Solar eclipse of December 6, 2067

Last updated
Solar eclipse of December 6, 2067
SE2067Dec06H.png
Map
Type of eclipse
NatureHybrid
Gamma 0.2845
Magnitude 1.0011
Maximum eclipse
Duration8 s (0 min 8 s)
Coordinates 6°00′S32°24′W / 6°S 32.4°W / -6; -32.4
Max. width of band4 km (2.5 mi)
Times (UTC)
Greatest eclipse14:03:43
References
Saros 143 (26 of 72)
Catalog # (SE5000) 9659

A total solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, December 6, 2067, [1] with a magnitude of 1.0011. It is a hybrid event, beginning and ending as an annular eclipse. 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 3.4 days before perigee (on December 10, 2067, at 0:40 UTC), the Moon's apparent diameter will be larger. [2]

Contents

The path of the eclipse will be visible as an annular eclipse from parts of southeastern Mexico, Guatemala, southern Belize, Honduras, Nicaragua, Colombia, Venezuela, Brazil, and Guyana before transitioning to a total eclipse. Totality will be visible from parts of Brazil before the eclipse transforms back to an annular eclipse, then passing over Nigeria, Cameroon, Chad, and Sudan. A partial solar eclipse will also be visible for parts of eastern North America, Central America, the Caribbean, northern and central South America, southern Europe, and Africa.

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]

December 6, 2067 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2067 December 06 at 11:18:45.6 UTC
First Umbral External Contact2067 December 06 at 12:19:30.5 UTC
First Central Line2067 December 06 at 12:20:00.2 UTC
Greatest Duration2067 December 06 at 12:20:00.2 UTC
First Umbral Internal Contact2067 December 06 at 12:20:29.9 UTC
First Penumbral Internal Contact2067 December 06 at 13:26:13.3 UTC
Equatorial Conjunction2067 December 06 at 14:03:13.4 UTC
Greatest Eclipse2067 December 06 at 14:03:43.3 UTC
Ecliptic Conjunction2067 December 06 at 14:06:46.9 UTC
Last Penumbral Internal Contact2067 December 06 at 14:41:15.1 UTC
Last Umbral Internal Contact2067 December 06 at 15:46:59.0 UTC
Last Central Line2067 December 06 at 15:47:26.0 UTC
Last Umbral External Contact2067 December 06 at 15:47:53.0 UTC
Last Penumbral External Contact2067 December 06 at 16:48:35.3 UTC
December 6, 2067 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.00113
Eclipse Obscuration1.00226
Gamma0.28446
Sun Right Ascension16h52m45.8s
Sun Declination-22°31'49.1"
Sun Semi-Diameter16'13.8"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension16h52m46.9s
Moon Declination-22°15'09.9"
Moon Semi-Diameter15'59.7"
Moon Equatorial Horizontal Parallax0°58'42.2"
ΔT96.0 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 2067
November 21
Descending node (full moon)
 December 6
Ascending node (new moon)
Lunar eclipse chart close-2067Nov21.png SE2067Dec06H.png
Penumbral lunar eclipse
Lunar Saros 117		 Hybrid solar eclipse
Solar Saros 143

Eclipses in 2067

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 143

Inex

Triad

Solar eclipses of 2065–2069

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 February 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2065 to 2069
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 July 3, 2065
SE2065Jul03P.png
Partial		1.4619123 December 27, 2065
SE2065Dec27P.png
Partial		−1.0688
128 June 22, 2066
SE2066Jun22A.png
Annular		0.733133 December 17, 2066
SE2066Dec17T.png
Total		−0.4043
138 June 11, 2067
SE2067Jun11A.png
Annular		−0.0387143 December 6, 2067
SE2067Dec06H.png
Hybrid		0.2845
148 May 31, 2068
SE2068May31T.png
Total		−0.797153 November 24, 2068
SE2068Nov24P.png
Partial		1.0299
158 May 20, 2069
SE2069May20P.png
Partial		−1.4852

Saros 143

This eclipse is a part of Saros series 143, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 7, 1617. It contains total eclipses from June 24, 1797 through October 24, 1995; hybrid eclipses from November 3, 2013 through December 6, 2067; and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2897. 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 16 at 3 minutes, 50 seconds on August 19, 1887, and the longest duration of annularity will be produced by member 51 at 4 minutes, 54 seconds on September 6, 2518. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 12–33 occur between 1801 and 2200:
121314
SE1815Jul06T.png
July 6, 1815		 SE1833Jul17T.png
July 17, 1833		 SE1851Jul28T.png
July 28, 1851
151617
SE1869Aug07T.png
August 7, 1869 		SE1887Aug19T.png
August 19, 1887 		SE1905Aug30T.png
August 30, 1905
181920
SE1923Sep10T.png
September 10, 1923 		SE1941Sep21T.png
September 21, 1941 		SE1959Oct02T.png
October 2, 1959
212223
SE1977Oct12T.png
October 12, 1977 		SE1995Oct24T.png
October 24, 1995 		SE2013Nov03H.png
November 3, 2013
242526
SE2031Nov14H.png
November 14, 2031 		SE2049Nov25H.png
November 25, 2049 		SE2067Dec06H.png
December 6, 2067
272829
SE2085Dec16A.png
December 16, 2085 		SE2103Dec29A.png
December 29, 2103		 SE2122Jan08A.png
January 8, 2122
303132
SE2140Jan20A.png
January 20, 2140		 SE2158Jan30A.png
January 30, 2158		 SE2176Feb10A.png
February 10, 2176
33
SE2194Feb21A.png
February 21, 2194

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
SE1805Dec21A.gif
December 21, 1805
(Saros 119)		 SE1816Nov19T.gif
November 19, 1816
(Saros 120)		 SE1827Oct20H.gif
October 20, 1827
(Saros 121)		 SE1838Sep18A.gif
September 18, 1838
(Saros 122)		 SE1849Aug18T.gif
August 18, 1849
(Saros 123)
SE1860Jul18T.gif
July 18, 1860
(Saros 124)		 SE1871Jun18A.gif
June 18, 1871
(Saros 125)		 SE1882May17T.png
May 17, 1882
(Saros 126)		 SE1893Apr16T.png
April 16, 1893
(Saros 127)		 SE1904Mar17A.png
March 17, 1904
(Saros 128)
SE1915Feb14A.png
February 14, 1915
(Saros 129)		 SE1926Jan14T.png
January 14, 1926
(Saros 130)		 SE1936Dec13A.png
December 13, 1936
(Saros 131)		 SE1947Nov12A.png
November 12, 1947
(Saros 132)		 SE1958Oct12T.png
October 12, 1958
(Saros 133)
SE1969Sep11A.png
September 11, 1969
(Saros 134)		 SE1980Aug10A.png
August 10, 1980
(Saros 135)		 SE1991Jul11T.png
July 11, 1991
(Saros 136)		 SE2002Jun10A.png
June 10, 2002
(Saros 137)		 SE2013May10A.png
May 10, 2013
(Saros 138)
SE2024Apr08T.png
April 8, 2024
(Saros 139)		 SE2035Mar09A.png
March 9, 2035
(Saros 140)		 SE2046Feb05A.png
February 5, 2046
(Saros 141)		 SE2057Jan05T.png
January 5, 2057
(Saros 142)		 SE2067Dec06H.png
December 6, 2067
(Saros 143)
SE2078Nov04A.png
November 4, 2078
(Saros 144)		 SE2089Oct04T.png
October 4, 2089
(Saros 145)		 SE2100Sep04T.png
September 4, 2100
(Saros 146)		 SE2111Aug04A.png
August 4, 2111
(Saros 147)		 Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
(Saros 148)
SE2133Jun03T.png
June 3, 2133
(Saros 149)		 Saros150 24van71 SE2144May03A.jpg
May 3, 2144
(Saros 150)		 SE2155Apr02A.png
April 2, 2155
(Saros 151)		 Saros152 21van70 SE2166Mar02T.jpg
March 2, 2166
(Saros 152)		 Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
(Saros 153)
Saros154 16van71 SE2187Dec29A.jpg
December 29, 2187
(Saros 154)		 SE2198Nov28T.png
November 28, 2198
(Saros 155)

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
SE1807Jun06H.gif
June 6, 1807
(Saros 134)		 SE1836May15A.gif
May 15, 1836
(Saros 135)		 SE1865Apr25T.png
April 25, 1865
(Saros 136)
SE1894Apr06H.gif
April 6, 1894
(Saros 137)		 SE1923Mar17A.png
March 17, 1923
(Saros 138)		 SE1952Feb25T.png
February 25, 1952
(Saros 139)
SE1981Feb04A.png
February 4, 1981
(Saros 140)		 SE2010Jan15A.png
January 15, 2010
(Saros 141)		 SE2038Dec26T.png
December 26, 2038
(Saros 142)
SE2067Dec06H.png
December 6, 2067
(Saros 143)		 SE2096Nov15A.png
November 15, 2096
(Saros 144)		 SE2125Oct26T.png
October 26, 2125
(Saros 145)
SE2154Oct07T.png
October 7, 2154
(Saros 146)		 Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)

Notes

  1. ↑ "December 6, 2067 Total Solar Eclipse". timeanddate. Retrieved 19 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 19 August 2024.
  3. ↑ "Hybrid Solar Eclipse of 2067 Dec 06". EclipseWise.com. Retrieved 19 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 143". eclipse.gsfc.nasa.gov.

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References

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