Solar eclipse of August 3, 2073

A total solar eclipse will occur at the Moon's ascending node of orbit on Thursday, August 3, 2073, with a magnitude of 1.0294. 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.

Solar eclipse of August 3, 2073
Map
Type of eclipse
NatureTotal
Gamma−0.8763
Magnitude1.0294
Maximum eclipse
Duration149 s (2 min 29 s)
Coordinates43.2°S 89.4°W / -43.2; -89.4
Max. width of band206 km (128 mi)
Times (UTC)
Greatest eclipse17:15:23
References
Saros127 (61 of 82)
Catalog # (SE5000)9672

Eclipses in 2073

Metonic

Tzolkinex

Half-Saros
  • Preceded by: Lunar eclipse of July 8, 2064
  • Followed by: Lunar eclipse of August 8, 2082

Tritos

Solar Saros 127

Inex

Triad

Solar eclipses of 2073–2076

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]

122February 7, 2073

Partial		 127August 3, 2073

Total
132January 27, 2074

Annular		 137July 24, 2074

Annular
142January 16, 2075

Total		 147July 13, 2075

Annular
152January 6, 2076

Total		 157July 1, 2076

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

April 28, 1911
May 9, 1929
May 20, 1947
55 56 57

May 30, 1965
June 11, 1983
June 21, 2001
58 59 60

July 2, 2019
July 13, 2037
July 24, 2055
61 62 63

August 3, 2073
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)

Notes
  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.

References
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