Solar eclipse of December 24, 1927
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.
| Solar eclipse of December 24, 1927 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | -1.2416 |
| Magnitude | 0.549 |
| Maximum eclipse | |
| Coordinates | 66.1°S 47.7°W |
| Times (UTC) | |
| Greatest eclipse | 3:59:41 |
| References | |
| Saros | 150 (12 of 71) |
| Catalog # (SE5000) | 9345 |
Related eclipses
Solar eclipses 1924–1928
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 | |||
References
- 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
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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