Solar eclipse of February 26, 1979

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Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse occurred at the Moon's descending node of orbit on Monday, February 26, 1979,[1] with a magnitude of 1.0391. A solar eclipse is an astronomical phenomenon that 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. Occurring about 19 hours after perigee (on February 25, 1979, at 22:20 UTC), the Moon's apparent diameter was larger.[2]

The central shadow of the Moon passed through Washington, Oregon, Idaho, Montana (where totality covered almost the entire state), North Dakota, Saskatchewan, Manitoba, Ontario, Quebec, the Northwest Territories of Canada (the portion that is now Nunavut), and Greenland. A partial eclipse was visible for parts of North America, Central America, the Caribbean, and Western Europe.

Visibility

File:Solar eclipse animate (1979-Feb-26).gif
Animation of eclipse path

United States

Many visitors traveled to the Pacific Northwest to view the Monday morning eclipse,[3] as it was the last chance to view a total solar eclipse in the contiguous United States for 38 years, 5 months, 26 days. The next opportunity was on August 21, 2017.[4] Several cities, including Lewiston, Idaho, and Goldendale, Washington, organized viewing events amid an expected bump in tourist traffic.[4] Television station KING-TV of Seattle produced a live broadcast of the eclipse from Goldendale and other cities in the Northwest.[5]

Although the path of totality passed through Portland shortly after sunrise (maximum at 8:14 am PST),[4] it was not directly observable due to overcast skies in northwestern Oregon.[6][7] At the Goldendale Observatory State Park in Washington, an estimated 10,000 people were able to view the eclipse after the overcast skies parted during totality.[8][9] Over 1,000 aircraft were guided around the path of totality by local air traffic control offices; the volume of flights in the area caused delays to passenger service at Seattle–Tacoma International Airport and Portland International Airport.[10][11] The Seattle-based Pacific Science Center chartered a Boeing 727 with 94 passengers to chase the eclipse.[12]

Canada

About a half hour later, the path of totality was in Manitoba and passed through cloudless Winnipeg in the late morning, maximum was at 10:48 am CST.[13] The greatest eclipse occurred seven minutes later at 10:55 am CST.

Canada's next total solar eclipse took place on August 1, 2008, after which Canada did not see another total solar eclipse until April 8, 2024.[14]

Observations

Portland, Oregon was the largest city within the path of totality. However, the thick clouds made observation unsuccessful. Only some areas outside the city could see the sun through the holes in the clouds. There were also charter flights allowing passengers to observe from the air.[15] Clouds covered most areas of the states of Oregon and Washington, and there were some clouds in western Montana. Observations were successful in places including North Dakota.[16][17] Jay Pasachoff led a team from Williams College in Massachusetts to Brandon University in Manitoba, Canada and successfully observed the total eclipse there.[18]

In literature

Writer Annie Dillard viewed the eclipse from the Yakima River Valley in central Washington state. She described her impressions of the eclipse in an essay, "Total Eclipse," first published in the magazine Antaeus and then in her collection, Teaching a Stone to Talk (1982). It was later selected for inclusion in The Best American Essays of the [20th] Century (2000).[19] Dillard describes a nearly overwhelming emotional experience, as suggested in this quotation: "I pray you will never see anything more awful in the sky." Describing the reactions of other onlookers, she relates "I heard screams."

The 1979 eclipse was also referenced in the opening pages of Douglas Coupland's novel, Generation X.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[20]

February 26, 1979 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1979 February 26 at 14:46:04.0 UTC
First Umbral External Contact 1979 February 26 at 16:08:06.6 UTC
First Central Line 1979 February 26 at 16:10:02.8 UTC
First Umbral Internal Contact 1979 February 26 at 16:12:03.2 UTC
Ecliptic Conjunction 1979 February 26 at 16:46:02.6 UTC
Greatest Duration 1979 February 26 at 16:54:19.3 UTC
Greatest Eclipse 1979 February 26 at 16:55:05.7 UTC
Equatorial Conjunction 1979 February 26 at 17:22:11.4 UTC
Last Umbral Internal Contact 1979 February 26 at 17:37:49.2 UTC
Last Central Line 1979 February 26 at 17:39:48.9 UTC
Last Umbral External Contact 1979 February 26 at 17:41:44.4 UTC
Last Penumbral External Contact 1979 February 26 at 19:03:56.4 UTC
February 26, 1979 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.03907
Eclipse Obscuration 1.07966
Gamma 0.89811
Sun Right Ascension 22h36m45.5s
Sun Declination -08°45'23.7"
Sun Semi-Diameter 16'09.1"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 22h35m43.5s
Moon Declination -07°52'47.4"
Moon Semi-Diameter 16'39.8"
Moon Equatorial Horizontal Parallax 1°01'09.4"
ΔT 49.7 s

Eclipse season

Script error: No such module "Labelled list hatnote". This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of February–March 1979
February 26
Descending node (new moon)
March 13
Ascending node (full moon)
File:SE1979Feb26T.png File:Lunar eclipse chart close-1979Mar13.png
Total solar eclipse
Solar Saros 120
Partial lunar eclipse
Lunar Saros 132

Related eclipses

Eclipses in 1979

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 120

Inex

Triad

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.[21]

The partial solar eclipses on June 21, 1982 and December 15, 1982 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1979 to 1982
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
120
File:1979 Solar eclipse, Brandon Manitoba Canada (35907221663).jpg
Totality in Brandon, MB,
Canada
February 26, 1979
File:SE1979Feb26T.png
Total
0.8981 125 August 22, 1979
File:SE1979Aug22A.png
Annular
−0.9632
130 February 16, 1980
File:SE1980Feb16T.png
Total
0.2224 135 August 10, 1980
File:SE1980Aug10A.png
Annular
−0.1915
140 February 4, 1981
File:SE1981Feb04A.png
Annular
−0.4838 145 July 31, 1981
File:SE1981Jul31T.png
Total
0.5792
150 January 25, 1982
File:SE1982Jan25P.png
Partial
−1.2311 155 July 20, 1982
File:SE1982Jul20P.png
Partial
1.2886

Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit.[22]

Series members 50–71 occur between 1801 and 2195:
50 51 52
File:SE1816Nov19T.gif
November 19, 1816
File:SE1834Nov30T.gif
November 30, 1834
File:SE1852Dec11T.gif
December 11, 1852
53 54 55
File:SE1870Dec22T.gif
December 22, 1870
File:SE1889Jan01T.png
January 1, 1889
File:SE1907Jan14T.png
January 14, 1907
56 57 58
File:SE1925Jan24T.png
January 24, 1925
File:SE1943Feb04T.png
February 4, 1943
File:SE1961Feb15T.png
February 15, 1961
59 60 61
File:SE1979Feb26T.png
February 26, 1979
File:SE1997Mar09T.png
March 9, 1997
File:SE2015Mar20T.png
March 20, 2015
62 63 64
File:SE2033Mar30T.png
March 30, 2033
File:SE2051Apr11P.png
April 11, 2051
File:SE2069Apr21P.png
April 21, 2069
65 66 67
File:SE2087May02P.png
May 2, 2087
File:Saros120 66van71 SE2105May14P.jpg
May 14, 2105
File:Saros120 67van71 SE2123May25P.jpg
May 25, 2123
68 69 70
File:Saros120 68van71 SE2141Jun04P.jpg
June 4, 2141
File:Saros120 69van71 SE2159Jun16P.jpg
June 16, 2159
File:Saros120 70van71 SE2177Jun26P.jpg
June 26, 2177
71
File:Saros120 71van71 SE2195Jul07P.jpg
July 7, 2195

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 descending node.

21 eclipse events between July 22, 1971 and July 22, 2047
July 22 May 9–11 February 26–27 December 14–15 October 2–3
116 118 120 122 124
File:SE1971Jul22P.png
July 22, 1971
File:SE1975May11P.png
May 11, 1975
File:SE1979Feb26T.png
February 26, 1979
File:SE1982Dec15P.png
December 15, 1982
File:SE1986Oct03H.png
October 3, 1986
126 128 130 132 134
File:SE1990Jul22T.png
July 22, 1990
File:SE1994May10A.png
May 10, 1994
File:SE1998Feb26T.png
February 26, 1998
File:SE2001Dec14A.png
December 14, 2001
File:SE2005Oct03A.png
October 3, 2005
136 138 140 142 144
File:SE2009Jul22T.png
July 22, 2009
File:SE2013May10A.png
May 10, 2013
File:SE2017Feb26A.png
February 26, 2017
File:SE2020Dec14T.png
December 14, 2020
File:SE2024Oct02A.png
October 2, 2024
146 148 150 152 154
File:SE2028Jul22T.png
July 22, 2028
File:SE2032May09A.png
May 9, 2032
File:SE2036Feb27P.png
February 27, 2036
File:SE2039Dec15T.png
December 15, 2039
File:SE2043Oct03A.png
October 3, 2043
156
File:SE2047Jul22P.png
July 22, 2047

Tritos series

Template:Solar Tritos series 2000 December 25

Inex series

Template:Solar Inex series 2008 February 7

Notes

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References

External links

Photos/observations:

Narrative Descriptions:

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