Jump to content

Solar eclipse of June 12, 2029: Difference between revisions

From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
No edit summary
Line 50: Line 50:


=== Saros 118 ===
=== Saros 118 ===
{{Solar Saros series 118}}
It is a part of [[Solar Saros 118|Saros cycle 118]], repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on May 24, 803 [[Common Era|CE]]. It contains total eclipses from August 19, 947 CE through October 25, 1650, hybrid eclipses on November 4, 1668, and November 15, 1686, and annular eclipses from November 27, 1704, through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. The longest duration of total was 6 minutes, 59 seconds on May 16, 1398.
{| class="wikitable collapsible collapsed"
!colspan=3|Series members 62–72 occur between 1901 and 2083:
|-
!62
!63
!64
|- style="text-align:center;"
|[[File:SE1903Mar29A.png|150px]]<br />[[solar eclipse of March 29, 1903|Mar 29, 1903]]
|[[File:SE1921Apr08A.png|150px]]<br />[[solar eclipse of April 8, 1921|Apr 8, 1921]]
|[[File:SE1939Apr19A.png|150px]]<br />[[solar eclipse of April 19, 1939|Apr 19, 1939]]
|-
!65
!66
!67
|- style="text-align:center;"
|[[File:SE1957Apr30A.png|150px]]<br />[[solar eclipse of April 30, 1957|Apr 30, 1957]]
|[[File:SE1975May11P.png|150px]]<br />[[solar eclipse of May 11, 1975|May 11, 1975]]
|[[File:SE1993May21P.png|150px]]<br />[[solar eclipse of May 21, 1993|May 21, 1993]]
|-
!68
!69
!70
|- style="text-align:center;"
|[[File:SE2011Jun01P.png|150px]]<br />[[solar eclipse of June 1, 2011|Jun 1, 2011]]
|[[File:SE2029Jun12P.png|150px]]<br />Jun 12, 2029
|[[File:SE2047Jun23P.png|150px]]<br />[[solar eclipse of June 23, 2047|Jun 23, 2047]]
|-
!71
!72
|- style="text-align:center;"
|[[File:SE2065Jul03P.png|150px]]<br />[[solar eclipse of July 3, 2065|Jul 3, 2065]]
|[[File:SE2083Jul15P.png|150px]]<br />[[solar eclipse of July 15, 2083|Jul 15, 2083]]
|}


=== Metonic series ===
=== Metonic series ===

Revision as of 02:22, 13 July 2024

Solar eclipse of June 12, 2029
Map
Type of eclipse
NaturePartial
Gamma1.2943
Magnitude0.4576
Maximum eclipse
Coordinates66°48′N 66°12′W / 66.8°N 66.2°W / 66.8; -66.2
Times (UTC)
Greatest eclipse4:06:13
References
Saros118 (69 of 72)
Catalog # (SE5000)9572

A partial solar eclipse will occur at the Moon's descending node of orbit on Tuesday, June 12, 2029, with a magnitude of 0.4576. 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. The eclipse will be visible from Northern and Central Europe, northern Russia, Arctic, Greenland, and northern North America.

This will be the second of four partial solar eclipses in 2029, with the others occurring on January 14, July 11, and December 5.

It also precedes the two total lunar eclipses occurring on June 26 and December 20.

Images


Animated path

Eclipses in 2029

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 118

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
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 118

This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

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).

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 118". eclipse.gsfc.nasa.gov.
Wikimedia Commons has media related to Solar eclipse of 2029 June 12.
Stub icon

This solar eclipse–related article is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=Solar_eclipse_of_June_12,_2029&oldid=1234193023"