Solar eclipse of November 4, 2078

Last updated
Solar eclipse of November 4, 2078
SE2078Nov04A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.2285
Magnitude 0.9255
Maximum eclipse
Duration509 s (8 min 29 s)
Coordinates 27°48′S83°18′W / 27.8°S 83.3°W / -27.8; -83.3
Max. width of band287 km (178 mi)
Times (UTC)
Greatest eclipse16:55:44
References
Saros 144 (20 of 70)
Catalog # (SE5000) 9684

An annular solar eclipse will occur at the Moon's descending node of orbit on Friday, November 4, 2078, [1] with a magnitude of 0.9255. 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. 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 only about 22 hours before apogee (on November 5, 2078, at 14:45 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Chile, Argentina, and Tristan da Cunha. A partial solar eclipse will also be visible for parts of eastern Oceania, Mexico, the southwestern United States, Central America, 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. [3]

November 4, 2078 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2078 November 04 at 13:50:30.4 UTC
First Umbral External Contact2078 November 04 at 14:56:36.8 UTC
First Central Line2078 November 04 at 14:59:50.8 UTC
First Umbral Internal Contact2078 November 04 at 15:03:05.2 UTC
First Penumbral Internal Contact2078 November 04 at 16:12:46.9 UTC
Greatest Eclipse2078 November 04 at 16:55:44.4 UTC
Ecliptic Conjunction2078 November 04 at 16:58:29.7 UTC
Equatorial Conjunction2078 November 04 at 17:07:32.6 UTC
Greatest Duration2078 November 04 at 17:13:29.5 UTC
Last Penumbral Internal Contact2078 November 04 at 17:38:24.2 UTC
Last Umbral Internal Contact2078 November 04 at 18:48:15.5 UTC
Last Central Line2078 November 04 at 18:51:30.7 UTC
Last Umbral External Contact2078 November 04 at 18:54:45.5 UTC
Last Penumbral External Contact2078 November 04 at 20:00:55.0 UTC
November 4, 2078 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.92551
Eclipse Obscuration0.85657
Gamma−0.22852
Sun Right Ascension14h40m53.9s
Sun Declination-15°38'07.6"
Sun Semi-Diameter16'07.5"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension14h40m33.5s
Moon Declination-15°49'24.5"
Moon Semi-Diameter14'42.4"
Moon Equatorial Horizontal Parallax0°53'58.5"
ΔT104.5 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 October–November 2078
October 21
Ascending node (full moon)
 November 4
Descending node (new moon)
 November 19
Ascending node (full moon)
SE2078Nov04A.png
Penumbral lunar eclipse
Lunar Saros 118		 Annular solar eclipse
Solar Saros 144		 Penumbral lunar eclipse
Lunar Saros 156

Eclipses in 2078

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 144

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 144

This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 5–26 occur between 1801 and 2200:
567
SE1808May25P.png
May 25, 1808		 SE1826Jun05P.png
June 5, 1826		 SE1844Jun16P.png
June 16, 1844
8910
SE1862Jun27P.png
June 27, 1862		 SE1880Jul07A.png
July 7, 1880		 SE1898Jul18A.png
July 18, 1898
111213
SE1916Jul30A.png
July 30, 1916 		SE1934Aug10A.png
August 10, 1934 		SE1952Aug20A.png
August 20, 1952
141516
SE1970Aug31A.png
August 31, 1970 		SE1988Sep11A.png
September 11, 1988 		SE2006Sep22A.png
September 22, 2006
171819
SE2024Oct02A.png
October 2, 2024 		SE2042Oct14A.png
October 14, 2042 		SE2060Oct24A.png
October 24, 2060
202122
SE2078Nov04A.png
November 4, 2078 		SE2096Nov15A.png
November 15, 2096 		SE2114Nov27A.png
November 27, 2114
232425
SE2132Dec07A.png
December 7, 2132		 SE2150Dec19A.png
December 19, 2150		 SE2168Dec29A.png
December 29, 2168
26
SE2187Jan09A.png
January 9, 2187

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
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
SE1818May05A.png
May 5, 1818
(Saros 135)		 SE1847Apr15T.png
April 15, 1847
(Saros 136)		 SE1876Mar25A.png
March 25, 1876
(Saros 137)
SE1905Mar06A.png
March 6, 1905
(Saros 138)		 SE1934Feb14T.png
February 14, 1934
(Saros 139)		 SE1963Jan25A.png
January 25, 1963
(Saros 140)
SE1992Jan04A.png
January 4, 1992
(Saros 141)		 SE2020Dec14T.png
December 14, 2020
(Saros 142)		 SE2049Nov25H.png
November 25, 2049
(Saros 143)
SE2078Nov04A.png
November 4, 2078
(Saros 144)		 SE2107Oct16T.png
October 16, 2107
(Saros 145)		 SE2136Sep26T.png
September 26, 2136
(Saros 146)
Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
(Saros 147)		 Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

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References

  1. ↑ "November 4, 2078 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 2078 Nov 04". 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 144". eclipse.gsfc.nasa.gov.
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