Solar eclipse of June 10, 2002

Last updated
Solar eclipse of June 10, 2002
Gregmote - 20020610 002 (by).jpg
Partial from Los Angeles, California
SE2002Jun10A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.1993
Magnitude 0.9962
Maximum eclipse
Duration23 s (0 min 23 s)
Coordinates 34°30′N178°36′W / 34.5°N 178.6°W / 34.5; -178.6
Max. width of band13 km (8.1 mi)
Times (UTC)
Greatest eclipse23:45:22
References
Saros 137 (35 of 70)
Catalog # (SE5000) 9513

An annular solar eclipse occurred on Monday, June 10, 2002. 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. Annularity was visible in Indonesia, Palau (Kayangel Atoll), Northern Mariana on June 11 (Tuesday), and the western tip of Jalisco, Mexico, on June 10 (Monday). This eclipse was during the 2002 FIFA World Cup. The closest apogee occurred on June 4, 2002. It was the first annular solar eclipse visible in the Pacific in 6 months.

Contents

It was partially visible in some areas of the United States; in Ventura, in southern California, some observation stations were set up for public viewing. [1] In Palm Desert, in the Coachella Valley, it was clearly visible, and it "got dark, it got cool, and it got eerie". [2] A "solar eclipse party" in Fresno drew around 400 attendees, [3] and as far north as Napa Valley, dozens of people went outside to watch the eclipse., [4] and it was visible in Utah. [5] Canada's National Post predicted a "substantial crowd" for Vancouver, despite the eclipse there being less than 60%; [6] even in Victoria, where the eclipse was as low as 30%, dozens attended a show at the Dominion Astrophysical Observatory. [7]

Observations

During this eclipse, the apex of the moon's umbral cone was close to the Earth's surface, and the magnitude was large. The edges of the moon and the sun were close to each other as seen from the Earth. Baily's beads on the lunar limb, which are usually only visible during a total solar eclipse, could also be seen. Since the path of annularity was mostly on the sea and covered very little land, and the Maluku sectarian conflict prevented many observers from going to the Maluku Islands, Indonesia, observations were mainly concentrated in Palau, Northern Mariana Islands and Mexico. A Japanese team made a live webcast on Tinian Island [8] . The local weather was clear at sunrise. The sun was completely covered by clouds 20 minutes before the maximum eclipse, but finally came out from the clouds shortly before the maximum [9] [10] . In Mexico，because the annular eclipse occurred shortly before sunrise and the solar zenith angle was extremely low on land, many people observed at sea off the ports including Puerto Vallarta. However, the eclipse was mostly clouded out due to the Tropical Storm Boris, and it even rained in some places. The sun only appeared occasionally [11] .

Images

SolarEclipse2002Jun10A.GIF

Eclipses of 2002

Tzolkinex

Half-Saros

Tritos

Solar Saros 137

Inex

Solar eclipses 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. [12]

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

Solar eclipse series sets from 2000 to 2003
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 2000 July 01
SE2000Jul01P.png
Partial (south)		−1.28214122 2000 December 25
SE2000Dec25P.png
Partial (north)		1.13669
127
Williams College wl.jpg
Totality from Lusaka, Zambia 		2001 June 21
SE2001Jun21T.png
Total		−0.57013132
Partial solar eclipse December 14 2001 Minneapolis.jpg
Partial from Minneapolis, MN 		2001 December 14
SE2001Dec14A.png
Annular		0.40885
137
Gregmote - 20020610 002 (by).jpg
Partial from Los Angeles, CA 		2002 June 10
SE2002Jun10A.png
Annular		0.19933142
Eclipse 4-12-2002 Woomera.jpg
Totality from Woomera 		2002 December 04
SE2002Dec04T.png
Total		−0.30204
147
Annular 2003-05-31 Culloden.png
Culloden, Scotland 		2003 May 31
SE2003May31A.png
Annular		0.99598152 2003 November 23
SE2003Nov23T.png
Total		−0.96381

Saros 137

It is a part of Saros cycle 137, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on May 25, 1389. It contains total eclipses from August 20, 1533, through December 6, 1695, first set of hybrid eclipses from December 17, 1713, through February 11, 1804, first set of annular eclipses from February 21, 1822, through March 25, 1876, second set of hybrid eclipses from April 6, 1894, through April 28, 1930, and second set of annular eclipses from May 9, 1948, through April 13, 2507. The series ends at member 70 as a partial eclipse on June 28, 2633. The longest duration of totality was 2 minutes, 55 seconds on September 10, 1569. Solar Saros 137 has 55 umbral eclipses from August 20, 1533, through April 13, 2507 (973.62 years). That's almost 1 millennium!

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 2100
SE1805Dec21A.gif
December 21, 1805
(Saros 119)		 SE1816Nov19T.gif
November 19, 1816
(Saros 120)		 SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1838Sep18A.gif
September 18, 1838
(Saros 122)		 SE1849Aug18T.gif
August 18, 1849
(Saros 123)		 SE1860Jul18T.gif
July 18, 1860
(Saros 124)
SE1871Jun18A.gif
June 18, 1871
(Saros 125)		 SE1882May17T.png
May 17, 1882
(Saros 126)		 SE1893Apr16T.png
April 16, 1893
(Saros 127)
SE1904Mar17A.png
March 17, 1904
(Saros 128)		 SE1915Feb14A.png
February 14, 1915
(Saros 129)		 SE1926Jan14T.png
January 14, 1926
(Saros 130)
SE1936Dec13A.png
December 13, 1936
(Saros 131)		 SE1947Nov12A.png
November 12, 1947
(Saros 132)		 SE1958Oct12T.png
October 12, 1958
(Saros 133)
SE1969Sep11A.png
September 11, 1969
(Saros 134)		 SE1980Aug10A.png
August 10, 1980
(Saros 135)		 SE1991Jul11T.png
July 11, 1991
(Saros 136)
SE2002Jun10A.png
June 10, 2002
(Saros 137)		 SE2013May10A.png
May 10, 2013
(Saros 138)		 SE2024Apr08T.png
April 8, 2024
(Saros 139)
SE2035Mar09A.png
March 9, 2035
(Saros 140)		 SE2046Feb05A.png
February 5, 2046
(Saros 141)		 SE2057Jan05T.png
January 5, 2057
(Saros 142)
SE2067Dec06H.png
December 6, 2067
(Saros 143)		 SE2078Nov04A.png
November 4, 2078
(Saros 144)		 SE2089Oct04T.png
October 4, 2089
(Saros 145)
SE2100Sep04T.png
September 4, 2100
(Saros 146)

In the 22nd century:

In the 23rd century:

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. ↑ "Eclipse observation station being set up in Grant Park today". Ventura County Star. Ventura, California. 2002-06-10. p. 11. Retrieved 2023-10-15– via Newspapers.com.
  2. ↑ Velush, Lukas (2002-06-11). "Solar phenomenon awes local residents". The Desert Sun. p. 11. Retrieved 2023-10-24– via Newspapers.com.
  3. ↑ Yahaira Castro (2002-06-11). "Discovery Center's solar eclipse party proves popular". The Fresno Bee.
  4. ↑ Roseann Langlois (2002-06-11). "Solar eclipse covers Napa Valley". The Napa Valley Register.
  5. ↑ "Solar eclipse tonight last to be visible in Utah for 10 years". The Daily Spectrum. Saint George, Utah. 2002-06-10. p. 1. Retrieved 2023-10-15– via Newspapers.com.
  6. ↑ "West will have best view of solar eclipse". National Post. Ontario, Canada. 2002-06-10. p. 2. Retrieved 2023-10-15– via Newspapers.com.
  7. ↑ Gerard Young (2002-06-11). "Celestial show draws curious". Times Colonist. Victoria, British Columbia.
  8. ↑ "Ringförmige Sonnenfinsternis am 10.06.2002" (in German). Sonnenfinsternis.org. Archived from the original on 4 March 2016.
  9. ↑ "The 2002 Annular Solar Eclipse in the Marianas Islands". Eclipse Tours. Archived from the original on 22 December 2015.
  10. ↑ "闇を支配するリング" (in Japanese). Archived from the original on 22 December 2015.
  11. ↑ "Eclipse Expedition to Mexico 2002". Argelander-Instituts für Astronomie. Archived from the original on 30 June 2013.
  12. ↑ 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.

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