Solar eclipse of August 11, 1961

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Solar eclipse of August 11, 1961
SE1961Aug11A.png
Map
Type of eclipse
NatureAnnular
Gamma-0.8859
Magnitude0.9375
Maximum eclipse
Duration395 sec (6 m 35 s)
Coordinates45°48′S 4°00′E / 45.8°S 4°E / -45.8; 4
Max. width of band499 km (310 mi)
Times (UTC)
Greatest eclipse10:46:47
References
Saros125 (51 of 73)
Catalog # (SE5000)9423

An annular solar eclipse occurred on August 11, 1961. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. A small annular eclipse covered only 94% of the Sun in a very broad path, 499 km wide at maximum, and lasted 6 minutes and 35 seconds.

Related eclipses[]

Solar eclipses of 1961–1964[]

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 1961–1964
Descending node   Ascending node
Saros Map Saros Map
120 SE1961Feb15T.png
1961 February 15
Total
125 SE1961Aug11A.png
1961 August 11
Annular
130 SE1962Feb05T.png
1962 February 5
Total
135 SE1962Jul31A.png
1962 July 31
Annular
140 SE1963Jan25A.png
1963 January 25
Annular
145 SE1963Jul20T.png
1963 July 20
Total
150 SE1964Jan14P.png
1964 January 14
Partial
155 SE1964Jul09P.png
1964 July 9
Partial
Partial solar eclipses of June 10, 1964 and December 4, 1964 belong in the next lunar year set.

Saros 125[]

Solar saros 125, repeating every about 18 years and 11 days, contains 73 events. The series started with a partial solar eclipse on February 4, 1060. It has total eclipses from June 13, 1276, to July 16, 1330. It has hybrid eclipses on July 26, 1348, and August 7, 1366, and annular eclipses from August 17, 1384, to August 22, 1979. The series ends at member 73 as a partial eclipse on April 9, 2358. The longest total eclipse occurred on June 25, 1294, at 1 minute and 11 seconds; the longest annular eclipse occurred on July 10, 1907, at 7 minutes and 23 seconds.[2]

Series members 47–58 occur between 1881 and 2100:
47 48 49
SE1889Jun28A.png
June 28, 1889
SE1907Jul10A.png
July 10, 1907
SE1925Jul20A.png
July 20, 1925
50 51 52
SE1943Aug01A.png
August 1, 1943
SE1961Aug11A.png
August 11, 1961
SE1979Aug22A.png
August 22, 1979
53 54 55
SE1997Sep02P.png
September 2, 1997
SE2015Sep13P.png
September 13, 2015
SE2033Sep23P.png
September 23, 2033
56 57 58
SE2051Oct04P.png
October 4, 2051
SE2069Oct15P.png
October 15, 2069
SE2087Oct26P.png
October 26, 2087

Inex series[]

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

In the 19th century:

  • Solar Saros 120: Total Solar Eclipse of 1816 Nov 19
  • Solar Saros 121: Hybrid Solar Eclipse of 1845 Oct 30
  • Solar Saros 122: Annular Solar Eclipse of 1874 Oct 10

In the 22nd century:

  • Solar Saros 130: Total Solar Eclipse of 2106 May 03
  • Solar Saros 131: Annular Solar Eclipse of 2135 Apr 13
  • Solar Saros 132: Hybrid Solar Eclipse of 2164 Mar 23
  • Solar Saros 133: Total Solar Eclipse of 2193 Mar 03

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). All eclipses in this table occur at the Moon's ascending node.

22 eclipse events between January 5, 1935 and August 11, 2018
January 4-5 October 23-24 August 10-12 May 30-31 March 18-19
111 113 115 117 119
SE1935Jan05P.png
January 5, 1935
SE1942Aug12P.png
August 12, 1942
SE1946May30P.png
May 30, 1946
SE1950Mar18A.png
March 18, 1950
121 123 125 127 129
SE1954Jan05A.png
January 5, 1954
SE1957Oct23T.png
October 23, 1957
SE1961Aug11A.png
August 11, 1961
SE1965May30T.png
May 30, 1965
SE1969Mar18A.png
March 18, 1969
131 133 135 137 139
SE1973Jan04A.png
January 4, 1973
SE1976Oct23T.png
October 23, 1976
SE1980Aug10A.png
August 10, 1980
SE1984May30A.png
May 30, 1984
SE1988Mar18T.png
March 18, 1988
141 143 145 147 149
SE1992Jan04A.png
January 4, 1992
SE1995Oct24T.png
October 24, 1995
SE1999Aug11T.png
August 11, 1999
SE2003May31A.png
May 31, 2003
SE2007Mar19P.png
March 19, 2007
151 153 155
SE2011Jan04P.png
January 4, 2011
SE2014Oct23P.png
October 23, 2014
SE2018Aug11P.png
August 11, 2018

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. ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.

References[]

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