Solar eclipse of February 25, 1952 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.4697 |
Magnitude | 1.0366 |
Maximum eclipse | |
Duration | 189 s (3 min 9 s) |
Coordinates | 15°36′N 32°42′E / 15.6°N 32.7°E |
Max. width of band | 138 km (86 mi) |
Times (UTC) | |
Greatest eclipse | 9:11:35 |
References | |
Saros | 139 (26 of 71) |
Catalog # (SE5000) | 9402 |
A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, February 25, 1952,[1][2][3][4][5][6] with a magnitude of 1.0366. 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. Occurring 1.4 days after perigee (on February 23, 1952, at 22:30 UTC), the Moon's apparent diameter was larger.[7]
The path of totality crossed French Equatorial Africa, Belgian Congo, Anglo-Egyptian Sudan, Arabia, Persia and the Soviet Union. A partial eclipse was visible for parts of Africa, Europe, West Asia, Central Asia, and South Asia.
The Vancouver News Herald 1952-02-26 p4
was invoked but never defined (see the help page).Richmond Times Dispatch 1952-02-26 p15
was invoked but never defined (see the help page).The Guardian 1952-02-26 p5
was invoked but never defined (see the help page).The News 1952-02-26 p1
was invoked but never defined (see the help page).St Louis Globe Democrat 1952-02-26 p1
was invoked but never defined (see the help page).