| Solar eclipse of January 27, 2093 | |
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Map
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| Type of eclipse | |
| Nature | Total |
| Gamma | -0.2737 |
| Magnitude | 1.034 |
| Maximum eclipse | |
| Duration | 2m 58s |
| Coordinates | 34.1S 136.4E |
| Max. width of band | 119 km |
| Times (UTC) | |
| Greatest eclipse | 3:22:16 |
| References | |
| Saros | 142 (27 of 72) |
| Catalog # (SE5000) | 9716 |
A total solar eclipse will occur on January 27, 2093. 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.
| 122 | February 18, 2091 Partial |
127 | August 15, 2091 Total |
| 132 | February 7, 2092 Annular |
137 | August 3, 2092 Annular |
| 142 | January 27, 2093 Total |
147 | July 23, 2093 Annular |
| 152 | January 16, 2094 Total |
157 | July 12, 2094 Partial |
It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291.[1]
Series members 17-27 occur between 1901 and 2100:
| 17 | 18 | 19 |
|---|---|---|
October 10, 1912 |
October 21, 1930 |
November 1, 1948 |
| 20 | 21 | 22 |
November 12, 1966 |
November 22, 1984 |
December 4, 2002 |
| 23 | 24 | 25 |
December 14, 2020 |
December 26, 2038 |
January 5, 2057 |
| 26 | 27 | |
January 16, 2075 |
January 27, 2093 |
