Solar eclipse of October 24, 1995

Solar eclipse of October 24, 1995
Solar eclipse of October 24, 1995
	Corona during total solar eclipse by Fred Espenak from Dundlod, India
	Map
Type of eclipse
Nature	Total
Gamma	0.3518
Magnitude	1.0213
Maximum eclipse
Duration	130 sec (2 m 10 s)
Coordinates	8°24′N 113°12′E / 8.4°N 113.2°E
Max. width of band	78 km (48 mi)
Times (UTC)
Greatest eclipse	4:33:30
References
Saros	143 (22 of 72)
Catalog # (SE5000)	9498

A total solar eclipse occurred on October 24, 1995. 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 Iran, Afghanistan, Pakistan, India, southwestern tip of Bangladesh, Burma, Thailand, Cambodia, Vietnam, Spratly Islands, northeastern tip of Sabah of Malaysia, Philippines and Indonesia.

An aerial observation of this eclipse was done over India,^[1] when a MiG-25 reconnaissance aircraft of the Indian Air Force was used to take images of this eclipse at an altitude of 25 km.^[2]

Images[]

Related eclipses[]

Eclipses of 1995[]

A partial lunar eclipse on April 15.
An annular solar eclipse on April 29.
A penumbral lunar eclipse on October 8.
A total solar eclipse on October 24.

Solar eclipses 1993–1996[]

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.^[3]

Solar eclipse series sets from 1993–1996
Descending node			Ascending node
Saros	Map	Gamma	Saros	Map	Gamma
118	1993 May 21 Partial	1.13720	123	1993 November 13 Partial	-1.04114
128 Partial from Bismarck, ND	1994 May 10 Annular	0.40771	133 Totality at Bolivia	1994 November 3 Total	-0.35216
138	1995 April 29 Annular	-0.33821	143 Totality at Dundlod, India	1995 October 24 Total	0.35176
148	1996 April 17 Partial	-1.05796	153	1996 October 12 Partial	1.12265

Solar 143[]

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887. All eclipses in this series occurs at the Moon’s ascending node.

Series members 17–28 occur between 1741 and 2100
8	9	10
May 23, 1743	June 3, 1761	June 14, 1779
11	12	13
June 24, 1797	July 6, 1815	July 17, 1833
14	15	16
July 28, 1851	August 7, 1869	August 19, 1887
17	18	19
August 30, 1905	September 10, 1923	September 21, 1941
20	21	22
October 2, 1959	October 12, 1977	October 24, 1995
23	24	25
November 3, 2013	November 14, 2031	November 25, 2049
26	27	28
December 6, 2067	December 16, 2085

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.

22 eclipse events between January 5, 1935 and August 11, 2018
January 4-5	October 23-24	August 10-12	May 30-31	March 18-19
111	113	115	117	119
January 5, 1935		August 12, 1942	May 30, 1946	March 18, 1950
121	123	125	127	129
January 5, 1954	October 23, 1957	August 11, 1961	May 30, 1965	March 18, 1969
131	133	135	137	139
January 4, 1973	October 23, 1976	August 10, 1980	May 30, 1984	March 18, 1988
141	143	145	147	149
January 4, 1992	October 24, 1995	August 11, 1999	May 31, 2003	March 19, 2007
151	153	155
January 4, 2011	October 23, 2014	August 11, 2018

In popular culture[]

Phil Whitaker's prize-winning debut novel Eclipse of the Sun published in 1997 and set in India has at its centre a dramatic attempt to organize a public viewing of the eclipse.

Notes[]

^ The MIGnificient Flying Machines - MiG-25R Bharat Rakshak.com 22 August 2017
^ Bhatnagar, A; Livingston, William Charles (2005). Fundamentals of Solar Astronomy. World Scientific. p. 157. ISBN 9812382445.
^ 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.

References[]

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

Photos:

[1] The MIGnificient Flying Machines - MiG-25R Bharat Rakshak.com 22 August 2017

[2] Bhatnagar, A; Livingston, William Charles (2005). Fundamentals of Solar Astronomy. World Scientific. p. 157. ISBN 9812382445.

[3] 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.

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