Solar eclipse of October 25, 2041

Last updated
Solar eclipse of October 25, 2041
SE2041Oct25A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.4133
Magnitude 0.9467
Maximum eclipse
Duration367 s (6 min 7 s)
Coordinates 9°54′N162°54′E / 9.9°N 162.9°E / 9.9; 162.9
Max. width of band213 km (132 mi)
Times (UTC)
Greatest eclipse1:36:22
References
Saros 134 (45 of 71)
Catalog # (SE5000) 9600

An annular solar eclipse will occur at the Moon's descending node of orbit between Thursday, October 24 and Friday, October 25, 2041, [1] with a magnitude of 0.9467. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 4.3 days after apogee (on October 20, 2041, at 17:10 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Mongolia, northeastern China, North Korea, Japan, the Marshall Islands, and Kiribati. A partial solar eclipse will be visible for parts of East Asia, Southeast Asia, northeastern Australia, Oceania, and Hawaii.

Images

SE2041Oct25A.gif
Animated path

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]

October 25, 2041 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2041 October 24 at 22:41:02.8 UTC
First Umbral External Contact2041 October 24 at 23:48:18.5 UTC
First Central Line2041 October 24 at 23:50:49.8 UTC
First Umbral Internal Contact2041 October 24 at 23:53:21.7 UTC
Equatorial Conjunction2041 October 25 at 01:13:01.1 UTC
First Penumbral Internal Contact2041 October 25 at 01:22:11.2 UTC
Ecliptic Conjunction2041 October 25 at 01:31:31.7 UTC
Greatest Eclipse2041 October 25 at 01:36:21.7 UTC
Last Penumbral Internal Contact2041 October 25 at 01:51:07.0 UTC
Greatest Duration2041 October 25 at 01:51:55.5 UTC
Last Umbral Internal Contact2041 October 25 at 03:19:38.3 UTC
Last Central Line2041 October 25 at 03:22:07.7 UTC
Last Umbral External Contact2041 October 25 at 03:24:36.3 UTC
Last Penumbral External Contact2041 October 25 at 04:31:44.8 UTC
October 25, 2041 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.94666
Eclipse Obscuration0.89617
Gamma0.41332
Sun Right Ascension13h59m22.0s
Sun Declination-12°10'20.1"
Sun Semi-Diameter16'04.9"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension14h00m02.5s
Moon Declination-11°49'54.3"
Moon Semi-Diameter15'00.8"
Moon Equatorial Horizontal Parallax0°55'06.0"
ΔT79.5 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.

Eclipse season of October–November 2041
October 25
Descending node (new moon)
 November 8
Ascending node (full moon)
SE2041Oct25A.png Lunar eclipse chart close-2041Nov08.png
Annular solar eclipse
Solar Saros 134		 Partial lunar eclipse
Lunar Saros 146

Eclipses in 2041

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 134

Inex

Triad

Solar eclipses of 2040–2043

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]

Solar eclipse series sets from 2040 to 2043
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 May 11, 2040
SE2040May11P.png
Partial		−1.2529124 November 4, 2040
SE2040Nov04P.png
Partial		1.0993
129 April 30, 2041
SE2041Apr30T.png
Total		−0.4492134 October 25, 2041
SE2041Oct25A.png
Annular		0.4133
139 April 20, 2042
SE2042Apr20T.png
Total		0.2956144 October 14, 2042
SE2042Oct14A.png
Annular		−0.303
149 April 9, 2043
SE2043Apr09T.png
Total (non-central)		1.0031154 October 3, 2043
SE2043Oct03A.png
Annular (non-central)		1.0102

Saros 134

This eclipse is a part of Saros series 134, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554; hybrid eclipses from January 3, 1573 through June 27, 1843; and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 72 as a partial eclipse on August 6, 2510. 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 11 at 1 minutes, 30 seconds on October 9, 1428, and the longest duration of annularity will be produced by member 52 at 10 minutes, 55 seconds on January 10, 2168. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 32–53 occur between 1801 and 2200:
323334
SE1807Jun06H.png
June 6, 1807		 SE1825Jun16H.png
June 16, 1825		 SE1843Jun27H.png
June 27, 1843
353637
SE1861Jul08A.png
July 8, 1861		 SE1879Jul19A.png
July 19, 1879		 SE1897Jul29A.png
July 29, 1897
383940
SE1915Aug10A.png
August 10, 1915 		SE1933Aug21A.png
August 21, 1933 		SE1951Sep01A.png
September 1, 1951
414243
SE1969Sep11A.png
September 11, 1969 		SE1987Sep23A.png
September 23, 1987 		SE2005Oct03A.png
October 3, 2005
444546
SE2023Oct14A.png
October 14, 2023 		SE2041Oct25A.png
October 25, 2041 		SE2059Nov05A.png
November 5, 2059
474849
SE2077Nov15A.png
November 15, 2077 		SE2095Nov27A.png
November 27, 2095 		SE2113Dec08A.png
December 8, 2113
505152
SE2131Dec19A.png
December 19, 2131		 SE2149Dec30A.png
December 30, 2149		 SE2168Jan10A.png
January 10, 2168
53
SE2186Jan20A.png
January 20, 2186

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 June 1, 2011 and October 24, 2098
May 31–June 1March 19–20January 5–6October 24–25August 12–13
118120122124126
SE2011Jun01P.png
June 1, 2011 		SE2015Mar20T.png
March 20, 2015 		SE2019Jan06P.png
January 6, 2019 		SE2022Oct25P.png
October 25, 2022 		SE2026Aug12T.png
August 12, 2026
128130132134136
SE2030Jun01A.png
June 1, 2030 		SE2034Mar20T.png
March 20, 2034 		SE2038Jan05A.png
January 5, 2038 		SE2041Oct25A.png
October 25, 2041 		SE2045Aug12T.png
August 12, 2045
138140142144146
SE2049May31A.png
May 31, 2049 		SE2053Mar20A.png
March 20, 2053 		SE2057Jan05T.png
January 5, 2057 		SE2060Oct24A.png
October 24, 2060 		SE2064Aug12T.png
August 12, 2064
148150152154156
SE2068May31T.png
May 31, 2068 		SE2072Mar19P.png
March 19, 2072 		SE2076Jan06T.png
January 6, 2076 		SE2079Oct24A.png
October 24, 2079 		SE2083Aug13P.png
August 13, 2083
158160162164
SE2087Jun01P.png
June 1, 2087 		SE2098Oct24P.png
October 24, 2098

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
SE1810Apr04A.gif
April 4, 1810
(Saros 126)		 SE1839Mar15T.gif
March 15, 1839
(Saros 127)		 SE1868Feb23A.gif
February 23, 1868
(Saros 128)
SE1897Feb01A.gif
February 1, 1897
(Saros 129)		 SE1926Jan14T.png
January 14, 1926
(Saros 130)		 SE1954Dec25A.png
December 25, 1954
(Saros 131)
SE1983Dec04A.png
December 4, 1983
(Saros 132)		 SE2012Nov13T.png
November 13, 2012
(Saros 133)		 SE2041Oct25A.png
October 25, 2041
(Saros 134)
SE2070Oct04A.png
October 4, 2070
(Saros 135)		 SE2099Sep14T.png
September 14, 2099
(Saros 136)		 SE2128Aug25A.png
August 25, 2128
(Saros 137)
SE2157Aug05A.png
August 5, 2157
(Saros 138)		 SE2186Jul16T.png
July 16, 2186
(Saros 139)

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References

  1. ↑ "October 24–25, 2041 Annular Solar Eclipse". timeanddate. Retrieved 14 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 August 2024.
  3. ↑ "Annular Solar Eclipse of 2041 Oct 25". EclipseWise.com. Retrieved 14 August 2024.
  4. ↑ 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.
  5. ↑ "NASA - Catalog of Solar Eclipses of Saros 134". eclipse.gsfc.nasa.gov.
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