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{{short description|Future annular solar eclipse}}
{{Solareclipse205_db|Infobox Solar eclipse2|2089Apr10}}
{{Infobox solar eclipse|2089Apr10}}
An annular [[solar eclipse]] will occur on April 10, 2089. {{Annular solar eclipse summary}}
An [[Annulus (mathematics)|annular]] [[solar eclipse]] will occur on April 10, [[2089]]. 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 (mathematics)|annulus]] (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.


== Related eclipses==
== Related eclipses==
=== Solar eclipses 2087-2090===
{{Solar eclipse set 2087-2090}}


=== Solar eclipses 2087–2090===
==References==
{{Solar eclipse set 2087–2090}}

=== Saros 140 ===

It is a part of [[Solar Saros 140|Saros cycle 140]], repeating every 18 years, 11 days, containing 71 events. The series started with 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. The longest duration of totality was 4 minutes, 10 seconds on August 12, 1692.
{| class="wikitable collapsible collapsed"
!colspan=3|Series members 23–53 occur between 1901 and 2450:
|-
!23
!24
!25
|- style="text-align:center;"
|[[File:SE1908Dec23H.png|150px]]<br />[[solar eclipse of December 23, 1908|Dec 23, 1908]]
|[[File:SE1927Jan03A.png|150px]]<br />[[solar eclipse of January 3, 1927|Jan 3, 1927]]
|[[File:SE1945Jan14A.png|150px]]<br />[[solar eclipse of January 14, 1945|Jan 14, 1945]]
|-
!26
!27
!28
|- style="text-align:center;"
|[[File:SE1963Jan25A.png|150px]]<br />[[solar eclipse of January 25, 1963|Jan 25, 1963]]
|[[File:SE1981Feb04A.png|150px]]<br />[[solar eclipse of February 4, 1981|Feb 4, 1981]]
|[[File:SE1999Feb16A.png|150px]]<br />[[solar eclipse of February 16, 1999|Feb 16, 1999]]
|-
!29
!30
!31
|- style="text-align:center;"
|[[File:SE2017Feb26A.png|150px]]<br />[[solar eclipse of February 26, 2017|Feb 26, 2017]]
|[[File:SE2035Mar09A.png|150px]]<br />[[solar eclipse of March 9, 2035|Mar 9, 2035]]
|[[File:SE2053Mar20A.png|150px]]<br />[[solar eclipse of March 20, 2053|Mar 20, 2053]]
|-
!32
!33
!34
|- style="text-align:center;"
|[[File:SE2071Mar31A.png|150px]]<br />[[solar eclipse of March 31, 2071|Mar 31, 2071]]
|[[File:SE2089Apr10A.png|150px]]<br />Apr 10, 2089
|[[File:SE2107Apr23A.png|150px]]<br />Apr 23, 2107
|-
!35
!36
!37
|- style="text-align:center;"
|[[File:SE2125May03A.png|150px]]<br />May 3, 2125
|[[File:SE2143May14A.png|150px]]<br />May 14, 2143
|[[File:SE2161May25A.png|150px]]<br />May 25, 2161
|-
!38
!39
!40
|- style="text-align:center;"
|[[File:SE2179Jun05A.png|150px]]<br />Jun 5, 2179
|[[File:SE2197Jun15A.png|150px]]<br />Jun 15, 2197
|[[File:SE2215Jun28A.png|150px]]<br />Jun 28, 2215
|-
!41
!42
!43
|- style="text-align:center;"
|[[File:SE2233Jul08A.png|150px]]<br />Jul 8, 2233
|[[File:SE2251Jul19A.png|150px]]<br />Jul 19, 2251
|[[File:SE2269Jul29A.png|150px]] <br />Jul 29, 2269
|-
!44
!45
!46
|- style="text-align:center;"
|[[File:SE2287Aug10A.png|150px]]<br />Aug 10, 2287
|[[File:SE2305Aug21A.png|150px]]<br />Aug 21, 2305
|[[File:SE2323Sep01A.png|150px]]<br />Sep 1, 2323
|-
!47
!48
!49
|- style="text-align:center;"
|[[File:SE2341Sep12A.png|150px]]<br />Sep 12, 2341
|[[File:SE2359Sep23A.png|150px]]<br />Sep 23, 2359
|[[File:SE2377Oct03A.png|150px]] <br />Oct 3, 2377
|-
!50
!51
!52
|- style="text-align:center;"
|[[File:SE2395Oct14A.png|150px]]<br />Oct 14, 2395
|[[File:SE2413Oct25A.png|150px]]<br />Oct 25, 2413
|[[File:SE2431Nov05A.png|150px]] <br />Nov 5, 2431
|-
!53
|- style="text-align:center;"
|[[File:SE2449Nov15A.png|150px]] <br />Nov 15, 2449
|}

=== Tritos series ===
{{Tritos eclipse set info}}
{| class="wikitable collapsible collapsed"
!colspan=4|Series members between 1901 and 2100
|- style="text-align:center;"
|[[File:SE1903Sep21T.png|150px]]<br />[[solar eclipse of September 21, 1903|September 21, 1903]]<br />(Saros 123)
|[[File:SE1914Aug21T.png|150px]]<br />[[solar eclipse of August 21, 1914|August 21, 1914]]<br />(Saros 124)
|[[File:SE1925Jul20A.png|150px]]<br />[[solar eclipse of July 20, 1925|July 20, 1925]]<br />(Saros 125)
|- style="text-align:center;"
|[[File:SE1936Jun19T.png|150px]]<br />[[solar eclipse of June 19, 1936|June 19, 1936]]<br />(Saros 126)
|[[File:SE1947May20T.png|150px]]<br />[[solar eclipse of May 20, 1947|May 20, 1947]]<br />(Saros 127)
|[[File:SE1958Apr19A.png|150px]]<br />[[solar eclipse of April 19, 1958|April 19, 1958]]<br />(Saros 128)
|- style="text-align:center;"
|[[File:SE1969Mar18A.png|150px]]<br />[[solar eclipse of March 18, 1969|March 18, 1969]]<br />(Saros 129)
|[[File:SE1980Feb16T.png|150px]]<br />[[solar eclipse of February 16, 1980|February 16, 1980]]<br />(Saros 130)
|[[File:SE1991Jan15A.png|150px]]<br />[[solar eclipse of January 15, 1991|January 15, 1991]]<br />(Saros 131)
|- style="text-align:center;"
|[[File:SE2001Dec14A.png|150px]]<br />[[solar eclipse of December 14, 2001|December 14, 2001]]<br />(Saros 132)
|[[File:SE2012Nov13T.png|150px]]<br />[[solar eclipse of November 13, 2012|November 13, 2012]]<br />(Saros 133)
|[[File:SE2023Oct14A.png|150px]]<br />[[solar eclipse of October 14, 2023|October 14, 2023]]<br />(Saros 134)
|- style="text-align:center;"
|[[File:SE2034Sep12A.png|150px]]<br />[[solar eclipse of September 12, 2034|September 12, 2034]]<br />(Saros 135)
|[[File:SE2045Aug12T.png|150px]]<br />[[solar eclipse of August 12, 2045|August 12, 2045]]<br />(Saros 136)
|[[File:SE2056Jul12A.png|150px]]<br />[[solar eclipse of July 12, 2056|July 12, 2056]]<br />(Saros 137)
|- style="text-align:center;"
|[[File:SE2067Jun11A.png|150px]]<br />[[solar eclipse of June 11, 2067|June 11, 2067]]<br />(Saros 138)
|[[File:SE2078May11T.png|150px]]<br />[[solar eclipse of May 11, 2078|May 11, 2078]]<br />(Saros 139)
|[[File:SE2089Apr10A.png|150px]]<br />April 10, 2089<br />(Saros 140)
|- style="text-align:center;"
|[[File:SE2100Mar10A.png|150px]]<br />[[solar eclipse of March 10, 2100|March 10, 2100]]<br />(Saros 141)
|
|}

==Notes==
{{reflist}}
{{reflist}}


==References==
== External links ==
{{Solar eclipse NASA reference|2001/SE2089Apr10A|20890410}}
{{Solar eclipse NASA reference|2001/SE2089Apr10A|20890410}}


{{Solar eclipses}}
{{Solar eclipses}}
{{commonscat|Solar eclipse of 2089 April 10}}
{{astronomy-stub}}


[[Category:Annular solar eclipses|2089 4 10]]
[[Category:2089 in science]]
[[Category:2089 in science]]
[[Category:Solar eclipses|2089 4 10]]
[[Category:21st-century solar eclipses|2089 4 10]]
[[Category:Future solar eclipses|2089 4 10]]
{{Solar-eclipse-stub}}

Latest revision as of 18:01, 2 January 2022

Solar eclipse of April 10, 2089
Map
Type of eclipse
NatureAnnular
Gamma−0.3319
Magnitude0.9919
Maximum eclipse
Duration53 s (0 min 53 s)
Coordinates10°12′S 154°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
Saros140 (33 of 71)
Catalog # (SE5000)9708

An annular solar eclipse will occur on April 10, 2089. 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.

Related eclipses[edit]

Solar eclipses 2087–2090[edit]

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]

120 May 2, 2087

Partial
125 October 26, 2087

Partial
130 April 21, 2088

Total
135 October 14, 2088

Annular
140 April 10, 2089

Annular
145 October 4, 2089

Total
150 March 31, 2090

Partial
155 September 23, 2090

Total

Saros 140[edit]

It is a part of Saros cycle 140, repeating every 18 years, 11 days, containing 71 events. The series started with 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. The longest duration of totality was 4 minutes, 10 seconds on August 12, 1692.

Tritos series[edit]

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.

Notes[edit]

  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.

References[edit]