Solar eclipse of November 15, 2077

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Solar eclipse of November 15, 2077
SE2077Nov15A.png
Map
Type of eclipse
Nature Annular
Gamma 0.4705
Magnitude 0.9371
Maximum eclipse
Duration 474 sec (7 m 54 s)
Coordinates 7°48′N 70°48′W / 7.8°N 70.8°W / 7.8; -70.8
Max. width of band 262 km (163 mi)
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 partly 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's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

Related eclipses[edit]

Solar eclipses 2076-2079[edit]

Each member 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.

119 June 1, 2076
SE2076Jun01P.png
Partial
124 November 26, 2076
SE2076Nov26P.png
Partial
129 May 22, 2077
SE2077May22T.png
Total
134 November 15, 2077
SE2077Nov15A.png
Annular
139 May 11, 2078
SE2078May11T.png
Total
144 November 4, 2078
SE2078Nov04A.png
Annular
149 May 1, 2079
SE2079May01T.png
Total
154 October 24, 2079
SE2079Oct24A.png
Annular

Saros 134[edit]

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]

References[edit]

External links[edit]