Solar eclipse of March 17, 1923

20th-century annular solar eclipse
33°00′S 2°24′E / 33°S 2.4°E / -33; 2.4Max. width of band305 km (190 mi)Times (UTC)Greatest eclipse12:44:58ReferencesSaros138 (26 of 70)Catalog # (SE5000)9334

An annular solar eclipse occurred on March 17, 1923. 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 Chile, Argentina, Falkland Islands including capital Stanley, Gough Island in Tristan da Cunha, South West Africa (today's Namibia), Bechuanaland Protectorate (today's Botswana, Southern Rhodesia (today's Zimbabwe) including capital Salisbury, Portuguese Mozambique (today's Mozambique), Nyasaland (today's Malawi), French Madagascar (the part now belonging to Madagascar, and the Islands of Juan de Nova and Tromelin).

Related eclipses

Solar eclipses 1921–1924

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 1921 to 1924
Descending node   Ascending node
118 April 8, 1921

Annular
123 October 1, 1921

Total
128 March 28, 1922

Annular
133 September 21, 1922

Total
138 March 17, 1923

Annular
143 September 10, 1923

Total
148 March 5, 1924

Partial
153 August 30, 1924

Partial

Saros 138

It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.

Series members 25–35 occur between 1901 and 2100:
25 26 27

March 6, 1905

March 17, 1923

March 27, 1941
28 29 30

April 8, 1959

April 18, 1977

April 29, 1995
31 32 33

May 10, 2013

May 21, 2031

May 31, 2049
34 35

June 11, 2067

June 22, 2085

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
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