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Solar eclipse of November 3, 1994

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Solar eclipse of November 3, 1994
Map
Type of eclipse
NatureTotal
Gamma−0.3522
Magnitude1.0535
Maximum eclipse
Duration263 s (4 min 23 s)
Coordinates35°24′S 34°12′W / 35.4°S 34.2°W / -35.4; -34.2
Max. width of band189 km (117 mi)
Times (UTC)
Greatest eclipse13:40:06
References
Saros133 (44 of 72)
Catalog # (SE5000)9496

A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, November 3, 1994, with a magnitude of 1.0535. 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. Totality was visible in Peru, northern Chile, Bolivia, northern Argentina, Paraguay, Brazil and Gough Island of British overseas territory of Saint Helena, Ascension and Tristan da Cunha. The Iguazu Falls, one of the largest waterfalls systems in the world, lay in the path of totality. Totality lasted about 4.4 minutes, so it was a relatively long total solar eclipse. Occurring only 10 hours and 2 minutes before perigee (on November 3, 1994, at 23:41 UTC, while greatest eclipse at 13:39 UTC), the moon's apparent diameter was also larger. [1] [2] [3] [4] [5] [6] [7] [8] [9] [10]

Images[edit]

Eclipse details[edit]

  • Eclipse Magnitude: 1.05351
  • Eclipse Obscuration: 1.10989
  • Gamma: -0.35216
  • Greatest Eclipse: 1994 November 3 at 13:39:05.4 UTC
  • Greatest Eclipse: 1994 November 3 at 13:39:05.4 UTC
  • Location of Greatest Eclipse: 35º21′22″ S, 34º13′21″ W, South Atlantic Ocean, 1,586 km (985.5 mi) off the coast of Brazil
  • Duration of Totality: 4 minutes, 23.28 seconds (263.28 seconds)
  • Sun Right Ascension: 14.57
  • Sun Declination: −15.1
  • Sun Diameter: 1934.8 arc-seconds
  • Moon Right Ascension: 14.56
  • Moon Declination: −15.4
  • Moon Diameter: 2006.0 arc-seconds
  • Saros Series: 133rd (44 of 72)

Observations[edit]

Jay Pasachoff led an observation team from Williams College in Massachusetts, observing the total eclipse at a military base near Putre, Chile, in the Atacama Desert. The team took images of the corona and measured its brightness. Teams from Japan and South Korea also conducted observations nearby.[11] The Russian Academy of Sciences sent a team to Criciúma, Brazil, taking images of the corona in polarized light and proposing reconstruction of its ray structure.[12]

Related eclipses[edit]

Eclipses in 1994[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 133[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 1993–1996[edit]

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.[13]

Solar eclipse series sets from 1993 to 1996
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 May 21, 1993

Partial
1.1372 123 November 13, 1993

Partial
−1.0411
128

Partial in Bismarck, ND, USA
May 10, 1994

Annular
0.4077 133

Totality in Bolivia
November 3, 1994

Total
−0.3522
138 April 29, 1995

Annular
−0.3382 143

Totality in Dundlod, India
October 24, 1995

Total
0.3518
148 April 17, 1996

Partial
−1.058 153 October 12, 1996

Partial
1.1227

Saros 133[edit]

This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. 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 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’s ascending node of orbit.[14]

Series members 34–55 occur between 1801 and 2200:
34 35 36

July 17, 1814

July 27, 1832

August 7, 1850
37 38 39

August 18, 1868

August 29, 1886

September 9, 1904
40 41 42

September 21, 1922

October 1, 1940

October 12, 1958
43 44 45

October 23, 1976

November 3, 1994

November 13, 2012
46 47 48

November 25, 2030

December 5, 2048

December 17, 2066
49 50 51

December 27, 2084

January 8, 2103

January 19, 2121
52 53 54

January 30, 2139

February 9, 2157

February 21, 2175
55

March 3, 2193

Inex series[edit]

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.

Metonic series[edit]

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 10–11 March 27–29 January 15–16 November 3 August 21–22
117 119 121 123 125

June 10, 1964

March 28, 1968

January 16, 1972

November 3, 1975

August 22, 1979
127 129 131 133 135

June 11, 1983

March 29, 1987

January 15, 1991

November 3, 1994

August 22, 1998
137 139 141 143 145

June 10, 2002

March 29, 2006

January 15, 2010

November 3, 2013

August 21, 2017
147 149 151 153 155

June 10, 2021

March 29, 2025

January 14, 2029

November 3, 2032

August 21, 2036

References[edit]

  1. ^ "Ultimo eclipse total de sol del siglo". La Prensa. Panama City, Panama, Panama. 1994-11-03. p. 27. Retrieved 2023-10-18 – via Newspapers.com.
  2. ^ "Two Sunrises: Dawn Breaks Twice In South America In Rare Solar Eclipse". The Tyler Courier-Times. Tyler, Texas. 1994-11-03. p. 18. Retrieved 2023-10-18 – via Newspapers.com.
  3. ^ "Rare Solar Eclipse Amazes People In South America". Hickory Daily Record. Hickory, North Carolina. 1994-11-03. p. 35. Retrieved 2023-10-18 – via Newspapers.com.
  4. ^ "Sun rises twice in rare solar eclipse". The Times. Streator, Illinois. 1994-11-03. p. 9. Retrieved 2023-10-18 – via Newspapers.com.
  5. ^ "S. America captivated by rare eclipse of the sun". Fort Worth Star-Telegram. Fort Worth, Texas. 1994-11-03. p. 27. Retrieved 2023-10-18 – via Newspapers.com.
  6. ^ "Rare solar eclipse yields two sunrises". The Galion Inquirer. Galion, Ohio. 1994-11-03. p. 3. Retrieved 2023-10-18 – via Newspapers.com.
  7. ^ "Eclipse de sol oscurecerá hoy a cinco países sudamericanos". La Prensa. Panama City, Panama, Panama. 1994-11-03. p. 43. Retrieved 2023-10-18 – via Newspapers.com.
  8. ^ "Brazilian sky watchers wait for eclipse". The Pantagraph. Bloomington, Illinois. 1994-11-03. p. 5. Retrieved 2023-10-18 – via Newspapers.com.
  9. ^ "Eclipse shrouds South America". The Daily Herald-Tribune. Grande Prairie, Alberta, Canada. 1994-11-03. p. 9. Retrieved 2023-10-18 – via Newspapers.com.
  10. ^ "A day with 2 sunrises". The South Bend Tribune. South Bend, Indiana. 1994-11-03. p. 6. Retrieved 2023-10-18 – via Newspapers.com.
  11. ^ "1994 total eclipse". Williams College. Archived from the original on 1 September 2019.
  12. ^ "ON THE STRUCTURE OF 3.11.94 ECLIPSE CORONA". IZMIRAN. Archived from the original on 22 November 2020.
  13. ^ 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.
  14. ^ "NASA - Catalog of Solar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.

External links[edit]

Photos: