Solar eclipse of June 11, 1983

Solar eclipse of June 11, 1983
Map
Type of eclipse
Nature	Total
Gamma	−0.4947
Magnitude	1.0524
Maximum eclipse
Duration	311 s (5 min 11 s)
Coordinates	6.2°S 114.2°E / -6.2; 114.2
Max. width of band	199 km (124 mi)
Times (UTC)
Greatest eclipse	4:43:33
References
Saros	127 (56 of 82)
Catalog # (SE5000)	9472

A total solar eclipse occurred on June 11, 1983. 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. The path of totality went through the Papua New Guinea, Solomon Islands, Indonesia.

Related eclipses

Solar eclipses of 1982-1985

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.

Note: Partial solar eclipses on January 25, 1982 and July 20, 1982 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1982 to 1985
Ascending node				Descending node
Saros	Map	Gamma		Saros	Map	Gamma
117	1982 June 21 Partial	−1.21017		122	1982 December 15 Partial	1.12928
127	1983 June 11 Total	−0.49475		132	1983 December 4 Annular	0.40150
137	1984 May 30 Annular	0.27552		142 Partial from Gisborne, NZ	1984 November 22 Total	−0.31318
147	1985 May 19 Partial	1.07197		152	1985 November 12 Total	−0.97948

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. There are no annular eclipses in this series. 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. All eclipses in this series occurs at the Moon’s ascending node.

Series members 52–68 occur between 1901 and 2200
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	63
August 3, 2073	August 15, 2091	August 26, 2109 (Partial)
64	65	66
September 6, 2127 (Partial	September 16, 2145 (Partial)	September 28, 2163 (Partial)
67	68
October 8, 2181 (Partial)	October 19, 2199 (Partial)

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.

21 eclipse events, progressing from south to north 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

References

• Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
  • Google interactive map
  • Besselian elements

Photos:

• Prof. Druckmüller's eclipse photography site
• Solar Corona Shape
• The 1983 Eclipse in Java