Solar eclipse of October 1, 1940

A total solar eclipse occurred on Tuesday, October 1, 1940. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible from Colombia, Brazil, Venezuela and South Africa.

Solar eclipse of October 1, 1940
Map
Type of eclipse
NatureTotal
Gamma−0.2573
Magnitude1.0645
Maximum eclipse
Duration335 s (5 min 35 s)
Coordinates17°30′S 18°12′W / 17.5°S 18.2°W / -17.5; -18.2
Max. width of band218 km (135 mi)
Times (UTC)
Greatest eclipse12:44:06
References
Saros133 (41 of 72)
Catalog # (SE5000)9376

Observation edit

Members of the Joint Permanent Eclipse Committee of the Royal Society and Royal Astronomical Society made observations in Brazil with interferometers and spectrometers. Teams of the Royal Observatory, Greenwich and Royal Observatory, Cape of Good Hope (now combined into the South African Astronomical Observatory) went to Calvinia, South Africa to study the gravitational lens proposed by the general relativity. Other scientists went to the edge of the path of totality to study the spectral lines of the solar chromosphere. A joint team of the Heliophysical Observatory of the University of Cambridge and the Radcliffe Observatory in Pretoria, South Africa (now combined into the South African Astronomical Observatory) went to Nelspoort to study the extreme ultraviolet spectrum of the chromosphere and corona, and conducted polarization studies of the corona and sky around the sun[1].

Related eclipses edit

Solar eclipses 1939–1942 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.[2]

Solar eclipse series sets from 1939 to 1942
Descending node   Ascending node
Saros Map Saros Map
118 April 19, 1939
 
Annular
123 October 12, 1939
 
Total
128 April 7, 1940
 
Annular
133 October 1, 1940
 
Total
138 March 27, 1941
 
Annular
143 September 21, 1941
 
Total
148 March 16, 1942
 
Partial
153 September 10, 1942
 
Partial
The partial solar eclipse on August 12, 1942 occurs in the next lunar year eclipse set.

Saros 133 edit

Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850.[3] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.

Series members 30–56 occur between 1742 and 2211
30 31 32
June 3, 1742 June 13, 1760  
June 24, 1778
33 34 35
July 4, 1796 July 17, 1814 July 27, 1832
36 37 38
August 7, 1850  
August 18, 1868
 
August 29, 1886
39 40 41
 
September 9, 1904
 
September 21, 1922
 
October 1, 1940
42 43 44
 
October 12, 1958
 
October 23, 1976
 
November 3, 1994
45 46 47
 
November 13, 2012
 
November 25, 2030
 
December 5, 2048
48 49 50
 
December 17, 2066
 
December 27, 2084
 
January 8, 2103
51 52 53
 
January 19, 2121
 
January 30, 2139
 
February 9, 2157
54 55 56
 
February 21, 2175
 
March 3, 2193
 
March 15, 2211

Metonic series edit

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).

Notes edit

  1. ^ Stratton, F. J. M. (1940). "Total Solar Eclipse of October 1, 1940". Nature. 145 (3662): 32. Archived from the original on 27 August 2019. Retrieved 2016-04-05.
  2. ^ 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.
  3. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros133.html

References edit