Solar eclipse of May 20, 2012

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Solar eclipse of May 20, 2012
SE2012May20A.png
Map
Type of eclipse
Nature Annular
Gamma 0.4828
Magnitude 0.9439
Maximum eclipse
Duration 5m 46s
Coordinates 49.1N 176.3E
Max. width of band 237 km
Times (UTC)
(P1) Partial begin 20:56:07
(U1) Total begin 22:06:17
Greatest eclipse 23:53:54
(U4) Total end 1:39:11
(P4) Partial end 2:49:21
References
Saros 128 (58 of 73)
Catalog # (SE5000) 9535

An annular solar eclipse took place on May 20, 2012 (May 21, 2012 for local time in Eastern Hemisphere), with a magnitude of 0.9439. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, causing the Sun to look like an annulus (ring), blocking most of the Sun's light. An annular eclipse appears as a partial eclipse over a region thousands of kilometres wide. This is also known as Ring of Fire.[1]

Contents

[edit] Visibility

The annular phase was visible at sunrise on May 21 from the Chinese coast, northern Taiwan, the south of Japan, and before sunset on May 20th from the western part of the United States. Guangzhou, Taipei, Tokyo and Albuquerque were on the central path. Its maximum occurred in part of the North Pacific, south of the Aleutian islands for 5 min and 46.3 s, and finished in the western United States.[2]

North America

It was the first central eclipse of the 21st century in the continental USA, and also the first annular eclipse there since the solar eclipse of May 10, 1994 which was also the previous eclipse of this series Solar Saros 128.

Eclipse2012animation.gif
Animation as viewed from Albuquerque, New Mexico, showing sunset before the eclipse ends
SE2012May20A.gif
Animation of eclipse path from space

[edit] Photo Gallery

Asia

North America

[edit] Related eclipses

[edit] Solar eclipses 2011-2014

This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.

Note: Partial solar eclipses on January 4, 2011 and July 1, 2011 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2011–2014
Descending node   Ascending node
118 June 1, 2011
SE2011Jun01P.png
Partial
123 November 25, 2011
SE2011Nov25P.png
Partial
128 May 20, 2012
SE2012May20A.png
Annular
133 November 13, 2012
SE2012Nov13T.png
Total
138 May 10, 2013
SE2013May10A.png
Annular
143 November 3, 2013
SE2013Nov03H.png
Hybrid
148 April 29, 2014
SE2014Apr29A.png
Annular
153 October 23, 2014
SE2014Oct23P.png
Partial

[edit] Saros 128

It is a part of Saros cycle 128, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471 and hybrid eclipses from June 28, 1489 through July 31, 1543. Then it progresses into annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. The longest duration of totality was 1 minutes, 45 seconds on June 7, 1453.[3]

Series members 52-62 occur between 1901 and 2100:

52 53 54
SE1904Mar17A.png
March 17, 1904
SE1922Mar28A.png
March 28, 1922
SE1940Apr07A.png
April 7, 1940
55 56 57
SE1958Apr19A.png
April 19, 1958
SE1976Apr29A.png
April 29, 1976
SE1994May10A.png
May 10, 1994
58 59 60
SE2012May20A.png
May 20, 2012
SE2030Jun01A.png
June 1, 2030
SE2048Jun11A.png
June 11, 2048
61 62
SE2066Jun22A.png
June 22, 2066
SE2084Jul03A.png
July 3, 2084

[edit] 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).

This series has 21 eclipse events between May 21, 1993 and May 20, 2069.

May 20-21 March 9 December 25-26 October 13-14 August 1-2
118 120 122 124 126
SE1993May21P.png
May 21, 1993
SE1997Mar09T.png
March 9, 1997
SE2000Dec25P.png
December 25, 2000
SE2004Oct14P.png
October 14, 2004
SE2008Aug01T.png
August 1, 2008
128 130 132 134 136
SE2012May20A.png
May 20, 2012
SE2016Mar09T.png
March 9, 2016
SE2019Dec26A.png
December 26, 2019
SE2023Oct14A.png
October 14, 2023
SE2027Aug02T.png
August 2, 2027
138 140 142 144 146
SE2031May21A.png
May 21, 2031
SE2035Mar09A.png
March 9, 2035
SE2038Dec26T.png
December 26, 2038
SE2042Oct14A.png
October 14, 2042
SE2046Aug02T.png
August 2, 2046
148 150 152 154 156
SE2050May20H.png
May 20, 2050
SE2054Mar09P.png
March 9, 2054
SE2057Dec26T.png
December 26, 2057
SE2061Oct13A.png
October 13, 2061
SE2065Aug02P.png
August 2, 2065
158
SE2069May20P.png
May 20, 2069

[edit] Notes

[edit] References

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