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Solar eclipse of December 13, 1974

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Solar eclipse of December 13, 1974
Map
Type of eclipse
NaturePartial
Gamma1.0797
Magnitude0.8266
Maximum eclipse
Coordinates66°48′N 69°24′W / 66.8°N 69.4°W / 66.8; -69.4
Times (UTC)
Greatest eclipse16:13:13
References
Saros151 (12 of 72)
Catalog # (SE5000)9453

A partial solar eclipse occurred at the Moon's ascending node of orbit on Friday, December 13, 1974, with a magnitude of 0.8266. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Related eclipses[edit]

Eclipses in 1974[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 151[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 1971–1974[edit]

This eclipse is a member of a semester series. An eclipse 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.[1]

Note: Partial solar eclipses on February 25, 1971 and August 20, 1971 occur in the next lunar year set.

Solar eclipse series sets from 1971 to 1974
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
116
1971 July 22
Partial
1.51298 121
1972 January 16
Annular
−0.93651
126
1972 July 10
Total
0.68719 131
1973 January 4
Annular
−0.26441
136
1973 June 30
Total
−0.07853 141
1973 December 24
Annular
0.41710
146
1974 June 20
Total
−0.82388 151
1974 December 13
Partial
1.07974

Saros 151[edit]

It is a part of Saros cycle 151, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on August 14, 1776. It contains annular eclipses from February 28, 2101, through April 23, 2191, a hybrid eclipse on May 5, 2209, and total eclipses from May 16, 2227, through July 6, 2912. The series ends at member 72 as a partial eclipse on October 1, 3056. The longest duration of totality will be 5 minutes, 41 seconds on May 22, 2840.

Metonic series[edit]

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).

References[edit]

  1. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.

External links[edit]