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Solar eclipse of November 27, 2095

An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, November 27, 2095, with a magnitude of 0.933. 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.

Solar eclipse of November 27, 2095
Map
Type of eclipse
NatureAnnular
Gamma0.4903
Magnitude0.933
Maximum eclipse
Duration527 s (8 min 47 s)
Coordinates7°12′N 169°48′E / 7.2°N 169.8°E / 7.2; 169.8
Max. width of band285 km (177 mi)
Times (UTC)
Greatest eclipse1:02:57
References
Saros134 (48 of 71)
Catalog # (SE5000)9723
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Eclipses in 2095

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 134

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Inex

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Triad

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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.[1]

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 134

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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.[2]

Series members 32–53 occur between 1801 and 2200:
32 33 34
 
June 6, 1807
 
June 16, 1825
 
June 27, 1843
35 36 37
 
July 8, 1861
 
July 19, 1879
 
July 29, 1897
38 39 40
 
August 10, 1915
 
August 21, 1933
 
September 1, 1951
41 42 43
 
September 11, 1969
 
September 23, 1987
 
October 3, 2005
44 45 46
 
October 14, 2023
 
October 25, 2041
 
November 5, 2059
47 48 49
 
November 15, 2077
 
November 27, 2095
 
December 8, 2113
50 51 52
 
December 19, 2131
 
December 30, 2149
 
January 10, 2168
53
 
January 20, 2186

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 July 3, 2065 and November 26, 2152
July 3–4 April 21–23 February 7–8 November 26–27 September 13–15
118 120 122 124 126
 
July 3, 2065
 
April 21, 2069
 
February 7, 2073
 
November 26, 2076
 
September 13, 2080
128 130 132 134 136
 
July 3, 2084
 
April 21, 2088
 
February 7, 2092
 
November 27, 2095
 
September 14, 2099
138 140 142 144 146
 
July 4, 2103
 
April 23, 2107
 
February 8, 2111
 
November 27, 2114
 
September 15, 2118
148 150 152 154 156
 
July 4, 2122
 
April 22, 2126
 
February 8, 2130
 
November 26, 2133
 
September 15, 2137
158 160 162 164
 
July 3, 2141
 
November 26, 2152

Notes

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  1. ^ 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.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 134". eclipse.gsfc.nasa.gov.

References

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