Solar eclipse of May 18, 1901

Solar eclipse of May 18, 1901
Map
Type of eclipse
Nature Total
Gamma -0.3626
Magnitude 1.068
Maximum eclipse
Duration 389 sec (6 m 29 s)
Coordinates 1°42′S 98°24′E / 1.7°S 98.4°E / -1.7; 98.4
Max. width of band 238 km (148 mi)
Times (UTC)
Greatest eclipse 5:33:48
References
Saros 136 (31 of 71)
Catalog # (SE5000) 9283

A total solar eclipse occurred on May 18, 1901. 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. The path of totality crossed Madagascar, Réunion, Mauritius, Indonesia, Papua, New Guinea.

Solar eclipses 1901-1902

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 1901-1902
Descending node   Ascending node
136May 18, 1901

Total
141November 11, 1901

Annular
146May 7, 1902

Partial
151October 31, 1902

Partial

Saros 136

Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on Jun 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, 8 seconds.[1]

Notes

References

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