Solar eclipse of April 21, 2069

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Solar eclipse of April 21, 2069
SE2069Apr21P.png
Map
Type of eclipse
NaturePartial
Gamma1.0624
Magnitude0.8992
Maximum eclipse
Coordinates71°00′N 101°18′W / 71°N 101.3°W / 71; -101.3
Times (UTC)
Greatest eclipse10:11:09
References
Saros120 (64 of 71)
Catalog # (SE5000)9663

A partial solar eclipse will occur on April 21, 2069. 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.

Related eclipses[edit]

Solar eclipses 2069–2072[edit]

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 April 21, 2069
SE2069Apr21P.png
Partial
125 October 15, 2069
SE2069Oct15P.png
Partial
130 April 11, 2070
SE2070Apr11T.png
Total
135 October 4, 2070
SE2070Oct04A.png
Annular
140 March 31, 2071
SE2071Mar31A.png
Annular
145 September 23, 2071
SE2071Sep23T.png
Total
150 March 19, 2072
SE2072Mar19P.png
Partial
155 September 12, 2072
SE2072Sep12T.png
Total

Saros 120[edit]

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[edit]

  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.

External links[edit]