Solar eclipse of October 4, 2051 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | -1.2094 |
Magnitude | 0.6024 |
Maximum eclipse | |
Coordinates | 72°00′S117°42′E / 72°S 117.7°E |
Times (UTC) | |
Greatest eclipse | 21:02:14 |
References | |
Saros | 125 (56 of 73) |
Catalog # (SE5000) | 9622 |
A partial solar eclipse will occur on Wednesday, October 4, 2051. 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 2051–2054 | ||||
---|---|---|---|---|
Descending node | Ascending node | |||
Saros | Map | Saros | Map | |
120 | April 11, 2051 Partial | 125 | October 4, 2051 Partial | |
130 | March 30, 2052 Total | 135 | September 22, 2052 Annular | |
140 | March 20, 2053 Annular | 145 | September 12, 2053 Total | |
150 | March 9, 2054 Partial | 155 | September 2, 2054 Partial |
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