Solar eclipse of February 16, 2045

Solar eclipse of February 16, 2045
Map
Type of eclipse
Nature Annular
Gamma -0.3125
Magnitude 0.9285
Maximum eclipse
Duration 467 sec (7 m 47 s)
Coordinates 28°18′S 166°12′W / 28.3°S 166.2°W / -28.3; -166.2
Max. width of band 281 km (175 mi)
Times (UTC)
Greatest eclipse 23:56:07
References
Saros 131 (52 of 70)
Catalog # (SE5000) 9607

An annular solar eclipse will occur on 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

Each member 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.

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.[1]

References

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