Solar eclipse of February 28, 2044

An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, February 28, 2044, with a magnitude of 0.96. 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 February 28, 2044
Map
Type of eclipse
NatureAnnular
Gamma−0.9954
Magnitude0.96
Maximum eclipse
Duration147 s (2 min 27 s)
Coordinates62°12′S 25°36′W / 62.2°S 25.6°W / -62.2; -25.6
Max. width of band- km
Times (UTC)
Greatest eclipse20:24:40
References
Saros121 (62 of 71)
Catalog # (SE5000)9605

This is the last of 55 umbral eclipses of Solar Saros 121. The 1st was in 1070 and the 55th will be in 2044. The total duration is 974 years.

Images

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Animated path

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Eclipses in 2044

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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 121

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Inex

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Triad

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Solar eclipses of 2044–2047

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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]

Solar eclipse series sets from 2044 to 2047
Ascending node   Descending node
121 February 28, 2044
 
Annular
126 August 23, 2044
 
Total
131 February 16, 2045
 
Annular
136 August 12, 2045
 
Total
141 February 5, 2046
 
Annular
146 August 2, 2046
 
Total
151 January 26, 2047
 
Partial
156 July 22, 2047
 
Partial
Partial solar eclipses on June 23, 2047 and December 16, 2047 occur on the next lunar year eclipse set.

Saros 121

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Solar saros 121, repeating every about 18 years, 11 days, and 8 hours, contains 71 events. The series started with a partial solar eclipse on April 25, 944. It contains total eclipses from July 10, 1070, to October 9, 1809. It contains hybrid eclipses on October 20, 1827, and October 30, 1845. It contains annular eclipses from November 11, 1863, to February 28, 2044. The series ends at member 71 as a partial eclipse on June 7, 2206. The longest total eclipse occurred on June 21, 1629, with greatest duration of totality at 6 minutes and 20 seconds. The longest annular eclipse will occur on February 28, 2044, with greatest duration of annularity at 2 minutes and 27 seconds.[2]

Series members 49–65 occur between 1801 and 2100:
49 50 51
 
October 9, 1809
 
October 20, 1827
 
October 30, 1845
52 53 54
 
November 11, 1863
 
November 21, 1881
 
December 3, 1899
55 56 57
 
December 14, 1917
 
December 25, 1935
 
January 5, 1954
58 59 60
 
January 16, 1972
 
January 26, 1990
 
February 7, 2008
61 62 63
 
February 17, 2026
 
February 28, 2044
 
March 11, 2062
64 65
 
March 21, 2080
 
April 1, 2098

References

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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. ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
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