Solar eclipse of July 24, 2055

From Wikipedia, the free encyclopedia
Solar eclipse of July 24, 2055
SE2055Jul24T.png
Map
Type of eclipse
NatureTotal
Gamma-0.8012
Magnitude1.0359
Maximum eclipse
Duration197 sec (3 m 17 s)
Coordinates33°18′S 25°48′E / 33.3°S 25.8°E / -33.3; 25.8
Max. width of band202 km (126 mi)
Times (UTC)
Greatest eclipse9:57:50
References
Saros127 (60 of 82)
Catalog # (SE5000)9631

A total solar eclipse will occur on July 24, 2055. 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[]

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 2054-58
Ascending node   Descending node
Saros Map Saros Map
117 August 3, 2054
SE2054Aug03P.png
Partial
122 January 27, 2055
SE2055Jan27P.png
Partial
127 July 24, 2055
SE2055Jul24T.png
Total
132 January 16, 2056
SE2056Jan16A.png
Annular
137 July 12, 2056
SE2056Jul12A.png
Annular
142 January 5, 2057
SE2057Jan05T.png
Total
147 July 1, 2057
SE2057Jul01A.png
Annular
152 December 26, 2057
SE2057Dec26T.png
Total
157 June 21, 2058
SE2058Jun21P.png
Partial

Saros 127[]

It is a part of Saros cycle 127, repeating every 18 years, 11 days, containing 82 events. The series started with partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular eclipses in this series. The series ends at member 82 as a partial eclipse on March 21, 2452. The longest duration of totality was 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occurs at the Moon’s ascending node.[2]

Series members 52–68 occur between 1901 and 2200
52 53 54
SE1911Apr28T.png
April 28, 1911
SE1929May09T.png
May 9, 1929
SE1947May20T.png
May 20, 1947
55 56 57
SE1965May30T.png
May 30, 1965
SE1983Jun11T.png
June 11, 1983
SE2001Jun21T.png
June 21, 2001
58 59 60
SE2019Jul02T.png
July 2, 2019
SE2037Jul13T.png
July 13, 2037
SE2055Jul24T.png
July 24, 2055
61 62 63
SE2073Aug03T.png
August 3, 2073
SE2091Aug15T.png
August 15, 2091
August 26, 2109 (Partial)
64 65 66
September 6, 2127 (Partial September 16, 2145 (Partial) September 28, 2163 (Partial)
67 68
October 8, 2181 (Partial) October 19, 2199 (Partial)

References[]

  1. ^ 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.
  2. ^ "Solar Saros series 127". NASA Goddard Space Flight Center. NASA. Retrieved 2 November 2017.

External links[]

Retrieved from ""