Solar eclipse of June 11, 1983 | |
---|---|
Map
|
|
Type of eclipse | |
Nature | Total |
Gamma | -0.4947 |
Magnitude | 1.0524 |
Maximum eclipse | |
Duration | 5m 11s |
Coordinates | 6.2S 114.2E |
Max. width of band | 199 km |
Times (UTC) | |
Greatest eclipse | 4:43:33 |
References | |
Saros | 127 (56 of 82) |
Catalog # (SE5000) | 9472 |
An annual solar eclipse occurred on June 11, 1983. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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.
Contents |
This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.
Note: Partial solar eclipses on January 25, 1982 and July 20, 1982 occur in the previous lunar year eclipse set.
Ascending node | Descending node | |||
---|---|---|---|---|
Saros | Map | Saros | Map | |
117 | June 21, 1982 Partial |
122 | December 15, 1982 Partial |
|
127 | June 11, 1983 Total |
132 | December 4, 1983 Annular |
|
137 | May 30, 1984 Annular |
142 | November 22, 1984 Total |
|
147 | May 19, 1985 Partial |
152 | November 12, 1985 Total |
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 |
---|---|---|
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 | |
August 3, 2073 |
August 15, 2091 |
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 20 eclipse events between June 10, 1964 and August 21, 2036.
June 10-11 | March 27-29 | January 15-16 | November 3 | August 21-22 |
---|---|---|---|---|
117 | 119 | 121 | 123 | 125 |
June 10, 1964 |
March 28, 1968 |
January 16, 1972 |
November 3, 1975 |
August 22, 1979 |
127 | 129 | 131 | 133 | 135 |
June 11, 1983 |
March 29, 1987 |
January 15, 1991 |
November 3, 1994 |
August 22, 1998 |
137 | 139 | 141 | 143 | 145 |
June 10, 2002 |
March 29, 2006 |
January 15, 2010 |
November 3, 2013 |
August 21, 2017 |
147 | 149 | 151 | 153 | 155 |
June 10, 2021 |
March 29, 2025 |
January 14, 2029 |
November 3, 2032 |
August 21, 2036 |
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