Solar eclipse of November 15, 2077

Last updated
Solar eclipse of November 15, 2077
SE2077Nov15A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.4705
Magnitude 0.9371
Maximum eclipse
Duration474 s (7 min 54 s)
Coordinates 7°48′N70°48′W / 7.8°N 70.8°W / 7.8; -70.8
Max. width of band262 km (163 mi)
Times (UTC)
Greatest eclipse17:07:56
References
Saros 134 (47 of 71)
Catalog # (SE5000) 9682

An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, November 15, 2077, [1] with a magnitude of 0.9371. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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 4 days after apogee (on November 11, 2077, at 17:20 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Oregon, southwestern Washington, northeastern California, Idaho, Nevada, Utah, Colorado, Arizona, New Mexico, Texas in the United States, the northeastern Yucatán Peninsula, the western tip of Cuba, Colombia, Venezuela, northern Brazil, Guyana, southern Suriname, and extreme southern French Guiana. A partial solar eclipse will also be visible for parts of North America, Central America, the Caribbean, South America, and West 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]

November 15, 2077 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2077 November 15 at 14:13:10.5 UTC
First Umbral External Contact2077 November 15 at 15:22:03.8 UTC
First Central Line2077 November 15 at 15:25:03.1 UTC
First Umbral Internal Contact2077 November 15 at 15:28:03.6 UTC
Equatorial Conjunction2077 November 15 at 16:47:52.0 UTC
Ecliptic Conjunction2077 November 15 at 17:02:23.8 UTC
Greatest Eclipse2077 November 15 at 17:07:56.2 UTC
Greatest Duration2077 November 15 at 17:21:02.7 UTC
Last Umbral Internal Contact2077 November 15 at 18:48:03.6 UTC
Last Central Line2077 November 15 at 18:51:01.7 UTC
Last Umbral External Contact2077 November 15 at 18:53:58.6 UTC
Last Penumbral External Contact2077 November 15 at 20:02:45.4 UTC
November 15, 2077 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.93707
Eclipse Obscuration0.87810
Gamma0.47047
Sun Right Ascension15h26m24.3s
Sun Declination-18°45'33.3"
Sun Semi-Diameter16'10.1"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension15h27m01.5s
Moon Declination-18°21'22.3"
Moon Semi-Diameter14'56.9"
Moon Equatorial Horizontal Parallax0°54'51.8"
ΔT103.7 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 2077
November 15
Descending node (new moon)
 November 29
Ascending node (full moon)
SE2077Nov15A.png
Annular solar eclipse
Solar Saros 134		 Partial lunar eclipse
Lunar Saros 146

Eclipses in 2077

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 134

Inex

Triad

Solar eclipses of 2076–2079

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 January 6, 2076 and July 1, 2076 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2076 to 2079
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 June 1, 2076
SE2076Jun01P.png
Partial		−1.3897124 November 26, 2076
SE2076Nov26P.png
Partial		1.1401
129 May 22, 2077
SE2077May22T.png
Total		−0.5725134 November 15, 2077
SE2077Nov15A.png
Annular		0.4705
139 May 11, 2078
SE2078May11T.png
Total		0.1838144 November 4, 2078
SE2078Nov04A.png
Annular		−0.2285
149 May 1, 2079
SE2079May01T.png
Total		0.9081154 October 24, 2079
SE2079Oct24A.png
Annular		−0.9243

Saros 134

This eclipse is a part of Saros series 134, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554; hybrid eclipses from January 3, 1573 through June 27, 1843; and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 72 as a partial eclipse on August 6, 2510. 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 11 at 1 minutes, 30 seconds on October 9, 1428, and the longest duration of annularity will be produced by member 52 at 10 minutes, 55 seconds on January 10, 2168. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 32–53 occur between 1801 and 2200:
323334
SE1807Jun06H.png
June 6, 1807		 SE1825Jun16H.png
June 16, 1825		 SE1843Jun27H.png
June 27, 1843
353637
SE1861Jul08A.png
July 8, 1861		 SE1879Jul19A.png
July 19, 1879		 SE1897Jul29A.png
July 29, 1897
383940
SE1915Aug10A.png
August 10, 1915 		SE1933Aug21A.png
August 21, 1933 		SE1951Sep01A.png
September 1, 1951
414243
SE1969Sep11A.png
September 11, 1969 		SE1987Sep23A.png
September 23, 1987 		SE2005Oct03A.png
October 3, 2005
444546
SE2023Oct14A.png
October 14, 2023 		SE2041Oct25A.png
October 25, 2041 		SE2059Nov05A.png
November 5, 2059
474849
SE2077Nov15A.png
November 15, 2077 		SE2095Nov27A.png
November 27, 2095 		SE2113Dec08A.png
December 8, 2113
505152
SE2131Dec19A.png
December 19, 2131		 SE2149Dec30A.png
December 30, 2149		 SE2168Jan10A.png
January 10, 2168
53
SE2186Jan20A.png
January 20, 2186

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 23, 2047 and November 16, 2134
June 22–23April 10–11January 27–29November 15–16September 3–5
118120122124126
SE2047Jun23P.png
June 23, 2047 		SE2051Apr11P.png
April 11, 2051 		SE2055Jan27P.png
January 27, 2055 		SE2058Nov16P.png
November 16, 2058 		SE2062Sep03P.png
September 3, 2062
128130132134136
SE2066Jun22A.png
June 22, 2066 		SE2070Apr11T.png
April 11, 2070 		SE2074Jan27A.png
January 27, 2074 		SE2077Nov15A.png
November 15, 2077 		SE2081Sep03T.png
September 3, 2081
138140142144146
SE2085Jun22A.png
June 22, 2085 		SE2089Apr10A.png
April 10, 2089 		SE2093Jan27T.png
January 27, 2093 		SE2096Nov15A.png
November 15, 2096 		SE2100Sep04T.png
September 4, 2100
148150152154156
SE2104Jun22T.png
June 22, 2104		 SE2108Apr11P.gif
April 11, 2108		 Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112		 SE2115Nov16A.png
November 16, 2115		 Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
158160162164
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123		 Saros164 03van80 SE2134Nov16P.jpg
November 16, 2134

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
SE1805Jan01P.gif
January 1, 1805
(Saros 109)		 SE1826Oct31P.gif
October 31, 1826
(Saros 111)		 SE1848Aug28P.gif
August 28, 1848
(Saros 113)
SE1859Jul29P.gif
July 29, 1859
(Saros 114)		 SE1870Jun28P.gif
June 28, 1870
(Saros 115)		 SE1881May27P.gif
May 27, 1881
(Saros 116)		 SE1892Apr26T.png
April 26, 1892
(Saros 117)		 SE1903Mar29A.png
March 29, 1903
(Saros 118)
SE1914Feb25A.png
February 25, 1914
(Saros 119)		 SE1925Jan24T.png
January 24, 1925
(Saros 120)		 SE1935Dec25A.png
December 25, 1935
(Saros 121)		 SE1946Nov23P.png
November 23, 1946
(Saros 122)		 SE1957Oct23T.png
October 23, 1957
(Saros 123)
SE1968Sep22T.png
September 22, 1968
(Saros 124)		 SE1979Aug22A.png
August 22, 1979
(Saros 125)		 SE1990Jul22T.png
July 22, 1990
(Saros 126)		 SE2001Jun21T.png
June 21, 2001
(Saros 127)		 SE2012May20A.png
May 20, 2012
(Saros 128)
SE2023Apr20H.png
April 20, 2023
(Saros 129)		 SE2034Mar20T.png
March 20, 2034
(Saros 130)		 SE2045Feb16A.png
February 16, 2045
(Saros 131)		 SE2056Jan16A.png
January 16, 2056
(Saros 132)		 SE2066Dec17T.png
December 17, 2066
(Saros 133)
SE2077Nov15A.png
November 15, 2077
(Saros 134)		 SE2088Oct14A.png
October 14, 2088
(Saros 135)		 SE2099Sep14T.png
September 14, 2099
(Saros 136)		 SE2110Aug15A.png
August 15, 2110
(Saros 137)		 SE2121Jul14A.png
July 14, 2121
(Saros 138)
SE2132Jun13T.png
June 13, 2132
(Saros 139)		 SE2143May14A.png
May 14, 2143
(Saros 140)		 SE2154Apr12A.png
April 12, 2154
(Saros 141)		 SE2165Mar12T.png
March 12, 2165
(Saros 142)		 SE2176Feb10A.png
February 10, 2176
(Saros 143)
SE2187Jan09A.png
January 9, 2187
(Saros 144)		 SE2197Dec09T.png
December 9, 2197
(Saros 145)

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
SE1817May16A.gif
May 16, 1817
(Saros 125)		 SE1846Apr25H.gif
April 25, 1846
(Saros 126)		 SE1875Apr06T.png
April 6, 1875
(Saros 127)
SE1904Mar17A.png
March 17, 1904
(Saros 128)		 SE1933Feb24A.png
February 24, 1933
(Saros 129)		 SE1962Feb05T.png
February 5, 1962
(Saros 130)
SE1991Jan15A.png
January 15, 1991
(Saros 131)		 SE2019Dec26A.png
December 26, 2019
(Saros 132)		 SE2048Dec05T.png
December 5, 2048
(Saros 133)
SE2077Nov15A.png
November 15, 2077
(Saros 134)		 SE2106Oct26A.png
October 26, 2106
(Saros 135)		 SE2135Oct07T.png
October 7, 2135
(Saros 136)
SE2164Sep16A.png
September 16, 2164
(Saros 137)		 SE2193Aug26A.png
August 26, 2193
(Saros 138)

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References

  1. ↑ "November 15, 2077 Annular Solar Eclipse". timeanddate. Retrieved 22 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 22 August 2024.
  3. ↑ "Annular Solar Eclipse of 2077 Nov 15". EclipseWise.com. Retrieved 22 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 134". eclipse.gsfc.nasa.gov.
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