Solar eclipse of April 28, 1930

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Solar eclipse of April 28, 1930
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Map
Type of eclipse
Nature Hybrid
Gamma 0.473
Magnitude 1.0003
Maximum eclipse
Duration 1 sec (0 m 1 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 1 km (0.62 mi)
Times (UTC)
Greatest eclipse 19:03:34
References
Saros 137 (31 of 70)
Catalog # (SE5000) 9351

A total solar eclipse occurred on April 28, 1930. 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. This event is a hybrid, starting and ending as an annular eclipse.

The path of totality crossed the eastern pacific ocean, northwestern United States, and across central and eastern Canada, and northern Labrador of the Dominion of Newfoundland (today's Newfoundland and Labrador in Canada).

Related eclipses

Solar eclipses 1928-1931

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 1928-1931
Ascending node   Descending node
117 May 19, 1928
SE1928May19T.png
Total
122 November 12, 1928
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Partial
127 May 9, 1929
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Total
132 November 1, 1929
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Annular
137 April 28, 1930
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Hybrid
142 October 21, 1930
SE1930Oct21T.png
Total
147 April 18, 1931
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Partial
152 October 11, 1931
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Partial

Saros series 142

It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291.[1]

Series members 17-27 occur between 1901 and 2100:

17 18 19
SE1912Oct10T.png
October 10, 1912
SE1930Oct21T.png
October 21, 1930
SE1948Nov01T.png
November 1, 1948
20 21 22
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November 12, 1966
SE1984Nov22T.png
November 22, 1984
SE2002Dec04T.png
December 4, 2002
23 24 25
SE2020Dec14T.png
December 14, 2020
SE2038Dec26T.png
December 26, 2038
SE2057Jan05T.png
January 5, 2057
26 27
SE2075Jan16T.png
January 16, 2075
SE2093Jan27T.png
January 27, 2093

Notes

References