Solar eclipse of July 18, 1860

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Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, July 18, 1860, with a magnitude of 1.0500. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.2 days before perigee (on July 20, 1860, at 19:15 UTC), the Moon's apparent diameter was larger.[1]

The path of totality was visible from parts of modern-day northwestern Oregon, Washington, northern Idaho, northwestern Montana, Canada, Spain, Algeria, Tunisia, Libya, Egypt, Sudan, and Eritrea. A partial solar eclipse was also visible for parts of North America, Europe, West Asia, North Africa, and West Africa.

Coronal Mass Ejection

The first coronal mass ejection may have been observed as coronal loops progressing during this total eclipse.[2]

File:Toulouse - L'éclipse de La lunette M. Raux (Baux ^) et ... (illisible) coll. humide - Fonds Trutat - MHNT.PHa.814.105.jpg
People watching an eclipse in 1860 at Toulouse, France. Picture by Eugène Trutat, Muséum de Toulouse.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[3]

July 18, 1860 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1860 July 18 at 11:54:56.3 UTC
First Umbral External Contact 1860 July 18 at 12:57:13.1 UTC
First Central Line 1860 July 18 at 12:58:21.9 UTC
First Umbral Internal Contact 1860 July 18 at 12:59:31.0 UTC
Equatorial Conjunction 1860 July 18 at 14:09:18.4 UTC
Ecliptic Conjunction 1860 July 18 at 14:20:40.8 UTC
Greatest Duration 1860 July 18 at 14:24:54.3 UTC
Greatest Eclipse 1860 July 18 at 14:26:24.2 UTC
Last Umbral Internal Contact 1860 July 18 at 15:53:26.2 UTC
Last Central Line 1860 July 18 at 15:54:37.2 UTC
Last Umbral External Contact 1860 July 18 at 15:55:48.0 UTC
Last Penumbral External Contact 1860 July 18 at 16:57:54.9 UTC
July 18, 1860 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.05000
Eclipse Obscuration 1.10249
Gamma 0.54871
Sun Right Ascension 07h52m23.3s
Sun Declination +20°56'51.5"
Sun Semi-Diameter 15'44.4"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 07h53m03.2s
Moon Declination +21°28'15.4"
Moon Semi-Diameter 16'18.0"
Moon Equatorial Horizontal Parallax 0°59'49.1"
ΔT 7.7 s

Eclipse season

Script error: No such module "Labelled list hatnote". This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of July–August 1860
July 18
Descending node (new moon)
August 1
Ascending node (full moon)
File:SE1860Jul18T.png
Total solar eclipse
Solar Saros 124
Partial lunar eclipse
Lunar Saros 136

Related eclipses

Eclipses in 1860

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 124

Inex

Triad

Solar eclipses of 1859–1862

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[4]

The partial solar eclipses on March 4, 1859 and August 28, 1859 occur in the previous lunar year eclipse set, and the partial solar eclipse on November 21, 1862 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1859 to 1862
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
109 February 3, 1859
File:SE1859Feb03Pe.gif
Partial
−1.5659 114 July 29, 1859
File:SE1859Jul29P.gif
Partial
1.2598
119 January 23, 1860
File:SE1860Jan23A.png
Annular
−0.8969 124 July 18, 1860
File:SE1860Jul18T.png
Total
0.5487
129 January 11, 1861
File:SE1861Jan11A.gif
Annular
−0.1766 134 July 8, 1861
File:SE1861Jul08A.gif
Annular
−0.2231
139 December 31, 1861
File:SE1861Dec31T.gif
Total
0.5187 144 June 27, 1862
File:SE1862Jun27P.gif
Partial
−1.0252
149 December 21, 1862
File:SE1862Dec21P.gif
Partial
1.1633

Saros 124

Template:Solar Saros series 124

Metonic series

Template:Solar Metonic series 1830–1917

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
File:SE1805Dec21A.gif
December 21, 1805
(Saros 119)
File:SE1816Nov19T.gif
November 19, 1816
(Saros 120)
File:SE1827Oct20H.gif
October 20, 1827
(Saros 121)
File:SE1838Sep18A.gif
September 18, 1838
(Saros 122)
File:SE1849Aug18T.gif
August 18, 1849
(Saros 123)
File:SE1860Jul18T.gif
July 18, 1860
(Saros 124)
File:SE1871Jun18A.gif
June 18, 1871
(Saros 125)
File:SE1882May17T.png
May 17, 1882
(Saros 126)
File:SE1893Apr16T.png
April 16, 1893
(Saros 127)
File:SE1904Mar17A.png
March 17, 1904
(Saros 128)
File:SE1915Feb14A.png
February 14, 1915
(Saros 129)
File:SE1926Jan14T.png
January 14, 1926
(Saros 130)
File:SE1936Dec13A.png
December 13, 1936
(Saros 131)
File:SE1947Nov12A.png
November 12, 1947
(Saros 132)
File:SE1958Oct12T.png
October 12, 1958
(Saros 133)
File:SE1969Sep11A.png
September 11, 1969
(Saros 134)
File:SE1980Aug10A.png
August 10, 1980
(Saros 135)
File:SE1991Jul11T.png
July 11, 1991
(Saros 136)
File:SE2002Jun10A.png
June 10, 2002
(Saros 137)
File:SE2013May10A.png
May 10, 2013
(Saros 138)
File:SE2024Apr08T.png
April 8, 2024
(Saros 139)
File:SE2035Mar09A.png
March 9, 2035
(Saros 140)
File:SE2046Feb05A.png
February 5, 2046
(Saros 141)
File:SE2057Jan05T.png
January 5, 2057
(Saros 142)
File:SE2067Dec06H.png
December 6, 2067
(Saros 143)
File:SE2078Nov04A.png
November 4, 2078
(Saros 144)
File:SE2089Oct04T.png
October 4, 2089
(Saros 145)
File:SE2100Sep04T.png
September 4, 2100
(Saros 146)
File:SE2111Aug04A.png
August 4, 2111
(Saros 147)
File:Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
(Saros 148)
File:SE2133Jun03T.png
June 3, 2133
(Saros 149)
File:Saros150 24van71 SE2144May03A.jpg
May 3, 2144
(Saros 150)
File:SE2155Apr02A.png
April 2, 2155
(Saros 151)
File:Saros152 21van70 SE2166Mar02T.jpg
March 2, 2166
(Saros 152)
File:Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
(Saros 153)
File:Saros154 16van71 SE2187Dec29A.jpg
December 29, 2187
(Saros 154)
File:SE2198Nov28T.png
November 28, 2198
(Saros 155)

Inex series

Template:Solar Inex series 2005 April 8

See also

References

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  2. Coronal Mass Ejections from the Sun - Propagation and Near Earth Effects
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