Solar eclipse of January 14, 1945

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.

Solar eclipse of January 14, 1945
Map
Type of eclipse
NatureAnnular
Gamma−0.4937
Magnitude0.997
Maximum eclipse
Duration15 s (0 min 15 s)
Coordinates51°06′S 110°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
Saros140 (25 of 71)
Catalog # (SE5000)9386

Related eclipses edit

Solar eclipses 1942–1946 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]

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

Solar eclipse series sets from 1942 to 1946
Ascending node   Descending node
115 August 12, 1942
 
Partial
120 February 4, 1943
 
Total
125 August 1, 1943
 
Annular
130 January 25, 1944
 
Total
135 July 20, 1944
 
Annular
140 January 14, 1945
 
Annular
145 July 9, 1945
 
Total
150 January 3, 1946
 
Partial
155 June 29, 1946
 
Partial

Saros 140 edit

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 edit

  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 edit