Solar eclipse of May 2, 2087

Last updated
Solar eclipse of May 2, 2087
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Map
Type of eclipse
NaturePartial
Gamma 1.1139
Magnitude 0.8011
Maximum eclipse
Coordinates 70°18′N127°36′E / 70.3°N 127.6°E / 70.3; 127.6
Times (UTC)
Greatest eclipse18:04:42
References
Saros 120 (65 of 71)
Catalog # (SE5000) 9704

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.

Contents

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]

120 May 2, 2087
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Partial
125 October 26, 2087
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Partial
130 April 21, 2088
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Total
135 October 14, 2088
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Annular
140 April 10, 2089
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Annular
145 October 4, 2089
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Total
150 March 31, 2090
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Partial
155 September 23, 2090
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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.

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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.