Solar eclipse of March 7, 1932

Last updated
Solar eclipse of March 7, 1932
SE1932Mar07A.png
Map
Type of eclipse
NatureAnnular
Gamma -0.9673
Magnitude 0.9277
Maximum eclipse
Duration319 sec (5 m 19 s)
Coordinates 60°42′S134°24′E / 60.7°S 134.4°E / -60.7; 134.4
Max. width of band1,083 km (673 mi)
Times (UTC)
Greatest eclipse7:55:50
References
Saros 119 (61 of 71)
Catalog # (SE5000) 9356

An annular solar eclipse occurred on March 7, 1932. 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.

Contents

Solar eclipses 1931–1935

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 1931–1935
Descending node Ascending node
114 September 12, 1931
SE1931Sep12P.png
Partial
119 March 7, 1932
SE1932Mar07A.png
Annular
124 August 31, 1932
SE1932Aug31T.png
Total
129 February 24, 1933
SE1933Feb24A.png
Annular
134 August 21, 1933
SE1933Aug21A.png
Annular
139 February 14, 1934
SE1934Feb14T.png
Total
144 August 10, 1934
SE1934Aug10A.png
Annular
149 February 3, 1935
SE1935Feb03P.png
Partial
154 July 30, 1935
SE1935Jul30P.png
Partial

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.

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 24–25October 12–13July 31-Aug 1May 18–20March 7–8
9193959799
December 23, 1878October 12, 1882July 31, 1886May 18, 1890March 7, 1894
101103105107109
December 23, 1897October 12, 1901August 1, 1905May 19, 1909March 8, 1913
111113115117119
SE1916Dec24P.png
December 24, 1916
October 12, 1920 SE1924Jul31P.png
July 31, 1924
SE1928May19T.png
May 19, 1928
SE1932Mar07A.png
March 7, 1932
121123125127129
SE1935Dec25A.png
December 25, 1935
SE1939Oct12T.png
October 12, 1939
SE1943Aug01A.png
August 1, 1943
SE1947May20T.png
May 20, 1947
SE1951Mar07A.png
March 7, 1951
131133135137139
SE1954Dec25A.png
December 25, 1954
SE1958Oct12T.png
October 12, 1958
SE1962Jul31A.png
July 31, 1962
SE1966May20A.png
May 20, 1966
SE1970Mar07T.png
March 7, 1970
141143145147149
SE1973Dec24A.png
December 24, 1973
SE1977Oct12T.png
October 12, 1977
SE1981Jul31T.png
July 31, 1981
SE1985May19P.png
May 19, 1985
SE1989Mar07P.png
March 7, 1989
151153155157159
SE1992Dec24P.png
December 24, 1992
SE1996Oct12P.png
October 12, 1996
SE2000Jul31P.png
July 31, 2000
May 19, 2004March 7, 2008
161163165167169
December 24, 2011October 13, 2015August 1, 2019May 19, 2023March 8, 2027

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.

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References