Solar eclipse of September 8, 1801

Last updated
Solar eclipse of September 8, 1801
SE1801Sep08P.png
Map
Type of eclipse
NaturePartial
Gamma 1.4657
Magnitude 0.1614
Maximum eclipse
Coordinates 61°06′N168°30′W / 61.1°N 168.5°W / 61.1; -168.5
Times (UTC)
Greatest eclipse5:54:40
References
Saros 112 (71 of 72)
Catalog # (SE5000) 9044

A partial solar eclipse occurred at the Moon's descending node of orbit on Tuesday, September 8, 1801, with a magnitude of 0.1614. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

The partial solar eclipse was visible for parts of modern-day eastern Russia and western Alaska. [1]

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. [2]

September 8, 1801 Solar Eclipse Times
EventTime (UTC)
Equatorial Conjunction1801 September 08 at 04:23:25.3 UTC
First Penumbral External Contact1801 September 08 at 04:53:32.8 UTC
Ecliptic Conjunction1801 September 08 at 05:38:08.2 UTC
Greatest Eclipse1801 September 08 at 05:54:39.3 UTC
Last Penumbral External Contact1801 September 08 at 06:56:17.9 UTC
September 8, 1801 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.16147
Eclipse Obscuration0.07489
Gamma1.46568
Sun Right Ascension11h04m58.3s
Sun Declination+05°53'39.8"
Sun Semi-Diameter15'53.2"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension11h07m32.9s
Moon Declination+07°04'46.3"
Moon Semi-Diameter15'03.7"
Moon Equatorial Horizontal Parallax0°55'16.6"
ΔT12.8 s

Eclipse season

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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of September–October 1801
September 8
Descending node (new moon)
 September 22
Ascending node (full moon)
 October 7
Descending node (new moon)
SE1801Sep08P.png SE1801Oct07P.png
Partial solar eclipse
Solar Saros 112		 Total lunar eclipse
Lunar Saros 124		 Partial solar eclipse
Solar Saros 150

Eclipses in 1801

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 112

Inex

Triad

Solar eclipses of 1801–1805

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. [3]

The partial solar eclipses on April 13, 1801 and October 7, 1801 occur in the previous lunar year eclipse set, and the solar eclipses on January 1, 1805 (partial); June 26, 1805 (partial); and December 21, 1805 (annular) occur in the next lunar year eclipse set.

Solar eclipse series sets from 1801 to 1805
Ascending node Descending node
SarosMapGammaSarosMapGamma
107March 14, 1801
SE1801Mar14P.png
Partial		−1.4434112 September 8, 1801
SE1801Sep08P.png
Partial		1.4657
117 March 4, 1802
SE1802Mar04T.png
Total		−0.6943122 August 28, 1802
SE1802Aug28A.png
Annular		0.7569
127 February 21, 1803
SE1803Feb21T.png
Total		−0.0075132 August 17, 1803
SE1803Aug17A.png
Annular		−0.0048
137February 11, 1804
SE1804Feb11H.png
Hybrid		0.7053142August 5, 1804
SE1804Aug05T.gif
Total		−0.7622
147January 30, 1805
SE1805Jan30P.gif
Partial		1.4651152July 26, 1805
SE1805Jul26Pb.gif
Partial		−1.4571

Saros 112

This eclipse is a part of Saros series 112, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 31, 539 AD. It contains total eclipses from March 15, 918 AD through November 18, 1332; hybrid eclipses from November 30, 1350 through April 29, 1585; and annular eclipses from May 11, 1603 through June 23, 1675. The series ends at member 72 as a partial eclipse on September 19, 1819. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of totality was produced by member 30 at 7 minutes, 20 seconds on June 9, 1062, and the longest duration of annularity was produced by member 64 at 1 minute, 1 second on June 23, 1675. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

22 eclipse events between September 8, 1801 and September 7, 1877
September 7–8June 26–27April 14–15January 31–February 1November 19–20
112114116118120
SE1801Sep08P.png
September 8, 1801 		SE1805Jun26P.gif
June 26, 1805		 SE1809Apr14A.gif
April 14, 1809		 SE1813Feb01A.gif
February 1, 1813		 SE1816Nov19T.png
November 19, 1816
122124126128130
SE1820Sep07A.png
September 7, 1820 		SE1824Jun26T.png
June 26, 1824 		Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828		 SE1832Feb01A.gif
February 1, 1832		 SE1835Nov20T.gif
November 20, 1835
132134136138140
SE1839Sep07A.png
September 7, 1839		 SE1843Jun27H.gif
June 27, 1843		 SE1847Apr15T.gif
April 15, 1847		 SE1851Feb01A.gif
February 1, 1851		 SE1854Nov20H.png
November 20, 1854
142144146148150
SE1858Sep07T.png
September 7, 1858 		SE1862Jun27P.gif
June 27, 1862		 SE1866Apr15P.gif
April 15, 1866		 SE1870Jan31P.gif
January 31, 1870		 SE1873Nov20P.png
November 20, 1873
152
SE1877Sep07P.gif
September 7, 1877

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
SE1801Sep08P.png
September 8, 1801
(Saros 112)		 SE1812Aug07P.gif
August 7, 1812
(Saros 113)		 SE1823Jul08P.gif
July 8, 1823
(Saros 114)		 SE1834Jun07P.gif
June 7, 1834
(Saros 115)		 SE1845May06An.gif
May 6, 1845
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)		 SE1867Mar06A.gif
March 6, 1867
(Saros 118)		 SE1878Feb02A.gif
February 2, 1878
(Saros 119)		 SE1889Jan01T.png
January 1, 1889
(Saros 120)		 SE1899Dec03A.png
December 3, 1899
(Saros 121)
SE1910Nov02P.png
November 2, 1910
(Saros 122)		 SE1921Oct01T.png
October 1, 1921
(Saros 123)		 SE1932Aug31T.png
August 31, 1932
(Saros 124)		 SE1943Aug01A.png
August 1, 1943
(Saros 125)		 SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1965May30T.png
May 30, 1965
(Saros 127)		 SE1976Apr29A.png
April 29, 1976
(Saros 128)		 SE1987Mar29H.png
March 29, 1987
(Saros 129)		 SE1998Feb26T.png
February 26, 1998
(Saros 130)		 SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2019Dec26A.png
December 26, 2019
(Saros 132)		 SE2030Nov25T.png
November 25, 2030
(Saros 133)		 SE2041Oct25A.png
October 25, 2041
(Saros 134)		 SE2052Sep22A.png
September 22, 2052
(Saros 135)		 SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2074Jul24A.png
July 24, 2074
(Saros 137)		 SE2085Jun22A.png
June 22, 2085
(Saros 138)		 SE2096May22T.png
May 22, 2096
(Saros 139)		 SE2107Apr23A.png
April 23, 2107
(Saros 140)		 SE2118Mar22A.png
March 22, 2118
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)		 SE2140Jan20A.png
January 20, 2140
(Saros 143)		 SE2150Dec19A.png
December 19, 2150
(Saros 144)		 SE2161Nov17T.png
November 17, 2161
(Saros 145)		 SE2172Oct17H.png
October 17, 2172
(Saros 146)
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)		 Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
SE1801Sep08P.png
September 8, 1801
(Saros 112)		 SE1830Aug18P.gif
August 18, 1830
(Saros 113)		 SE1859Jul29P.gif
July 29, 1859
(Saros 114)
SE1888Jul09P.gif
July 9, 1888
(Saros 115)		 SE1917Jun19P.png
June 19, 1917
(Saros 116)		 SE1946May30P.png
May 30, 1946
(Saros 117)
SE1975May11P.png
May 11, 1975
(Saros 118)		 SE2004Apr19P.png
April 19, 2004
(Saros 119)		 SE2033Mar30T.png
March 30, 2033
(Saros 120)
SE2062Mar11P.png
March 11, 2062
(Saros 121)		 SE2091Feb18P.png
February 18, 2091
(Saros 122)		 Saros123 59van70 SE2120Jan30P.jpg
January 30, 2120
(Saros 123)
Saros124 62van73 SE2149Jan09P.jpg
January 9, 2149
(Saros 124)		 Saros125 63van73 SE2177Dec20P.jpg
December 20, 2177
(Saros 125)

See also

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References

  1. ↑ "Solar eclipse of September 8, 1801". NASA . Retrieved June 15, 2012.
  2. ↑ "Partial Solar Eclipse of 1801 Sep 08". EclipseWise.com. Retrieved 28 September 2024.
  3. ↑ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  4. ↑ "NASA - Catalog of Solar Eclipses of Saros 112". eclipse.gsfc.nasa.gov.
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