Solar eclipse of July 23, 2093

Last updated
Solar eclipse of July 23, 2093
SE2093Jul23A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.5717
Magnitude 0.9463
Maximum eclipse
Duration311 s (5 min 11 s)
Coordinates 54°36′N1°18′E / 54.6°N 1.3°E / 54.6; 1.3
Max. width of band241 km (150 mi)
Times (UTC)
Greatest eclipse12:32:04
References
Saros 147 (27 of 80)
Catalog # (SE5000) 9717

An annular solar eclipse will occur at the Moon's ascending node of orbit on Thursday, July 23, 2093, [1] with a magnitude of 0.9463. 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 1.1 days after apogee (on July 22, 2093, at 10:10 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Illinois, Indiana, Ohio, Michigan, Pennsylvania, New York, Vermont, New Hampshire, and Maine in the United States, southeastern Canada, Ireland, the United Kingdom, the Netherlands, Germany, the Czech Republic, Poland, Slovakia, Hungary, Ukraine, Romania, Moldova, Turkey, Iraq, Iran, Pakistan, and western India. A partial solar eclipse will also be visible for parts of eastern North America, the Caribbean, Europe, North Africa, Central Asia, North Asia, and South Asia.

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. [3]

July 23, 2093 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2093 July 23 at 09:39:24.9 UTC
First Umbral External Contact2093 July 23 at 10:52:14.3 UTC
First Central Line2093 July 23 at 10:55:00.8 UTC
First Umbral Internal Contact2093 July 23 at 10:57:48.8 UTC
Equatorial Conjunction2093 July 23 at 12:23:43.7 UTC
Greatest Duration2093 July 23 at 12:27:42.7 UTC
Greatest Eclipse2093 July 23 at 12:32:03.8 UTC
Ecliptic Conjunction2093 July 23 at 12:38:51.2 UTC
Last Umbral Internal Contact2093 July 23 at 14:06:25.3 UTC
Last Central Line2093 July 23 at 14:09:12.6 UTC
Last Umbral External Contact2093 July 23 at 14:11:58.3 UTC
Last Penumbral External Contact2093 July 23 at 15:24:45.2 UTC
July 23, 2093 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.94634
Eclipse Obscuration0.89557
Gamma0.57165
Sun Right Ascension08h14m45.4s
Sun Declination+19°49'29.6"
Sun Semi-Diameter15'44.6"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension08h15m01.4s
Moon Declination+20°20'03.3"
Moon Semi-Diameter14'43.0"
Moon Equatorial Horizontal Parallax0°54'00.8"
ΔT117.4 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 July 2093
July 8
Descending node (full moon)
July 23
Ascending node (new moon)
SE2093Jul23A.png
Partial lunar eclipse
Lunar Saros 121
Annular solar eclipse
Solar Saros 147

Eclipses in 2093

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 147

Inex

Triad

Solar eclipses of 2091–2094

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. [4]

The partial solar eclipses on June 13, 2094 and December 7, 2094 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2091 to 2094
Descending node Ascending node
SarosMapGammaSarosMapGamma
122 February 18, 2091
SE2091Feb18P.png
Partial
1.1779127 August 15, 2091
SE2091Aug15T.png
Total
−0.949
132 February 7, 2092
SE2092Feb07A.png
Annular
0.4322137 August 3, 2092
SE2092Aug03A.png
Annular
−0.2044
142 January 27, 2093
SE2093Jan27T.png
Total
−0.2737147 July 23, 2093
SE2093Jul23A.png
Annular
0.5717
152 January 16, 2094
SE2094Jan16T.png
Total
−0.9333157 July 12, 2094
SE2094Jul12P.png
Partial
1.3150

Saros 147

This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. 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 will be produced by member 38 at 9 minutes, 41 seconds on November 21, 2291. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 11–32 occur between 1801 and 2200:
111213
SE1805Jan30P.gif
January 30, 1805
SE1823Feb11P.gif
February 11, 1823
SE1841Feb21P.gif
February 21, 1841
141516
SE1859Mar04P.gif
March 4, 1859
SE1877Mar15P.gif
March 15, 1877
SE1895Mar26P.gif
March 26, 1895
171819
SE1913Apr06P.png
April 6, 1913
SE1931Apr18P.png
April 18, 1931
SE1949Apr28P.png
April 28, 1949
202122
SE1967May09P.png
May 9, 1967
SE1985May19P.png
May 19, 1985
SE2003May31A.png
May 31, 2003
232425
SE2021Jun10A.png
June 10, 2021
SE2039Jun21A.png
June 21, 2039
SE2057Jul01A.png
July 1, 2057
262728
SE2075Jul13A.png
July 13, 2075
SE2093Jul23A.png
July 23, 2093
SE2111Aug04A.png
August 4, 2111
293031
SE2129Aug15A.png
August 15, 2129
Saros147 30van80 SE2147Aug26A.jpg
August 26, 2147
Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
32
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183

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 ascending node.

21 eclipse events between July 23, 2036 and July 23, 2112
July 23–24May 11February 27–28December 16–17October 4–5
117119121123125
SE2036Jul23P.png
July 23, 2036
SE2040May11P.png
May 11, 2040
SE2044Feb28A.png
February 28, 2044
SE2047Dec16P.png
December 16, 2047
SE2051Oct04P.png
October 4, 2051
127129131133135
SE2055Jul24T.png
July 24, 2055
SE2059May11T.png
May 11, 2059
SE2063Feb28A.png
February 28, 2063
SE2066Dec17T.png
December 17, 2066
SE2070Oct04A.png
October 4, 2070
137139141143145
SE2074Jul24A.png
July 24, 2074
SE2078May11T.png
May 11, 2078
SE2082Feb27A.png
February 27, 2082
SE2085Dec16A.png
December 16, 2085
SE2089Oct04T.png
October 4, 2089
147149151153155
SE2093Jul23A.png
July 23, 2093
SE2097May11T.png
May 11, 2097
SE2101Feb28A.png
February 28, 2101
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108
157
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112

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
SE1804Feb11H.png
February 11, 1804
(Saros 137)
SE1833Jan20A.gif
January 20, 1833
(Saros 138)
SE1861Dec31T.gif
December 31, 1861
(Saros 139)
SE1890Dec12H.gif
December 12, 1890
(Saros 140)
SE1919Nov22A.png
November 22, 1919
(Saros 141)
SE1948Nov01T.png
November 1, 1948
(Saros 142)
SE1977Oct12T.png
October 12, 1977
(Saros 143)
SE2006Sep22A.png
September 22, 2006
(Saros 144)
SE2035Sep02T.png
September 2, 2035
(Saros 145)
SE2064Aug12T.png
August 12, 2064
(Saros 146)
SE2093Jul23A.png
July 23, 2093
(Saros 147)
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
(Saros 148)
Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
(Saros 149)
Saros150 26van71 SE2180May24A.jpg
May 24, 2180
(Saros 150)

Notes

  1. "July 23, 2093 Annular Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. "Annular Solar Eclipse of 2093 Jul 23". EclipseWise.com. Retrieved 24 August 2024.
  4. 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.
  5. "NASA - Catalog of Solar Eclipses of Saros 147". eclipse.gsfc.nasa.gov.

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References