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Solar eclipse of August 3, 2073

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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°12′S 89°24′W / 43.2°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

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.

Related eclipses[edit]

Eclipses in 2073[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 127[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 2073–2076[edit]

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]

122 February 7, 2073

Partial
127 August 3, 2073

Total
132 January 27, 2074

Annular
137 July 24, 2074

Annular
142 January 16, 2075

Total
147 July 13, 2075

Annular
152 January 6, 2076

Total
157 July 1, 2076

Partial

Saros 127[edit]

This eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 82 events. The series started with a partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular or hybrid eclipses in this set. The series ends at member 82 as a partial eclipse on March 21, 2452. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of totality was produced by member 31 at 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 46–68 occur between 1801 and 2200:
46 47 48

February 21, 1803

March 4, 1821

March 15, 1839
49 50 51

March 25, 1857

April 6, 1875

April 16, 1893
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
64 65 66

September 6, 2127

September 16, 2145

September 28, 2163
67 68

October 8, 2181

October 19, 2199

Notes[edit]

  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. ^ "NASA - Catalog of Solar Eclipses of Saros 127". eclipse.gsfc.nasa.gov.

References[edit]