Solar eclipse of November 27, 2095

Solar eclipse of November 27, 2095
Map
Type of eclipse
Nature Annular
Gamma 0.4903
Magnitude 0.933
Maximum eclipse
Duration 527 sec (8 m 47 s)
Coordinates 7°12′N 169°48′E / 7.2°N 169.8°E / 7.2; 169.8
Max. width of band 285 km (177 mi)
Times (UTC)
Greatest eclipse 1:02:57
References
Saros 134 (48 of 71)
Catalog # (SE5000) 9723

An annular solar eclipse will occur on November 28, 2095. 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.

Solar eclipses 2094-2098

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.

119June 13, 2094

Partial
124December 7, 2094

Partial
129June 2, 2095

Total
134November 27, 2095

Annular
139May 22, 2096

Total
144November 15, 2096

Annular
149May 11, 2097

Total
154November 4, 2097

Annular
  164October 24, 2098

Partial

Saros 134

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]

Notess

References


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