Solar eclipse of March 7, 1951

Solar eclipse of March 7, 1951
Solar eclipse of March 7, 1951
	Map
Type of eclipse
Nature	Annular
Gamma	-0.242
Magnitude	0.9896
Maximum eclipse
Duration	59 sec (0 m 59 s)
Coordinates	17°42′S 123°30′W / 17.7°S 123.5°W
Max. width of band	38 km (24 mi)
Times (UTC)
Greatest eclipse	20:53:40
References
Saros	129 (48 of 80)
Catalog # (SE5000)	9400

An annular solar eclipse occurred on March 7, 1951 with a magnitude of 0.9896. 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 from New Zealand on March 8th (Thursday), and northern Costa Rica, Nicaragua, and San Andrés Island in Colombia on March 7th (Wednesday).

Related eclipses[]

Solar eclipses of 1950–1953[]

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 1950–1953
Ascending node		Descending node
Saros	Map	Saros	Map
119	1950 March 18 Annular (non-central)	124	1950 September 12 Total
129	1951 March 7 Annular	134	1951 September 1 Annular
139	1952 February 25 Total	144	1952 August 20 Annular
149	1953 February 14 Partial	154	1953 August 9 Partial
Solar eclipse of July 11, 1953 belongs to the next lunar year set

Saros 129[]

It is a part of Saros cycle 129, repeating every 18 years, 11 days, containing 80 events. The series started with partial solar eclipse on October 3, 1103. It contains annular eclipses on May 6, 1464 through March 18, 1969, hybrid eclipses from March 29, 1987 through April 20, 2023 and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. The longest duration of totality was 3 minutes, 43 seconds on June 25, 2131 . All eclipses in this series occurs at the Moon’s ascending node.^[2]

Series members 46–56 occur between 1901 and 2100:
46	47	48
February 14, 1915	February 24, 1933	March 7, 1951
49	50	51
March 18, 1969	March 29, 1987	April 8, 2005
52	53	54
April 20, 2023	April 30, 2041	May 11, 2059
55	56
May 22, 2077	June 2, 2095

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 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