Solar eclipse of August 13, 2083

Last updated
Solar eclipse of August 13, 2083
Partial eclipse
SE2083Aug13P.png
Map
Gamma −1.2064
Magnitude 0.6146
Maximum eclipse
Coordinates 62°06′S67°30′W / 62.1°S 67.5°W / -62.1; -67.5
Times (UTC)
Greatest eclipse12:34:41
References
Saros 156 (5 of 69)
Catalog # (SE5000) 9694

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, August 13, 2083, [1] with a magnitude of 0.6146. 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

The partial solar eclipse will be visible for parts of southern and central South America and Antarctica.

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]

August 13, 2083 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2083 August 13 at 10:45:02.9 UTC
Greatest Eclipse2083 August 13 at 12:34:41.2 UTC
Ecliptic Conjunction2083 August 13 at 12:47:43.2 UTC
Equatorial Conjunction2083 August 13 at 13:35:18.6 UTC
Last Penumbral External Contact2083 August 13 at 14:23:49.7 UTC
August 13, 2083 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.61464
Eclipse Obscuration0.51798
Gamma−1.20640
Sun Right Ascension09h33m34.6s
Sun Declination+14°29'20.4"
Sun Semi-Diameter15'47.0"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension09h31m40.1s
Moon Declination+13°27'06.6"
Moon Semi-Diameter15'25.9"
Moon Equatorial Horizontal Parallax0°56'37.9"
ΔT108.5 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of July–August 2083
July 15
Descending node (new moon)
July 29
Ascending node (full moon)
August 13
Descending node (new moon)
SE2083Jul15P.png Lunar eclipse chart close-2083Jul29.png SE2083Aug13P.png
Partial solar eclipse
Solar Saros 118
Total lunar eclipse
Lunar Saros 130
Partial solar eclipse
Solar Saros 156

Eclipses in 2083

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 156

Inex

Triad

Solar eclipses 2080–2083

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]

The partial solar eclipse on July 15, 2083 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 2080 to 2083
Ascending node Descending node
SarosMapGammaSarosMapGamma
121 March 21, 2080
SE2080Mar21P.png
Partial
−1.0578126 September 13, 2080
SE2080Sep13P.png
Partial
1.0723
131 March 10, 2081
SE2081Mar10A.png
Annular
−0.3653136 September 3, 2081
SE2081Sep03T.png
Total
0.3378
141 February 27, 2082
SE2082Feb27A.png
Annular
0.3361146 August 24, 2082
SE2082Aug24T.png
Total
−0.4004
151 February 16, 2083
SE2083Feb16P.png
Partial
1.017156 August 13, 2083
SE2083Aug13P.png
Partial
−1.2064

Saros 156

This eclipse is a part of Saros series 156, repeating every 18 years, 11 days, and containing 69 events. The series started with a partial solar eclipse on July 1, 2011. It contains annular eclipses from September 26, 2155 through April 7, 3075. There are no hybrid or total eclipses in this set. The series ends at member 69 as a partial eclipse on July 14, 3237. 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 29 at 8 minutes, 28 seconds on May 3, 2516. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 1–11 occur between 2011 and 2200:
123
SE2011Jul01P.png
July 1, 2011
SE2029Jul11P.png
July 11, 2029
SE2047Jul22P.png
July 22, 2047
456
SE2065Aug02P.png
August 2, 2065
SE2083Aug13P.png
August 13, 2083
Saros156 06van69 SE2101Aug24P.jpg
August 24, 2101
789
Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
Saros156 09van69 SE2155Sep26A.jpg
September 26, 2155
1011
Saros156 10van69 SE2173Oct07A.jpg
October 7, 2173
Saros156 11van69 SE2191Oct18A.jpg
October 18, 2191

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 1, 2011 and October 24, 2098
May 31–June 1March 19–20January 5–6October 24–25August 12–13
118120122124126
SE2011Jun01P.png
June 1, 2011
SE2015Mar20T.png
March 20, 2015
SE2019Jan06P.png
January 6, 2019
SE2022Oct25P.png
October 25, 2022
SE2026Aug12T.png
August 12, 2026
128130132134136
SE2030Jun01A.png
June 1, 2030
SE2034Mar20T.png
March 20, 2034
SE2038Jan05A.png
January 5, 2038
SE2041Oct25A.png
October 25, 2041
SE2045Aug12T.png
August 12, 2045
138140142144146
SE2049May31A.png
May 31, 2049
SE2053Mar20A.png
March 20, 2053
SE2057Jan05T.png
January 5, 2057
SE2060Oct24A.png
October 24, 2060
SE2064Aug12T.png
August 12, 2064
148150152154156
SE2068May31T.png
May 31, 2068
SE2072Mar19P.png
March 19, 2072
SE2076Jan06T.png
January 6, 2076
SE2079Oct24A.png
October 24, 2079
SE2083Aug13P.png
August 13, 2083
158160162164
SE2087Jun01P.png
June 1, 2087
SE2098Oct24P.png
October 24, 2098

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 December 7, 2170 (part of Saros 164) and November 7, 2181 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2105
SE1810Sep28A.gif
September 28, 1810
(Saros 131)
SE1821Aug27A.gif
August 27, 1821
(Saros 132)
SE1832Jul27T.gif
July 27, 1832
(Saros 133)
SE1843Jun27H.gif
June 27, 1843
(Saros 134)
SE1854May26A.png
May 26, 1854
(Saros 135)
SE1865Apr25T.png
April 25, 1865
(Saros 136)
SE1876Mar25A.gif
March 25, 1876
(Saros 137)
SE1887Feb22A.png
February 22, 1887
(Saros 138)
SE1898Jan22T.png
January 22, 1898
(Saros 139)
SE1908Dec23H.png
December 23, 1908
(Saros 140)
SE1919Nov22A.png
November 22, 1919
(Saros 141)
SE1930Oct21T.png
October 21, 1930
(Saros 142)
SE1941Sep21T.png
September 21, 1941
(Saros 143)
SE1952Aug20A.png
August 20, 1952
(Saros 144)
SE1963Jul20T.png
July 20, 1963
(Saros 145)
SE1974Jun20T.png
June 20, 1974
(Saros 146)
SE1985May19P.png
May 19, 1985
(Saros 147)
SE1996Apr17P.png
April 17, 1996
(Saros 148)
SE2007Mar19P.png
March 19, 2007
(Saros 149)
SE2018Feb15P.png
February 15, 2018
(Saros 150)
SE2029Jan14P.png
January 14, 2029
(Saros 151)
SE2039Dec15T.png
December 15, 2039
(Saros 152)
SE2050Nov14P.png
November 14, 2050
(Saros 153)
SE2061Oct13A.png
October 13, 2061
(Saros 154)
SE2072Sep12T.png
September 12, 2072
(Saros 155)
SE2083Aug13P.png
August 13, 2083
(Saros 156)
SE2094Jul12P.png
July 12, 2094
(Saros 157)
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105
(Saros 158)

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
SE1823Feb11P.gif
February 11, 1823
(Saros 147)
SE1852Jan21P.png
January 21, 1852
(Saros 148)
SE1880Dec31P.gif
December 31, 1880
(Saros 149)
SE1909Dec12P.png
December 12, 1909
(Saros 150)
SE1938Nov21P.png
November 21, 1938
(Saros 151)
SE1967Nov02T.png
November 2, 1967
(Saros 152)
SE1996Oct12P.png
October 12, 1996
(Saros 153)
SE2025Sep21P.png
September 21, 2025
(Saros 154)
SE2054Sep02P.png
September 2, 2054
(Saros 155)
SE2083Aug13P.png
August 13, 2083
(Saros 156)
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112
(Saros 157)
Saros158 05van70 SE2141Jul03P.jpg
July 3, 2141
(Saros 158)
Saros159 03van70 SE2170Jun14P.jpg
June 14, 2170
(Saros 159)
Saros160 02van71 SE2199May24P.jpg
May 24, 2199
(Saros 160)

References

  1. "August 13, 2083 Partial Solar Eclipse". timeanddate. Retrieved 23 August 2024.
  2. "Partial Solar Eclipse of 2083 Aug 13". EclipseWise.com. Retrieved 23 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 156". eclipse.gsfc.nasa.gov.