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 |
| 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.
Related eclipses
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.
| 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]
Notess
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
