Solar eclipse of February 26, 1979

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Solar eclipse of February 26, 1979
Totality as seen from Brandon, Manitoba
Map
Type of eclipse
NatureTotal
Gamma0.8981
Magnitude1.0391
Maximum eclipse
Duration169 s (2 min 49 s)
Coordinates52°06′N 94°30′W / 52.1°N 94.5°W / 52.1; -94.5
Max. width of band298 km (185 mi)
Times (UTC)
Greatest eclipse16:55:06
References
Saros120 (59 of 71)
Catalog # (SE5000)9462

In astronomy, a total solar eclipse occurred on Monday, February 26, 1979. 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. The central shadow of the moon passed through the northwestern U.S. states of Washington, Oregon, Idaho, Montana (where totality covered almost the entire state), the north-central state of North Dakota, parts of the Canadian provinces of Saskatchewan, Manitoba, Ontario, Quebec, and what is now the Canadian Territory of Nunavut, and Greenland.



Visibility

Many visitors traveled to the Pacific Northwest to view the eclipse,[1] since it would be the last chance to view a total solar eclipse in the United States for almost four decades. The next over the United States will be the total solar eclipse of August 21, 2017.

Although the path of totality passed through Portland, Oregon in early morning, it was not directly observable from the Portland area due to overcast skies.[2]

The path of totality passed through Winnipeg, Manitoba in the early afternoon.

Gallery

Related eclipses

A partial lunar eclipse occurred on March 13, 1979, 15 days later, visible over Africa, Europe and Asia. A total lunar eclipse followed on September 6, 1979.

Solar eclipses of 1979–1982

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.[3] There were 8 solar eclipses between February 26, 1979 and July 20, 1982. Were there: February 26, 1979 (total solar eclipse, 0.8 days after perigee, 103.9%, 0.89811 gamma, saros 120), August 22, 1979 (small annular solar eclipse, 0.6 days before apogee, 93.3%, −0.96319 gamma, saros 125), February 16, 1980 (total solar eclipse, 1 day before perigee, 104.3%, 0.22244 gamma, saros 130), August 10, 1980 (large annular solar eclipse, 5 days before apogee, 97.3%, −0.19154 gamma, saros 135), February 4, 1981 (large annular solar eclipse, 4 days before perigee, 99.4%, −0.48375 gamma, saros 140), July 31, 1981 (total solar eclipse, 3.8 days after perigee, 102.6%, 0.57917 gamma, saros 145), January 25, 1982 (moderate partial solar eclipse, 4.7 days after apogee, 56.6%, −1.23110 gamma, saros 150) and July 20, 1982 (small partial solar eclipse, 0.9 days after perigee, 46.4%, 1.28859 gamma, saros 155).

Solar eclipse series sets from 1979 to 1982
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
120
1979 February 26
Total
0.89811 125
1979 August 22
Annular
−0.96319
130
1980 February 16
Total
0.22244 135
1980 August 10
Annular
−0.19154
140
1981 February 4
Annular
−0.48375 145
1981 July 31
Total
0.57917
150
1982 January 25
Partial
−1.23110 155
1982 July 20
Partial
1.28859
Partial solar eclipses on June 21, 1982 and December 15, 1982 occur in the next lunar year eclipse set.

Saros 120

This eclipse is a part of Saros cycle 120, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 27, 933 AD, and reached an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and total eclipses from June 8, 1564, through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occurs at the Moon’s descending node.

Series members 55–65 occur between 1901 and 2100
55 56 57

January 14, 1907

January 24, 1925

February 4, 1943
58 59 60

February 15, 1961

February 26, 1979

March 9, 1997
61 62 63

March 20, 2015

March 30, 2033

April 11, 2051
64 65

April 21, 2069

May 2, 2087

Metonic cycle

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 descending node.

21 events between July 22, 1971 and July 22, 2047
July 21–22 May 9–11 February 26–27 December 14–15 October 2–3
116 118 120 122 124

July 22, 1971

May 11, 1975

February 26, 1979

December 15, 1982

October 3, 1986
126 128 130 132 134

July 22, 1990

May 10, 1994

February 26, 1998

December 14, 2001

October 3, 2005
136 138 140 142 144

July 22, 2009

May 10, 2013

February 26, 2017

December 14, 2020

October 2, 2024
146 148 150 152 154

July 22, 2028

May 9, 2032

February 27, 2036

December 15, 2039

October 3, 2043
156

July 22, 2047

Notes

  1. ^ "Eclipse chased across Northwest". Daytona Beach Morning Journal. New York Times. February 27, 1979. p. 1A.
  2. ^ "Thick clouds hide eclipse from many". Eugene Register-Guard. Associated Press. February 26, 1979. p. 1A.
  3. ^ 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.

See also

References

Photos/observations: