Solar eclipse of September 25, 2098

Last updated
Solar eclipse of September 25, 2098
SE2098Sep25P.png
Map
Type of eclipse
NaturePartial
Gamma 1.14
Magnitude 0.7871
Maximum eclipse
Coordinates 61°06′N101°00′W / 61.1°N 101°W / 61.1; -101
Times (UTC)
Greatest eclipse0:31:16
References
Saros 126 (52 of 72)
Catalog # (SE5000) 9729

A partial solar eclipse will occur at the Moon's descending node of orbit between Wednesday, September 24 and Thursday, September 25, 2098, [1] with a magnitude of 0.7871. 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 will be visible for parts of the Russian Far East, Hawaii, and western North America.

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 25, 2098 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2098 September 24 at 22:41:16.8 UTC
Equatorial Conjunction2098 September 24 at 23:26:40.4 UTC
Ecliptic Conjunction2098 September 25 at 00:20:01.8 UTC
Greatest Eclipse2098 September 25 at 00:31:16.2 UTC
Last Penumbral External Contact2098 September 25 at 02:21:44.9 UTC
September 25, 2098 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.78710
Eclipse Obscuration0.73803
Gamma1.11845
Sun Right Ascension12h09m17.5s
Sun Declination-01°00'22.0"
Sun Semi-Diameter15'56.5"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension12h11m27.7s
Moon Declination-00°01'23.2"
Moon Semi-Diameter16'27.0"
Moon Equatorial Horizontal Parallax1°00'22.3"
ΔT122.3 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 2098
September 25
Descending node (new moon)
October 10
Ascending node (full moon)
October 24
Descending node (new moon)
SE2098Sep25P.png Lunar eclipse chart close-2098Oct10.png SE2098Oct24P.png
Partial solar eclipse
Solar Saros 126
Total lunar eclipse
Lunar Saros 138
Partial solar eclipse
Solar Saros 164

Eclipses in 2098

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 126

Inex

Triad

Solar eclipses of 2098–2101

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 eclipse on October 24, 2098 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2098 to 2101
Ascending node Descending node
SarosMapGammaSarosMapGamma
121 April 1, 2098
SE2098Apr01P.png
Partial
−1.1005126 September 25, 2098
SE2098Sep25P.png
Partial
1.14
131 March 21, 2099
SE2099Mar21A.png
Annular
−0.4016136 September 14, 2099
SE2099Sep14T.png
Total
0.3942
141 March 10, 2100
SE2100Mar10A.png
Annular
0.3077146 September 4, 2100
SE2100Sep04T.png
Total
−0.3384
151February 28, 2101
SE2101Feb28A.png
Annular
0.9964156August 24, 2101
Saros156 06van69 SE2101Aug24P.jpg
Partial
−1.1392

Saros 126

This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810; hybrid eclipses from April 14, 1828 through May 6, 1864; and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. 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 annularity was produced by member 11 at 6 minutes, 30 seconds on June 26, 1359, and the longest duration of totality was produced by member 45 at 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 36–57 occur between 1801 and 2200:
363738
SE1810Apr04A.gif
April 4, 1810
Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828
SE1846Apr25H.gif
April 25, 1846
394041
SE1864May06H.gif
May 6, 1864
SE1882May17T.png
May 17, 1882
SE1900May28T.png
May 28, 1900
424344
SE1918Jun08T.png
June 8, 1918
SE1936Jun19T.png
June 19, 1936
SE1954Jun30T.png
June 30, 1954
454647
SE1972Jul10T.png
July 10, 1972
SE1990Jul22T.png
July 22, 1990
SE2008Aug01T.png
August 1, 2008
484950
SE2026Aug12T.png
August 12, 2026
SE2044Aug23T.png
August 23, 2044
SE2062Sep03P.png
September 3, 2062
515253
SE2080Sep13P.png
September 13, 2080
SE2098Sep25P.png
September 25, 2098
Saros126 53van72 SE2116Oct06P.jpg
October 6, 2116
545556
Saros126 54van72 SE2134Oct17P.jpg
October 17, 2134
Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
Saros126 56van72 SE2170Nov08P.jpg
November 8, 2170
57
Saros126 57van72 SE2188Nov18P.jpg
November 18, 2188

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 July 15, 2083 and December 7, 2170
July 14–15May 2–3February 18–19December 7–8September 25–26
118120122124126
SE2083Jul15P.png
July 15, 2083
SE2087May02P.png
May 2, 2087
SE2091Feb18P.png
February 18, 2091
SE2094Dec07P.png
December 7, 2094
SE2098Sep25P.png
September 25, 2098
128130132134136
SE2102Jul15A.png
July 15, 2102
SE2106May03T.png
May 3, 2106
SE2110Feb18A.png
February 18, 2110
SE2113Dec08A.png
December 8, 2113
SE2117Sep26T.png
September 26, 2117
138140142144146
SE2121Jul14A.png
July 14, 2121
SE2125May03A.png
May 3, 2125
SE2129Feb18T.png
February 18, 2129
SE2132Dec07A.png
December 7, 2132
SE2136Sep26T.png
September 26, 2136
148150152154156
Saros148 28van75 SE2140Jul14T.jpg
July 14, 2140
Saros150 24van71 SE2144May03A.jpg
May 3, 2144
Saros152 20van70 SE2148Feb19T.jpg
February 19, 2148
Saros154 14van71 SE2151Dec08A.jpg
December 8, 2151
Saros156 09van69 SE2155Sep26A.jpg
September 26, 2155
158160162164
Saros158 06van70 SE2159Jul15P.jpg
July 15, 2159
Saros164 05van80 SE2170Dec07P.jpg
December 7, 2170

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.

The partial solar eclipses on April 8, 1902 (part of Saros 108) and January 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 2000 and 2200
SE2000Jul01P.png
July 1, 2000
(Saros 117)
SE2011Jun01P.png
June 1, 2011
(Saros 118)
SE2022Apr30P.png
April 30, 2022
(Saros 119)
SE2033Mar30T.png
March 30, 2033
(Saros 120)
SE2044Feb28A.png
February 28, 2044
(Saros 121)
SE2055Jan27P.png
January 27, 2055
(Saros 122)
SE2065Dec27P.png
December 27, 2065
(Saros 123)
SE2076Nov26P.png
November 26, 2076
(Saros 124)
SE2087Oct26P.png
October 26, 2087
(Saros 125)
SE2098Sep25P.png
September 25, 2098
(Saros 126)
Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
(Saros 127)
SE2120Jul25A.png
July 25, 2120
(Saros 128)
Saros129 58van80 SE2131Jun25T.jpg
June 25, 2131
(Saros 129)
SE2142May25T.png
May 25, 2142
(Saros 130)
SE2153Apr23A.png
April 23, 2153
(Saros 131)
SE2164Mar23H.png
March 23, 2164
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)
SE2186Jan20A.png
January 20, 2186
(Saros 134)
SE2196Dec19A.png
December 19, 2196
(Saros 135)

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
SE1809Apr14A.gif
April 14, 1809
(Saros 116)
SE1838Mar25T.gif
March 25, 1838
(Saros 117)
SE1867Mar06A.gif
March 6, 1867
(Saros 118)
Saros119 59van71 SE1896Feb13A.jpg
February 13, 1896
(Saros 119)
SE1925Jan24T.png
January 24, 1925
(Saros 120)
SE1954Jan05A.png
January 5, 1954
(Saros 121)
SE1982Dec15P.png
December 15, 1982
(Saros 122)
SE2011Nov25P.png
November 25, 2011
(Saros 123)
SE2040Nov04P.png
November 4, 2040
(Saros 124)
SE2069Oct15P.png
October 15, 2069
(Saros 125)
SE2098Sep25P.png
September 25, 2098
(Saros 126)
Saros127 64van82 SE2127Sep06P.jpg
September 6, 2127
(Saros 127)
Saros128 66van73 SE2156Aug16P.jpg
August 16, 2156
(Saros 128)
Saros129 61van80 SE2185Jul26T.jpg
July 26, 2185
(Saros 129)

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References

  1. "September 24–25, 2098 Partial Solar Eclipse". timeanddate. Retrieved 25 August 2024.
  2. "Partial Solar Eclipse of 2098 Sep 25". EclipseWise.com. Retrieved 25 August 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 126". eclipse.gsfc.nasa.gov.