Solar eclipse of September 1, 1951

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Solar eclipse of September 1, 1951
SE1951Sep01A.png
Map
Type of eclipse
Nature Annular
Gamma 0.1557
Magnitude 0.9747
Maximum eclipse
Duration 156 sec (2 m 36 s)
Coordinates 16°30′N 8°30′W / 16.5°N 8.5°W / 16.5; -8.5
Max. width of band 91 km (57 mi)
Times (UTC)
Greatest eclipse 12:51:51
References
Saros 134 (40 of 71)
Catalog # (SE5000) 9401

An annular solar eclipse occurred on September 1, 1951. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

Related eclipses[edit]

Solar eclipses of 1950-1953[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.

Solar eclipse series sets from 1950–1953
Ascending node   Descending node
Saros Map Saros Map
119 SE1950Mar18A.png
March 18, 1950
Annular
124 SE1950Sep12T.png
September 12, 1950
Total
129 SE1951Mar07A.png
March 7, 1951
Annular
134 SE1951Sep01A.png
September 1, 1951
Annular
139 SE1952Feb25T.png
February 25, 1952
Total
144 SE1952Aug20A.png
August 20, 1952
Annular
149 SE1953Feb14P.png
February 14, 1953
Partial
154 SE1953Aug09P.png
August 9, 1953
Partial
Solar eclipse of July 11, 1953 belongs to the next lunar year set

Saros 134[edit]

It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428.[1]

Notes[edit]

References[edit]