figure, an angle might be defined as: the opening between the rays; the area of the plane that lies between the rays; or the amount of rotation about the vertex of one ray to the other.

More generally, angles are also formed wherever two line segments come together, such as at the corners of triangles and other polygons,[2] or at the intersection of two planes or curves, in which case the rays lying tangent to each curve at the point of intersection define the angle.Template:Sfn

It is common to consider that the sides of the angle divide the plane into two regions called the interior of the angle and the exterior of the angle. The interior of the angle is also referred to as an angular sector.[6][7]Template:Efn

Notation and measurement

File:Angle diagram.svg
BAC is formed by rays AB and AC. θ is the conventional measure of BAC and β is an alternative measure.

An angle symbol ( or ^, read as "angle") together with one or three defining points is used to identify angles in geometric figures. For example, the angle with vertex A formed by the rays AB and AC is denoted as A (using the vertex alone) or BAC (with the vertex always named in the middle). The size or measure of the angle is denoted mA or mBAC.

In geometric figures and mathematical expressions, it is also common to use Greek letters (α, β, γ, θ, φ, ...) or lower case Roman letters (abc, ...) as variables to represent the size of an angle.Template:Sfn Angular measure is commonly a scalar quantity,[8] although in physics and some fields of mathematics, signed angles are used by convention to indicate a direction of rotation: positive for anti-clockwise; negative for clockwise.[9]

Units of measurement

Angles are measured in various units, the most common being the degree (denoted by the symbol °), radian (denoted by the symbol rad) and turn. These units differ in the way they divide up a full angle, an angle where one ray, initially congruent to the other, performs a compete rotation about the vertex to return back to its starting position.[10]

Degrees and turns are defined directly with reference to a full angle, which measures 1 turn or 360°.[11] A measure in turns gives an angle's size as a proportion of a full angle and a degree can be considered as a subdivision of a turn. Radians are not defined directly in relation to a full angle (see Template:Section link), but in such a way that its measure is 2Template:Math rad, approximately 6.28 rad.[12]

Addition and subtraction

Script error: No such module "anchor".

File:Angle addition.svg
The angle addition postulate defines addition and subtraction of angles: θ + α = φ; φα = θ.

The angle addition postulate states that if D is a point lying in the interior of BAC then:[13] mBAC=mBAD+mDAC. This relationship defines what it means to add any two angles: their vertices are placed together while sharing a side to create a new larger angle. The measure of the new larger angle is the sum of the measures of the two angles. Subtraction follows from rearrangement of the formula.[13]

Types

Script error: No such module "redirect hatnote".

Common angles

Diagram visualizing common angles: zero, acute, right, obtuse, straight, reflex, full
Common types of angles
  • An angle equal to 0° or not turned is called a zero angle.Template:Sfn
  • An angle smaller than a right angle (less than 90°) is called an acute angle.Template:Sfn
  • An angle equal to Template:Sfrac turn (90° or Template:Sfrac rad) is called a right angle. Two lines that form a right angle are said to be normal, orthogonal, or perpendicular.Template:Sfn
  • An angle larger than a right angle and smaller than a straight angle (between 90° and 180°) is called an obtuse angleTemplate:Sfn ("obtuse" meaning "blunt").
  • An angle equal to Template:Sfrac turn (180° or Template:Math rad) is called a straight angle.Template:Sfn
  • An angle larger than a straight angle but less than 1 turn (between 180° and 360°) is called a reflex angle.
  • An angle equal to 1 turn (360° or 2Template:Math rad) is called a full angle, complete angle, round angle or perigon.
  • An angle that is not a multiple of a right angle is called an oblique angle.

Adjacent and vertical angles

Template:Redirect-distinguish Script error: No such module "Gallery". Adjacent angles (abbreviated adj. ∠s), are angles that share a common vertex and edge but do not share any interior points. In other words, they are angles side by side or adjacent, sharing an "arm".

Vertical angles are formed when two straight lines intersect at a point producing four angles. A pair of angles opposite each other are called vertical angles, opposite angles or vertically opposite angles (abbreviated vert. opp. ∠s),[14] where "vertical" refers to the sharing of a vertex, rather than an up-down orientation. A theorem states that vertical angles are always congruent or equal to each other.Template:Sfn A transversal is a line that intersects a pair of (often parallel) lines and is associated with exterior angles, interior angles, alternate exterior angles, alternate interior angles, corresponding angles, and consecutive interior angles.Template:Sfn

Combining angle pairs

When summing two angles (either adjacent or separated in space), three special cases are named complementary, supplementary, and explementary angles.

Complementary angles are angle pairs whose measures sum to a right angle (Template:Sfrac turn, 90°, or Template:Sfrac rad). If the two complementary angles are adjacent, their non-shared sides form a right angle. In a right-angle triangle the two acute angles are complementary as the sum of the internal angles of a triangle is 180°. The difference between an angle and a right angle is termed the complement of the angle.Template:Sfn

Supplementary angles sum to a straight angle (Template:Sfrac turn, 180°, or Template:Math rad). If the two supplementary angles are adjacent, their non-shared sides form a straight angle or straight line and are called a linear pair of angles.Template:Sfn The difference between an angle and a straight angle is termed the supplement of the angle.[15]

Explementary angles or conjugate angles sum to a full angle (1 turn, 360°, or 2Template:Math radians).[16] The difference between an angle and a full angle is termed the explement or conjugate of the angle.[17][18]

Examples of non-adjacent supplementary angles include the consecutive angles of a parallelogram and opposite angles of a cyclic quadrilateral. For a circle with center O, and tangent lines from an exterior point P touching the circle at points T and Q, the resulting angles ∠TPQ and ∠TOQ are supplementary.

Polygon-related angles

File:ExternalAngles.svg
Internal and external angles
  • An angle that is part of a simple polygon is called an interior angle if it lies on the inside of that simple polygon. A simple concave polygon has at least one interior angle, that is, a reflex angle. Template:Pb In Euclidean geometry, the measures of the interior angles of a triangle add up to Template:Math radians, 180°, or Template:Sfrac turn; the measures of the interior angles of a simple convex quadrilateral add up to 2Template:Math radians, 360°, or 1 turn. In general, the measures of the interior angles of a simple convex polygon with n sides add up to (n − 2)Template:Math radians, or (n − 2)180 degrees, (n − 2)2 right angles, or (n − 2)Template:Sfrac turn.
  • The supplement of an interior angle is called an exterior angle; that is, an interior angle and an exterior angle form a linear pair of angles. There are two exterior angles at each vertex of the polygon, each determined by extending one of the two sides of the polygon that meet at the vertex; these two angles are vertical and hence are equal. An exterior angle measures the amount of rotation one must make at a vertex to trace the polygon.Template:Sfn If the corresponding interior angle is a reflex angle, the exterior angle should be considered negative. Even in a non-simple polygon, it may be possible to define the exterior angle. Still, one will have to pick an orientation of the plane (or surface) to decide the sign of the exterior angle measure. Template:Pb In Euclidean geometry, the sum of the exterior angles of a simple convex polygon, if only one of the two exterior angles is assumed at each vertex, will be one full turn (360°). The exterior angle here could be called a supplementary exterior angle. Exterior angles are commonly used in Logo Turtle programs when drawing regular polygons.
  • In a triangle, the bisectors of two exterior angles and the bisector of the other interior angle are concurrent (meet at a single point).[19]Template:Rp
  • In a triangle, three intersection points, each of an external angle bisector with the opposite extended side, are collinear.[19]Template:Rp
  • In a triangle, three intersection points, two between an interior angle bisector and the opposite side, and the third between the other exterior angle bisector and the opposite side extended are collinear.[19]Template:Rp
  • Some authors use the name exterior angle of a simple polygon to mean the explement exterior angle (not supplement!) of the interior angle.[20] This conflicts with the above usage.

Plane-related angles

  • The angle between two planes (such as two adjacent faces of a polyhedron) is called a dihedral angle.Template:Sfn It may be defined as the acute angle between two lines normal to the planes.
  • The angle between a plane and an intersecting straight line is complementary to the angle between the intersecting line and the normal to the plane.

Measuring angles

Script error: No such module "Labelled list hatnote". Angle measurement encompasses both direct physical measurement using a measuring instrument such as a protractor, as well as the theoretical calculation of angle size from other known quantities. While the measurement of angles is intrinsically linked with rotation and circles, there are various perspectives as to exactly what is being measured, including amongst others: the amount of rotation about the vertex of one ray to the other;[21] the amount of opening between the rays;[22] or the length of the arc that subtends the angle at the centre of a unit circle.[23]

The measurement of angles is inherently different from the measurement of other physical quantities such as length.[24] Angles of special significance (such as the right angle) inform the systems and units of angular measurement, which is not the case for length where the units of measurement (metres, feet) are arbitrary.

Broadly there are two approaches to measuring angles: relative to a reference angle (such as a right angle); and circular measurement.

Reference angle

A chosen reference angle (right angle, straight angle or full angle) can be divided into equal parts, and the size of one part used as a unit for measurement of other angles.

In the most common method of practical angular measurement a right angle is divided into 90 equal parts called degrees, while in the rarely used centesimal system, a right angle is divided into 100 equal parts called gradians.[25][26]

Circular measurement

File:Basic angle in circle.svg
The angle size θ can be measured as s/r radians or s/C turns

With circular measurement an angle is placed within a circle of any size, with the vertex at the circle's centre and the sides intersecting the perimeter.

An arc with length s is formed as the perimeter between the two points of intersection, which is said to subtend the angle. The length s can be used to measure the angle's size θ, however as s is dependent on the size of the circle chosen, the measure must be scaled. This can be done by taking the ratio of s to either the radius r or circumference C of the circle.

The ratio of the length s by the radius r is the number of radians in the angle,[23] while the ratio of length s by the circumference C is the number of turns: θ=srrad=sCturn=s2πrturn

File:Radian measurement.svg
The radian measure of Template:Mathθ=sr=ssN

The value of Template:Math thus defined is independent of the size of the circle: if the length of the radius is changed, then both the circumference and the arc length change in the same proportion, so the ratios Template:Sfrac and Template:Sfrac are unaltered.Template:Refn

The ratio Template:Sfrac is called the "radian measure"[13] or "circular measure"[27][26][28] of an angle, but is also used to define a unit of measurement called a radian, which is defined as an angle for which the ratio Template:Sfrac = 1.[27] Thus, the measurement of an angle given by Template:Sfrac can be thought of in two ways: firstly as a measure in terms of the angle's own proportions (ratio of arc length to radius), or secondly as the quantity of units in the angle (ratio of arc length of measured angle to arc length of unit angle).[29][26]

Units

The following table lists some notable units used to represent angles.

Name (symbol) Number in one turn 1 unit in degrees Description
turn 1 360° The turn is the angle subtended by the circumference of a circle at its centre. A turn is equal to 2Template:Pi or [[Tau (mathematics)|Template:Tau]] radians.
degree ( ° ) 360 The degree may be defined such that one turn is equal to 360 degrees.
radian (rad) Template:Math Template:Val The radian is the angle subtended by an arc of a circle that has the same length as the circle's radius.
grad (gon) 400 0.9° The grad, also called grade, gradian, or gon, is defined such that a right angle is equal to as 100 gradians. The grad is used mostly in triangulation and continental surveying.
arcminute ( ′ ) Template:Val Template:Sfrac° The minute of arc (or arcminute, or just minute) is a sexagesimal subunit of a degree.
arcsecond ( ″ ) Template:Val Template:Sfrac° The second of arc (or arcsecond, or just second) is a sexagesimal subunit of a minute of arc.
milliradian (mrad) Template:Math Template:Val The milliradian is a thousandth of a radian. For artillery and navigation a unit is used, often called a 'mil', which are approximately equal to a milliradian. One turn is exactly 6000, 6300, or 6400 mils, depending on which definition is used.

Dimensional analysis

Script error: No such module "labelled list hatnote". In mathematics and the International System of Quantities, an angle is defined as a dimensionless quantity,[30] and in particular, the radian is defined as dimensionless in the International System of Units.[31] This convention prevents angles providing information for dimensional analysis. For example, when one measures an angle in radians by dividing the arc length by the radius, one is essentially dividing a length by another length, and the units of length cancel each other out. Therefore the result—the angle—doesn't have a physical "dimension" like meters or seconds.[32] This holds true with all angle units, such as radians, degrees, or turns—they all represent a pure number quantifying how much something has turned.[33] This is why, in many equations, angle units seem to "disappear" during calculations, which feels inconsistent and can lead to mixing up angle units.[34][35]

This has led to significant discussion among scientists and educators. Some scientists have suggested treating the angle as having its own fundamental dimension, similar to length or time.[36] This would mean that angle units like radians would always be explicitly present in calculations, facilitating dimensional analysis. However, this approach would also require changing many well-known mathematical and physics formulas, making them longer and perhaps a bit less familiar.[37] For now, the established practice is to write angle units where appropriate but consider them dimensionless, understanding that these units are important but behave differently from meters or kilograms.[38]

Signed angles

Script error: No such module "Labelled list hatnote". Script error: No such module "Labelled list hatnote".

File:Angles on the unit circle.svg
Measuring from the x-axis, angles on the unit circle count as positive in the counterclockwise direction, and negative in the clockwise direction.

An angle denoted as Template:Math might refer to any of four angles: the clockwise angle from B to C about A, the anticlockwise angle from B to C about A, the clockwise angle from C to B about A, or the anticlockwise angle from C to B about A, It is therefore frequently helpful to impose a convention that allows positive and negative angular values to represent orientations and/or rotations in opposite directions or "sense" relative to some reference.

In a two-dimensional Cartesian coordinate system, an angle is typically defined by its two sides, with its vertex at the origin. The initial side is on the positive x-axis, while the other side or terminal side is defined by the measure from the initial side in radians, degrees, or turns, with positive angles representing rotations toward the positive y-axis and negative angles representing rotations toward the negative y-axis. When Cartesian coordinates are represented by standard position, defined by the x-axis rightward and the y-axis upward, positive rotations are anticlockwise, and negative cycles are clockwise.

In many contexts, an angle of −θ is effectively equivalent to an angle of "one full turn minus θ". For example, an orientation represented as −45° is effectively equal to an orientation defined as 360° − 45° or 315°. Although the final position is the same, a physical rotation (movement) of −45° is not the same as a rotation of 315° (for example, the rotation of a person holding a broom resting on a dusty floor would leave visually different traces of swept regions on the floor).

In three-dimensional geometry, "clockwise" and "anticlockwise" have no absolute meaning, so the direction of positive and negative angles must be defined in terms of an orientation, which is typically determined by a normal vector passing through the angle's vertex and perpendicular to the plane in which the rays of the angle lie.

In navigation, bearings or azimuth are measured relative to north. By convention, viewed from above, bearing angles are positive clockwise, so a bearing of 45° corresponds to a north-east orientation. Negative bearings are not used in navigation, so a north-west orientation corresponds to a bearing of 315°.

Equivalent angles

  • Angles that have the same measure (i.e., the same magnitude) are said to be equal or congruent. An angle is defined by its measure and is not dependent upon the lengths of the sides of the angle (e.g., all right angles are equal in measure).
  • Two angles that share terminal sides, but differ in size by an integer multiple of a turn, are called coterminal angles.
  • The reference angle (sometimes called related angle) for any angle θ in standard position is the positive acute angle between the terminal side of θ and the x-axis (positive or negative).[39] Procedurally, the magnitude of the reference angle for a given angle may determined by taking the angle's magnitude modulo Template:Sfrac turn, 180°, or Template:Math radians, then stopping if the angle is acute, otherwise taking the supplementary angle, 180° minus the reduced magnitude. For example, an angle of 30 degrees is already a reference angle, and an angle of 150 degrees also has a reference angle of 30 degrees (180° − 150°). Angles of 210° and 510° correspond to a reference angle of 30 degrees as well (210° mod 180° = 30°, 510° mod 180° = 150° whose supplementary angle is 30°).

Related quantities

For an angular unit, it is definitional that the angle addition postulate holds, however some measurements or quantities related to angles are in use that do not satisfy this postulate:

  • The slope or gradient is equal to the tangent of the angle and is often expressed as a percentage ("rise" over "run"). For very small values (less than 5%), the slope of a line is approximately the measure in radians of its angle with the horizontal direction. An elevation grade is a slope used to indicate the steepness of roads, paths and railway lines.
  • The spread between two lines is defined in rational geometry as the square of the sine of the angle between the lines. As the sine of an angle and the sine of its supplementary angle are the same, any angle of rotation that maps one of the lines into the other leads to the same value for the spread between the lines.
  • Although done rarely, one can report the direct results of trigonometric functions, such as the sine of the angle.

Angles between curves

File:Curve angles.svg
The angle between the two curves at P is defined as the angle between the tangents A and B at P.

The angle between a line and a curve (mixed angle) or between two intersecting curves (curvilinear angle) is defined to be the angle between the tangents at the point of intersection. Various names (now rarely, if ever, used) have been given to particular cases:—amphicyrtic (Gr. Script error: No such module "Lang"., on both sides, κυρτός, convex) or cissoidal (Gr. κισσός, ivy), biconvex; xystroidal or sistroidal (Gr. ξυστρίς, a tool for scraping), concavo-convex; amphicoelic (Gr. κοίλη, a hollow) or angulus lunularis, biconcave.[40]

Bisecting and trisecting angles

Script error: No such module "Labelled list hatnote".

The ancient Greek mathematicians knew how to bisect an angle (divide it into two angles of equal measure) using only a compass and straightedge but could only trisect certain angles. In 1837, Pierre Wantzel showed that this construction could not be performed for most angles.

Dot product and generalisations

In the Euclidean space, the angle θ between two Euclidean vectors u and v is related to their dot product and their lengths by the formula 𝐮𝐯=cos(θ)𝐮𝐯.

This formula supplies an easy method to find the angle between two planes (or curved surfaces) from their normal vectors and between skew lines from their vector equations.

Inner product

To define angles in an abstract real inner product space, we replace the Euclidean dot product ( · ) by the inner product ,, i.e. 𝐮,𝐯=cos(θ) 𝐮𝐯.

In a complex inner product space, the expression for the cosine above may give non-real values, so it is replaced with Re(𝐮,𝐯)=cos(θ)𝐮𝐯. or, more commonly, using the absolute value, with |𝐮,𝐯|=|cos(θ)|𝐮𝐯.

The latter definition ignores the direction of the vectors. It thus describes the angle between one-dimensional subspaces span(𝐮) and span(𝐯) spanned by the vectors 𝐮 and 𝐯 correspondingly.

Angles between subspaces

The definition of the angle between one-dimensional subspaces span(𝐮) and span(𝐯) given by |𝐮,𝐯|=|cos(θ)|𝐮𝐯 in a Hilbert space can be extended to subspaces of finite number of dimensions. Given two subspaces 𝒰, 𝒲 with dim(𝒰):=kdim(𝒲):=l, this leads to a definition of k angles called canonical or principal angles between subspaces.

Angles in Riemannian geometry

In Riemannian geometry, the metric tensor is used to define the angle between two tangents. Where U and V are tangent vectors and gij are the components of the metric tensor G, cosθ=gijUiVj|gijUiUj||gijViVj|.

Hyperbolic angle

File:Hyperbolic rotation.gif
A constant hyperbolic angle (0.2), under hyperbolic rotation, corresponds to a variable circular angle.

A hyperbolic angle is an argument of a hyperbolic function just as the circular angle is the argument of a circular function. The comparison can be visualized as the size of the openings of a hyperbolic sector and a circular sector since the areas of these sectors correspond to the angle magnitudes in each case.[41] Unlike the circular angle, the hyperbolic angle is unbounded. When the circular and hyperbolic functions are viewed as infinite series in their angle argument, the circular ones are just alternating series forms of the hyperbolic functions. This comparison of the two series corresponding to functions of angles was described by Leonhard Euler in Introduction to the Analysis of the Infinite (1748).

History and etymology

The word angle comes from the Latin word Script error: No such module "Lang"., meaning "corner". Cognate words include the Greek Script error: No such module "Lang". (Script error: No such module "Lang".) meaning "crooked, curved" and the English word "ankle". Both are connected with the Proto-Indo-European root *ank-, meaning "to bend" or "bow".[42]

Philosophers have debated the nature of angles for millennia, with some arguing that angles are a measure (quantity), and others saying they are a kind of shape defined by the lines that bound it (qualitative relation), and still others saying an angle is both.[43] Pedagogically, the accepted answer is that angles are defined as figures, and the measure of an angle is defined as the number of congruent non-overlapping copies of a unit angle necessary to cover the angle and its interior. Angles are said to be equal in measure and similar or congruent in shape.[44]

Euclid defines a plane angle as the inclination to each other, in a plane, of two lines that meet each other and do not lie straight with respect to each other. According to the Neoplatonic metaphysician Proclus, an angle must be either a quality, a quantity, or a relationship. The first concept, angle as quality, was used by Eudemus of Rhodes, who regarded an angle as a deviation from a straight line; the second, angle as quantity, by Carpus of Antioch, who regarded it as the interval or space between the intersecting lines; Euclid adopted the third: angle as a relationship.[45]

Vertical angle theorem

The equality of vertically opposite angles is called the vertical angle theorem. Eudemus of Rhodes attributed the proof to Thales of Miletus.[46]Template:Sfn The proposition showed that since both of a pair of vertical angles are supplementary to both of the adjacent angles, the vertical angles are equal in measure. According to a historical note,Template:Sfn when Thales visited Egypt, he observed that whenever the Egyptians drew two intersecting lines, they would measure the vertical angles to make sure that they were equal. Thales concluded that one could prove that all vertical angles are equal if one accepted some general notions such as:

  • All straight angles are equal.
  • Equals added to equals are equal.
  • Equals subtracted from equals are equal.

When two adjacent angles form a straight line, they are supplementary. Therefore, if we assume that the measure of angle A equals x, the measure of angle C would be 180° − x. Similarly, the measure of angle D would be 180° − x. Both angle C and angle D have measures equal to 180° − x and are congruent. Since angle B is supplementary to both angles C and D, either of these angle measures may be used to determine the measure of Angle B. Using the measure of either angle C or angle D, we find the measure of angle B to be 180° − (180° − x) = x. Therefore, both angle A and angle B have measures equal to x and are equal in measure.

Angles in geography and astronomy

In geography, the location of any point on the Earth can be identified using a geographic coordinate system. This system specifies the latitude and longitude of any location in terms of angles subtended at the center of the Earth, using the equator and (usually) the Greenwich meridian as references.

In astronomy, a given point on the celestial sphere (that is, the apparent position of an astronomical object) can be identified using any of several astronomical coordinate systems, where the references vary according to the particular system. Astronomers measure the angular separation of two stars by imagining two lines through the center of the Earth, each intersecting one of the stars. The angle between those lines and the angular separation between the two stars can be measured.

In both geography and astronomy, a sighting direction can be specified in terms of a vertical angle such as altitude angle or elevation with respect to the horizon as well as the azimuth with respect to north.

Astronomers also measure objects' apparent size as an angular diameter. For example, the full moon has an angular diameter of approximately 0.5° when viewed from Earth. One could say, "The Moon's diameter subtends an angle of half a degree." The small-angle formula can convert such an angular measurement into a distance/size ratio.

Other astronomical approximations include:

  • 0.5° is the approximate angular diameter of the Sun and of the Moon as viewed from Earth.
  • 1° is the approximate angular width of the little finger at arm's length.
  • 10° is the approximate angular width of a closed fist at arm's length.
  • 20° is the approximate angular width of a handspan at arm's length.

These measurements depend on the individual subject, and the above should be treated as rough rule of thumb approximations only.

In astronomy, right ascension is usually measured in angular units that are expressed in terms of time based on a 24-hour day.[47]

Unit Symbol Degrees Radians Turns Other
Hour h 15° <templatestyles src="Fraction/styles.css" />Template:Pi12 rad <templatestyles src="Fraction/styles.css" />124 turn
Minute m 0°15′ <templatestyles src="Fraction/styles.css" />Template:Pi720 rad <templatestyles src="Fraction/styles.css" />1Template:Val turn <templatestyles src="Fraction/styles.css" />160 hour
Second s 0°0′15″ <templatestyles src="Fraction/styles.css" />Template:PiTemplate:Val rad <templatestyles src="Fraction/styles.css" />1Template:Val turn <templatestyles src="Fraction/styles.css" />160 minute

See also

Template:Div col

Template:Div col end

Notes

Template:Reflist Template:Notelist

References

Template:Reflist

Bibliography

Template:Refbegin

  • Script error: No such module "citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1"..
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1".
  • Script error: No such module "Template wrapper".Template:Main other
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1".

File:Wikisource-logo.svg This article incorporates text from a publication now in the public domainScript error: No such module "template wrapper". Template:Refend

Further reading

Template:Refbegin

  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".
  • Script error: No such module "Citation/CS1".

Template:Refend

External links

Template:Sister project Template:Sister project

Template:Authority control

  1. Script error: No such module "citation/CS1".
  2. a b Script error: No such module "citation/CS1".
  3. Script error: No such module "Footnotes".
  4. Script error: No such module "citation/CS1".
  5. Script error: No such module "citation/CS1".
  6. Script error: No such module "citation/CS1".
  7. Script error: No such module "citation/CS1".
  8. Script error: No such module "citation/CS1".
  9. Script error: No such module "Citation/CS1".
  10. Script error: No such module "citation/CS1".
  11. Script error: No such module "citation/CS1".
  12. Script error: No such module "citation/CS1".
  13. a b c Script error: No such module "citation/CS1".
  14. Script error: No such module "Footnotes".
  15. Script error: No such module "citation/CS1".
  16. Script error: No such module "citation/CS1".
  17. Script error: No such module "citation/CS1".
  18. Template:Cite thesis
  19. a b c Johnson, Roger A. Advanced Euclidean Geometry, Dover Publications, 2007.
  20. Script error: No such module "citation/CS1". as cited in Script error: No such module "Template wrapper".
  21. Script error: No such module "citation/CS1".
  22. Script error: No such module "citation/CS1".
  23. a b Script error: No such module "citation/CS1".
  24. Script error: No such module "Citation/CS1".
  25. Script error: No such module "citation/CS1".
  26. a b c Script error: No such module "citation/CS1".
  27. a b Script error: No such module "citation/CS1".
  28. Script error: No such module "citation/CS1".
  29. Script error: No such module "Citation/CS1".
  30. Script error: No such module "citation/CS1".
  31. Template:SIbrochure9th
  32. Script error: No such module "citation/CS1".
  33. Script error: No such module "Citation/CS1".
  34. Script error: No such module "Citation/CS1".
  35. Script error: No such module "Citation/CS1".
  36. Script error: No such module "Citation/CS1".
  37. Script error: No such module "Citation/CS1".
  38. Script error: No such module "Citation/CS1".
  39. Script error: No such module "citation/CS1".
  40. Script error: No such module "Footnotes".; Script error: No such module "Footnotes".
  41. Robert Baldwin Hayward (1892) The Algebra of Coplanar Vectors and Trigonometry, chapter six
  42. Script error: No such module "Footnotes".
  43. Script error: No such module "citation/CS1".
  44. Script error: No such module "Citation/CS1".
  45. Script error: No such module "Footnotes".; Script error: No such module "Footnotes".
  46. Script error: No such module "citation/CS1". Proposition I:13.
  47. Script error: No such module "citation/CS1".