Solar eclipse of December 14, 2001

Last updated
Solar eclipse of December 14, 2001
Partial solar eclipse December 14 2001 Minneapolis.jpg
SE2001Dec14A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.4089
Magnitude 0.9681
Maximum eclipse
Duration233 s (3 min 53 s)
Coordinates 0°36′N130°42′W / 0.6°N 130.7°W / 0.6; -130.7
Max. width of band126 km (78 mi)
Times (UTC)
Greatest eclipse20:53:01
References
Saros 132 (45 of 71)
Catalog # (SE5000) 9512

An annular solar eclipse occurred on December 14, 2001. [1] [2] [3] 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. It 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.

Contents

The moon's apparent diameter was near the average diameter because the eclipse occurred 7.9 days after perigee (December 6, 2001 at 22:49 UTC) and 6.7 days before apogee (December 21, 2001 at 13:03 UTC).

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 [4] . 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. [5] . 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 [6] .

Coincidentally, the 2001 Geminids peaked in the early morning of December 14 local time, less than 24 hours before the annular solar eclipse [5] .

Images

SE2001Dec14A.gif

Eclipses of 2001

Tzolkinex

Half-Saros

Tritos

Solar Saros 132

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. [7]

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 132

This eclipse is a part of Saros cycle 132, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146, hybrid on March 22, 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. The longest duration of annularity was 6 minutes, 56 seconds on May 9, 1641, and totality will be 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occurs at the Moon’s descending node.

Series members 28–50 occur between 1690 and 2100:
282930
SE1695Jun11A.png
June 11, 1695
SE1713Jun22A.png
June 22, 1713
SE1731Jul04A.png
July 4, 1731
313233
SE1749Jul14A.png
July 14, 1749
SE1767Jul25A.png
July 25, 1767
SE1785Aug05A.png
August 5, 1785
343536
SE1803Aug17A.png
August 17, 1803
SE1821Aug27A.png
August 27, 1821
SE1839Sep07A.png
September 7, 1839
373839
SE1857Sep18A.png
September 18, 1857
SE1875Sep29A.png
September 29, 1875
SE1893Oct09A.png
October 9, 1893
404142
SE1911Oct22A.png
October 22, 1911
SE1929Nov01A.png
November 1, 1929
SE1947Nov12A.png
November 12, 1947
434445
SE1965Nov23A.png
November 23, 1965
SE1983Dec04A.png
December 4, 1983
SE2001Dec14A.png
December 14, 2001
464748
SE2019Dec26A.png
December 26, 2019
SE2038Jan05A.png
January 5, 2038
SE2056Jan16A.png
January 16, 2056
4950
SE2074Jan27A.png
January 27, 2074
SE2092Feb07A.png
February 7, 2092

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.

Metonic cycle

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 events between July 22, 1971 and July 22, 2047
July 21–22May 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

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References

  1. "Eclipse anular". La Prensa. 2001-12-09. p. 71. Retrieved 2023-10-25 via Newspapers.com.
  2. "Moon shadow". South Florida Sun Sentinel. 2001-12-15. p. 15. Retrieved 2023-10-25 via Newspapers.com.
  3. "Hawaii, Costa Rica had best views". The Orlando Sentinel. 2001-12-15. p. 35. Retrieved 2023-10-25 via Newspapers.com.
  4. Paul Maley. "2001 Annular Solar Eclipse in Costa Rica". Eclipse Tours. Archived from the original on 22 December 2015.
  5. 1 2 "Eclipse Expedition to Costa Rica 2001". Argelander-Instituts für Astronomie. Archived from the original on 28 June 2013.
  6. Jay M. Pasachoff. "Costa Rica Annular Eclipse Trip". ICSTARS Astronomy. Archived from the original on 4 March 2016.
  7. 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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