Solar eclipse of April 10, 2089

Last updated
Solar eclipse of April 10, 2089
SE2089Apr10A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.3319
Magnitude 0.9919
Maximum eclipse
Duration53 s (0 min 53 s)
Coordinates 10°12′S154°48′W / 10.2°S 154.8°W / -10.2; -154.8
Max. width of band30 km (19 mi)
Times (UTC)
Greatest eclipse22:44:42
References
Saros 140 (33 of 71)
Catalog # (SE5000) 9708

An annular solar eclipse will occur at the Moon's descending node of orbit between Sunday, April 10 and Monday, April 11, 2089, [1] with a magnitude of 0.9919. 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 7 days after apogee (on April 3, 2089, at 23:20 UTC) and 6.8 days before perigee (on April 17, 2089, at 17:00 UTC). [2]

Contents

The path of annularity will be visible from parts of southeastern Australia, Tonga, and Niue. A partial solar eclipse will also be visible for parts of Australia, Oceania, Antarctica, Mexico, and Central America.

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]

April 10, 2089 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2089 April 10 at 19:56:15.6 UTC
First Umbral External Contact2089 April 10 at 20:59:15.4 UTC
First Central Line2089 April 10 at 21:00:03.3 UTC
Greatest Duration2089 April 10 at 21:00:03.3 UTC
First Umbral Internal Contact2089 April 10 at 21:00:51.4 UTC
First Penumbral Internal Contact2089 April 10 at 22:11:51.4 UTC
Equatorial Conjunction2089 April 10 at 22:33:57.5 UTC
Greatest Eclipse2089 April 10 at 22:44:41.5 UTC
Ecliptic Conjunction2089 April 10 at 22:48:21.4 UTC
Last Penumbral Internal Contact2089 April 10 at 23:17:50.5 UTC
Last Umbral Internal Contact2089 April 11 at 00:28:41.8 UTC
Last Central Line2089 April 11 at 00:29:26.8 UTC
Last Umbral External Contact2089 April 11 at 00:30:11.6 UTC
Last Penumbral External Contact2089 April 11 at 01:33:05.8 UTC
April 10, 2089 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.99192
Eclipse Obscuration0.98391
Gamma−0.33186
Sun Right Ascension01h20m36.9s
Sun Declination+08°29'24.5"
Sun Semi-Diameter15'57.8"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension01h20m58.3s
Moon Declination+08°11'12.9"
Moon Semi-Diameter15'35.9"
Moon Equatorial Horizontal Parallax0°57'14.7"
ΔT113.5 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.

Eclipse season of March–April 2089
March 26
Ascending node (full moon)
 April 10
Descending node (new moon)
SE2089Apr10A.png
Penumbral lunar eclipse
Lunar Saros 114		 Annular solar eclipse
Solar Saros 140

Eclipses in 2089

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 140

Inex

Triad

Solar eclipses of 2087–2090

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 eclipse on June 1, 2087 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2087 to 2090
Descending node Ascending node
SarosMapGammaSarosMapGamma
120 May 2, 2087
SE2087May02P.png
Partial		1.1139125 October 26, 2087
SE2087Oct26P.png
Partial		−1.2882
130 April 21, 2088
SE2088Apr21T.png
Total		0.4135135 October 14, 2088
SE2088Oct14A.png
Annular		−0.5349
140 April 10, 2089
SE2089Apr10A.png
Annular		−0.3319145 October 4, 2089
SE2089Oct04T.png
Total		0.2167
150 March 31, 2090
SE2090Mar31P.png
Partial		−1.1028155 September 23, 2090
SE2090Sep23T.png
Total		0.9157

Saros 140

This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836; hybrid eclipses from November 20, 1854 through December 23, 1908; and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. 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 totality was produced by member 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 18–39 occur between 1801 and 2200:
181920
SE1818Oct29T.png
October 29, 1818		 SE1836Nov09T.png
November 9, 1836		 SE1854Nov20H.png
November 20, 1854
212223
SE1872Nov30H.png
November 30, 1872		 SE1890Dec12H.png
December 12, 1890		 SE1908Dec23H.png
December 23, 1908
242526
SE1927Jan03A.png
January 3, 1927 		SE1945Jan14A.png
January 14, 1945 		SE1963Jan25A.png
January 25, 1963
272829
SE1981Feb04A.png
February 4, 1981 		SE1999Feb16A.png
February 16, 1999 		SE2017Feb26A.png
February 26, 2017
303132
SE2035Mar09A.png
March 9, 2035 		SE2053Mar20A.png
March 20, 2053 		SE2071Mar31A.png
March 31, 2071
333435
SE2089Apr10A.png
April 10, 2089 		SE2107Apr23A.png
April 23, 2107		 SE2125May03A.png
May 3, 2125
363738
SE2143May14A.png
May 14, 2143		 SE2161May25A.png
May 25, 2161		 SE2179Jun05A.png
June 5, 2179
39
SE2197Jun15A.png
June 15, 2197

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 23, 2047 and November 16, 2134
June 22–23April 10–11January 27–29November 15–16September 3–5
118120122124126
SE2047Jun23P.png
June 23, 2047 		SE2051Apr11P.png
April 11, 2051 		SE2055Jan27P.png
January 27, 2055 		SE2058Nov16P.png
November 16, 2058 		SE2062Sep03P.png
September 3, 2062
128130132134136
SE2066Jun22A.png
June 22, 2066 		SE2070Apr11T.png
April 11, 2070 		SE2074Jan27A.png
January 27, 2074 		SE2077Nov15A.png
November 15, 2077 		SE2081Sep03T.png
September 3, 2081
138140142144146
SE2085Jun22A.png
June 22, 2085 		SE2089Apr10A.png
April 10, 2089 		SE2093Jan27T.png
January 27, 2093 		SE2096Nov15A.png
November 15, 2096 		SE2100Sep04T.png
September 4, 2100
148150152154156
SE2104Jun22T.png
June 22, 2104		 SE2108Apr11P.gif
April 11, 2108		 Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112		 SE2115Nov16A.png
November 16, 2115		 Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
158160162164
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123		 Saros164 03van80 SE2134Nov16P.jpg
November 16, 2134

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
SE1805Jun26P.gif
June 26, 1805
(Saros 114)		 SE1816May27A.gif
May 27, 1816
(Saros 115)		 SE1827Apr26A.gif
April 26, 1827
(Saros 116)		 SE1838Mar25T.gif
March 25, 1838
(Saros 117)		 SE1849Feb23A.gif
February 23, 1849
(Saros 118)
SE1860Jan23A.png
January 23, 1860
(Saros 119)		 SE1870Dec22T.png
December 22, 1870
(Saros 120)		 SE1881Nov21A.gif
November 21, 1881
(Saros 121)		 SE1892Oct20P.gif
October 20, 1892
(Saros 122)		 SE1903Sep21T.png
September 21, 1903
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)		 SE1925Jul20A.png
July 20, 1925
(Saros 125)		 SE1936Jun19T.png
June 19, 1936
(Saros 126)		 SE1947May20T.png
May 20, 1947
(Saros 127)		 SE1958Apr19A.png
April 19, 1958
(Saros 128)
SE1969Mar18A.png
March 18, 1969
(Saros 129)		 SE1980Feb16T.png
February 16, 1980
(Saros 130)		 SE1991Jan15A.png
January 15, 1991
(Saros 131)		 SE2001Dec14A.png
December 14, 2001
(Saros 132)		 SE2012Nov13T.png
November 13, 2012
(Saros 133)
SE2023Oct14A.png
October 14, 2023
(Saros 134)		 SE2034Sep12A.png
September 12, 2034
(Saros 135)		 SE2045Aug12T.png
August 12, 2045
(Saros 136)		 SE2056Jul12A.png
July 12, 2056
(Saros 137)		 SE2067Jun11A.png
June 11, 2067
(Saros 138)
SE2078May11T.png
May 11, 2078
(Saros 139)		 SE2089Apr10A.png
April 10, 2089
(Saros 140)		 SE2100Mar10A.png
March 10, 2100
(Saros 141)		 SE2111Feb08T.png
February 8, 2111
(Saros 142)		 SE2122Jan08A.png
January 8, 2122
(Saros 143)
SE2132Dec07A.png
December 7, 2132
(Saros 144)		 SE2143Nov07T.png
November 7, 2143
(Saros 145)		 SE2154Oct07T.png
October 7, 2154
(Saros 146)		 Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
(Saros 147)		 Saros148 30van75 SE2176Aug04T.jpg
August 4, 2176
(Saros 148)
Saros149 30van71 SE2187Jul06T.jpg
July 6, 2187
(Saros 149)		 Saros150 27van71 SE2198Jun04A.jpg
June 4, 2198
(Saros 150)

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
SE1828Oct09A.gif
October 9, 1828
(Saros 131)		 SE1857Sep18A.gif
September 18, 1857
(Saros 132)		 SE1886Aug29T.png
August 29, 1886
(Saros 133)
SE1915Aug10A.png
August 10, 1915
(Saros 134)		 SE1944Jul20A.png
July 20, 1944
(Saros 135)		 SE1973Jun30T.png
June 30, 1973
(Saros 136)
SE2002Jun10A.png
June 10, 2002
(Saros 137)		 SE2031May21A.png
May 21, 2031
(Saros 138)		 SE2060Apr30T.png
April 30, 2060
(Saros 139)
SE2089Apr10A.png
April 10, 2089
(Saros 140)		 SE2118Mar22A.png
March 22, 2118
(Saros 141)		 SE2147Mar02T.png
March 2, 2147
(Saros 142)
SE2176Feb10A.png
February 10, 2176
(Saros 143)

Notes

  1. ↑ "April 10–11, 2089 Annular Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. ↑ "Annular Solar Eclipse of 2089 Apr 10". EclipseWise.com. Retrieved 24 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 140". eclipse.gsfc.nasa.gov.

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References

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