Solar eclipse of March 18, 1950

Solar eclipse of March 18, 1950
Map
Type of eclipse
Nature	Annular
Gamma	0.9988
Magnitude	0.962
Maximum eclipse
Duration	-
Coordinates	60°54′S40°54′E / 60.9°S 40.9°E / -60.9; 40.9
Max. width of band	- km
Times (UTC)
Greatest eclipse	15:32:01
References
Saros	119 (62 of 71)
Catalog # (SE5000)	9398

An annular solar eclipse occurred on March 18, 1950. 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.

While it was an annular solar eclipse, it was a non-central solar eclipse (when the gamma is 0.9972 or larger).

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 119

It is a part of Saros cycle 119, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012, with a hybrid eclipse on August 31, 1030. It has annular eclipses from September 10, 1048, through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. The longest duration of totality was only 32 seconds on August 20, 1012. The longest duration of annularity was 7 minutes, 37 seconds on September 1, 1625. The longest duration of hybridity was only 18 seconds on August 31, 1030.

Series members 54–70 occur between 1801 and 2100:
54	55	56
December 21, 1805	January 1, 1824	January 11, 1842
57	58	59
January 23, 1860	February 2, 1878	February 13, 1896
60	61	62
February 25, 1914	March 7, 1932	March 18, 1950
63	64	65
March 28, 1968	April 9, 1986	April 19, 2004
66	67	68
April 30, 2022	May 11, 2040	May 22, 2058
69	70
June 1, 2076	June 13, 2094

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

Notes

1. 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