Solar eclipse of February 16, 2045
Map
Type of eclipse
NatureAnnular
Gamma−0.3125
Magnitude0.9285
Maximum eclipse
Duration467 sec (7 m 47 s)
Coordinates28°18′S 166°12′W / 28.3°S 166.2°W / -28.3; -166.2
Max. width of band281 km (175 mi)
Times (UTC)
Greatest eclipse23:56:07
References
Saros131 (52 of 70)
Catalog # (SE5000)9607

An annular solar eclipse will occur on Thursday, February 16, 2045. 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.

Images


Animated path

Solar eclipses of 2044–2047

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 2044–2047
Ascending node   Descending node
121February 28, 2044

Annular
126August 23, 2044

Total
131February 16, 2045

Annular
136August 12, 2045

Total
141February 5, 2046

Annular
146August 2, 2046

Total
151January 26, 2047

Partial
156July 22, 2047

Partial
Partial solar eclipses on June 23, 2047 and December 16, 2047 occur on the next lunar year eclipse set.

Saros 131

It is a part of Saros cycle 131, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on August 1, 1125. It contains total eclipses from March 27, 1522 through May 30, 1612 and hybrid eclipses from June 10, 1630 through July 24, 1702, and annular eclipses from August 4, 1720 through June 18, 2243. The series ends at member 70 as a partial eclipse on September 2, 2369. The longest duration of totality was only 58 seconds on May 30, 1612. All eclipses in this series occurs at the Moon’s ascending node.

Series members 33–70 occur between 1702 and 2369
33 34 35

July 24, 1702

August 4, 1720

August 15, 1738
36 37 38

August 25, 1756

September 6, 1774

September 16, 1792
39 40 41

September 28, 1810

October 9, 1828

October 20, 1846
42 43 44

October 30, 1864

November 10, 1882

November 22, 1900
45 46 47

December 3, 1918

December 13, 1936

December 25, 1954
48 49 50

January 4, 1973

January 15, 1991

January 26, 2009
51 52 53

February 6, 2027

February 16, 2045

February 28, 2063
54 55 56

March 10, 2081

March 21, 2099

April 2, 2117
57 58 59

April 13, 2135

April 23, 2153

May 5, 2171
60 61 62

May 15, 2189

May 27, 2207

June 6, 2225
63 64 65

June 18, 2243

June 28, 2261

July 9, 2279
66 67 68

July 20, 2297

August 1, 2315

August 11, 2333
69 70

August 22, 2351

September 2, 2369

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.

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 ascending node.

References

  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.
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