Solar eclipse of November 27, 2095
An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, November 27, 2095, with a magnitude of 0.933. 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
Eclipses in 2095
- A total solar eclipse on June 2, 2095.
- A partial lunar eclipse on June 17, 2095.
- An annular solar eclipse on November 27, 2095.
- A partial lunar eclipse on December 11, 2095.
Metonic
- Preceded by: Solar eclipse of February 7, 2092
- Followed by: Solar eclipse of September 14, 2099
Tzolkinex
- Preceded by: Solar eclipse of October 14, 2088
- Followed by: Solar eclipse of January 8, 2103
Half-Saros
- Preceded by: Lunar eclipse of November 20, 2086
- Followed by: Lunar eclipse of December 2, 2104
Tritos
- Preceded by: Solar eclipse of December 27, 2084
- Followed by: Solar eclipse of October 26, 2106
Solar Saros 134
- Preceded by: Solar eclipse of November 15, 2077
- Followed by: Solar eclipse of December 8, 2113
Inex
- Preceded by: Solar eclipse of December 17, 2066
- Followed by: Solar eclipse of November 6, 2124
Triad
- Preceded by: Solar eclipse of January 26, 2009
- Followed by: Solar eclipse of September 27, 2182
Solar eclipses of 2094–2098
This eclipse is a member of a semester series. An eclipse 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.[1]
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 a 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. All eclipses in this series occur at the Moon’s descending node.[2]
Series members 32–48 occur between 1801 and 2100: | ||
---|---|---|
32 | 33 | 34 |
![]() June 6, 1807 | ![]() June 16, 1825 | ![]() June 27, 1843 |
35 | 36 | 37 |
![]() July 8, 1861 | ![]() July 19, 1879 | ![]() July 29, 1897 |
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 |
Notes
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements
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By era | |
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Saros series (list) | |
Visibility | |
Historical |
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![21 August 2017 total solar eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/4/42/Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg/80px-Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg)
Total/hybrid eclipses
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- 1133
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- 2186
Annular eclipses
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- 1820
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- 1889
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![23 October 2014 partial eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png/80px-Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png)
Partial eclipses
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