Solar eclipse of December 14, 2001

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Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, December 14, 2001,[1][2][3][4] with a magnitude of 0.9681. 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 7.9 days after perigee (on December 6, 2001, at 22:40 UTC) and 6.7 days before apogee (on December 21, 2001, at 13:00 UTC).[5]

Annularity was visible across the Pacific Ocean, southern Costa Rica, northern Nicaragua and San Andrés Island, Colombia. The central shadow passed just south of Hawaii in early morning and ended over Central America near sunset. A partial eclipse was visible for parts of North America, Central America, northwestern South America, and Hawaii.

Observation

The path of annularity was mostly on the sea, so observers were concentrated in Central America, the only land covered by the path, especially in Costa Rica with the largest area covered by the path and highest solar zenith angle. However, it was cloudy or rainy in many parts of the country during the eclipse, and only a few observers saw the annular eclipse.[6] The International Occultation Timing Association made up of scientists from different countries planned to measure the diameter of the sun with Baily's beads that appeared at the moment of the second and third contacts in Santa Rosa National Park on the northern edge of the path of annularity, but failed.[7] A team of professors from the University of Costa Rica and abroad traveled to Ostional Mixed Wildlife Refuge, kilometres north of Nosara. The sun could be seen through the clouds after the eclipse started, but it was completely clouded out when 80% was blocked by the moon. All the stages after that, including the annularity, could not be seen.[8]

Coincidentally, the 2001 Geminids peaked in the early morning of December 14 local time, less than 24 hours before the annular solar eclipse.[7]

Images

File:SE2001Dec14A.gif

Gallery

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 December 2001
December 14
Descending node (new moon)
December 30
Ascending node (full moon)
File:SE2001Dec14A.png File:Lunar eclipse chart close-2001Dec30.png
Annular solar eclipse
Solar Saros 132
Penumbral lunar eclipse
Lunar Saros 144

Related eclipses

Eclipses in 2001

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 132

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.[9]

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
Saros Map Gamma Saros Map Gamma
117 July 1, 2000
File:SE2000Jul01P.png
Partial
−1.28214 122
File:2000-12-25-partial solar eclipse Minnesota TLR.jpg
Partial projection in Minneapolis, MN, USA
December 25, 2000
File:SE2000Dec25P.png
Partial
1.13669
127
File:Williams College wl.jpg
Totality in Lusaka, Zambia
June 21, 2001
File:SE2001Jun21T.png
Total
−0.57013 132
File:Partial solar eclipse December 14 2001 Minneapolis.jpg
Partial in Minneapolis, MN, USA
December 14, 2001
File:SE2001Dec14A.png
Annular
0.40885
137
File:Gregmote - 20020610 002 (by).jpg
Partial in Los Angeles, CA, USA
June 10, 2002
File:SE2002Jun10A.png
Annular
0.19933 142
File:Eclipse 4-12-2002 Woomera.jpg
Totality in Woomera, South Australia
December 4, 2002
File:SE2002Dec04T.png
Total
−0.30204
147
File:Annular 2003-05-31 Culloden.png
Annularity in Culloden, Scotland
May 31, 2003
File:SE2003May31A.png
Annular
0.99598 152
File:ECLIPSE LUNAR (3254112650).jpg
November 23, 2003
File:SE2003Nov23T.png
Total
−0.96381

Saros 132

This eclipse is a part of Saros series 132, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146; hybrid eclipses on March 23, 2164 and April 3, 2182; and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. 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 25 at 6 minutes, 56 seconds on May 9, 1641, and the longest duration of totality will be produced by member 61 at 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occur at the Moon’s descending node of orbit.[10]

Series members 34–56 occur between 1801 and 2200:
34 35 36
File:SE1803Aug17A.png
August 17, 1803
File:SE1821Aug27A.png
August 27, 1821
File:SE1839Sep07A.png
September 7, 1839
37 38 39
File:SE1857Sep18A.png
September 18, 1857
File:SE1875Sep29A.png
September 29, 1875
File:SE1893Oct09A.png
October 9, 1893
40 41 42
File:SE1911Oct22A.png
October 22, 1911
File:SE1929Nov01A.png
November 1, 1929
File:SE1947Nov12A.png
November 12, 1947
43 44 45
File:SE1965Nov23A.png
November 23, 1965
File:SE1983Dec04A.png
December 4, 1983
File:SE2001Dec14A.png
December 14, 2001
46 47 48
File:SE2019Dec26A.png
December 26, 2019
File:SE2038Jan05A.png
January 5, 2038
File:SE2056Jan16A.png
January 16, 2056
49 50 51
File:SE2074Jan27A.png
January 27, 2074
File:SE2092Feb07A.png
February 7, 2092
File:SE2110Feb18A.png
February 18, 2110
52 53 54
File:SE2128Mar01A.png
March 1, 2128
File:SE2146Mar12A.png
March 12, 2146
File:SE2164Mar23H.png
March 23, 2164
55 56
File:SE2182Apr03H.png
April 3, 2182
File:SE2200Apr14T.png
April 14, 2200

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 2001 December 14

Inex series

Template:Solar Inex series 2001 December 14

References

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