Solar eclipse of October 12, 1996

Solar eclipse of October 12, 1996
Solar eclipse of October 12, 1996
	Map
Type of eclipse
Nature	Partial
Gamma	1.1227
Magnitude	0.7575
Maximum eclipse
Coordinates	71°42′N 32°06′E / 71.7°N 32.1°E
Times (UTC)
Greatest eclipse	14:03:04
References
Saros	153 (8 of 70)
Catalog # (SE5000)	9500

A partial solar eclipse occurred at the Moon's ascending node of orbit on Saturday, October 12, 1996, with a magnitude of 0.7575. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Images[edit]

A child viewing solar eclipse with smoked glass in western Poland

Animation

Related eclipses[edit]

Solar eclipses of 1993–1996[edit]

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 1993 to 1996
Descending node			Ascending node
Saros	Map	Gamma	Saros	Map	Gamma
118	May 21, 1993 Partial	1.1372	123	November 13, 1993 Partial	−1.0411
128 Partial in Bismarck, ND, USA	May 10, 1994 Annular	0.4077	133 Totality in Bolivia	November 3, 1994 Total	−0.3522
138	April 29, 1995 Annular	−0.3382	143 Totality in Dundlod, India	October 24, 1995 Total	0.3518
148	April 17, 1996 Partial	−1.058	153	October 12, 1996 Partial	1.1227

Saros 153[edit]

This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 38 at 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit.^[2]

Series members 1–19 occur between 1870 and 2200:
1	2	3
July 28, 1870	August 7, 1888	August 20, 1906
4	5	6
August 30, 1924	September 10, 1942	September 20, 1960
7	8	9
October 2, 1978	October 12, 1996	October 23, 2014
10	11	12
November 3, 2032	November 14, 2050	November 24, 2068
13	14	15
December 6, 2086	December 17, 2104	December 28, 2122
16	17	18
January 8, 2141	January 19, 2159	January 29, 2177
19
February 10, 2195

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 ascending node.

22 eclipse events between December 24, 1916 and July 31, 2000
December 24–25	October 12–13	July 31-Aug 1	May 18–20	March 7–8
91	93	95	97	99
December 23, 1878	October 12, 1882	July 31, 1886	May 18, 1890	March 7, 1894
101	103	105	107	109
December 23, 1897	October 12, 1901	August 1, 1905	May 19, 1909	March 8, 1913
111	113	115	117	119
December 24, 1916	October 12, 1920	July 31, 1924	May 19, 1928	March 7, 1932
121	123	125	127	129
December 25, 1935	October 12, 1939	August 1, 1943	May 20, 1947	March 7, 1951
131	133	135	137	139
December 25, 1954	October 12, 1958	July 31, 1962	May 20, 1966	March 7, 1970
141	143	145	147	149
December 24, 1973	October 12, 1977	July 31, 1981	May 19, 1985	March 7, 1989
151	153	155	157	159
December 24, 1992	October 12, 1996	July 31, 2000	May 19, 2004	March 7, 2008
161	163	165	167	169
December 24, 2011	October 13, 2015	August 1, 2019	May 19, 2023	March 8, 2027