Solar eclipse of December 24, 1927 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | -1.2416 |
Magnitude | 0.549 |
Maximum eclipse | |
Coordinates | 66°06′S47°42′W / 66.1°S 47.7°W |
Times (UTC) | |
Greatest eclipse | 3:59:41 |
References | |
Saros | 150 (12 of 71) |
Catalog # (SE5000) | 9345 |
A partial solar eclipse occurred on December 24, 1927. 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.
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]
Solar eclipse series sets from 1924–1928 | ||||
---|---|---|---|---|
Ascending node | Descending node | |||
115 | July 31, 1924 Partial | 120 | January 24, 1925 Total | |
125 | July 20, 1925 Annular | 130 | January 14, 1926 Total | |
135 | July 9, 1926 Annular | 140 | January 3, 1927 Annular | |
145 | June 29, 1927 Total | 150 | December 24, 1927 Partial | |
155 | June 17, 1928 Partial |
It is a part of Saros cycle 150, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126, through June 22, 2829. There are no total eclipses in this series. The series ends at member 71 as a partial eclipse on September 29, 2991. The longest duration of annularity will be 9 minutes, 58 seconds on December 19, 2522.
Series members 11-21 occur between 1901 and 2100: | ||
---|---|---|
11 | 12 | 13 |
December 12, 1909 | December 24, 1927 | January 3, 1946 |
14 | 15 | 16 |
January 14, 1964 | January 25, 1982 | February 5, 2000 |
17 | 18 | 19 |
February 15, 2018 | February 27, 2036 | March 9, 2054 |
20 | 21 | |
March 19, 2072 | March 31, 2090 |
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