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Solar eclipse of November 4, 2097

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Solar eclipse of November 4, 2097
Map
Type of eclipse
NatureAnnular
Gamma−0.8926
Magnitude0.9494
Maximum eclipse
Duration216 s (3 min 36 s)
Coordinates65°48′S 86°48′E / 65.8°S 86.8°E / -65.8; 86.8
Max. width of band411 km (255 mi)
Times (UTC)
Greatest eclipse2:01:25
References
Saros154 (11 of 71)
Catalog # (SE5000)9727

An annular solar eclipse will occur at the Moon's descending node of orbit between Sunday, November 3 and Monday, November 4, 2097,[1] with a magnitude of 0.9494. 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 about 5.4 days before apogee (on November 9, 2097, at 12:15 UTC), the Moon's apparent diameter will be smaller.[2]

The path of annularity will be visible from parts of Antarctica. A partial solar eclipse will also be visible for parts of southwestern Australia and Antarctica. This annular eclipse is notable in that the path of annularity passes over the South Pole.

Eclipse details

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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, 2097 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2097 November 03 at 23:34:35.1 UTC
First Umbral External Contact 2097 November 04 at 01:06:01.0 UTC
First Central Line 2097 November 04 at 01:10:07.9 UTC
First Umbral Internal Contact 2097 November 04 at 01:14:32.3 UTC
Greatest Eclipse 2097 November 04 at 02:01:25.2 UTC
Greatest Duration 2097 November 04 at 02:10:27.8 UTC
Ecliptic Conjunction 2097 November 04 at 02:11:36.5 UTC
Equatorial Conjunction 2097 November 04 at 02:45:40.7 UTC
Last Umbral Internal Contact 2097 November 04 at 02:47:47.0 UTC
Last Central Line 2097 November 04 at 02:52:14.7 UTC
Last Umbral External Contact 2097 November 04 at 02:56:25.0 UTC
Last Penumbral External Contact 2097 November 04 at 04:28:03.3 UTC
November 4, 2097 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.94941
Eclipse Obscuration 0.90138
Gamma −0.89264
Sun Right Ascension 14h40m01.3s
Sun Declination -15°33'59.2"
Sun Semi-Diameter 16'07.3"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 14h38m39.0s
Moon Declination -16°19'33.5"
Moon Semi-Diameter 15'12.3"
Moon Equatorial Horizontal Parallax 0°55'48.3"
ΔT 121.5 s

Eclipse season

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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 October–November 2097
October 21
Ascending node (full moon)
November 4
Descending node (new moon)
Total lunar eclipse
Lunar Saros 128
Annular solar eclipse
Solar Saros 154
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Eclipses in 2097

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 154

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Inex

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Triad

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Solar eclipses of 2094–2098

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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 solar eclipses on January 16, 2094 (total) and July 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses on April 1, 2098 and September 25, 2098 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2094 to 2098
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 June 13, 2094

Partial
−1.4613 124 December 7, 2094

Partial
1.1547
129 June 2, 2095

Total
−0.6396 134 November 27, 2095

Annular
0.4903
139 May 22, 2096

Total
0.1196 144 November 15, 2096

Annular
−0.20
149 May 11, 2097

Total
0.8516 154 November 4, 2097

Annular
−0.8926
159 May 1, 2098 164 October 24, 2098

Partial
−1.5407

Saros 154

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This eclipse is a part of Saros series 154, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 19, 1917. It contains annular eclipses from October 3, 2043 through March 27, 2332; hybrid eclipses from April 7, 2350 through April 29, 2386; and total eclipses from May 9, 2404 through May 29, 3035. The series ends at member 71 as a partial eclipse on August 25, 3179. 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 9 at 3 minutes, 41 seconds on October 13, 2061, and the longest duration of totality will be produced by member 35 at 4 minutes, 50 seconds on July 25, 2530. All eclipses in this series occur at the Moon’s descending node of orbit.[5]

Series members 1–16 occur between 1917 and 2200:
1 2 3

July 19, 1917

July 30, 1935

August 9, 1953
4 5 6

August 20, 1971

August 31, 1989

September 11, 2007
7 8 9

September 21, 2025

October 3, 2043

October 13, 2061
10 11 12

October 24, 2079

November 4, 2097

November 16, 2115
13 14 15

November 26, 2133

December 8, 2151

December 18, 2169
16

December 29, 2187

Metonic series

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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 11–12 March 30–31 January 16 November 4–5 August 23–24
118 120 122 124 126

June 12, 2029

March 30, 2033

January 16, 2037

November 4, 2040

August 23, 2044
128 130 132 134 136

June 11, 2048

March 30, 2052

January 16, 2056

November 5, 2059

August 24, 2063
138 140 142 144 146

June 11, 2067

March 31, 2071

January 16, 2075

November 4, 2078

August 24, 2082
148 150 152 154 156

June 11, 2086

March 31, 2090

January 16, 2094

November 4, 2097

August 24, 2101
158 160 162 164

June 12, 2105

November 4, 2116

Tritos series

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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

February 21, 1803
(Saros 127)

January 21, 1814
(Saros 128)

December 20, 1824
(Saros 129)

November 20, 1835
(Saros 130)

October 20, 1846
(Saros 131)

September 18, 1857
(Saros 132)

August 18, 1868
(Saros 133)

July 19, 1879
(Saros 134)

June 17, 1890
(Saros 135)

May 18, 1901
(Saros 136)

April 17, 1912
(Saros 137)

March 17, 1923
(Saros 138)

February 14, 1934
(Saros 139)

January 14, 1945
(Saros 140)

December 14, 1955
(Saros 141)

November 12, 1966
(Saros 142)

October 12, 1977
(Saros 143)

September 11, 1988
(Saros 144)

August 11, 1999
(Saros 145)

July 11, 2010
(Saros 146)

June 10, 2021
(Saros 147)

May 9, 2032
(Saros 148)

April 9, 2043
(Saros 149)

March 9, 2054
(Saros 150)

February 5, 2065
(Saros 151)

January 6, 2076
(Saros 152)

December 6, 2086
(Saros 153)

November 4, 2097
(Saros 154)

October 5, 2108
(Saros 155)

September 5, 2119
(Saros 156)

August 4, 2130
(Saros 157)

July 3, 2141
(Saros 158)

June 3, 2152
(Saros 159)

April 1, 2174
(Saros 161)

Inex series

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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

May 25, 1808
(Saros 144)

May 4, 1837
(Saros 145)

April 15, 1866
(Saros 146)

March 26, 1895
(Saros 147)

March 5, 1924
(Saros 148)

February 14, 1953
(Saros 149)

January 24, 1982
(Saros 150)

January 4, 2011
(Saros 151)

December 15, 2039
(Saros 152)

November 24, 2068
(Saros 153)

November 4, 2097
(Saros 154)

October 16, 2126
(Saros 155)

September 26, 2155
(Saros 156)

September 4, 2184
(Saros 157)

Notes

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  1. ^ "November 3–4, 2097 Annular Solar Eclipse". timeanddate. Retrieved 25 August 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 25 August 2024.
  3. ^ "Annular Solar Eclipse of 2097 Nov 04". EclipseWise.com. Retrieved 25 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 154". eclipse.gsfc.nasa.gov.

References

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