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Solar eclipse of November 3, 2032

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Solar eclipse of November 3, 2032
Map
Type of eclipse
NaturePartial
Gamma1.0643
Magnitude0.8554
Maximum eclipse
Coordinates70°24′N 132°36′E / 70.4°N 132.6°E / 70.4; 132.6
Times (UTC)
Greatest eclipse5:34:13
References
Saros153 (10 of 70)
Catalog # (SE5000)9580

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, November 3, 2032,[1] with a magnitude of 0.8554. 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.

A partial eclipse will be visible for most of Asia.

Images

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Animated path

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.[2]

November 3, 2032 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2032 November 03 at 03:23:35.3 UTC
Equatorial Conjunction 2032 November 03 at 05:07:21.3 UTC
Greatest Eclipse 2032 November 03 at 05:34:12.9 UTC
Ecliptic Conjunction 2032 November 03 at 05:46:07.8 UTC
Last Penumbral External Contact 2032 November 03 at 07:44:57.6 UTC
November 3, 2032 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.85543
Eclipse Obscuration 0.79712
Gamma 1.06431
Sun Right Ascension 14h35m40.9s
Sun Declination -15°13'54.9"
Sun Semi-Diameter 16'07.4"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 14h36m33.6s
Moon Declination -14°16'01.1"
Moon Semi-Diameter 15'13.0"
Moon Equatorial Horizontal Parallax 0°55'50.8"
ΔT 75.1 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 2032
October 18
Descending node (full moon)
November 3
Ascending node (new moon)
Total lunar eclipse
Lunar Saros 127
Partial solar eclipse
Solar Saros 153
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Eclipses in 2032

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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 153

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Inex

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Triad

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Solar eclipses of 2029–2032

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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.[3]

The partial solar eclipses on January 14, 2029 and July 11, 2029 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2029 to 2032
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 June 12, 2029

Partial
1.29431 123 December 5, 2029

Partial
−1.06090
128 June 1, 2030

Annular
0.56265 133 November 25, 2030

Total
−0.38669
138 May 21, 2031

Annular
−0.19699 143 November 14, 2031

Hybrid
0.30776
148 May 9, 2032

Annular
−0.93748 153 November 3, 2032

Partial
1.06431

Saros 153

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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:
1 2 3

July 28, 1870

August 7, 1888

August 20, 1906
4 5 6

August 30, 1924

September 10, 1942

September 20, 1960
7 8 9

October 2, 1978

October 12, 1996

October 23, 2014
10 11 12

November 3, 2032

November 14, 2050

November 24, 2068
13 14 15

December 6, 2086

December 17, 2104

December 28, 2122
16 17 18

January 8, 2141

January 19, 2159

January 29, 2177
19

February 10, 2195

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 ascending node.

20 eclipse events between June 10, 1964 and August 21, 2036
June 10–11 March 28–29 January 14–16 November 3 August 21–22
117 119 121 123 125

June 10, 1964

March 28, 1968

January 16, 1972

November 3, 1975

August 22, 1979
127 129 131 133 135

June 11, 1983

March 29, 1987

January 15, 1991

November 3, 1994

August 22, 1998
137 139 141 143 145

June 10, 2002

March 29, 2006

January 15, 2010

November 3, 2013

August 21, 2017
147 149 151 153 155

June 10, 2021

March 29, 2025

January 14, 2029

November 3, 2032

August 21, 2036

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 2087

August 17, 1803
(Saros 132)

July 17, 1814
(Saros 133)

June 16, 1825
(Saros 134)

May 15, 1836
(Saros 135)

April 15, 1847
(Saros 136)

March 15, 1858
(Saros 137)

February 11, 1869
(Saros 138)

January 11, 1880
(Saros 139)

December 12, 1890
(Saros 140)

November 11, 1901
(Saros 141)

October 10, 1912
(Saros 142)

September 10, 1923
(Saros 143)

August 10, 1934
(Saros 144)

July 9, 1945
(Saros 145)

June 8, 1956
(Saros 146)

May 9, 1967
(Saros 147)

April 7, 1978
(Saros 148)

March 7, 1989
(Saros 149)

February 5, 2000
(Saros 150)

January 4, 2011
(Saros 151)

December 4, 2021
(Saros 152)

November 3, 2032
(Saros 153)

October 3, 2043
(Saros 154)

September 2, 2054
(Saros 155)

August 2, 2065
(Saros 156)

July 1, 2076
(Saros 157)

June 1, 2087
(Saros 158)

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

April 13, 1801
(Saros 145)

March 24, 1830
(Saros 146)

March 4, 1859
(Saros 147)

February 11, 1888
(Saros 148)

January 23, 1917
(Saros 149)

January 3, 1946
(Saros 150)

December 13, 1974
(Saros 151)

November 23, 2003
(Saros 152)

November 3, 2032
(Saros 153)

October 13, 2061
(Saros 154)

September 23, 2090
(Saros 155)

September 5, 2119
(Saros 156)

August 14, 2148
(Saros 157)

July 25, 2177
(Saros 158)

References

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  1. ^ "November 3, 2032 Partial Solar Eclipse". timeanddate. Retrieved 14 August 2024.
  2. ^ "Partial Solar Eclipse of 2032 Nov 03". EclipseWise.com. Retrieved 14 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.
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