| Solar eclipse of October 26, 2087 | |
|---|---|
 Map | |
| 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 |
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