Solar eclipse of September 11, 1988

An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, September 11, 1988, with a magnitude of 0.9377. 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. Annularity was visible in southeastern Somalia (including the capital city Mogadishu), the Indian Ocean and Macquarie Island of Australia.

Solar eclipse of September 11, 1988
Map
Type of eclipse
NatureAnnular
Gamma−0.4681
Magnitude0.9377
Maximum eclipse
Duration417 s (6 min 57 s)
Coordinates20°00′S 94°24′E / 20°S 94.4°E / -20; 94.4
Max. width of band258 km (160 mi)
Times (UTC)
Greatest eclipse4:44:29
References
Saros144 (15 of 70)
Catalog # (SE5000)9483
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Eclipses in 1988

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 144

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Inex

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Triad

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Solar eclipses of 1986–1989

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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 1986 to 1989
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 April 9, 1986
 
Partial
−1.0822 124 October 3, 1986
 
Hybrid
0.9931
129 March 29, 1987
 
Hybrid
−0.3053 134 September 23, 1987
 
Annular
0.2787
139 March 18, 1988
 
Total
0.4188 144 September 11, 1988
 
Annular
−0.4681
149 March 7, 1989
 
Partial
1.0981 154 August 31, 1989
 
Partial
−1.1928

Saros 144

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This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

Series members 5–26 occur between 1801 and 2200:
5 6 7
 
May 25, 1808
 
June 5, 1826
 
June 16, 1844
8 9 10
 
June 27, 1862
 
July 7, 1880
 
July 18, 1898
11 12 13
 
July 30, 1916
 
August 10, 1934
 
August 20, 1952
14 15 16
 
August 31, 1970
 
September 11, 1988
 
September 22, 2006
17 18 19
 
October 2, 2024
 
October 14, 2042
 
October 24, 2060
20 21 22
 
November 4, 2078
 
November 15, 2096
 
November 27, 2114
23 24 25
 
December 7, 2132
 
December 19, 2150
 
December 29, 2168
26
 
January 9, 2187

Inex series

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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.

Metonic series

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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 September 12, 1931 and July 1, 2011.
September 11-12 June 30-July 1 April 17-19 February 4-5 November 22-23
114 116 118 120 122
 
September 12, 1931
 
June 30, 1935
 
April 19, 1939
 
February 4, 1943
 
November 23, 1946
124 126 128 130 132
 
September 12, 1950
 
June 30, 1954
 
April 19, 1958
 
February 5, 1962
 
November 23, 1965
134 136 138 140 142
 
September 11, 1969
 
June 30, 1973
 
April 18, 1977
 
February 4, 1981
 
November 22, 1984
144 146 148 150 152
 
September 11, 1988
 
June 30, 1992
 
April 17, 1996
 
February 5, 2000
 
November 23, 2003
154 156
 
September 11, 2007
 
July 1, 2011

Notes

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  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. ^ "NASA - Catalog of Solar Eclipses of Saros 144". eclipse.gsfc.nasa.gov.

References

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