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Solar eclipse of May 9, 2032

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Solar eclipse of May 9, 2032
Map
Type of eclipse
NatureAnnular
Gamma−0.9375
Magnitude0.9957
Maximum eclipse
Duration22 s (0 min 22 s)
Coordinates51°18′S 7°06′W / 51.3°S 7.1°W / -51.3; -7.1
Max. width of band44 km (27 mi)
Times (UTC)
Greatest eclipse13:26:42
References
Saros148 (22 of 75)
Catalog # (SE5000)9579

An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, May 9, 2032,[1] with a magnitude of 0.9957. 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. The Moon's apparent diameter will be near the average diameter because it will occur 5.7 days after perigee (on May 3, 2032, at 21:40 UTC) and 7.4 days before apogee (on May 16, 2032, at 23:20 UTC).[2]

Since most of the path of this eclipse is narrow and passes over the South Atlantic Ocean, no land areas will witness annularity. However, a partial eclipse will be visible for parts of southern South America and Southern Africa.

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.[3]

May 9, 2032 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2032 May 09 at 11:11:06.6 UTC
First Umbral External Contact 2032 May 09 at 12:48:26.6 UTC
First Central Line 2032 May 09 at 12:49:18.2 UTC
Greatest Duration 2032 May 09 at 12:49:18.2 UTC
First Umbral Internal Contact 2032 May 09 at 12:50:10.9 UTC
Equatorial Conjunction 2032 May 09 at 13:08:19.5 UTC
Greatest Eclipse 2032 May 09 at 13:26:42.4 UTC
Ecliptic Conjunction 2032 May 09 at 13:36:54.7 UTC
Last Umbral Internal Contact 2032 May 09 at 14:03:24.2 UTC
Last Central Line 2032 May 09 at 14:04:19.8 UTC
Last Umbral External Contact 2032 May 09 at 14:05:14.2 UTC
Last Penumbral External Contact 2032 May 09 at 15:42:32.2 UTC
May 9, 2032 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.99570
Eclipse Obscuration 0.99143
Gamma −0.93748
Sun Right Ascension 03h08m06.7s
Sun Declination +17°35'43.5"
Sun Semi-Diameter 15'50.4"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 03h08m46.1s
Moon Declination +16°42'42.0"
Moon Semi-Diameter 15'41.5"
Moon Equatorial Horizontal Parallax 0°57'35.4"
ΔT 74.9 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 April–May 2032
April 25
Ascending node (full moon)
May 9
Descending node (new moon)
Total lunar eclipse
Lunar Saros 122
Annular solar eclipse
Solar Saros 148
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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 148

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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.[4]

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 148

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This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. 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 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit.[5]

Series members 10–31 occur between 1801 and 2200:
10 11 12

December 30, 1815

January 9, 1834

January 21, 1852
13 14 15

January 31, 1870

February 11, 1888

February 23, 1906
16 17 18

March 5, 1924

March 16, 1942

March 27, 1960
19 20 21

April 7, 1978

April 17, 1996

April 29, 2014
22 23 24

May 9, 2032

May 20, 2050

May 31, 2068
25 26 27

June 11, 2086

June 22, 2104

July 4, 2122
28 29 30

July 14, 2140

July 25, 2158

August 4, 2176
31

August 16, 2194

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.

21 eclipse events between July 22, 1971 and July 22, 2047
July 22 May 9–11 February 26–27 December 14–15 October 2–3
116 118 120 122 124

July 22, 1971

May 11, 1975

February 26, 1979

December 15, 1982

October 3, 1986
126 128 130 132 134

July 22, 1990

May 10, 1994

February 26, 1998

December 14, 2001

October 3, 2005
136 138 140 142 144

July 22, 2009

May 10, 2013

February 26, 2017

December 14, 2020

October 2, 2024
146 148 150 152 154

July 22, 2028

May 9, 2032

February 27, 2036

December 15, 2039

October 3, 2043
156

July 22, 2047

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

September 28, 1829
(Saros 141)

September 7, 1858
(Saros 142)

August 19, 1887
(Saros 143)

July 30, 1916
(Saros 144)

July 9, 1945
(Saros 145)

June 20, 1974
(Saros 146)

May 31, 2003
(Saros 147)

May 9, 2032
(Saros 148)

April 20, 2061
(Saros 149)

March 31, 2090
(Saros 150)

March 11, 2119
(Saros 151)

February 19, 2148
(Saros 152)

January 29, 2177
(Saros 153)

See also

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References

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  1. ^ "May 9, 2032 Annular Solar Eclipse". timeanddate. Retrieved 14 August 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 August 2024.
  3. ^ "Annular Solar Eclipse of 2032 May 09". EclipseWise.com. Retrieved 14 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 148". eclipse.gsfc.nasa.gov.
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