Solar eclipse of September 23, 2071

A total solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, September 23, 2071, with a magnitude of 1.0333. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Solar eclipse of September 23, 2071
Map
Type of eclipse
NatureTotal
Gamma0.262
Magnitude1.0333
Maximum eclipse
Duration191 s (3 min 11 s)
Coordinates14°12′N 76°42′W / 14.2°N 76.7°W / 14.2; -76.7
Max. width of band116 km (72 mi)
Times (UTC)
Greatest eclipse17:20:28
References
Saros145 (25 of 77)
Catalog # (SE5000)9668
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Eclipses in 2071

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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 145

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Inex

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Triad

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Solar eclipses of 2069–2072

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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]

120 April 21, 2069
 
Partial
125 October 15, 2069
 
Partial
130 April 11, 2070
 
Total
135 October 4, 2070
 
Annular
140 March 31, 2071
 
Annular
145 September 23, 2071
 
Total
150 March 19, 2072
 
Partial
155 September 12, 2072
 
Total

Saros 145

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This eclipse is a part of Saros series 145, repeating every 18 years, 11 days, and containing 77 events. The series started with a partial solar eclipse on January 4, 1639. It contains an annular eclipse on June 6, 1891; a hybrid eclipse on June 17, 1909; and total eclipses from June 29, 1927 through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. 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 15 at 6 seconds (by default) on June 6, 1891, and the longest duration of totality will be produced by member 50 at 7 minutes, 12 seconds on June 25, 2522. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 10–32 occur between 1801 and 2200:
10 11 12
 
April 13, 1801
 
April 24, 1819
 
May 4, 1837
13 14 15
 
May 16, 1855
 
May 26, 1873
 
June 6, 1891
16 17 18
 
June 17, 1909
 
June 29, 1927
 
July 9, 1945
19 20 21
 
July 20, 1963
 
July 31, 1981
 
August 11, 1999
22 23 24
 
August 21, 2017
 
September 2, 2035
 
September 12, 2053
25 26 27
 
September 23, 2071
 
October 4, 2089
 
October 16, 2107
28 29 30
 
October 26, 2125
 
November 7, 2143
 
November 17, 2161
31 32
 
November 28, 2179
 
December 9, 2197

Inex series

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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.

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 ascending node.

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 145". eclipse.gsfc.nasa.gov.

References

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