Solar eclipse of October 23, 2014
Solar eclipse of October 23, 2014 | |
---|---|
![]() From Minneapolis, near greatest eclipse | |
Type of eclipse | |
Nature | Partial |
Gamma | 1.0908 |
Magnitude | 0.8114 |
Maximum eclipse | |
Coordinates | 71°12′N 97°12′W / 71.2°N 97.2°W |
Times (UTC) | |
(P1) Partial begin | 19:37:30 |
Greatest eclipse | 21:45:39 |
(P4) Partial end | 23:51:36 |
References | |
Saros | 153 (9 of 70) |
Catalog # (SE5000) | 9540 |
A partial solar eclipse occurred at the Moon's ascending node of orbit on Thursday, October 23, 2014,[1][2] with a magnitude of 0.8114. 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. Occurring only 5.7 days after apogee (Apogee on October 18, 2014), the Moon's apparent diameter was smaller.
It was the 9th eclipse of the 153rd Saros cycle, which began with a partial eclipse on July 28, 1870 and will conclude with a partial eclipse on August 22, 3114.
Viewing[edit]
The center of the Moon's shadow missed the Earth, passing above the North Pole, but a partial eclipse was visible at sunrise (October 24 local time) in far eastern Russia, and before sunset (October 23) across most of North America.
![]() Animated path |
Gallery[edit]
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Photograph of the eclipse projected with binoculars in Puebla, Mexico
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Simulated greatest partiality from Nunavut, Canada at sunset
-
Seattle, Washington, 21:21 UTC
-
San Jose, California, 21:26 UTC. The eclipse coincided with giant sunspot region 2192, the largest seen in 24 years.[3]
-
Minneapolis, Minnesota at 21:34 UTC
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Buchanan, Virginia, 21:44 UTC
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Austin, Texas, 22:00 UTC
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Joshua Tree National Park, 22:14 UTC
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Mentor, Ohio, 22:15 UTC
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Los Altos, California, 22:16 UTC
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College of DuPage, 22:28 UTC
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Mountain View, California, 22:33 UTC
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Melbourne, Florida, 22:38 UTC
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Denver, Colorado, 22:40 UTC
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Palo Alto, California, 22:42 UTC
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Cupertino, California, 22:47 UTC
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Coralville, Iowa, 22:56 UTC
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Composite image from Melbourne, Florida
-
Composite image from Minneapolis, Minnesota
Related eclipses[edit]
Eclipses of 2014[edit]
- A total lunar eclipse on April 15.
- A non-central annular solar eclipse on April 29.
- A total lunar eclipse on October 8.
- A partial solar eclipse on October 23.
Metonic[edit]
- Preceded by: Solar eclipse of January 4, 2011
- Followed by: Solar eclipse of August 11, 2018
Tzolkinex[edit]
- Preceded by: Solar eclipse of September 11, 2007
- Followed by: Solar eclipse of December 4, 2021
Half-Saros[edit]
- Preceded by: Lunar eclipse of October 17, 2005
- Followed by: Lunar eclipse of October 28, 2023
Tritos[edit]
- Preceded by: Solar eclipse of November 23, 2003
- Followed by: Solar eclipse of September 21, 2025
Solar Saros 153[edit]
- Preceded by: Solar eclipse of October 12, 1996
- Followed by: Solar eclipse of November 3, 2032
Inex[edit]
- Preceded by: Solar eclipse of November 12, 1985
- Followed by: Solar eclipse of October 3, 2043
Triad[edit]
- Preceded by: Solar eclipse of December 24, 1927
- Followed by: Solar eclipse of August 24, 2101
Solar eclipses of 2011–2014[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.[4]
The 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 to 2014 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
118![]() Partial in Tromsø, Norway |
June 1, 2011![]() Partial |
1.21300 | 123![]() Hinode XRT footage |
November 25, 2011![]() Partial |
−1.05359 | |
128![]() Annularity in Red Bluff, CA, USA |
May 20, 2012![]() Annular |
0.48279 | 133![]() Totality in Mount Carbine, Queensland, Australia |
November 13, 2012![]() Total |
−0.37189 | |
138 Annularity in Churchills Head, Australia |
May 10, 2013![]() Annular |
−0.26937 | 143 Partial in Libreville, Gabon |
November 3, 2013![]() Hybrid |
0.32715 | |
148![]() Partial in Adelaide, Australia |
April 29, 2014![]() Annular (non-central) |
−0.99996 | 153![]() Partial in Minneapolis, MN, USA |
October 23, 2014![]() Partial |
1.09078 |
A total solar eclipse on March 20, 2015, and a partial solar eclipse of September 13, 2015 occur during the next lunar year set.
Saros 153[edit]
This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 annularity will be produced by member 38 at 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit.[5]
Series members 1–19 occur between 1870 and 2200: | ||
---|---|---|
1 | 2 | 3 |
![]() July 28, 1870 |
![]() August 7, 1888 |
![]() August 20, 1906 |
4 | 5 | 6 |
![]() August 30, 1924 |
![]() September 10, 1942 |
![]() September 20, 1960 |
7 | 8 | 9 |
![]() October 2, 1978 |
![]() October 12, 1996 |
![]() October 23, 2014 |
10 | 11 | 12 |
![]() November 3, 2032 |
![]() November 14, 2050 |
![]() November 24, 2068 |
13 | 14 | 15 |
![]() December 6, 2086 |
![]() December 17, 2104 |
![]() December 28, 2122 |
16 | 17 | 18 |
![]() January 8, 2141 |
![]() January 19, 2159 |
![]() January 29, 2177 |
19 | ||
![]() February 10, 2195 |
Metonic series[edit]
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 ascending node.
22 eclipse events between January 5, 1935 and August 11, 2018 | ||||
---|---|---|---|---|
January 4-5 | October 23-24 | August 10-12 | May 30-31 | March 18-19 |
111 | 113 | 115 | 117 | 119 |
![]() January 5, 1935 |
![]() August 12, 1942 |
![]() May 30, 1946 |
![]() March 18, 1950 | |
121 | 123 | 125 | 127 | 129 |
![]() January 5, 1954 |
![]() October 23, 1957 |
![]() August 11, 1961 |
![]() May 30, 1965 |
![]() March 18, 1969 |
131 | 133 | 135 | 137 | 139 |
![]() January 4, 1973 |
![]() October 23, 1976 |
![]() August 10, 1980 |
![]() May 30, 1984 |
![]() March 18, 1988 |
141 | 143 | 145 | 147 | 149 |
![]() January 4, 1992 |
![]() October 24, 1995 |
![]() August 11, 1999 |
![]() May 31, 2003 |
![]() March 19, 2007 |
151 | 153 | 155 | ||
![]() January 4, 2011 |
![]() October 23, 2014 |
![]() August 11, 2018 |
Notes[edit]
References[edit]
- ^ "Valpo glimpses eclipse". The Times. 2014-10-24. p. A9. Retrieved 2023-10-26 – via Newspapers.com.
- ^ "Sun and moon put on show". Merced Sun-Star. 2014-10-24. p. B1. Retrieved 2023-10-26 – via Newspapers.com.
- ^ "Gentle giant sunspot region 2192".
- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 153". eclipse.gsfc.nasa.gov.
![](https://cdn.statically.io/img/upload.wikimedia.org/wikipedia/en/thumb/4/4a/Commons-logo.svg/30px-Commons-logo.svg.png)
External links[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC