Solar eclipse of May 21, 1993

Last updated
Solar eclipse of May 21, 1993
SE1993May21P.png
Map
Type of eclipse
NaturePartial
Gamma 1.1372
Magnitude 0.7352
Maximum eclipse
Coordinates 68°48′N162°18′E / 68.8°N 162.3°E / 68.8; 162.3
Times (UTC)
Greatest eclipse14:20:15
References
Saros 118 (67 of 72)
Catalog # (SE5000) 9493

A partial solar eclipse occurred at the Moon's descending node of orbit on Friday, May 21, 1993, [1] with a magnitude of 0.7352. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

A partial eclipse was visible for parts of Alaska, Canada, Greenland, the United States, and Northern Europe.

Images

SE1993May21P.gif

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse. [2]

May 21, 1993 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1993 May 21 at 12:19:45.7 UTC
Ecliptic Conjunction1993 May 21 at 14:07:30.6 UTC
Greatest Eclipse1993 May 21 at 14:20:14.6 UTC
Equatorial Conjunction1993 May 21 at 14:34:45.0 UTC
Last Penumbral External Contact1993 May 21 at 16:20:31.6 UTC
May 21, 1993 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.73519
Eclipse Obscuration0.65896
Gamma1.13720
Sun Right Ascension03h53m29.8s
Sun Declination+20°15'44.4"
Sun Semi-Diameter15'48.0"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension03h52m59.3s
Moon Declination+21°18'54.5"
Moon Semi-Diameter15'16.2"
Moon Equatorial Horizontal Parallax0°56'02.5"
ΔT59.4 s

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 May–June 1993
May 21
Descending node (new moon)
June 4
Ascending node (full moon)
SE1993May21P.png Lunar eclipse chart close-1993Jun04.png
Partial solar eclipse
Solar Saros 118
Total lunar eclipse
Lunar Saros 130

Eclipses in 1993

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 118

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. [3]

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 118

This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 totality was produced by member 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

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 May 21, 1993 and May 20, 2069
May 20–21March 9December 25–26October 13–14August 1–2
118120122124126
SE1993May21P.png
May 21, 1993
SE1997Mar09T.png
March 9, 1997
SE2000Dec25P.png
December 25, 2000
SE2004Oct14P.png
October 14, 2004
SE2008Aug01T.png
August 1, 2008
128130132134136
SE2012May20A.png
May 20, 2012
SE2016Mar09T.png
March 9, 2016
SE2019Dec26A.png
December 26, 2019
SE2023Oct14A.png
October 14, 2023
SE2027Aug02T.png
August 2, 2027
138140142144146
SE2031May21A.png
May 21, 2031
SE2035Mar09A.png
March 9, 2035
SE2038Dec26T.png
December 26, 2038
SE2042Oct14A.png
October 14, 2042
SE2046Aug02T.png
August 2, 2046
148150152154156
SE2050May20H.png
May 20, 2050
SE2054Mar09P.png
March 9, 2054
SE2057Dec26T.png
December 26, 2057
SE2061Oct13A.png
October 13, 2061
SE2065Aug02P.png
August 2, 2065
158
SE2069May20P.png
May 20, 2069

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.

The partial solar eclipses on March 27, 1884 (part of Saros 108) and December 24, 1916 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 1971 and 2200
SE1971Jul22P.png
July 22, 1971
(Saros 116)
SE1982Jun21P.png
June 21, 1982
(Saros 117)
SE1993May21P.png
May 21, 1993
(Saros 118)
SE2004Apr19P.png
April 19, 2004
(Saros 119)
SE2015Mar20T.png
March 20, 2015
(Saros 120)
SE2026Feb17A.png
February 17, 2026
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2047Dec16P.png
December 16, 2047
(Saros 123)
SE2058Nov16P.png
November 16, 2058
(Saros 124)
SE2069Oct15P.png
October 15, 2069
(Saros 125)
SE2080Sep13P.png
September 13, 2080
(Saros 126)
SE2091Aug15T.png
August 15, 2091
(Saros 127)
SE2102Jul15A.png
July 15, 2102
(Saros 128)
SE2113Jun13T.png
June 13, 2113
(Saros 129)
SE2124May14T.png
May 14, 2124
(Saros 130)
SE2135Apr13A.png
April 13, 2135
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2157Feb09T.png
February 9, 2157
(Saros 133)
SE2168Jan10A.png
January 10, 2168
(Saros 134)
SE2178Dec09A.png
December 9, 2178
(Saros 135)
SE2189Nov08T.png
November 8, 2189
(Saros 136)
SE2200Oct09A.png
October 9, 2200
(Saros 137)

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
SE1819Sep19Pe.gif
September 19, 1819
(Saros 112)
SE1848Aug28P.gif
August 28, 1848
(Saros 113)
SE1877Aug09P.gif
August 9, 1877
(Saros 114)
SE1906Jul21P.png
July 21, 1906
(Saros 115)
SE1935Jun30P.png
June 30, 1935
(Saros 116)
SE1964Jun10P.png
June 10, 1964
(Saros 117)
SE1993May21P.png
May 21, 1993
(Saros 118)
SE2022Apr30P.png
April 30, 2022
(Saros 119)
SE2051Apr11P.png
April 11, 2051
(Saros 120)
SE2080Mar21P.png
March 21, 2080
(Saros 121)
Saros122 63van70 SE2109Mar01P.jpg
March 1, 2109
(Saros 122)
Saros123 60van70 SE2138Feb09P.jpg
February 9, 2138
(Saros 123)
Saros124 63van73 SE2167Jan21P.jpg
January 21, 2167
(Saros 124)
Saros125 64van73 SE2195Dec31P.jpg
December 31, 2195
(Saros 125)

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References

  1. "May 21, 1993 Partial Solar Eclipse". timeanddate. Retrieved 10 August 2024.
  2. "Partial Solar Eclipse of 1993 May 21". EclipseWise.com. Retrieved 10 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 118". eclipse.gsfc.nasa.gov.