Solar eclipse of December 6, 2086

Last updated
Solar eclipse of December 6, 2086
SE2086Dec06P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0194
Magnitude 0.9271
Maximum eclipse
Coordinates 67°24′N96°12′E / 67.4°N 96.2°E / 67.4; 96.2
Times (UTC)
Greatest eclipse5:38:55
References
Saros 153 (13 of 70)
Catalog # (SE5000) 9702

A partial solar eclipse will occur at the Moon's ascending node of orbit on Friday, December 6, 2086, [1] with a magnitude of 0.9271. 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 much of 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. [2]

December 6, 2086 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2086 December 06 at 03:21:35.8 UTC
Equatorial Conjunction2086 December 06 at 05:36:56.3 UTC
Greatest Eclipse2086 December 06 at 05:38:55.4 UTC
Ecliptic Conjunction2086 December 06 at 05:50:30.7 UTC
Last Penumbral External Contact2086 December 06 at 07:56:10.8 UTC
December 6, 2086 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.92711
Eclipse Obscuration0.86398
Gamma1.01940
Sun Right Ascension16h52m56.6s
Sun Declination-22°31'57.0"
Sun Semi-Diameter16'13.7"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension16h53m00.7s
Moon Declination-21°35'36.6"
Moon Semi-Diameter15'06.1"
Moon Equatorial Horizontal Parallax0°55'25.4"
ΔT111.4 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 November–December 2086
November 20
Descending node (full moon)
December 6
Ascending node (new moon)
SE2086Dec06P.png
Partial lunar eclipse
Lunar Saros 127
Partial solar eclipse
Solar Saros 153

Eclipses in 2086

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 153

Inex

Triad

Solar eclipses of 2083–2087

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 eclipses on February 16, 2083 and August 13, 2083 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 2, 2087 and October 26, 2087 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2083 to 2087
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 July 15, 2083
SE2083Jul15P.png
Partial
1.5465123 January 7, 2084
SE2084Jan07P.png
Partial
−1.0715
128 July 3, 2084
SE2084Jul03A.png
Annular
0.8208133 December 27, 2084
SE2084Dec27T.png
Total
−0.4094
138 June 22, 2085
SE2085Jun22A.png
Annular
0.0452143 December 16, 2085
SE2085Dec16A.png
Annular
0.2786
148 June 11, 2086
SE2086Jun11T.png
Total
−0.7215153 December 6, 2086
SE2086Dec06P.png
Partial
1.0194
158 June 1, 2087
SE2087Jun01P.png
Partial
−1.4186

Saros 153

This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–19 occur between 1870 and 2200:
123
SE1870Jul28Pb.gif
July 28, 1870
SE1888Aug07P.gif
August 7, 1888
SE1906Aug20P.png
August 20, 1906
456
SE1924Aug30P.png
August 30, 1924
SE1942Sep10P.png
September 10, 1942
SE1960Sep20P.png
September 20, 1960
789
SE1978Oct02P.png
October 2, 1978
SE1996Oct12P.png
October 12, 1996
SE2014Oct23P.png
October 23, 2014
101112
SE2032Nov03P.png
November 3, 2032
SE2050Nov14P.png
November 14, 2050
SE2068Nov24P.png
November 24, 2068
131415
SE2086Dec06P.png
December 6, 2086
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
161718
Saros153 16van70 SE2141Jan08A.jpg
January 8, 2141
Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
19
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195

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 13, 2018 and July 12, 2094
July 12–13April 30–May 1February 16–17December 5–6September 22–23
117119121123125
SE2018Jul13P.png
July 13, 2018
SE2022Apr30P.png
April 30, 2022
SE2026Feb17A.png
February 17, 2026
SE2029Dec05P.png
December 5, 2029
SE2033Sep23P.png
September 23, 2033
127129131133135
SE2037Jul13T.png
July 13, 2037
SE2041Apr30T.png
April 30, 2041
SE2045Feb16A.png
February 16, 2045
SE2048Dec05T.png
December 5, 2048
SE2052Sep22A.png
September 22, 2052
137139141143145
SE2056Jul12A.png
July 12, 2056
SE2060Apr30T.png
April 30, 2060
SE2064Feb17A.png
February 17, 2064
SE2067Dec06H.png
December 6, 2067
SE2071Sep23T.png
September 23, 2071
147149151153155
SE2075Jul13A.png
July 13, 2075
SE2079May01T.png
May 1, 2079
SE2083Feb16P.png
February 16, 2083
SE2086Dec06P.png
December 6, 2086
SE2090Sep23T.png
September 23, 2090
157
SE2094Jul12P.png
July 12, 2094

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
SE1803Feb21T.png
February 21, 1803
(Saros 127)
SE1814Jan21A.gif
January 21, 1814
(Saros 128)
SE1824Dec20Am.gif
December 20, 1824
(Saros 129)
SE1835Nov20T.png
November 20, 1835
(Saros 130)
SE1846Oct20A.png
October 20, 1846
(Saros 131)
SE1857Sep18A.png
September 18, 1857
(Saros 132)
SE1868Aug18T.png
August 18, 1868
(Saros 133)
SE1879Jul19A.png
July 19, 1879
(Saros 134)
SE1890Jun17A.png
June 17, 1890
(Saros 135)
SE1901May18T.png
May 18, 1901
(Saros 136)
SE1912Apr17H.png
April 17, 1912
(Saros 137)
SE1923Mar17A.png
March 17, 1923
(Saros 138)
SE1934Feb14T.png
February 14, 1934
(Saros 139)
SE1945Jan14A.png
January 14, 1945
(Saros 140)
SE1955Dec14A.png
December 14, 1955
(Saros 141)
SE1966Nov12T.png
November 12, 1966
(Saros 142)
SE1977Oct12T.png
October 12, 1977
(Saros 143)
SE1988Sep11A.png
September 11, 1988
(Saros 144)
SE1999Aug11T.png
August 11, 1999
(Saros 145)
SE2010Jul11T.png
July 11, 2010
(Saros 146)
SE2021Jun10A.png
June 10, 2021
(Saros 147)
SE2032May09A.png
May 9, 2032
(Saros 148)
SE2043Apr09T.png
April 9, 2043
(Saros 149)
SE2054Mar09P.png
March 9, 2054
(Saros 150)
SE2065Feb05P.png
February 5, 2065
(Saros 151)
SE2076Jan06T.png
January 6, 2076
(Saros 152)
SE2086Dec06P.png
December 6, 2086
(Saros 153)
SE2097Nov04A.png
November 4, 2097
(Saros 154)
Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108
(Saros 155)
Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
(Saros 156)
Saros157 05van70 SE2130Aug04P.jpg
August 4, 2130
(Saros 157)
Saros158 05van70 SE2141Jul03P.jpg
July 3, 2141
(Saros 158)
Saros159 02van70 SE2152Jun03P.jpg
June 3, 2152
(Saros 159)
Saros161 01van72 SE2174Apr01P.jpg
April 1, 2174
(Saros 161)

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
SE1826Jun05P.gif
June 5, 1826
(Saros 144)
SE1855May16P.gif
May 16, 1855
(Saros 145)
SE1884Apr25P.gif
April 25, 1884
(Saros 146)
SE1913Apr06P.png
April 6, 1913
(Saros 147)
SE1942Mar16P.png
March 16, 1942
(Saros 148)
SE1971Feb25P.png
February 25, 1971
(Saros 149)
SE2000Feb05P.png
February 5, 2000
(Saros 150)
SE2029Jan14P.png
January 14, 2029
(Saros 151)
SE2057Dec26T.png
December 26, 2057
(Saros 152)
SE2086Dec06P.png
December 6, 2086
(Saros 153)
Saros154 12van71 SE2115Nov16A.jpg
November 16, 2115
(Saros 154)
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
(Saros 155)
Saros156 10van69 SE2173Oct07A.jpg
October 7, 2173
(Saros 156)

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References

  1. "December 6, 2086 Partial Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. "Partial Solar Eclipse of 2086 Dec 06". EclipseWise.com. Retrieved 24 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 153". eclipse.gsfc.nasa.gov.