Solar eclipse of April 28, 1911

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Solar eclipse of April 28, 1911
SE1911Apr28T.png
Map
Type of eclipse
Nature Total
Gamma -0.2294
Magnitude 1.0562
Maximum eclipse
Duration 297 sec (4 m 57 s)
Coordinates 1°54′N 151°54′W / 1.9°N 151.9°W / 1.9; -151.9
Max. width of band 190 km (120 mi)
Times (UTC)
Greatest eclipse 22:27:22
References
Saros 127 (52 of 82)
Catalog # (SE5000) 9306

A total solar eclipse occurred on April 28, 1911. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Related eclipses[edit]

Solar eclipses 1910-1913[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.

Solar eclipse series sets from 1910-1913
Ascending node   Descending node
117 May 9, 1910
SE1910May09T.png
Total
122 November 2, 1910
SE1910Nov02P.png
Partial
127 April 28, 1911
SE1911Apr28T.png
Total
132 October 22, 1911
SE1911Oct22A.png
Annular
137 April 17, 1912
SE1912Apr17H.png
Hybrid
142 October 10, 1912
SE1912Oct10T.png
Total
147 April 6, 1913
SE1913Apr06P.png
Partial
152 September 30, 1913
SE1913Sep30P.png
Partial


Saros 127[edit]

It is a part of Saros cycle 127, repeating every 18 years, 11 days, containing 82 events. The series started with partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. The series ends at member 82 as a partial eclipse on March 21, 2452. The longest duration of totality was 5 minutes, 40 seconds on August 30, 1532.[1]

Notes[edit]

References[edit]