Solar eclipse of April 29, 1995

Last updated
Solar eclipse of April 29, 1995
SE1995Apr29A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.3382
Magnitude 0.9497
Maximum eclipse
Duration397 s (6 min 37 s)
Coordinates 4°48′S79°24′W / 4.8°S 79.4°W / -4.8; -79.4
Max. width of band196 km (122 mi)
Times (UTC)
Greatest eclipse17:33:20
References
Saros 138 (30 of 70)
Catalog # (SE5000) 9497

An annular solar eclipse occurred at the Moon's descending node of orbit on Saturday, April 29, 1995, [1] [2] [3] [4] [5] [6] [7] [8] with a magnitude of 0.9497. 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 3.5 days before apogee (on May 3, 1995, at 1:50 UTC), the Moon's apparent diameter was smaller. [9]

Contents

Annularity was visible in Peru, southeastern Ecuador, southeastern Colombia and Brazil. A partial eclipse was visible for parts of South America, Mexico, Central America, Florida, the Caribbean, and West Africa.

Images

SE1995Apr29A.gif

Observations

A team of NASA's Johnson Space Center observed the annular eclipse near Puinahua District in the Peruvian Amazon rainforest. The weather was clear and the observations were successful. [10]

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 April 1995
April 15
Ascending node (full moon)
 April 29
Descending node (new moon)
Lunar eclipse chart close-1995Apr15.png SE1995Apr29A.png
Partial lunar eclipse
Lunar Saros 112		 Annular solar eclipse
Solar Saros 138

Eclipses in 1995

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 138

Inex

Triad

Solar eclipses of 1993–1996

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. [11]

Solar eclipse series sets from 1993 to 1996
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 May 21, 1993
SE1993May21P.png
Partial		1.1372123 November 13, 1993
SE1993Nov13P.png
Partial		−1.0411
128
Solar Eclipse 1994 (7160293094).jpg
Partial in Bismarck, ND, USA 		May 10, 1994
SE1994May10A.png
Annular		0.4077133
Diamond Ring, Total Solar Eclipse, Bolivia, 1994 (3183977692).jpg
Totality in Bolivia 		November 3, 1994
SE1994Nov03T.png
Total		−0.3522
138 April 29, 1995
SE1995Apr29A.png
Annular		−0.3382143
Hao WLCC 941103.jpg
Totality in Dundlod, India 		October 24, 1995
SE1995Oct24T.png
Total		0.3518
148 April 17, 1996
SE1996Apr17P.png
Partial		−1.058153 October 12, 1996
SE1996Oct12P.png
Partial		1.1227

Saros 138

This eclipse is a part of Saros series 138, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482; a hybrid eclipse on March 1, 2500; and total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. 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 23 at 8 minutes, 2 seconds on February 11, 1869, and the longest duration of totality will be produced by member 61 at 56 seconds on April 3, 2554. All eclipses in this series occur at the Moon’s descending node of orbit. [12]

Series members 20–41 occur between 1801 and 2200:
202122
SE1815Jan10A.png
January 10, 1815		 SE1833Jan20A.png
January 20, 1833		 SE1851Feb01A.png
February 1, 1851
232425
SE1869Feb11A.png
February 11, 1869		 SE1887Feb22A.png
February 22, 1887		 SE1905Mar06A.png
March 6, 1905
262728
SE1923Mar17A.png
March 17, 1923 		SE1941Mar27A.png
March 27, 1941 		SE1959Apr08A.png
April 8, 1959
293031
SE1977Apr18A.png
April 18, 1977 		SE1995Apr29A.png
April 29, 1995 		SE2013May10A.png
May 10, 2013
323334
SE2031May21A.png
May 21, 2031 		SE2049May31A.png
May 31, 2049 		SE2067Jun11A.png
June 11, 2067
353637
SE2085Jun22A.png
June 22, 2085 		SE2103Jul04A.png
July 4, 2103		 SE2121Jul14A.png
July 14, 2121
383940
SE2139Jul25A.png
July 25, 2139		 SE2157Aug05A.png
August 5, 2157		 SE2175Aug16A.png
August 16, 2175
41
SE2193Aug26A.png
August 26, 2193

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 11, 1953 and July 11, 2029
July 10–11April 29–30February 15–16December 4September 21–23
116118120122124
SE1953Jul11P.png
July 11, 1953 		SE1957Apr30A.png
April 30, 1957 		SE1961Feb15T.png
February 15, 1961 		SE1964Dec04P.png
December 4, 1964 		SE1968Sep22T.png
September 22, 1968
126128130132134
SE1972Jul10T.png
July 10, 1972 		SE1976Apr29A.png
April 29, 1976 		SE1980Feb16T.png
February 16, 1980 		SE1983Dec04A.png
December 4, 1983 		SE1987Sep23A.png
September 23, 1987
136138140142144
SE1991Jul11T.png
July 11, 1991 		SE1995Apr29A.png
April 29, 1995 		SE1999Feb16A.png
February 16, 1999 		SE2002Dec04T.png
December 4, 2002 		SE2006Sep22A.png
September 22, 2006
146148150152154
SE2010Jul11T.png
July 11, 2010 		SE2014Apr29A.png
April 29, 2014 		SE2018Feb15P.png
February 15, 2018 		SE2021Dec04T.png
December 4, 2021 		SE2025Sep21P.png
September 21, 2025
156
SE2029Jul11P.png
July 11, 2029

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
SE1809Oct09T.gif
October 9, 1809
(Saros 121)		 SE1820Sep07A.png
September 7, 1820
(Saros 122)		 SE1831Aug07T.gif
August 7, 1831
(Saros 123)		 SE1842Jul08T.png
July 8, 1842
(Saros 124)		 SE1853Jun06A.gif
June 6, 1853
(Saros 125)
SE1864May06H.gif
May 6, 1864
(Saros 126)		 SE1875Apr06T.png
April 6, 1875
(Saros 127)		 SE1886Mar05A.gif
March 5, 1886
(Saros 128)		 SE1897Feb01A.gif
February 1, 1897
(Saros 129)		 SE1908Jan03T.png
January 3, 1908
(Saros 130)
SE1918Dec03A.png
December 3, 1918
(Saros 131)		 SE1929Nov01A.png
November 1, 1929
(Saros 132)		 SE1940Oct01T.png
October 1, 1940
(Saros 133)		 SE1951Sep01A.png
September 1, 1951
(Saros 134)		 SE1962Jul31A.png
July 31, 1962
(Saros 135)
SE1973Jun30T.png
June 30, 1973
(Saros 136)		 SE1984May30A.png
May 30, 1984
(Saros 137)		 SE1995Apr29A.png
April 29, 1995
(Saros 138)		 SE2006Mar29T.png
March 29, 2006
(Saros 139)		 SE2017Feb26A.png
February 26, 2017
(Saros 140)
SE2028Jan26A.png
January 26, 2028
(Saros 141)		 SE2038Dec26T.png
December 26, 2038
(Saros 142)		 SE2049Nov25H.png
November 25, 2049
(Saros 143)		 SE2060Oct24A.png
October 24, 2060
(Saros 144)		 SE2071Sep23T.png
September 23, 2071
(Saros 145)
SE2082Aug24T.png
August 24, 2082
(Saros 146)		 SE2093Jul23A.png
July 23, 2093
(Saros 147)		 SE2104Jun22T.png
June 22, 2104
(Saros 148)		 SE2115May24T.png
May 24, 2115
(Saros 149)		 Saros150 23van71 SE2126Apr22A.jpg
April 22, 2126
(Saros 150)
Saros151 21van72 SE2137Mar21A.jpg
March 21, 2137
(Saros 151)		 Saros152 20van70 SE2148Feb19T.jpg
February 19, 2148
(Saros 152)		 Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
(Saros 153)		 Saros154 15van71 SE2169Dec18A.jpg
December 18, 2169
(Saros 154)		 Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
(Saros 155)
Saros156 11van69 SE2191Oct18A.jpg
October 18, 2191
(Saros 156)

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
SE1821Aug27A.gif
August 27, 1821
(Saros 132)		 SE1850Aug07T.gif
August 7, 1850
(Saros 133)		 SE1879Jul19A.png
July 19, 1879
(Saros 134)
SE1908Jun28A.png
June 28, 1908
(Saros 135)		 SE1937Jun08T.png
June 8, 1937
(Saros 136)		 SE1966May20A.png
May 20, 1966
(Saros 137)
SE1995Apr29A.png
April 29, 1995
(Saros 138)		 SE2024Apr08T.png
April 8, 2024
(Saros 139)		 SE2053Mar20A.png
March 20, 2053
(Saros 140)
SE2082Feb27A.png
February 27, 2082
(Saros 141)		 SE2111Feb08T.png
February 8, 2111
(Saros 142)		 SE2140Jan20A.png
January 20, 2140
(Saros 143)
SE2168Dec29A.png
December 29, 2168
(Saros 144)		 SE2197Dec09T.png
December 9, 2197
(Saros 145)

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References

  1. ↑ "April 29, 1995 Annular Solar Eclipse". timeanddate. Retrieved 10 August 2024.
  2. ↑ "Hoy, eclipse solar parcial". La Prensa. Panama City, Panama, Panama. 1995-04-29. p. 44. Retrieved 2023-10-18– via Newspapers.com.
  3. ↑ "Eclipse anular de sol causa entusiasmo y advertencias en Perú". El Nuevo Herald. Miami, Florida. 1995-04-29. p. 21. Retrieved 2023-10-18– via Newspapers.com.
  4. ↑ "AstroData". The Morning Call. Allentown, Pennsylvania. 1995-04-29. p. 86. Retrieved 2023-10-18– via Newspapers.com.
  5. ↑ "UNH has another alternative paper". The Boston Globe. Boston, Massachusetts. 1995-04-30. p. 303. Retrieved 2023-10-18– via Newspapers.com.
  6. ↑ "Partial eclipse is seen at Deltona observatory". The Orlando Sentinel. Orlando, Florida. 1995-04-30. p. 283. Retrieved 2023-10-18– via Newspapers.com.
  7. ↑ "Annular eclipse in the limelight". Detroit Free Press. Detroit, Michigan. 1995-04-30. p. 5. Retrieved 2023-10-18– via Newspapers.com.
  8. ↑ "Peruvians see unusual eclipse". The Boston Globe. Boston, Massachusetts. 1995-04-30. p. 17. Retrieved 2023-10-18– via Newspapers.com.
  9. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 10 August 2024.
  10. ↑ Paul D. Maley. "Ring Eclipse in the Amazon Rainforest". Eclipse Tours. Archived from the original on 18 September 2020.
  11. ↑ 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.
  12. ↑ "NASA - Catalog of Solar Eclipses of Saros 138". eclipse.gsfc.nasa.gov.

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