Solar eclipse of February 26, 1979

Last updated
Solar eclipse of February 26, 1979
1979 Solar eclipse, Brandon Manitoba Canada (35907221663).jpg
Totality as seen from Brandon, Manitoba
SE1979Feb26T.png
Map
Type of eclipse
NatureTotal
Gamma 0.8981
Magnitude 1.0391
Maximum eclipse
Duration169 s (2 min 49 s)
Coordinates 52°06′N94°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
Saros 120 (59 of 71)
Catalog # (SE5000) 9462

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]

Contents

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

Animation of eclipse path 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
EventTime (UTC)
First Penumbral External Contact1979 February 26 at 14:46:04.0 UTC
First Umbral External Contact1979 February 26 at 16:08:06.6 UTC
First Central Line1979 February 26 at 16:10:02.8 UTC
First Umbral Internal Contact1979 February 26 at 16:12:03.2 UTC
Ecliptic Conjunction1979 February 26 at 16:46:02.6 UTC
Greatest Duration1979 February 26 at 16:54:19.3 UTC
Greatest Eclipse1979 February 26 at 16:55:05.7 UTC
Equatorial Conjunction1979 February 26 at 17:22:11.4 UTC
Last Umbral Internal Contact1979 February 26 at 17:37:49.2 UTC
Last Central Line1979 February 26 at 17:39:48.9 UTC
Last Umbral External Contact1979 February 26 at 17:41:44.4 UTC
Last Penumbral External Contact1979 February 26 at 19:03:56.4 UTC
February 26, 1979 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.03907
Eclipse Obscuration1.07966
Gamma0.89811
Sun Right Ascension22h36m45.5s
Sun Declination-08°45'23.7"
Sun Semi-Diameter16'09.1"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension22h35m43.5s
Moon Declination-07°52'47.4"
Moon Semi-Diameter16'39.8"
Moon Equatorial Horizontal Parallax1°01'09.4"
ΔT49.7 s

Eclipse season

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)
SE1979Feb26T.png Lunar eclipse chart close-1979Mar13.png
Total solar eclipse
Solar Saros 120
Partial lunar eclipse
Lunar Saros 132

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
SarosMapGammaSarosMapGamma
120
1979 Solar eclipse, Brandon Manitoba Canada (35907221663).jpg
Totality in Brandon, MB,
Canada
February 26, 1979
SE1979Feb26T.png
Total
0.8981125 August 22, 1979
SE1979Aug22A.png
Annular
−0.9632
130 February 16, 1980
SE1980Feb16T.png
Total
0.2224135 August 10, 1980
SE1980Aug10A.png
Annular
−0.1915
140 February 4, 1981
SE1981Feb04A.png
Annular
−0.4838145 July 31, 1981
SE1981Jul31T.png
Total
0.5792
150 January 25, 1982
SE1982Jan25P.png
Partial
−1.2311155 July 20, 1982
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:
505152
SE1816Nov19T.gif
November 19, 1816
SE1834Nov30T.gif
November 30, 1834
SE1852Dec11T.gif
December 11, 1852
535455
SE1870Dec22T.gif
December 22, 1870
SE1889Jan01T.png
January 1, 1889
SE1907Jan14T.png
January 14, 1907
565758
SE1925Jan24T.png
January 24, 1925
SE1943Feb04T.png
February 4, 1943
SE1961Feb15T.png
February 15, 1961
596061
SE1979Feb26T.png
February 26, 1979
SE1997Mar09T.png
March 9, 1997
SE2015Mar20T.png
March 20, 2015
626364
SE2033Mar30T.png
March 30, 2033
SE2051Apr11P.png
April 11, 2051
SE2069Apr21P.png
April 21, 2069
656667
SE2087May02P.png
May 2, 2087
Saros120 66van71 SE2105May14P.jpg
May 14, 2105
Saros120 67van71 SE2123May25P.jpg
May 25, 2123
686970
Saros120 68van71 SE2141Jun04P.jpg
June 4, 2141
Saros120 69van71 SE2159Jun16P.jpg
June 16, 2159
Saros120 70van71 SE2177Jun26P.jpg
June 26, 2177
71
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 22May 9–11February 26–27December 14–15October 2–3
116118120122124
SE1971Jul22P.png
July 22, 1971
SE1975May11P.png
May 11, 1975
SE1979Feb26T.png
February 26, 1979
SE1982Dec15P.png
December 15, 1982
SE1986Oct03H.png
October 3, 1986
126128130132134
SE1990Jul22T.png
July 22, 1990
SE1994May10A.png
May 10, 1994
SE1998Feb26T.png
February 26, 1998
SE2001Dec14A.png
December 14, 2001
SE2005Oct03A.png
October 3, 2005
136138140142144
SE2009Jul22T.png
July 22, 2009
SE2013May10A.png
May 10, 2013
SE2017Feb26A.png
February 26, 2017
SE2020Dec14T.png
December 14, 2020
SE2024Oct02A.png
October 2, 2024
146148150152154
SE2028Jul22T.png
July 22, 2028
SE2032May09A.png
May 9, 2032
SE2036Feb27P.png
February 27, 2036
SE2039Dec15T.png
December 15, 2039
SE2043Oct03A.png
October 3, 2043
156
SE2047Jul22P.png
July 22, 2047

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1837 and 2200
SE1837Apr05P.png
April 5, 1837
(Saros 107)
SE1848Mar05P.gif
March 5, 1848
(Saros 108)
SE1859Feb03P.png
February 3, 1859
(Saros 109)
SE1880Dec02P.gif
December 2, 1880
(Saros 111)
SE1913Aug31P.png
August 31, 1913
(Saros 114)
SE1924Jul31P.png
July 31, 1924
(Saros 115)
SE1935Jun30P.png
June 30, 1935
(Saros 116)
SE1946May30P.png
May 30, 1946
(Saros 117)
SE1957Apr30A.png
April 30, 1957
(Saros 118)
SE1968Mar28P.png
March 28, 1968
(Saros 119)
SE1979Feb26T.png
February 26, 1979
(Saros 120)
SE1990Jan26A.png
January 26, 1990
(Saros 121)
SE2000Dec25P.png
December 25, 2000
(Saros 122)
SE2011Nov25P.png
November 25, 2011
(Saros 123)
SE2022Oct25P.png
October 25, 2022
(Saros 124)
SE2033Sep23P.png
September 23, 2033
(Saros 125)
SE2044Aug23T.png
August 23, 2044
(Saros 126)
SE2055Jul24T.png
July 24, 2055
(Saros 127)
SE2066Jun22A.png
June 22, 2066
(Saros 128)
SE2077May22T.png
May 22, 2077
(Saros 129)
SE2088Apr21T.png
April 21, 2088
(Saros 130)
SE2099Mar21A.png
March 21, 2099
(Saros 131)
SE2110Feb18A.png
February 18, 2110
(Saros 132)
SE2121Jan19T.png
January 19, 2121
(Saros 133)
SE2131Dec19A.png
December 19, 2131
(Saros 134)
SE2142Nov17A.png
November 17, 2142
(Saros 135)
SE2153Oct17T.png
October 17, 2153
(Saros 136)
SE2164Sep16A.png
September 16, 2164
(Saros 137)
SE2175Aug16A.png
August 16, 2175
(Saros 138)
SE2186Jul16T.png
July 16, 2186
(Saros 139)
SE2197Jun15A.png
June 15, 2197
(Saros 140)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
SE1805Jun26P.gif
June 26, 1805
(Saros 114)
SE1834Jun07P.gif
June 7, 1834
(Saros 115)
SE1863May17P.gif
May 17, 1863
(Saros 116)
SE1892Apr26T.png
April 26, 1892
(Saros 117)
SE1921Apr08A.png
April 8, 1921
(Saros 118)
SE1950Mar18A.png
March 18, 1950
(Saros 119)
SE1979Feb26T.png
February 26, 1979
(Saros 120)
SE2008Feb07A.png
February 7, 2008
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2065Dec27P.png
December 27, 2065
(Saros 123)
SE2094Dec07P.png
December 7, 2094
(Saros 124)
Saros125 60van73 SE2123Nov18P.jpg
November 18, 2123
(Saros 125)
Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
(Saros 126)
Saros127 67van82 SE2181Oct08P.jpg
October 8, 2181
(Saros 127)

Notes

  1. "February 26, 1979 Total Solar Eclipse". timeanddate. Retrieved 8 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 8 August 2024.
  3. "Eclipse chased across Northwest". Daytona Beach Morning Journal. New York Times. February 27, 1979. p. 1A.
  4. 1 2 3 "Total Eclipse". The Spokesman-Review . February 25, 1979. p. 6.
  5. Nast, Stan (February 26, 1979). "The Big Eclipse Cover-up". Seattle Post-Intelligencer . p. 1.
  6. "Thick clouds hide eclipse from many". Eugene Register-Guard. Associated Press. February 26, 1979. p. 1A.
  7. "Sun gives a wink to Northwest U.S." Spokane Daily Chronicle. Associated Press. February 26, 1979. p. 1.
  8. Hahn, Jon (February 27, 1979). "Goldendale's Heavens Opened For a Totaling Experience". Seattle Post-Intelligencer. p. A1.
  9. Richards, Leverett (February 27, 1979). "Moon devours sun above overcast NW". The Oregonian . p. A1.
  10. Crick, Rolla J. (February 26, 1979). "Sun watchers crowd skies". The Oregon Journal . p. 9.
  11. "Skies in path of eclipse aswarm with aircraft". The Seattle Times. February 26, 1979. p. A14.
  12. Connolly, Patrick (February 26, 1979). "Eclipse viewers aboard 727 play musical chairs". The Seattle Times. p. A14.
  13. Van, Jon (February 27, 1979). "Eclipse turns morning to night at 10:48 am". Chicago Tribune. p. 2, sec. 1.
  14. Dickinson, Terence (August 3, 2017). "Canada's last solar eclipse in 1979". Maclean's. Archived from the original on August 12, 2017. Retrieved August 24, 2017.
  15. "Thick clouds hide eclipse from many". The Register-Guard . 26 February 1979. p. 1. Archived from the original on 18 October 2020.
  16. "Tracking Our Last Eclipse of the Century" (PDF). Life : 110–118. April 1979. Archived from the original (PDF) on 13 March 2016.
  17. "Eclipse Chased Across Northwest". The Daytona Beach News-Journal . 27 February 1979. p. 1.
  18. "1979, Manitoba, Canada". Williams College. Archived from the original on 4 August 2020.
  19. Atwan, Robert (2001-10-10). Oates, Joyce Carol (ed.). The Best American Essays of the Century (Reprint ed.). Mariner Books. ISBN   9780618155873.
  20. "Total Solar Eclipse of 1979 Feb 26". EclipseWise.com. Retrieved 8 August 2024.
  21. 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.
  22. "NASA - Catalog of Solar Eclipses of Saros 120". eclipse.gsfc.nasa.gov.

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of March 9, 2016</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Tuesday, March 8 and Wednesday, March 9, 2016, with a magnitude of 1.045. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. 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 1.25 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of June 30, 1954</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, June 30, 1954, with a magnitude of 1.0357. 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. Occurring about 3.1 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of February 26, 1998</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Thursday, February 26, 1998, with a magnitude of 1.0441. 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. Occurring about 1.1 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of July 22, 1990</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Saturday, July 21 and Sunday, July 22, 1990, with a magnitude of 1.0391. 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. Occurring 2.7 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of May 22, 2096</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit between Monday, May 21 and Tuesday, May 22, 2096, with a magnitude of 1.0737. 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. Occurring about 13 hours after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of March 18, 1988</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit between Thursday, March 17 and Friday, March 18, 1988, with a magnitude of 1.0464. 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. Occurring only 1.1 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of February 14, 1934</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit between Tuesday, February 13 and Wednesday, February 14, 1934, with a magnitude of 1.0321. 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. Occurring only 1.6 days after perigee, the Moon's apparent diameter was smaller.

<span class="mw-page-title-main">Solar eclipse of December 14, 2020</span> Total eclipse

A total solar eclipse occurred at the Moon’s descending node of orbit on Monday, December 14, 2020, with a magnitude of 1.0254. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. 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 1.8 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of November 25, 2030</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, November 25, 2030, with a magnitude of 1.0468. 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. Occurring only about 14 hours before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of December 5, 2048</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Saturday, December 5, 2048, with a magnitude of 1.044. 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 greater than the Sun's, blocking all direct sunlight. 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 only about 16.5 hours before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of June 8, 1918</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Saturday, June 8 and Sunday, June 9, 1918, with a magnitude of 1.0292. 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. Occurring 3.7 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of December 26, 2038</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit between Saturday, December 25 and Sunday, December 26, 2038, with a magnitude of 1.0268. 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. Occurring about 1.7 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of December 15, 2039</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Thursday, December 15, 2039, with a magnitude of 1.0356. 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. Occurring about 4.5 hours before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of September 12, 1950</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Monday, September 11, 1950 and Tuesday, September 12, 1950, with a magnitude of 1.0182. 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. Occurring about 3.2 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of April 30, 2041</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, April 30, 2041, with a magnitude of 1.0189. 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. Occurring about 3.75 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of April 28, 1911</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit between Friday, April 28 and Saturday, April 29, 1911, with a magnitude of 1.0562. 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. Occurring about 1.4 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of January 16, 2075</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, January 16, 2075, with a magnitude of 1.0311. 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. Occurring about 1.5 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of January 16, 2094</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, January 16, 2094, with a magnitude of 1.0342. 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. Occurring about 10.5 hours before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of July 9, 1945</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, July 9, 1945, with a magnitude of 1.018. 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. Occurring about 4.4 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of November 19, 1816</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, November 19, 1816, with a magnitude of 1.0233. 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. Occurring about 1.7 days before perigee, the Moon's apparent diameter was larger.

References

Photos/observations:

Narrative Descriptions: