Solar eclipse of November 3, 2032

Last updated
Solar eclipse of November 3, 2032
SE2032Nov03P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0643
Magnitude 0.8554
Maximum eclipse
Coordinates 70°24′N132°36′E / 70.4°N 132.6°E / 70.4; 132.6
Times (UTC)
Greatest eclipse5:34:13
References
Saros 153 (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, 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.

Contents

Images

SE2032Nov03P.gif
Animated path

Eclipses in 2032

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 153

Inex

Triad

Solar eclipses of 2029–2032

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. [1]

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
SarosMapGammaSarosMapGamma
118 June 12, 2029
SE2029Jun12P.png
Partial
1.29431123 December 5, 2029
SE2029Dec05P.png
Partial
−1.06090
128 June 1, 2030
SE2030Jun01A.png
Annular
0.56265133 November 25, 2030
SE2030Nov25T.png
Total
−0.38669
138 May 21, 2031
SE2031May21A.png
Annular
−0.19699143 November 14, 2031
SE2031Nov14H.png
Hybrid
0.30776
148 May 9, 2032
SE2032May09A.png
Annular
−0.93748153 November 3, 2032
SE2032Nov03P.png
Partial
1.06431

Saros 153

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. [2]

Series members 1–19 occur between 1870 and 2200:
123
SE1870Jul28Pb.gif
July 28, 1870
SE1888Aug07P.gif
August 7, 1888
SE1906Aug20P.png
August 20, 1906
456
SE1924Aug30P.png
August 30, 1924
SE1942Sep10P.png
September 10, 1942
SE1960Sep20P.png
September 20, 1960
789
SE1978Oct02P.png
October 2, 1978
SE1996Oct12P.png
October 12, 1996
SE2014Oct23P.png
October 23, 2014
101112
SE2032Nov03P.png
November 3, 2032
SE2050Nov14P.png
November 14, 2050
SE2068Nov24P.png
November 24, 2068
131415
SE2086Dec06P.png
December 6, 2086
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
161718
Saros153 16van70 SE2141Jan08A.jpg
January 8, 2141
Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
19
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195

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.

20 eclipse events between June 10, 1964 and August 21, 2036
June 10–11March 28–29January 14–16November 3August 21–22
117119121123125
SE1964Jun10P.png
June 10, 1964
SE1968Mar28P.png
March 28, 1968
SE1972Jan16A.png
January 16, 1972
SE1975Nov03P.png
November 3, 1975
SE1979Aug22A.png
August 22, 1979
127129131133135
SE1983Jun11T.png
June 11, 1983
SE1987Mar29H.png
March 29, 1987
SE1991Jan15A.png
January 15, 1991
SE1994Nov03T.png
November 3, 1994
SE1998Aug22A.png
August 22, 1998
137139141143145
SE2002Jun10A.png
June 10, 2002
SE2006Mar29T.png
March 29, 2006
SE2010Jan15A.png
January 15, 2010
SE2013Nov03H.png
November 3, 2013
SE2017Aug21T.png
August 21, 2017
147149151153155
SE2021Jun10A.png
June 10, 2021
SE2025Mar29P.png
March 29, 2025
SE2029Jan14P.png
January 14, 2029
SE2032Nov03P.png
November 3, 2032
SE2036Aug21P.png
August 21, 2036

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 2087
SE1803Aug17A.png
August 17, 1803
(Saros 132)
SE1814Jul17T.png
July 17, 1814
(Saros 133)
SE1825Jun16H.png
June 16, 1825
(Saros 134)
SE1836May15A.png
May 15, 1836
(Saros 135)
SE1847Apr15T.png
April 15, 1847
(Saros 136)
SE1858Mar15A.png
March 15, 1858
(Saros 137)
SE1869Feb11A.png
February 11, 1869
(Saros 138)
SE1880Jan11T.png
January 11, 1880
(Saros 139)
SE1890Dec12H.png
December 12, 1890
(Saros 140)
SE1901Nov11A.png
November 11, 1901
(Saros 141)
SE1912Oct10T.png
October 10, 1912
(Saros 142)
SE1923Sep10T.png
September 10, 1923
(Saros 143)
SE1934Aug10A.png
August 10, 1934
(Saros 144)
SE1945Jul09T.png
July 9, 1945
(Saros 145)
SE1956Jun08T.png
June 8, 1956
(Saros 146)
SE1967May09P.png
May 9, 1967
(Saros 147)
SE1978Apr07P.png
April 7, 1978
(Saros 148)
SE1989Mar07P.png
March 7, 1989
(Saros 149)
SE2000Feb05P.png
February 5, 2000
(Saros 150)
SE2011Jan04P.png
January 4, 2011
(Saros 151)
SE2021Dec04T.png
December 4, 2021
(Saros 152)
SE2032Nov03P.png
November 3, 2032
(Saros 153)
SE2043Oct03A.png
October 3, 2043
(Saros 154)
SE2054Sep02P.png
September 2, 2054
(Saros 155)
SE2065Aug02P.png
August 2, 2065
(Saros 156)
SE2076Jul01P.png
July 1, 2076
(Saros 157)
SE2087Jun01P.png
June 1, 2087
(Saros 158)

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
SE1801Apr13P.png
April 13, 1801
(Saros 145)
SE1830Mar24P.gif
March 24, 1830
(Saros 146)
SE1859Mar04P.gif
March 4, 1859
(Saros 147)
SE1888Feb11P.gif
February 11, 1888
(Saros 148)
SE1917Jan23P.png
January 23, 1917
(Saros 149)
SE1946Jan03P.png
January 3, 1946
(Saros 150)
SE1974Dec13P.png
December 13, 1974
(Saros 151)
SE2003Nov23T.png
November 23, 2003
(Saros 152)
SE2032Nov03P.png
November 3, 2032
(Saros 153)
SE2061Oct13A.png
October 13, 2061
(Saros 154)
SE2090Sep23T.png
September 23, 2090
(Saros 155)
Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
(Saros 156)
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)
Saros158 07van70 SE2177Jul25P.jpg
July 25, 2177
(Saros 158)

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References

  1. 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.
  2. "NASA - Catalog of Solar Eclipses of Saros 153". eclipse.gsfc.nasa.gov.