Solar_eclipse_of_September_11,_1988 Knowpia

Solar eclipse of September 11, 1988
Solar eclipse of September 11, 1988
	Map
Type of eclipse
Nature	Annular
Gamma	−0.4681
Magnitude	0.9377
Maximum eclipse
Duration	417 s (6 min 57 s)
Coordinates	20°00′S 94°24′E / 20°S 94.4°E
Max. width of band	258 km (160 mi)
Times (UTC)
Greatest eclipse	4:44:29
References
Saros	144 (15 of 70)
Catalog # (SE5000)	9483

An annular solar eclipse occurred on September 11, 1988. 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.

Related eclipses edit

Eclipses of 1988 edit

A penumbral lunar eclipse on March 3.
A total solar eclipse on March 18.
A partial lunar eclipse on August 27.
An annular solar eclipse on September 11.

Solar eclipses of 1986–1989 edit

There were 8 solar eclipses between April 9, 1986 and August 31, 1989.

Solar eclipse series sets from 1986 to 1989
Ascending node			Descending node
Saros	Map	Gamma	Saros	Map	Gamma
119	1986 April 9 Partial	−1.08215	124	1986 October 3 Hybrid	0.99305
129	1987 March 29 Hybrid	−0.30531	134	1987 September 23 Annular	0.27869
139	1988 March 18 Total	0.41879	144	1988 September 11Annular −0.46811 149 1989 March 7 Partial	1.09815	154	1989 August 31 Partial	−1.19279

Saros 144 edit

It is a part of Saros cycle 144, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no total eclipses in the series. The series ends at member 70 as a partial eclipse on May 5, 2980. The longest duration of annularity will be 9 minutes, 52 seconds on December 29, 2168.

Series members 11–21 occur between 1901 and 2100:
11	12	13
Jul 30, 1916	Aug 10, 1934	Aug 20, 1952
14	15	16
Aug 31, 1970	Sep 11, 1988	Sep 22, 2006
17	18	19
Oct 2, 2024	Oct 14, 2042	Oct 24, 2060
20	21
Nov 4, 2078	Nov 15, 2096

Inex series edit

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.

Inex series members between 1901 and 2100:
November 11, 1901 (Saros 141)	October 21, 1930 (Saros 142)	October 2, 1959 (Saros 143)
September 11, 1988 (Saros 144)	August 21, 2017 (Saros 145)	August 2, 2046 (Saros 146)
July 13, 2075 (Saros 147)

Metonic series edit

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