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 8m 47s
Coordinates 7.2N 169.8E
Max. width of band 285 km
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 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

Related eclipses

Solar eclipses 2094-2098

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

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]

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

Notess

References