Solar eclipse of September 2, 2035

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Solar eclipse of September 2, 2035
SE2035Sep02T.png
Map
Type of eclipse
Nature Total
Gamma 0.3727
Magnitude 1.032
Maximum eclipse
Duration 2m 54s
Coordinates 29.1N 158E
Max. width of band 116 km
Times (UTC)
Greatest eclipse 1:56:46
References
Saros 145 (23 of 77)
Catalog # (SE5000) 9586

A total solar eclipse will occur on September 2, 2035. 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.

Images[edit]

SE2035Sep02T.gif
Animated path

Related eclipses[edit]

Solar eclipses of 2033-2036[edit]

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.

Solar eclipse series sets from 2033-2036
Ascending node   Descending node
120 March 30, 2033
SE2033Mar30T.png
Total
125 September 23, 2033
SE2033Sep23P.png
Partial
130 March 20, 2034
SE2034Mar20T.png
Total
136 September 12, 2034
SE2034Sep12A.png
Annular
140 March 9, 2035
SE2035Mar09A.png
Annular
145 September 2, 2035
SE2035Sep02T.png
Total
150 February 27, 2036
SE2036Feb27P.png
Partial
155 August 21, 2036
SE2036Aug21P.png
Partial
A partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set.

Saros 145[edit]

This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, containing 77 events. The series started with partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927 through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds. [1]

Series members 16–26 occur between 1901 and 2100:

16 17 18
SE1909Jun17H.png
June 17, 1909
SE1927Jun29T.png
June 29, 1927
1945Jul09T.png
July 9, 1945
19 20 21
SE1963Jul20T.png
July 20, 1963
SE1981Jul31T.png
July 31, 1981
SE1999Aug11T.png
August 11, 1999
22 23 24
SE2017Aug21T.png
August 21, 2017
SE2035Sep02T.png
September 2, 2035
SE2053Sep12T.png
September 12, 2053
25 26
SE2071Sep23T.png
September 23, 2071
SE2089Oct04T.png
October 4, 2089

Metonic series[edit]

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 21, 1982, and June 21, 2058.

June 21 April 8-9 January 26 November 13-14 September 1-2
117 119 121 123 125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127 129 131 133 135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
SE2016Sep01A.png
September 1, 2016
137 139 141 143 145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147 149 151 153 155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
SE2047Jan26P.png
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

References[edit]

  1. ^ Espenak, Fred (Project & Website Manager), Statistics for Solar Eclipses of Saros 145, NASA, updated 2009 September 26.

External links[edit]