Solar eclipse of January 25, 1944

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Solar eclipse of January 25, 1944
Type of eclipse
Nature Total
Gamma 0.2025
Magnitude 1.0428
Maximum eclipse
Duration 249 sec (4 m 9 s)
Coordinates 7°36′S 50°12′W / 7.6°S 50.2°W / -7.6; -50.2
Max. width of band 146 km (91 mi)
Times (UTC)
Greatest eclipse 15:26:42
Saros 130 (48 of 73)
Catalog # (SE5000) 9384

A total solar eclipse occurred on January 25, 1944. 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. Totality was visible from Peru, Brazil, British Sierra Leone (today's Sierra Leone), and French West Africa (the parts now belonging to Guinea, Mali, Burkina Faso and Niger, including Guinean capital Conakry).

Related eclipses[edit]

Solar eclipses 1942-1946[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.

Note: The partial solar eclipse on September 10, 1942 occurs in the previous lunar year eclipse set.

Saros 130[edit]

It is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619.[1]