Solar eclipse of January 25, 1944
Solar eclipse of January 25, 1944 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.2025 |
Magnitude | 1.0428 |
Maximum eclipse | |
Duration | 249 s (4 min 9 s) |
Coordinates | 7°36′S 50°12′W / 7.6°S 50.2°W |
Max. width of band | 146 km (91 mi) |
Times (UTC) | |
Greatest eclipse | 15:26:42 |
References | |
Saros | 130 (48 of 73) |
Catalog # (SE5000) | 9384 |
A total solar eclipse occurred on January 25, 1944. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
Related eclipses
Solar eclipses 1942-1946
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]
The partial solar eclipses on March 16, 1942 and September 10, 1942 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 30, 1946 and November 23, 1946 occur in the next lunar year eclipse set.
Solar eclipse series sets from 1942 to 1946 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
115 | August 12, 1942![]() Partial |
−1.5244 | 120 | February 4, 1943![]() Total |
0.8734 | |
125 | August 1, 1943![]() Annular |
−0.8041 | 130 | January 25, 1944![]() Total |
0.2025 | |
135 | July 20, 1944![]() Annular |
−0.0314 | 140 | January 14, 1945![]() Annular |
−0.4937 | |
145 | July 9, 1945![]() Total |
0.7356 | 150 | January 3, 1946![]() Partial |
−1.2392 | |
155 | June 29, 1946![]() Partial |
1.4361 |
Saros 130
This eclipse is a part of Saros series 130, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular or hybrid eclipses in this set. The series ends at member 73 as a partial eclipse on October 25, 2394. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 30 at 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 41–62 occur between 1801 and 2200: | ||
---|---|---|
41 | 42 | 43 |
![]() November 9, 1817 |
![]() November 20, 1835 |
![]() November 30, 1853 |
44 | 45 | 46 |
![]() December 12, 1871 |
![]() December 22, 1889 |
![]() January 3, 1908 |
47 | 48 | 49 |
![]() January 14, 1926 |
![]() January 25, 1944 |
![]() February 5, 1962 |
50 | 51 | 52 |
![]() February 16, 1980 |
![]() February 26, 1998 |
![]() March 9, 2016 |
53 | 54 | 55 |
![]() March 20, 2034 |
![]() March 30, 2052 |
![]() April 11, 2070 |
56 | 57 | 58 |
![]() April 21, 2088 |
![]() May 3, 2106 |
![]() May 14, 2124 |
59 | 60 | 61 |
![]() May 25, 2142 |
![]() June 4, 2160 |
![]() June 16, 2178 |
62 | ||
![]() June 26, 2196 |
Notes
- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 130". eclipse.gsfc.nasa.gov.
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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