| Solar eclipse of December 27, 2084 | |
|---|---|
|  Map | |
| Type of eclipse | |
| Nature | Total | 
| Gamma | −0.4094 | 
| Magnitude | 1.0396 | 
| Maximum eclipse | |
| Duration | 184 sec (3 m 4 s) | 
| Coordinates | 47°18′S 47°42′E / 47.3°S 47.7°E | 
| Max. width of band | 146 km (91 mi) | 
| Times (UTC) | |
| Greatest eclipse | 9:13:48 | 
| References | |
| Saros | 133 (49 of 72) | 
| Catalog # (SE5000) | 9698 | 
A total solar eclipse will occur on December 27, 2084. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
Related eclipses
Solar eclipses 2083–2087
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]
| Solar eclipse series sets from 2083–2087 | ||||
|---|---|---|---|---|
| Descending node | Ascending node | |||
| 118 | July 15, 2083  Partial | 123 | January 7, 2084  Partial | |
| 128 | July 3, 2084  Annular | 133 | December 27, 2084  Total | |
| 138 | June 22, 2085  Annular | 143 | December 16, 2085  Annular | |
| 148 | June 11, 2086  Total | 153 | December 6, 2086  Partial | |
| 158 | June 1, 2087  Partial | |||
Tritos
- Preceded: Solar eclipse of January 27, 2074
- Followed: Solar eclipse of November 27, 2095
Tzolkinex
- Preceded: Solar eclipse of November 15, 2077
- Followed: Solar eclipse of February 7, 2092
Saros 133
Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850.[2] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.
| Series members 30–56 occur between 1742 and 2211 | ||
|---|---|---|
| 30 | 31 | 32 | 
| June 3, 1742 | June 13, 1760 |  June 24, 1778 | 
| 33 | 34 | 35 | 
| July 4, 1796 | July 17, 1814 | July 27, 1832 | 
| 36 | 37 | 38 | 
| August 7, 1850 |  August 18, 1868 |  August 29, 1886 | 
| 39 | 40 | 41 | 
|  September 9, 1904 |  September 21, 1922 |  October 1, 1940 | 
| 42 | 43 | 44 | 
|  October 12, 1958 |  October 23, 1976 |  November 3, 1994 | 
| 45 | 46 | 47 | 
|  November 13, 2012 |  November 25, 2030 |  December 5, 2048 | 
| 48 | 49 | 50 | 
|  December 17, 2066 |  December 27, 2084 |  January 8, 2103 | 
| 51 | 52 | 53 | 
|  January 19, 2121 |  January 30, 2139 |  February 9, 2157 | 
| 54 | 55 | 56 | 
|  February 21, 2175 |  March 3, 2193 |  March 15, 2211 | 
Notes
- ↑ 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.
- ↑ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros133.html
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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