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