Solar eclipse of June 21, 2001

Last updated
Solar eclipse of June 21, 2001
Williams College wl.jpg
Totality from Lusaka, Zambia by the Williams College eclipse expedition
SE2001Jun21T.png
Map
Type of eclipse
NatureTotal
Gamma −0.5701
Magnitude 1.0495
Maximum eclipse
Duration297 s (4 min 57 s)
Coordinates 11°18′S2°42′E / 11.3°S 2.7°E / -11.3; 2.7
Max. width of band200 km (120 mi)
Times (UTC)
(P1) Partial begin9:33:04
(U1) Total begin10:35:59
Greatest eclipse12:04:46
(U4) Total end13:31:37
(P4) Partial end14:35:25
References
Saros 127 (57 of 82)
Catalog # (SE5000) 9511

A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, June 21, 2001, [1] with a magnitude of 1.0495. It was the first solar eclipse of the 21st century. 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 2.25 days before perigee (on June 23, 2001, at 18:20 UTC), the Moon's apparent diameter was larger. [2]

Contents

Many people traveled to Africa to watch the eclipse; [3] [4] [5] the Daily Telegraph reported that "while some tribesmen watch a celestial crocodile eating the sun, the modern African will be counting the cash brought in by thousands of visitors". [6]

Visibility

It was visible from a narrow corridor in the southern Atlantic Ocean and southern Africa, including Angola, Zambia, Zimbabwe, Mozambique, the southern tip of Malawi, and Madagascar. A partial eclipse was seen from the much broader path of the Moon's penumbra, including eastern South America and most of Africa.

Observations

Within the path of totality, Angola got the best conditions with the highest solar zenith angle, longest duration and largest chance of clear weather. Sumbe, capital of Cuanza Sul Province, where the path first touched land, was the best in Angola with 4 minutes and 34 seconds of totality. However, the Angolan Civil War [7] prevented many from traveling to the county, and only about 500 people observed the eclipse there. Besides tourists, there were also scientists from the United States, France, Brazil, South Africa, the Czech Republic, Portugal and Hungary. [8]

Zambia, though inferior to its neighbouring country Angola in the chance of clear weather, attracted many scientists and tourists due to its stable political situation and also the fact that its capital city Lusaka was also located within the path of totality. [7] The Zambian government made it a national holiday with one day off, and ZamPost also issues special postage stamps and first-day covers. [9] Scientists from the United States, the United Kingdom, Germany, Japan, South Korea and China observed it in Zambia. [9] The Chinese Academy of Sciences sent a team of 6 people, carrying 3 gravimeters, 2 nuclear gyromagnetometers, 4 digital acquisition systems and recording systems to study the gravity anomalies recorded by Indian scientists during the total solar eclipse of October 24, 1995, and by Chinese scientists during the total solar eclipse of March 9, 1997, in Mohe County. [10] [11] With continuous observation for more than 10 years after that, China obtained the first observational evidence that the gravity field propagates at the speed of light. [12]

Coincidence

Besides the eclipse, the day was also the June solstice (winter solstice in the Southern Hemisphere where the path of totality passed) when the sun was at the northernmost limit. It was also the closest approach of Mars since 1988. [13]

Images

SE2001Jun21T.gif

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. [14]

June 21, 2001 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2001 June 21 at 09:34:04.6 UTC
First Umbral External Contact2001 June 21 at 10:37:00.4 UTC
First Central Line2001 June 21 at 10:38:10.0 UTC
First Umbral Internal Contact2001 June 21 at 10:39:19.9 UTC
Ecliptic Conjunction2001 June 21 at 11:58:49.4 UTC
Equatorial Conjunction2001 June 21 at 11:58:54.2 UTC
Greatest Eclipse2001 June 21 at 12:04:46.3 UTC
Greatest Duration2001 June 21 at 12:07:11.5 UTC
Last Umbral Internal Contact2001 June 21 at 13:30:14.3 UTC
Last Central Line2001 June 21 at 13:31:26.2 UTC
Last Umbral External Contact2001 June 21 at 13:32:37.9 UTC
Last Penumbral External Contact2001 June 21 at 14:35:26.2 UTC
June 21, 2001 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.04954
Eclipse Obscuration1.10153
Gamma−0.57013
Sun Right Ascension06h00m46.1s
Sun Declination+23°26'18.2"
Sun Semi-Diameter15'44.3"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension06h01m00.5s
Moon Declination+22°52'27.2"
Moon Semi-Diameter16'17.6"
Moon Equatorial Horizontal Parallax0°59'47.9"
ΔT64.2 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 June–July 2001
June 21
Ascending node (new moon)
July 5
Descending node (full moon)
SE2001Jun21T.png Lunar eclipse chart close-2001Jul05.png
Total solar eclipse
Solar Saros 127
Partial lunar eclipse
Lunar Saros 139

Eclipses in 2001

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 127

Inex

Triad

Solar eclipses of 2000–2003

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. [15]

The partial solar eclipses on February 5, 2000 and July 31, 2000 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2000 to 2003
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 July 1, 2000
SE2000Jul01P.png
Partial
−1.28214122
2000-12-25-partial solar eclipse Minnesota TLR.jpg
Partial projection in Minneapolis, MN, USA
December 25, 2000
SE2000Dec25P.png
Partial
1.13669
127
Williams College wl.jpg
Totality in Lusaka, Zambia
June 21, 2001
SE2001Jun21T.png
Total
−0.57013132
Partial solar eclipse December 14 2001 Minneapolis.jpg
Partial in Minneapolis, MN, USA
December 14, 2001
SE2001Dec14A.png
Annular
0.40885
137
Gregmote - 20020610 002 (by).jpg
Partial in Los Angeles, CA, USA
June 10, 2002
SE2002Jun10A.png
Annular
0.19933142
Eclipse 4-12-2002 Woomera.jpg
Totality in Woomera, South Australia
December 4, 2002
SE2002Dec04T.png
Total
−0.30204
147
Annular 2003-05-31 Culloden.png
Annularity in Culloden, Scotland
May 31, 2003
SE2003May31A.png
Annular
0.99598152
ECLIPSE LUNAR (3254112650).jpg
November 23, 2003
SE2003Nov23T.png
Total
−0.96381

Saros 127

This eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 82 events. The series started with a partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular or hybrid eclipses in this set. The series ends at member 82 as a partial eclipse on March 21, 2452. 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 totality was produced by member 31 at 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occur at the Moon’s ascending node of orbit. [16]

Series members 46–68 occur between 1801 and 2200:
464748
SE1803Feb21T.png
February 21, 1803
SE1821Mar04T.gif
March 4, 1821
SE1839Mar15T.gif
March 15, 1839
495051
SE1857Mar25T.gif
March 25, 1857
SE1875Apr06T.png
April 6, 1875
SE1893Apr16T.png
April 16, 1893
525354
SE1911Apr28T.png
April 28, 1911
SE1929May09T.png
May 9, 1929
SE1947May20T.png
May 20, 1947
555657
SE1965May30T.png
May 30, 1965
SE1983Jun11T.png
June 11, 1983
SE2001Jun21T.png
June 21, 2001
585960
SE2019Jul02T.png
July 2, 2019
SE2037Jul13T.png
July 13, 2037
SE2055Jul24T.png
July 24, 2055
616263
SE2073Aug03T.png
August 3, 2073
SE2091Aug15T.png
August 15, 2091
Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
646566
Saros127 64van82 SE2127Sep06P.jpg
September 6, 2127
Saros127 65van82 SE2145Sep16P.jpg
September 16, 2145
Saros127 66van82 SE2163Sep28P.jpg
September 28, 2163
6768
Saros127 67van82 SE2181Oct08P.jpg
October 8, 2181
Saros127 68van82 SE2199Oct19P.jpg
October 19, 2199

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 between June 21, 1982 and June 21, 2058
June 21April 8–9January 26November 13–14September 1–2
117119121123125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127129131133135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
SE2016Sep01A.png
September 1, 2016
137139141143145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147149151153155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
SE2047Jan26P.png
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

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 1801 and 2200
SE1805Jan01P.gif
January 1, 1805
(Saros 109)
SE1826Oct31P.gif
October 31, 1826
(Saros 111)
SE1848Aug28P.gif
August 28, 1848
(Saros 113)
SE1859Jul29P.gif
July 29, 1859
(Saros 114)
SE1870Jun28P.gif
June 28, 1870
(Saros 115)
SE1881May27P.gif
May 27, 1881
(Saros 116)
SE1892Apr26T.png
April 26, 1892
(Saros 117)
SE1903Mar29A.png
March 29, 1903
(Saros 118)
SE1914Feb25A.png
February 25, 1914
(Saros 119)
SE1925Jan24T.png
January 24, 1925
(Saros 120)
SE1935Dec25A.png
December 25, 1935
(Saros 121)
SE1946Nov23P.png
November 23, 1946
(Saros 122)
SE1957Oct23T.png
October 23, 1957
(Saros 123)
SE1968Sep22T.png
September 22, 1968
(Saros 124)
SE1979Aug22A.png
August 22, 1979
(Saros 125)
SE1990Jul22T.png
July 22, 1990
(Saros 126)
SE2001Jun21T.png
June 21, 2001
(Saros 127)
SE2012May20A.png
May 20, 2012
(Saros 128)
SE2023Apr20H.png
April 20, 2023
(Saros 129)
SE2034Mar20T.png
March 20, 2034
(Saros 130)
SE2045Feb16A.png
February 16, 2045
(Saros 131)
SE2056Jan16A.png
January 16, 2056
(Saros 132)
SE2066Dec17T.png
December 17, 2066
(Saros 133)
SE2077Nov15A.png
November 15, 2077
(Saros 134)
SE2088Oct14A.png
October 14, 2088
(Saros 135)
SE2099Sep14T.png
September 14, 2099
(Saros 136)
SE2110Aug15A.png
August 15, 2110
(Saros 137)
SE2121Jul14A.png
July 14, 2121
(Saros 138)
SE2132Jun13T.png
June 13, 2132
(Saros 139)
SE2143May14A.png
May 14, 2143
(Saros 140)
SE2154Apr12A.png
April 12, 2154
(Saros 141)
SE2165Mar12T.png
March 12, 2165
(Saros 142)
SE2176Feb10A.png
February 10, 2176
(Saros 143)
SE2187Jan09A.png
January 9, 2187
(Saros 144)
SE2197Dec09T.png
December 9, 2197
(Saros 145)

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
SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1856Sep29A.gif
September 29, 1856
(Saros 122)
SE1885Sep08T.png
September 8, 1885
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)
SE1943Aug01A.png
August 1, 1943
(Saros 125)
SE1972Jul10T.png
July 10, 1972
(Saros 126)
SE2001Jun21T.png
June 21, 2001
(Saros 127)
SE2030Jun01A.png
June 1, 2030
(Saros 128)
SE2059May11T.png
May 11, 2059
(Saros 129)
SE2088Apr21T.png
April 21, 2088
(Saros 130)
SE2117Apr02A.png
April 2, 2117
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)

Notes

  1. "June 21, 2001 Total Solar Eclipse". timeanddate. Retrieved 11 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 11 August 2024.
  3. "Thousands gather in Zambia for total solar eclipse". The News and Advance. 2001-06-21. p. 5. Retrieved 2023-10-25 via Newspapers.com.
  4. "Solar eclipse: Day declared national holiday as thousands come to Zambia". Hickory Daily Record. 2001-06-22. p. 2. Retrieved 2023-10-25 via Newspapers.com.
  5. "First total eclipse of new millennium sweeps across Africa". Arizona Daily Sun. 2001-06-22. p. 7. Retrieved 2023-10-25 via Newspapers.com.
  6. "Tradition and tourism flourish in solar eclipse". The Daily Telegraph. 2001-06-21. p. 17. Retrieved 2023-10-25 via Newspapers.com.
  7. 1 2 "2001年6月21日非洲日全食" (in Chinese). Beijing Planetarium. Archived from the original on 23 September 2015.
  8. "各国科学家和游客云集安哥拉观看日全食". Xinhua News Agency (in Chinese). Sohu News. 21 June 2001. Archived from the original on 4 March 2016.
  9. 1 2 Zeng Wei (21 June 2001). "日全食搅热赞比亚". Beijing Youth Daily (in Chinese). People.cn. Archived from the original on 24 September 2015.
  10. "宇宙起源理论可能改写 6科学家赴非观测日全食". Beijing Youth Daily (in Chinese). Sohu News. 15 June 2001. Archived from the original on 4 March 2016.
  11. Chai Shikuan, Xiong Sihao (25 June 2001). "中科院日全食观测队获得高质量观测数据" (in Chinese). Xinhua News Agency. Archived from the original on 2003-11-03.
  12. Sun Zifa (26 December 2012). "中国科学家全球首获引力场以光速传播的观测证据" (in Chinese). China News Service. Archived from the original on 24 September 2015.
  13. "Diamond Ring in the Sun". APOD. 21 June 2001.
  14. "Total Solar Eclipse of 2001 Jun 21". EclipseWise.com. Retrieved 11 August 2024.
  15. 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.
  16. "NASA - Catalog of Solar Eclipses of Saros 127". eclipse.gsfc.nasa.gov.

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of March 29, 2006</span> Total eclipse

A total solar eclipse occurred at the Moon’s descending node of orbit on Wednesday, March 29, 2006, with a magnitude of 1.0515. 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 after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 11, 1999</span> Total eclipse

A total solar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, August 11, 1999, with a magnitude of 1.0286. 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 3.5 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of December 4, 2002</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, December 4, 2002, with a magnitude of 1.0244. 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 1.9 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of July 11, 2010</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Tuesday, July 11 and Wednesday, July 12, 2010, with a magnitude of 1.058. 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 1.6 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 1, 2008</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Friday, August 1, 2008, with a magnitude of 1.0394. 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 2.4 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of July 11, 1991</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Thursday, July 11, 1991, with a magnitude of 1.08. 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 8 hours after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of April 29, 2014</span> 21st-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Tuesday, April 29, 2014, with a magnitude of 0.9868. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The center of the Moon's shadow missed the Earth's South Pole, but the partial eclipse was visible from parts of Antarctica and Australia, and an annular eclipse was visible from a small part of Antarctica.

<span class="mw-page-title-main">Solar eclipse of November 3, 2013</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, November 3, 2013, with a magnitude of 1.0159. It was a hybrid eclipse of the Sun with a small portion over the western Atlantic Ocean at sunrise as an annular eclipse and the rest of the path as a narrow total solar eclipse. 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 hybrid solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's in sunrise and sunset, but at Greatest Eclipse the Moon's apparent diameter is larger than the Sun's.

<span class="mw-page-title-main">Solar eclipse of March 9, 1997</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Saturday, March 8 and Sunday, March 9, 1997, with a magnitude of 1.042. 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 18.5 hours after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of February 16, 1980</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Saturday, February 16, 1980, with a magnitude of 1.0434. 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 24 hours before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of April 29, 1976</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Thursday, April 29, 1976, with a magnitude of 0.9421. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 1.9 days after apogee, the Moon's apparent diameter was smaller.

<span class="mw-page-title-main">Solar eclipse of April 19, 1958</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Saturday, April 19, 1958, with a magnitude of 0.9408. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 2.2 days after apogee, the Moon's apparent diameter was smaller.

<span class="mw-page-title-main">Solar eclipse of October 24, 1995</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, October 24, 1995, with a magnitude of 1.0213. 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 2.7 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of June 11, 1983</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, June 11, 1983, with a magnitude of 1.0524. 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 2.1 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of September 23, 1987</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Wednesday, September 23, 1987, with a magnitude of 0.9634. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring only 5 days after apogee, the Moon's apparent diameter was smaller.

<span class="mw-page-title-main">Solar eclipse of September 22, 1968</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Sunday, September 22, 1968, with a magnitude of 1.0099. 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 3.4 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.

<span class="mw-page-title-main">Solar eclipse of February 4, 1943</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Thursday, February 4 and Friday, February 5, 1943, with a magnitude of 1.0331. 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 22 hours after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of September 21, 1941</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, September 21, 1941, with a magnitude of 1.0379. 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 2.25 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of May 9, 1948</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's ascending node of orbit between Saturday, May 8 and Sunday, May 9, 1948, with a magnitude of 0.9999. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The Moon's apparent diameter was near the average diameter because it occurred 7 days after apogee and 6.7 days before perigee.

References

Photos: