A partial solar eclipse occurred at the Moon's descending node of orbit between Friday, August 20 and Saturday, August 21, 1971, with a magnitude of 0.508. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

A partial eclipse was visible for parts of Australia, Oceania, and Antarctica.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.

August 20, 1971 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1971 August 20 at 20:52:59.2 UTC
Greatest Eclipse1971 August 20 at 22:39:31.5 UTC
Ecliptic Conjunction1971 August 20 at 22:54:02.4 UTC
Equatorial Conjunction1971 August 20 at 23:50:24.9 UTC
Last Penumbral External Contact1971 August 21 at 00:25:39.4 UTC
August 20, 1971 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.50797
Eclipse Obscuration0.39282
Gamma−1.26591
Sun Right Ascension09h57m48.0s
Sun Declination+12°25'50.7"
Sun Semi-Diameter15'48.4"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension09h55m45.7s
Moon Declination+11°23'25.4"
Moon Semi-Diameter14'56.3"
Moon Equatorial Horizontal Parallax0°54'49.4"
ΔT41.8 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of July–August 1971
July 22 Descending node (new moon)August 6 Ascending node (full moon)August 20 Descending node (new moon)
Partial solar eclipse Solar Saros 116Total lunar eclipse Lunar Saros 128Partial solar eclipse Solar Saros 154

Related eclipses

Eclipses in 1971

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 154

Inex

Triad

Solar eclipses of 1968–1971

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.

The partial solar eclipse on July 22, 1971 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1968 to 1971
Ascending nodeDescending node
SarosMapGammaSarosMapGamma
119March 28, 1968 Partial−1.037124September 22, 1968 Total0.9451
129March 18, 1969 Annular−0.2704134September 11, 1969 Annular0.2201
139 Totality in Williamston, NC USAMarch 7, 1970 Total0.4473144August 31, 1970 Annular−0.5364
149February 25, 1971 Partial1.1188154August 20, 1971 Partial−1.2659

Saros 154

This eclipse is a part of Saros series 154, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 19, 1917. It contains annular eclipses from October 3, 2043, through March 27, 2332; hybrid eclipses from April 7, 2350 through April 29, 2386; and total eclipses from May 9, 2404 through May 29, 3035. The series ends at member 71 as a partial eclipse on August 25, 3179. 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 annularity will be produced by member 9 at 3 minutes, 41 seconds on October 13, 2061, and the longest duration of totality will be produced by member 35 at 4 minutes, 50 seconds on July 25, 2530. All eclipses in this series occur at the Moon’s descending node of orbit.

Series members 1–16 occur between 1917 and 2200:
123
July 19, 1917July 30, 1935August 9, 1953
456
August 20, 1971August 31, 1989September 11, 2007
789
September 21, 2025October 3, 2043October 13, 2061
101112
October 24, 2079November 4, 2097November 16, 2115
131415
November 26, 2133December 8, 2151December 18, 2169
16
December 29, 2187

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 descending node.

22 eclipse events between March 27, 1884 and August 20, 1971
March 27–29January 14November 1–2August 20–21June 8
108110112114116
March 27, 1884August 20, 1895June 8, 1899
118120122124126
March 29, 1903January 14, 1907November 2, 1910August 21, 1914June 8, 1918
128130132134136
March 28, 1922January 14, 1926November 1, 1929August 21, 1933June 8, 1937
138140142144146
March 27, 1941January 14, 1945November 1, 1948August 20, 1952June 8, 1956
148150152154
March 27, 1960January 14, 1964November 2, 1967August 20, 1971

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 1982
November 29, 1807 (Saros 139)October 29, 1818 (Saros 140)September 28, 1829 (Saros 141)August 27, 1840 (Saros 142)July 28, 1851 (Saros 143)
June 27, 1862 (Saros 144)May 26, 1873 (Saros 145)April 25, 1884 (Saros 146)March 26, 1895 (Saros 147)February 23, 1906 (Saros 148)
January 23, 1917 (Saros 149)December 24, 1927 (Saros 150)November 21, 1938 (Saros 151)October 21, 1949 (Saros 152)September 20, 1960 (Saros 153)
August 20, 1971 (Saros 154)July 20, 1982 (Saros 155)

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.

Series members between 1801 and 2200
November 29, 1826 (Saros 149)November 9, 1855 (Saros 150)October 19, 1884 (Saros 151)
September 30, 1913 (Saros 152)September 10, 1942 (Saros 153)August 20, 1971 (Saros 154)
July 31, 2000 (Saros 155)July 11, 2029 (Saros 156)June 21, 2058 (Saros 157)
June 1, 2087 (Saros 158)
April 1, 2174 (Saros 161)

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