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	<title>53 Camelopardalis - Revision history</title>
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	<updated>2026-05-10T16:24:29Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<title>imported&gt;Loooke: add orbit</title>
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		<updated>2025-02-08T19:35:38Z</updated>

		<summary type="html">&lt;p&gt;add orbit&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Short description|Star in the constellation Camelopardalis}}&lt;br /&gt;
{{Starbox begin}}&lt;br /&gt;
{{Starbox image&lt;br /&gt;
| image = [[Image:AXCamLightCurve.png|250px]]&lt;br /&gt;
| caption = A [[light curve]] for AX Camelopardalis, plotted from &amp;#039;&amp;#039;[[Transiting Exoplanet Survey Satellite|TESS]]&amp;#039;&amp;#039; data&amp;lt;ref name=MAST/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox observe&lt;br /&gt;
 | epoch = [[J2000.0]]&lt;br /&gt;
 | constell = [[Camelopardalis (constellation)|Camelopardalis]]&lt;br /&gt;
 | ra = {{RA|08|01|42.43137}}&amp;lt;ref name=GaiaDR2/&amp;gt;&lt;br /&gt;
 | dec = {{DEC|+60|19|27.8016}}&amp;lt;ref name=GaiaDR2/&amp;gt;&lt;br /&gt;
 | appmag_v = {{nowrap|6.02&amp;lt;ref name=Anderson2012/&amp;gt; (6.3 + 7.5)&amp;lt;ref name=Malkov2012/&amp;gt;}}&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox character&lt;br /&gt;
 | type  = main sequence&lt;br /&gt;
 | class = A3VpSrSiCrEu&amp;lt;ref name=abt1995/&amp;gt;&lt;br /&gt;
 | b-v   = {{Val|0.158|0.005}}&amp;lt;ref name=Anderson2012/&amp;gt;&lt;br /&gt;
 | variable = [[Alpha2 Canum Venaticorum|α&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; CVn]]&amp;lt;ref name=Samus2017/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox astrometry&lt;br /&gt;
 | radial_v = {{Val|−2.2}}&amp;lt;ref name=Anderson2012/&amp;gt;&lt;br /&gt;
 | prop_mo_ra  = −21.367&amp;lt;ref name=GaiaDR2/&amp;gt;&lt;br /&gt;
 | prop_mo_dec = −26.386&amp;lt;ref name=GaiaDR2/&amp;gt;&lt;br /&gt;
 | parallax = 11.2327&lt;br /&gt;
 | p_error  = 0.1547&lt;br /&gt;
 | parallax_footnote = &amp;lt;ref name=GaiaDR2/&amp;gt;&lt;br /&gt;
 | absmag_v = 1.05&amp;lt;ref name=Anderson2012/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox orbit&lt;br /&gt;
 | reference = &amp;lt;ref name=ORB6&amp;gt;{{cite web|url=http://www.astro.gsu.edu/wds/orb6.html|title=Sixth Catalog of Orbits of Visual Binary Stars|publisher=United States Naval Observatory|accessdate=2025-02-08}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
 | period_unitless = {{Val|6.6504|0.0089}}&lt;br /&gt;
 | axis = {{val|0.055|0.018}}&lt;br /&gt;
 | inclination = {{val|55.4|2.9}}&lt;br /&gt;
 | node = {{val|118.3|20.1}}&lt;br /&gt;
 | periastron = {{Val|2001.2281|0.025}}&lt;br /&gt;
 | eccentricity = {{Val|0.706|0.024}}&lt;br /&gt;
 | periarg = {{Val|8.3|1.8}}&lt;br /&gt;
 | k1 = {{Val|12.08|0.45}}&amp;lt;ref name=Carrier2002/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox detail&lt;br /&gt;
 | source  = &amp;lt;ref name=Carrier2002/&amp;gt;&lt;br /&gt;
 | component1 = 53 Cam A&lt;br /&gt;
 | mass    = {{Val|2.074|0.012}}&lt;br /&gt;
 | radius  = {{Val|2.36|0.10}}&lt;br /&gt;
 | gravity = {{Val|3.70|0.10}}&lt;br /&gt;
 | luminosity  = {{Val|24.9|1.15}}&lt;br /&gt;
 | temperature = {{Val|8400|150|fmt=commas}}&lt;br /&gt;
 | metal_fe = &lt;br /&gt;
 | rotational_velocity = {{Val|12.5|0.5|fmt=commas}}&lt;br /&gt;
 | rotation = {{Val|8.02681|0.00004|u=days}}&lt;br /&gt;
 | age_myr  = {{Val|615|56|51}}&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox catalog&lt;br /&gt;
 | names = {{odlist | V=AX Cam | F=53 Cam | BD=+60°1105 | FK5=302 | HD=65339 | HIP=39261 | HR=3109 | SAO=14402 | GC=10822 | CCDM=08017+6019 | WDS=J08017+6019 }}&amp;lt;ref name=SIMBAD/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox reference&lt;br /&gt;
 | Simbad = 53+Cam&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox end}}&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;53 Camelopardalis&amp;#039;&amp;#039;&amp;#039; is a [[binary star]] system in the northern [[circumpolar constellation]] of [[Camelopardalis]],&amp;lt;ref name=SIMBAD/&amp;gt; located 290&amp;amp;nbsp;[[light year]]s away from the Sun as determined by [[stellar parallax|parallax]] measurements.&amp;lt;ref name=GaiaDR2/&amp;gt; It has the [[variable star designation]] &amp;#039;&amp;#039;&amp;#039;AX Camelopardalis&amp;#039;&amp;#039;&amp;#039;; &amp;#039;&amp;#039;53 Camelopardalis&amp;#039;&amp;#039; is the [[Flamsteed designation]].&amp;lt;ref name=SIMBAD/&amp;gt; This object is dimly visible to the [[naked eye]] as a white hued star with a baseline [[apparent visual magnitude]] of +6.02.&amp;lt;ref name=Anderson2012/&amp;gt; It is a single-lined [[spectroscopic binary]]&amp;lt;ref name=Kochukhov2004/&amp;gt; system with an [[orbital period]] of 6.63&amp;amp;nbsp;years and a high [[orbital eccentricity|eccentricity]] of about 0.7.&amp;lt;ref name=Carrier2002/&amp;gt; The &amp;quot;&amp;#039;&amp;#039;a&amp;#039;&amp;#039; sin &amp;#039;&amp;#039;i&amp;#039;&amp;#039;&amp;quot; value of the primary is {{Convert|280|Gm|AU|abbr=on|lk=on}}, where &amp;#039;&amp;#039;a&amp;#039;&amp;#039; is the [[semimajor axis]] and &amp;#039;&amp;#039;i&amp;#039;&amp;#039; is the [[orbital inclination]].&amp;lt;ref name=Carrier2002/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The visible component is a well-studied magnetic [[Ap star]]&amp;lt;ref name=Carrier2002/&amp;gt; with a [[stellar classification]] of A3VpSrSiCrEu&amp;lt;ref name=abt1995/&amp;gt; and a visual magnitude of 6.3.&amp;lt;ref name=Malkov2012/&amp;gt; The [[stellar magnetic field|magnetic field]] topology of 53 Camelopardalis is complex, and is accompanied by abundance variations across the surface of elements like silicon, calcium, titanium, iron, and neodymium.&amp;lt;ref name=Carrier2002/&amp;gt; &lt;br /&gt;
&lt;br /&gt;
Tadeusz Jarzębowski discovered that 53 Camelopardalis is a [[variable star]], in 1960.&amp;lt;ref name=&amp;quot;Jarzębowski1960&amp;quot;/&amp;gt; It is classified as an [[Alpha2 Canum Venaticorum variable|Alpha&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; Canum Venaticorum]] type variable star and the combined brightness of the system varies from magnitude +6.00 down to +6.05 with a rotationally-modulated period of 8.0278 days.&amp;lt;ref name=Samus2017/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The primary has 2.1 times the [[mass of the Sun]] and 2.4 times the [[Sun&amp;#039;s radius]]. It is spinning with a [[projected rotational velocity]] of 12.5&amp;amp;nbsp;km/s and a [[rotation period]] of 8.0268&amp;amp;nbsp;days. The inclination angle of the pole is estimated to be {{Val|57|5|u=°}}. The star is about 615&amp;amp;nbsp;million years old and is radiating 25 times the [[luminosity of the Sun]] from its [[photosphere]] at an [[effective temperature]] of 8,400&amp;amp;nbsp;K.&amp;lt;ref name=Carrier2002/&amp;gt; &lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist|refs=&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=GaiaDR2&amp;gt;{{cite DR2|1088465727807087744}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=SIMBAD&amp;gt;{{cite simbad | title=53 Cam | access-date=2019-04-22 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;Jarzębowski1960&amp;quot;&amp;gt;{{cite journal&lt;br /&gt;
 | last1=Jarzębowski | first1=T.&lt;br /&gt;
 | title=Relation between Light-variation and Magnetic Variation in Magnetic Alpha Variables&lt;br /&gt;
 | journal=Acta Astronomica | date=1960 | volume=10 | pages=31–52&lt;br /&gt;
 | bibcode=1960AcA....10...31J | url=https://articles.adsabs.harvard.edu/pdf/1960AcA....10...31J&lt;br /&gt;
 | access-date=29 December 2024}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=Anderson2012&amp;gt;{{citation&lt;br /&gt;
 | title=XHIP: An extended hipparcos compilation&lt;br /&gt;
 | last1=Anderson | first1=E. | last2=Francis | first2=Ch.&lt;br /&gt;
 | journal=Astronomy Letters | postscript=.&lt;br /&gt;
 | volume=38 | issue=5 | pages=331 | year=2012&lt;br /&gt;
 | bibcode=2012AstL...38..331A | arxiv=1108.4971&lt;br /&gt;
 | doi=10.1134/S1063773712050015 | s2cid=119257644 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=MAST&amp;gt;{{cite web&lt;br /&gt;
 | title=MAST: Barbara A. Mikulski Archive for Space Telescopes&lt;br /&gt;
 | url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html&lt;br /&gt;
 | publisher=Space Telescope Science Institute |access-date=8 December 2021}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=Carrier2002&amp;gt;{{citation&lt;br /&gt;
 | title=Multiplicity among chemically peculiar stars. II. Cool magnetic Ap stars&lt;br /&gt;
 | last1=Carrier | first1=F. | last2=North | first2=P.&lt;br /&gt;
 | last3=Udry | first3=S. | last4=Babel | first4=J.&lt;br /&gt;
 | display-authors=1 | journal=Astronomy and Astrophysics&lt;br /&gt;
 | volume=394 | pages=151–169 | date=October 2002&lt;br /&gt;
 | doi=10.1051/0004-6361:20021122 | postscript=.&lt;br /&gt;
 | bibcode=2002A&amp;amp;A...394..151C | arxiv=astro-ph/0208082 | s2cid=14223227 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=Kochukhov2004&amp;gt;{{citation&lt;br /&gt;
 | title=Magnetic Doppler imaging of 53 Camelopardalis in all four Stokes parameters&lt;br /&gt;
 | last1=Kochukhov | first1=O. | last2=Bagnulo | first2=S.&lt;br /&gt;
 | last3=Wade | first3=G. A. | last4=Sangalli | first4=L.&lt;br /&gt;
 | last5=Piskunov | first5=N. | last6=Landstreet | first6=J. D.&lt;br /&gt;
 | last7=Petit | first7=P. | last8=Sigut | first8=T. A. A.&lt;br /&gt;
 | display-authors=1 | journal=Astronomy and Astrophysics&lt;br /&gt;
 | volume=414 | pages=613–632 | date=February 2004&lt;br /&gt;
 | issue=2 | doi=10.1051/0004-6361:20031595 | bibcode=2004A&amp;amp;A...414..613K | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=abt1995&amp;gt;{{citation&lt;br /&gt;
 | last1=Abt | first1=Helmut A. | last2=Morrell | first2=Nidia I.&lt;br /&gt;
 | title=The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars&lt;br /&gt;
 | journal=Astrophysical Journal Supplement Series&lt;br /&gt;
 | volume=99 | pages=135 | year=1995&lt;br /&gt;
 | bibcode=1995ApJS...99..135A | doi=10.1086/192182 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=Samus2017&amp;gt;{{citation&lt;br /&gt;
 | display-authors=1 | last1=Samus | first1=N. N.&lt;br /&gt;
 | last2=Kazarovets | first2=E. V. | last3=Durlevich | first3=O. V.&lt;br /&gt;
 | last4=Kireeva | first4=N. N. | last5=Pastukhova | first5=E. N. &lt;br /&gt;
 | title=General Catalogue of Variable Stars&lt;br /&gt;
 | version=5.1 | journal=Astronomy Reports&lt;br /&gt;
 | year=2017 | volume=61 | issue=1 | pages=80–88&lt;br /&gt;
 | doi=10.1134/S1063772917010085 | bibcode=2017ARep...61...80S | s2cid=125853869 | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=Malkov2012&amp;gt;{{citation&lt;br /&gt;
 | last1=Malkov | first1=O. Yu. | last2=Tamazian | first2=V. S.&lt;br /&gt;
 | last3=Docobo | first3=J. A. | last4=Chulkov | first4=D. A.&lt;br /&gt;
 | title=Dynamical Masses of a Selected Sample of Orbital Binaries&lt;br /&gt;
 | display-authors=1 | journal=Astronomy &amp;amp; Astrophysics&lt;br /&gt;
 | volume=546 | id=A69 | pages=5 | date=2012&lt;br /&gt;
 | doi=10.1051/0004-6361/201219774 | bibcode=2012A&amp;amp;A...546A..69M | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
{{Stars of Camelopardalis}}&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:53 Camelopardalis}}&lt;br /&gt;
[[Category:A-type main-sequence stars]]&lt;br /&gt;
[[Category:Ap stars]]&lt;br /&gt;
[[Category:Alpha2 Canum Venaticorum variables]]&lt;br /&gt;
[[Category:Spectroscopic binaries]]&lt;br /&gt;
[[Category:Camelopardalis]]&lt;br /&gt;
[[Category:Durchmusterung objects]]&lt;br /&gt;
[[Category:Flamsteed objects|Camelopardalis, 53]]&lt;br /&gt;
[[Category:Henry Draper Catalogue objects|065339]]&lt;br /&gt;
[[Category:Hipparcos objects|039261]]&lt;br /&gt;
[[Category:Bright Star Catalogue objects|3109]]&lt;br /&gt;
[[Category:Objects with variable star designations|Camelopardalis, AX]]&lt;/div&gt;</summary>
		<author><name>imported&gt;Loooke</name></author>
	</entry>
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