Solar eclipse of March 28, 1968

Last updated
Solar eclipse of March 28, 1968
SE1968Mar28P.png
Map
Type of eclipse
NaturePartial
Gamma -1.037
Magnitude 0.899
Maximum eclipse
Coordinates 61°00′S79°48′W / 61°S 79.8°W / -61; -79.8
Times (UTC)
Greatest eclipse23:00:30
References
Saros 119 (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.

Contents

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
SarosMapGammaSarosMapGamma
119 SE1968Mar28P.png
1968 March 28
Partial
-1.03704124 SE1968Sep22T.png
1968 September 22
Total
0.94507
129 SE1969Mar18A.png
1969 March 18
Annular
-0.27037134 SE1969Sep11A.png
1969 September 11
Annular
0.22014
139 SE1970Mar07T.png
1970 March 7
Total
0.44728144 SE1970Aug31A.png
1970 August 31
Annular
-0.53640
149 SE1971Feb25P.png
1971 February 25
Partial
1.11876154 SE1971Aug20P.png
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 10–11March 27–29January 15–16November 3August 21–22
117119121123125
SE1964Jun10P.png
June 10, 1964
SE1968Mar28P.png
March 28, 1968
SE1972Jan16A.png
January 16, 1972
SE1975Nov03P.png
November 3, 1975
SE1979Aug22A.png
August 22, 1979
127129131133135
SE1983Jun11T.png
June 11, 1983
SE1987Mar29H.png
March 29, 1987
SE1991Jan15A.png
January 15, 1991
SE1994Nov03T.png
November 3, 1994
SE1998Aug22A.png
August 22, 1998
137139141143145
SE2002Jun10A.png
June 10, 2002
SE2006Mar29T.png
March 29, 2006
SE2010Jan15A.png
January 15, 2010
SE2013Nov03H.png
November 3, 2013
SE2017Aug21T.png
August 21, 2017
147149151153155
SE2021Jun10A.png
June 10, 2021
SE2025Mar29P.png
March 29, 2025
SE2029Jan14P.png
January 14, 2029
SE2032Nov03P.png
November 3, 2032
SE2036Aug21P.png
August 21, 2036

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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.