Solar eclipse of November 1, 1948

Solar eclipse of November 1, 1948
Map
Type of eclipse
Nature Total
Gamma -0.3517
Magnitude 1.0231
Maximum eclipse
Duration 1m 56s
Coordinates 33.1S 76.2E
Max. width of band 84 km
Times (UTC)
Greatest eclipse 5:59:18
References
Saros 142 (19 of 72)
Catalog # (SE5000) 9395

A total solar eclipse occurred on November 1, 1948. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.

Contents

Related eclipses

Solar eclipses 1946-1949

This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.

Solar eclipse series sets from 1946-1949
Ascending node   Descending node
117 May 30, 1946

Partial
122 November 23, 1946

Partial
127 May 20, 1947

Total
132 November 12, 1947

Annular
137 May 9, 1948

Annular
142 November 1, 1948

Total
147 April 28, 1949

Partial
152 October 21, 1949

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

October 10, 1912

October 21, 1930

November 1, 1948
20 21 22

November 12, 1966

November 22, 1984

December 4, 2002
23 24 25

December 14, 2020

December 26, 2038

January 5, 2057
26 27

January 16, 2075

January 27, 2093

Notes

References