Solar eclipse of August 30, 1905

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Solar eclipse of August 30, 1905
SE1905Aug30T.png
Map
Type of eclipse
Nature Total
Gamma 0.5708
Magnitude 1.0477
Maximum eclipse
Duration 226 sec (3 m 46 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 192 km (119 mi)
Times (UTC)
Greatest eclipse 13:07:26
References
Saros 143 (17 of 72)
Catalog # (SE5000) 9293

A total solar eclipse occurred on August 30, 1905. 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

Solar eclipses of 1902-1907

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 1902-1907
Descending node   Ascending node
108 April 8, 1902
SE1902Apr08P.png
Partial
118 March 29, 1903
SE1903Mar29A.png
Annular
123 September 21, 1903
SE1903Sep21T.png
Total
128 March 17, 1904
SE1904Mar17A.png
Annular
133 September 9, 1904
SE1904Sep09T.png
Total
138 March 6, 1905
SE1905Mar06A.png
Annular
143 August 30, 1905
SE1905Aug30T.png
Total
148 February 23, 1906
SE1906Feb23P.png
Partial
153 August 20, 1906
SE1906Aug20P.png
Partial

Solar 143

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887.[1]

Series members 17-28 occur between 1901 and 2100:

17 18 19
SE1905Aug30T.png
August 30, 1905
SE1923Sep10T.png
September 10, 1923
SE1941Sep21T.png
September 21, 1941
20 21 22
SE1959Oct02T.png
October 2, 1959
SE1977Oct12T.png
October 12, 1977
SE1995Oct24T.png
October 24, 1995
23 24 25
SE2013Nov03H.png
November 3, 2013
SE2031Nov14H.png
November 14, 2031
SE2049Nov25H.png
November 25, 2049
26 27 28
SE2067Dec06H.png
December 6, 2067
SE2085Dec16A.png
December 16, 2085

Notes

References