An annular solar eclipse will occur on November 27, 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 eclipse of November 27, 2095 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Annular |
| Gamma | 0.4903 |
| Magnitude | 0.933 |
| Maximum eclipse | |
| Duration | 527 s (8 min 47 s) |
| Coordinates | 7°12′N 169°48′E / 7.2°N 169.8°E |
| Max. width of band | 285 km (177 mi) |
| Times (UTC) | |
| Greatest eclipse | 1:02:57 |
| References | |
| Saros | 134 (48 of 71) |
| Catalog # (SE5000) | 9723 |
Related eclipses edit
Solar eclipses 2094–2098 edit
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 |
Tritos edit
- Preceded: Solar eclipse of December 27, 2084
- Followed: Solar eclipse of October 26, 2106
Tzolkinex edit
- Preceded: Solar eclipse of November 15, 2088
- Followed: Solar eclipse of January 19, 2102
Saros 134 edit
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 edit
- ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
- ^ "NASA - Catalog of Solar Eclipses of Saros 134". eclipse.gsfc.nasa.gov.
References edit
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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