Solar eclipse of October 24, 2098

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, October 24, 2098, with a magnitude of 0.0056. 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.

Solar eclipse of October 24, 2098
Map
Type of eclipse
NaturePartial
Gamma−1.5407
Magnitude0.0056
Maximum eclipse
Coordinates61°48′S 95°30′W / 61.8°S 95.5°W / -61.8; -95.5
Times (UTC)
Greatest eclipse10:36:11
References
Saros164 (1 of 80)
Catalog # (SE5000)9730

This minor eclipse is the first solar eclipse of Saros cycle 164. It is the shallowest solar eclipse of the 21st century; at best, in a remote location within the Southern Ocean the moon will block out 0.56% of the sun's diameter with the sun barely above the horizon. Gamma is equal to −1.5407, which is also farther from zero than any other solar eclipse in the century. The eclipse is not listed by some sources.[1] There will not be a shallower partial eclipse until August 23, 2883.

Eclipse details

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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]

October 24, 2098 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2098 October 24 at 10:25:24.3 UTC
Greatest Eclipse 2098 October 24 at 10:36:10.8 UTC
Last Penumbral External Contact 2098 October 24 at 10:46:29.2 UTC
Ecliptic Conjunction 2098 October 24 at 10:52:05.9 UTC
Equatorial Conjunction 2098 October 24 at 11:56:02.8 UTC
October 24, 2098 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.00568
Eclipse Obscuration 0.00051
Gamma −1.54072
Sun Right Ascension 13h57m42.1s
Sun Declination -12°01'06.6"
Sun Semi-Diameter 16'04.5"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 13h55m00.2s
Moon Declination -13°22'41.3"
Moon Semi-Diameter 16'04.0"
Moon Equatorial Horizontal Parallax 0°58'57.8"
ΔT 122.4 s

Eclipse season

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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)
     
Partial solar eclipse
Solar Saros 126
Total lunar eclipse
Lunar Saros 138
Partial solar eclipse
Solar Saros 164
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Eclipses in 2098

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Solar Saros 164

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Solar eclipses of 2094–2098

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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 solar eclipses on January 16, 2094 (total) and July 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses on April 1, 2098 and September 25, 2098 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2094 to 2098
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 June 13, 2094
 
Partial
−1.4613 124 December 7, 2094
 
Partial
1.1547
129 June 2, 2095
 
Total
−0.6396 134 November 27, 2095
 
Annular
0.4903
139 May 22, 2096
 
Total
0.1196 144 November 15, 2096
 
Annular
−0.20
149 May 11, 2097
 
Total
0.8516 154 November 4, 2097
 
Annular
−0.8926
159 May 1, 2098 164 October 24, 2098
 
Partial
−1.5407

Saros 164

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This eclipse is a part of Saros series 164, repeating every 18 years, 11 days, and containing 80 events. The series will start with a partial solar eclipse on October 24, 2098. It contains total eclipses from June 1, 2459 through June 20, 3090; hybrid eclipses from July 1, 3108 through August 3, 3162; and annular eclipses from August 13, 3180 through September 4, 3216. The series ends at member 80 as a partial eclipse on March 10, 3523. 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 26 at 6 minutes, 30 seconds on July 25, 2549, and the longest duration of annularity was produced by member 63 at 1 minutes, 21 seconds on September 4, 3216. All eclipses in this series occur at the Moon’s descending node of orbit.[4]

Metonic series

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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 1 March 19–20 January 5–6 October 24–25 August 12–13
118 120 122 124 126
 
June 1, 2011
 
March 20, 2015
 
January 6, 2019
 
October 25, 2022
 
August 12, 2026
128 130 132 134 136
 
June 1, 2030
 
March 20, 2034
 
January 5, 2038
 
October 25, 2041
 
August 12, 2045
138 140 142 144 146
 
May 31, 2049
 
March 20, 2053
 
January 5, 2057
 
October 24, 2060
 
August 12, 2064
148 150 152 154 156
 
May 31, 2068
 
March 19, 2072
 
January 6, 2076
 
October 24, 2079
 
August 13, 2083
158 160 162 164
 
June 1, 2087
 
October 24, 2098

Tritos series

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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 eclipse on October 24, 2098 (part of Saros 164) is also a part of this series but is not included in the table below.

Series members between 1801 and 2011
 
February 11, 1804
(Saros 137)
 
January 10, 1815
(Saros 138)
 
December 9, 1825
(Saros 139)
 
November 9, 1836
(Saros 140)
 
October 9, 1847
(Saros 141)
 
September 7, 1858
(Saros 142)
 
August 7, 1869
(Saros 143)
 
July 7, 1880
(Saros 144)
 
June 6, 1891
(Saros 145)
 
May 7, 1902
(Saros 146)
 
April 6, 1913
(Saros 147)
 
March 5, 1924
(Saros 148)
 
February 3, 1935
(Saros 149)
 
January 3, 1946
(Saros 150)
 
December 2, 1956
(Saros 151)
 
November 2, 1967
(Saros 152)
 
October 2, 1978
(Saros 153)
 
August 31, 1989
(Saros 154)
 
July 31, 2000
(Saros 155)
 
July 1, 2011
(Saros 156)

References

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  1. ^ "Solar and Lunar Eclipses Worldwide – 2098". www.timeanddate.com. Retrieved 2023-12-15.
  2. ^ "Partial Solar Eclipse of 2098 Oct 24". 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 164". eclipse.gsfc.nasa.gov.
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