Solar eclipse of January 14, 1945

Last updated
Solar eclipse of January 14, 1945
SE1945Jan14A.png
Map
Type of eclipse
NatureAnnular
Gamma -0.4937
Magnitude 0.997
Maximum eclipse
Duration15 sec (0 m 15 s)
Coordinates 51°06′S110°18′E / 51.1°S 110.3°E / -51.1; 110.3
Max. width of band12 km (7.5 mi)
Times (UTC)
Greatest eclipse5:01:43
References
Saros 140 (25 of 71)
Catalog # (SE5000) 9386

An annular solar eclipse occurred on Sunday, January 14, 1945. 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 Eastern Cape in South Africa, and northeastern Tasmania Island and Furneaux Group in Australia.

Contents

Solar eclipses 1942–1946

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]

Note: The partial solar eclipse on September 10, 1942 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 1942–1946
Ascending node Descending node
115 August 12, 1942
SE1942Aug12P.png
Partial
120 February 4, 1943
SE1943Feb04T.png
Total
125 August 1, 1943
SE1943Aug01A.png
Annular
130 January 25, 1944
SE1944Jan25T.png
Total
135 July 20, 1944
SE1944Jul20A.png
Annular
140 January 14, 1945
SE1945Jan14A.png
Annular
145 July 9, 1945
1945Jul09T.png
Total
150 January 3, 1946
SE1946Jan03P.png
Partial
155 June 29, 1946
SE1946Jun29P.png
Partial

Saros 140

It is a part of Saros cycle 140, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836, hybrid eclipses from November 20, 1854 through December 23, 1908, and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. The longest duration of totality was 4 minutes, 10 seconds on August 12, 1692.

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