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Solar eclipse of March 28, 1968

From Wikipedia, the free encyclopedia

Solar eclipse of March 28, 1968
Map
Type of eclipse
NaturePartial
Gamma−1.037
Magnitude0.899
Maximum eclipse
Coordinates61°00′S 79°48′W / 61°S 79.8°W / -61; -79.8
Times (UTC)
Greatest eclipse23:00:30
References
Saros119 (63 of 71)
Catalog # (SE5000)9438

A partial solar eclipse occurred on March 28, 1968. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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Transcription

Related eclipses

Solar eclipses of 1968–1971

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 1968–1971
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119

1968 March 28
Partial
−1.03704 124

1968 September 22
Total
0.94507
129

1969 March 18
Annular
−0.27037 134

1969 September 11
Annular
0.22014
139

1970 March 7
Total
0.44728 144

1970 August 31
Annular
−0.53640
149

1971 February 25
Partial
1.11876 154

1971 August 20
Partial
−1.26591
A partial solar eclipse of July 22, 1971 occurs in the next lunar year set.

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.

21 eclipse events, progressing from south to north between June 10, 1964, and August 21, 2036
June 10–11 March 27–29 January 15–16 November 3 August 21–22
117 119 121 123 125

June 10, 1964

March 28, 1968

January 16, 1972

November 3, 1975

August 22, 1979
127 129 131 133 135

June 11, 1983

March 29, 1987

January 15, 1991

November 3, 1994

August 22, 1998
137 139 141 143 145

June 10, 2002

March 29, 2006

January 15, 2010

November 3, 2013

August 21, 2017
147 149 151 153 155

June 10, 2021

March 29, 2025

January 14, 2029

November 3, 2032

August 21, 2036

References

  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.

External links

This page was last edited on 25 May 2023, at 20:38
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