Solar eclipse of April 10, 2089: Difference between revisions

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=== Saros 140 ===
=== Saros 140 ===
{{Template talk:Solar Saros series 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 23-33 occur between 1901 and 2100:
|-
!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
|- style="text-align:center;"
|[[File:SE2071Mar31A.png|150px]]<BR>[[solar eclipse of March 31, 2071|Mar 31, 2071]]
|[[File:SE2089Apr10A.png|150px]]<BR>[[solar eclipse of April 10, 2089|Apr 10, 2089]]
|}<noinclude>

{{template reference list}}

[[Category:Solar eclipse templates]]
</noinclude>


==Notes==
==Notes==

Revision as of 23:12, 30 May 2019

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

Solar eclipses 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.[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

Template talk:Solar Saros series 140

Notes

  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


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