Solar eclipse of May 2, 2087

A partial solar eclipse will occur on Friday 2 May 2087. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Solar eclipse of May 2, 2087
Map
Type of eclipse
NaturePartial
Gamma1.1139
Magnitude0.8011
Maximum eclipse
Coordinates70.3°N 127.6°E / 70.3; 127.6
Times (UTC)
Greatest eclipse18:04:42
References
Saros120 (65 of 71)
Catalog # (SE5000)9704

Solar eclipses 2087–2090

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]

120May 2, 2087

Partial
125October 26, 2087

Partial
130April 21, 2088

Total
135October 14, 2088

Annular
140April 10, 2089

Annular
145October 4, 2089

Total
150March 31, 2090

Partial
155September 23, 2090

Total

Saros 120

This eclipse is a part of Saros cycle 120, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 27, 933 AD, and reached an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and total eclipses from June 8, 1564, through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occurs at the Moon’s descending 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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