Solar eclipse of April 25, 1865

A total solar eclipse occurred on April 25, 1865. 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.

Solar eclipse of April 25, 1865
Map
Type of eclipse
NatureTotal
Gamma−0.4826
Magnitude1.0584
Maximum eclipse
Duration323 sec (5 m 23 s)
Coordinates14.8°S 25.8°W / -14.8; -25.8
Max. width of band219 km (136 mi)
Times (UTC)
Greatest eclipse14:08:34
References
Saros136 (29 of 71)
Catalog # (SE5000)9199

Observations

The total eclipse was also witnessed by the passengers and crew of the SS Great Britain, passing the coastline of Brazil en route from Australia to England;[1] they were able to observe stars in the daytime.

Saros 136

Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on June 14, 1360, and reached a first annular eclipse on September 8, 1504. It was a hybrid event from November 22, 1612, through January 17, 1703, and total eclipses from January 27, 1721, through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622, with the entire series lasting 1262 years. The longest eclipse occurred on June 20, 1955, with a maximum duration of totality at 7 minutes, 7.74 seconds. All eclipses in this series occurs at the Moon's descending node.[2]

Series members 29–43 occur between 1865 and 2117
29 30 31

Apr 25, 1865

May 6, 1883

May 18, 1901
32 33 34

May 29, 1919

Jun 8, 1937

Jun 20, 1955
35 36 37

Jun 30, 1973

Jul 11, 1991

Jul 22, 2009
38 39 40

Aug 2, 2027

Aug 12, 2045

Aug 24, 2063
41 42 43

Sep 3, 2081

Sep 14, 2099

Sep 26, 2117

References

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