Solar eclipse of November 15, 2077 | |
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Map
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|
Type of eclipse | |
Nature | Annular |
Gamma | 0.4705 |
Magnitude | 0.9371 |
Maximum eclipse | |
Duration | 7m 54s |
Coordinates | 7.8N 70.8W |
Max. width of band | 262 km |
Times (UTC) | |
Greatest eclipse | 17:07:56 |
References | |
Saros | 134 (47 of 71) |
Catalog # (SE5000) | 9682 |
An annular solar eclipse will occur on November 15, 2077. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun, causing the sun to look like an annulus (ring), blocking most of the Sun's light. An annular eclipse appears as a partial eclipse 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 1, 2076 Partial |
124 | November 26, 2076 Partial |
129 | May 22, 2077 Total |
134 | November 15, 2077 Annular |
139 | May 11, 2078 Total |
144 | November 4, 2078 Annular |
149 | May 1, 2079 Total |
154 | October 24, 2079 Annular |
It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428.[1]
Series members 38-48 occur between 1901 and 2100:
38 | 39 | 40 |
---|---|---|
August 10, 1915 |
August 21, 1933 |
September 1, 1951 |
41 | 42 | 43 |
September 11, 1969 |
September 23, 1987 |
October 3, 2005 |
44 | 45 | 46 |
October 14, 2023 |
October 25, 2041 |
November 5, 2059 |
47 | 48 | |
November 15, 2077 |
November 27, 2095 |