Solar eclipse of July 2, 2019

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Solar eclipse of July 2, 2019
SE2019Jul02T.png
Map
Type of eclipse
Nature Total
Gamma -0.6466
Magnitude 1.0459
Maximum eclipse
Duration 273 sec (4 m 33 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 201 km (125 mi)
Times (UTC)
Greatest eclipse 19:24:08
References
Saros 127 (58 of 82)
Catalog # (SE5000) 9551

A total solar eclipse will occur on July 2, 2019 with a magnitude of 1.0459. 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. Totality will be visible from the southern Pacific Ocean east of New Zealand to the Coquimbo Region in Chile and Argentina at sunset, with the maximum of 4 minutes 32 seconds visible from the Pacific Ocean.

Images

File:SE2019Jul02T.gif

Related eclipses

Solar eclipses of 2018-2021

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.

Note: Partial solar eclipses on February 15, 2018, and August 11, 2018, occur during the previous semester series.

Solar eclipse series sets from 2018–2021
Ascending node   Descending node
117 July 13, 2018
SE2018Jul13P.png
Partial
122 January 6, 2019
SE2019Jan06P.png
Partial
127 July 2, 2019
SE2019Jul02T.png
Total
132 December 26, 2019
SE2019Dec26A.png
Annular
137 June 21, 2020
SE2020Jun21A.png
Annular
142 December 14, 2020
SE2020Dec14T.png
Total
147 June 10, 2021
SE2021Jun10A.png
Annular
152 December 4, 2021
SE2021Dec04T.png
Total

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. 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.[1]

Series members 52-62 occur between 1901 and 2100:

52 53 54
SE1911Apr28T.png
April 28, 1911
150px
May 9, 1929
SE1947May20T.png
May 20, 1947
55 56 57
150px
May 30, 1965
SE1983Jun11T.png
June 11, 1983
SE2001Jun21T.png
June 21, 2001
58 59 60
SE2019Jul02T.png
July 2, 2019
150px
July 13, 2037
SE2055Jul24T.png
July 24, 2055
61 62
150px
August 3, 2073
SE2091Aug15T.png
August 15, 2091

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, progressing from north to south between July 1, 2000 and July 1, 2076.

July 1-2 April 19-20 February 5-7 November 24-25 September 12-13
117 119 121 123 125
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127 129 131 133 135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137 139 141 143 145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147 149 151 153 155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

Notes

References


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