Solar eclipse of January 5, 2057

Solar eclipse of January 5, 2057
Map
Type of eclipse
Nature	Total
Gamma	-0.2837
Magnitude	1.0287
Maximum eclipse
Duration	149 sec (2 m 29 s)
Coordinates
Max. width of band	102 km (63 mi)
Times (UTC)
Greatest eclipse	9:47:52
References
Saros	142 (25 of 72)
Catalog # (SE5000)	9634

A total solar eclipse will occur on January 5, 2057. 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 2054-2058

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.

117	August 3, 2054 Partial	122	January 27, 2055 Partial
127	July 24, 2055 Total	132	January 16, 2056 Annular
137	July 12, 2056 Annular	142	January 5, 2057 Total
147	July 1, 2057 Annular	152	December 26, 2057 Total
157	June 21, 2058 Partial

Saros series 142

It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291.

Series members 17-27 occur between 1901 and 2100:

17	18	19
October 10, 1912	October 21, 1930	November 1, 1948
20	21	22
150px November 12, 1966	November 22, 1984	December 4, 2002
23	24	25
December 14, 2020	December 26, 2038	January 5, 2057
26	27
January 16, 2075	January 27, 2093

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1901 and 2100 are:

March 17, 1904 (Saros 128)	February 14, 1915 (Saros 129)	January 14, 1926 (Saros 130)
December 13, 1936 (Saros 131)	November 12, 1947 (Saros 132)	October 12, 1958 (Saros 133)
September 11, 1969 (Saros 134)	August 10, 1980 (Saros 135)	July 11, 1991 (Saros 136)
June 10, 2002 (Saros 137)	May 10, 2013 (Saros 138)	April 8, 2024 (Saros 139)
March 9, 2035 (Saros 140)	February 5, 2046 (Saros 141)	January 5, 2057 (Saros 142)
December 6, 2067 (Saros 143)	November 4, 2078 (Saros 144)	October 4, 2089 (Saros 145)
September 4, 2100 (Saros 146)

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).

This series has 21 eclipse events between June 1, 2011 and June 1, 2087.

May 31 – June 1	March 19–20	January 5–6	October 24–25	August 12–13
118	119	121	123	125
June 1, 2011	March 20, 2015	January 6, 2019	October 25, 2022	August 12, 2026
128	129	131	133	135
June 1, 2030	March 20, 2034	January 5, 2038	October 25, 2041	August 12, 2045
138	139	141	143	145
May 31, 2049	March 20, 2053	January 5, 2057	October 24, 2060	August 12, 2064
148	149	151	153	155
May 31, 2068	March 19, 2072	January 6, 2076	October 24, 2079	August 13, 2083
157
June 1, 2087

External links

• NASA graphics