| Solar eclipse of May 11, 2097 | |
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Map
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| Type of eclipse | |
| Nature | Total |
| Gamma | 0.8516 |
| Magnitude | 1.0538 |
| Maximum eclipse | |
| Duration | 3m 10s |
| Coordinates | 67.4N 149.5W |
| Max. width of band | 339 km |
| Times (UTC) | |
| Greatest eclipse |
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| References | |
| Saros | 149 (25 of 71) |
| Catalog # (SE5000) | 9726 |
A total solar eclipse will occur on May 11, 2097. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.
Contents |
This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.
| 119 | June 13, 2094 Partial |
124 | December 7, 2094 Partial |
| 129 | June 2, 2095 Total |
134 | November 27, 2095 Annular |
| 139 | May 22, 2096 Total |
144 | November 15, 2096 Annular |
| 149 | May 11, 2097 Total |
154 | November 4, 2097 Annular |
| 164 | October 24, 2098 Partial |
