Solar eclipse of October 26, 2087 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | −1.2882 |
Magnitude | 0.4696 |
Maximum eclipse | |
Coordinates | 71°00′S 130°30′W / 71°S 130.5°W |
Times ( UTC) | |
Greatest eclipse | 11:46:57 |
References | |
Saros | 125 (58 of 73) |
Catalog # (SE5000) | 9705 |
A partial solar eclipse will occur on October 26, 2087. 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]
120 |
May 2, 2087 Partial |
125 |
October 26, 2087 Partial |
130 |
April 21, 2088 Total |
135 |
October 14, 2088 Annular |
140 |
April 10, 2089 Annular |
145 |
October 4, 2089 Total |
150 |
March 31, 2090 Partial |
155 |
September 23, 2090 Total |