Solar eclipse of August 24, 2063

Last updated
Solar eclipse of August 24, 2063
SE2063Aug24T.png
Map
Type of eclipse
NatureTotal
Gamma 0.2771
Magnitude 1.075
Maximum eclipse
Duration349 s (5 min 49 s)
Coordinates 25°36′N168°24′E / 25.6°N 168.4°E / 25.6; 168.4
Max. width of band252 km (157 mi)
Times (UTC)
Greatest eclipse1:22:11
References
Saros 136 (40 of 71)
Catalog # (SE5000) 9649

A total solar eclipse will occur at the Moon's descending node of orbit between Thursday, August 23 and Friday, August 24, 2063, [1] with a magnitude of 1.075. 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. Occurring about 2.5 hours before perigee (on August 24, 2063, at 3:50 UTC), the Moon's apparent diameter will be larger. [2] Perigee did occur near the very end of this eclipse.

Contents

The path of totality will be visible from parts of northern China, Mongolia, the northeastern tip of North Korea, southern Primorsky Krai of Russia, northern Japan, and parts of French Polynesia. A partial solar eclipse will also be visible for parts of East Asia, North Asia, Hawaii, and Oceania.

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]

August 24, 2063 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2063 August 23 at 22:47:34.7 UTC
First Umbral External Contact2063 August 23 at 23:42:04.1 UTC
First Central Line2063 August 23 at 23:43:38.1 UTC
First Umbral Internal Contact2063 August 23 at 23:45:12.3 UTC
First Penumbral Internal Contact2063 August 24 at 00:43:41.8 UTC
Equatorial Conjunction2063 August 24 at 01:08:02.8 UTC
Greatest Duration2063 August 24 at 01:17:30.5 UTC
Ecliptic Conjunction2063 August 24 at 01:19:21.7 UTC
Greatest Eclipse2063 August 24 at 01:22:10.6 UTC
Last Penumbral Internal Contact2063 August 24 at 02:00:58.2 UTC
Last Umbral Internal Contact2063 August 24 at 02:59:17.7 UTC
Last Central Line2063 August 24 at 03:00:51.8 UTC
Last Umbral External Contact2063 August 24 at 03:02:25.7 UTC
Last Penumbral External Contact2063 August 24 at 03:56:52.1 UTC
August 24, 2063 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.07497
Eclipse Obscuration1.15557
Gamma0.27715
Sun Right Ascension10h12m03.7s
Sun Declination+11°07'34.9"
Sun Semi-Diameter15'48.9"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension10h12m34.5s
Moon Declination+11°22'46.8"
Moon Semi-Diameter16'43.4"
Moon Equatorial Horizontal Parallax1°01'22.6"
ΔT92.9 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 August–September 2063
August 24
Descending node (new moon)
 September 7
Ascending node (full moon)
SE2063Aug24T.png
Total solar eclipse
Solar Saros 136		 Penumbral lunar eclipse
Lunar Saros 148

Eclipses in 2063

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 136

Inex

Triad

Solar eclipses of 2062–2065

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 July 3, 2065 and December 27, 2065 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2062 to 2065
Ascending node Descending node
SarosMapGammaSarosMapGamma
121 March 11, 2062
SE2062Mar11P.png
Partial		−1.0238126 September 3, 2062
SE2062Sep03P.png
Partial		1.0191
131 February 28, 2063
SE2063Feb28A.png
Annular		−0.336136 August 24, 2063
SE2063Aug24T.png
Total		0.2771
141 February 17, 2064
SE2064Feb17A.png
Annular		0.3597146 August 12, 2064
SE2064Aug12T.png
Total		−0.4652
151 February 5, 2065
SE2065Feb05P.png
Partial		1.0336156 August 2, 2065
SE2065Aug02P.png
Partial		−1.2759

Saros 136

This eclipse is a part of Saros series 136, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 14, 1360. It contains annular eclipses from September 8, 1504 through November 12, 1594; hybrid eclipses from November 22, 1612 through January 17, 1703; and total eclipses from January 27, 1721 through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622. 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 9 at 32 seconds on September 8, 1504, and the longest duration of totality was produced by member 34 at 7 minutes, 7.74 seconds on June 20, 1955. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 26–47 occur between 1801 and 2200:
262728
SE1811Mar24T.png
March 24, 1811		 SE1829Apr03T.png
April 3, 1829		 SE1847Apr15T.png
April 15, 1847
293031
SE1865Apr25T.gif
April 25, 1865 		SE1883May06T.png
May 6, 1883 		SE1901May18T.png
May 18, 1901
323334
SE1919May29T.png
May 29, 1919 		SE1937Jun08T.png
June 8, 1937 		SE1955Jun20T.png
June 20, 1955
353637
SE1973Jun30T.png
June 30, 1973 		SE1991Jul11T.png
July 11, 1991 		SE2009Jul22T.png
July 22, 2009
383940
SE2027Aug02T.png
August 2, 2027 		SE2045Aug12T.png
August 12, 2045 		SE2063Aug24T.png
August 24, 2063
414243
SE2081Sep03T.png
September 3, 2081 		SE2099Sep14T.png
September 14, 2099 		SE2117Sep26T.png
September 26, 2117
444546
SE2135Oct07T.png
October 7, 2135		 SE2153Oct17T.png
October 17, 2153		 SE2171Oct29T.png
October 29, 2171
47
SE2189Nov08T.png
November 8, 2189

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.

22 eclipse events between June 12, 2029 and November 4, 2116
June 11–12March 30–31January 16November 4–5August 23–24
118120122124126
SE2029Jun12P.png
June 12, 2029 		SE2033Mar30T.png
March 30, 2033 		SE2037Jan16P.png
January 16, 2037 		SE2040Nov04P.png
November 4, 2040 		SE2044Aug23T.png
August 23, 2044
128130132134136
SE2048Jun11A.png
June 11, 2048 		SE2052Mar30T.png
March 30, 2052 		SE2056Jan16A.png
January 16, 2056 		SE2059Nov05A.png
November 5, 2059 		SE2063Aug24T.png
August 24, 2063
138140142144146
SE2067Jun11A.png
June 11, 2067 		SE2071Mar31A.png
March 31, 2071 		SE2075Jan16T.png
January 16, 2075 		SE2078Nov04A.png
November 4, 2078 		SE2082Aug24T.png
August 24, 2082
148150152154156
SE2086Jun11T.png
June 11, 2086 		SE2090Mar31P.png
March 31, 2090 		SE2094Jan16T.png
January 16, 2094 		SE2097Nov04A.png
November 4, 2097 		Saros156 06van69 SE2101Aug24P.jpg
August 24, 2101
158160162164
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105		 Saros164 02van80 SE2116Nov04P.jpg
November 4, 2116

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
SE1801Sep08P.png
September 8, 1801
(Saros 112)		 SE1812Aug07P.gif
August 7, 1812
(Saros 113)		 SE1823Jul08P.gif
July 8, 1823
(Saros 114)		 SE1834Jun07P.gif
June 7, 1834
(Saros 115)		 SE1845May06An.gif
May 6, 1845
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)		 SE1867Mar06A.gif
March 6, 1867
(Saros 118)		 SE1878Feb02A.gif
February 2, 1878
(Saros 119)		 SE1889Jan01T.png
January 1, 1889
(Saros 120)		 SE1899Dec03A.png
December 3, 1899
(Saros 121)
SE1910Nov02P.png
November 2, 1910
(Saros 122)		 SE1921Oct01T.png
October 1, 1921
(Saros 123)		 SE1932Aug31T.png
August 31, 1932
(Saros 124)		 SE1943Aug01A.png
August 1, 1943
(Saros 125)		 SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1965May30T.png
May 30, 1965
(Saros 127)		 SE1976Apr29A.png
April 29, 1976
(Saros 128)		 SE1987Mar29H.png
March 29, 1987
(Saros 129)		 SE1998Feb26T.png
February 26, 1998
(Saros 130)		 SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2019Dec26A.png
December 26, 2019
(Saros 132)		 SE2030Nov25T.png
November 25, 2030
(Saros 133)		 SE2041Oct25A.png
October 25, 2041
(Saros 134)		 SE2052Sep22A.png
September 22, 2052
(Saros 135)		 SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2074Jul24A.png
July 24, 2074
(Saros 137)		 SE2085Jun22A.png
June 22, 2085
(Saros 138)		 SE2096May22T.png
May 22, 2096
(Saros 139)		 SE2107Apr23A.png
April 23, 2107
(Saros 140)		 SE2118Mar22A.png
March 22, 2118
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)		 SE2140Jan20A.png
January 20, 2140
(Saros 143)		 SE2150Dec19A.png
December 19, 2150
(Saros 144)		 SE2161Nov17T.png
November 17, 2161
(Saros 145)		 SE2172Oct17H.png
October 17, 2172
(Saros 146)
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)		 Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

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
SE1803Feb21T.png
February 21, 1803
(Saros 127)		 SE1832Feb01A.gif
February 1, 1832
(Saros 128)		 SE1861Jan11A.gif
January 11, 1861
(Saros 129)
SE1889Dec22T.png
December 22, 1889
(Saros 130)		 SE1918Dec03A.png
December 3, 1918
(Saros 131)		 SE1947Nov12A.png
November 12, 1947
(Saros 132)
SE1976Oct23T.png
October 23, 1976
(Saros 133)		 SE2005Oct03A.png
October 3, 2005
(Saros 134)		 SE2034Sep12A.png
September 12, 2034
(Saros 135)
SE2063Aug24T.png
August 24, 2063
(Saros 136)		 SE2092Aug03A.png
August 3, 2092
(Saros 137)		 SE2121Jul14A.png
July 14, 2121
(Saros 138)
SE2150Jun25T.png
June 25, 2150
(Saros 139)		 SE2179Jun05A.png
June 5, 2179
(Saros 140)

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References

  1. ↑ "August 23–24, 2063 Total Solar Eclipse". timeanddate. Retrieved 18 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 18 August 2024.
  3. ↑ "Total Solar Eclipse of 2063 Aug 24". EclipseWise.com. Retrieved 18 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 136". eclipse.gsfc.nasa.gov.
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