Solar eclipse of April 11, 2051

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Solar eclipse of April 11, 2051
SE2051Apr11P.png
Map
Type of eclipse
Nature Partial
Gamma 1.0169
Magnitude 0.9849
Maximum eclipse
Coordinates 71°36′N 32°12′E / 71.6°N 32.2°E / 71.6; 32.2
Times (UTC)
Greatest eclipse 2:10:39
References
Saros 120 (63 of 71)
Catalog # (SE5000) 9621

A partial solar eclipse will occur on April 11, 2051. The umbral shadow of the moon will pass just above the north pole of the earth.

Related eclipses[edit]

Solar eclipses 2051-2054[edit]

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.

120 April 11, 2051
SE2051Apr11P.png
Partial
125 October 4, 2051
SE2051Oct04P.png
Partial
130 March 30, 2052
SE2052Mar30T.png
Total
135 September 22, 2052
SE2052Sep22A.png
Annular
140 March 20, 2053
SE2053Mar20A.png
Annular
145 September 12, 2053
SE2053Sep12T.png
Total
150 March 9, 2054
SE2054Mar09P.png
Partial
155 September 2, 2054
SE2054Sep02P.png
Partial

Saros 120[edit]

It 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.[1]

Series members 55–65 occur between 1901 and 2100:

55 56 57
SE1907Jan14T.png
January 14, 1907
SE1925Jan24T.png
January 24, 1925
SE1943Feb04T.png
February 4, 1943
58 59 60
SE1961Feb15T.png
February 15, 1961
SE1979Feb26T.png
February 26, 1979
SE1997Mar09T.png
March 9, 1997
61 62 63
SE2015Mar20T.png
March 20, 2015
SE2033Mar30T.png
March 30, 2033
SE2051Apr11P.png
April 11, 2051
64 65
SE2069Apr21P.png
April 21, 2069
SE2087May02P.png
May 2, 2087

References[edit]

External links[edit]