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 the Middle East, Asia, Indonesia.

Images

Related eclipses

Solar eclipses 1993-1996

Each member 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.

Solar eclipse series sets from 1993–1996

Ascending node			Descending node
Saros	Map		Saros	Map
118	May 21, 1993 Partial		123	November 13, 1993 Partial
128	May 10, 1994 Annular		133	November 3, 1994 Total
138	April 29, 1995 Annular		143 Totality at Dundlod, India	October 24, 1995 Total
148	April 17, 1996 Partial		153	October 12, 1996 Partial

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.^[1]

Series members 17-28 occur between 1901 and 2100: 

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).

21 eclipse events between August 12, 1942 and August 11, 2018 

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

Notes

1. http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros143.html

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
• Rušin from Nim Ka Thana, India
• Russian scientist had no successful observation of the eclipse
• Russian scientist had no successful observation of the eclipse (2)
• The 1995 Eclipse in India