Solar eclipse of January 4, 2011

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Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, January 4, 2011,[1][2][3] with a magnitude of 0.8576. 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.

This was the first of four partial solar eclipses in 2011, with the others occurring on June 1, July 1, and November 25.

The greatest eclipse occurred at 08:51 UTC in northern Sweden. At that time, the axis of the Moon's shadow passed a mere 510 km above Earth's surface.[4]

The eclipse was visible near sunrise over most of Europe before moving over central Asia. It ended at sunset over east Asia. It was visible as a minor partial eclipse over north Africa and the Middle East.

Visibility

File:SE2011Jan04P.gif
Animated path

Photo gallery

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[5]

January 4, 2011 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2011 January 4 at 06:41:18.7 UTC
Greatest Eclipse 2011 January 4 at 08:51:42.4 UTC
Ecliptic Conjunction 2011 January 4 at 09:03:43.1 UTC
Equatorial Conjunction 2011 January 4 at 09:16:20.6 UTC
Last Penumbral External Contact 2011 January 4 at 11:02:01.4 UTC
January 4, 2011 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.85759
Eclipse Obscuration 0.79839
Gamma 1.06265
Sun Right Ascension 18h59m14.9s
Sun Declination -22°44'21.1"
Sun Semi-Diameter 16'15.9"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 18h58m23.8s
Moon Declination -21°46'01.2"
Moon Semi-Diameter 15'18.1"
Moon Equatorial Horizontal Parallax 0°56'09.6"
ΔT 66.3 s

Eclipse season

Script error: No such module "Labelled list hatnote". This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of December 2010–January 2011
December 21
Descending node (full moon)
January 4
Ascending node (new moon)
File:Lunar eclipse chart close-10dec21.png File:SE2011Jan04P.png
Total lunar eclipse
Lunar Saros 125
Partial solar eclipse
Solar Saros 151

Related eclipses

Eclipses in 2011

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 151

Inex

Triad

Solar eclipses of 2008–2011

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.[6]

The partial solar eclipses on June 1, 2011 and November 25, 2011 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2008 to 2011
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
121
File:Solar eclipse 2008Feb07-New Zealand-partial-Greg Hewgill.jpg
Partial in Christchurch, New Zealand
February 7, 2008
File:SE2008Feb07A.png
Annular
−0.95701 126
File:Corona.jpg
Totality in Kumul, Xinjiang, China
August 1, 2008
File:SE2008Aug01T.png
Total
0.83070
131
File:Annular solar eclipse pky.png
Annularity in Palangka Raya, Indonesia
January 26, 2009
File:SE2009Jan26A.png
Annular
−0.28197 136
File:Solar eclipse 22 July 2009 taken by Lutfar Rahman Nirjhar from Bangladesh.jpg
Totality in Kurigram District, Bangladesh
July 22, 2009
File:SE2009Jul22T.png
Total
0.06977
141
File:Solar annular eclipse of January 15, 2010 in Jinan, China.jpg
Annularity in Jinan, Shandong, China
January 15, 2010
File:SE2010Jan15A.png
Annular
0.40016 146
File:Eclipse 2010 Hao 1.JPG
Totality in Hao, French Polynesia
July 11, 2010
File:SE2010Jul11T.png
Total
−0.67877
151
File:Solar eclipse poland 4thjan2011.jpg
Partial in Poland
January 4, 2011
File:SE2011Jan04P.png
Partial
1.06265 156 July 1, 2011
File:SE2011Jul01P.png
Partial
−1.49171

Saros 151

Template:Solar Saros series 151

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). 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
File:SE1935Jan05P.png
January 5, 1935
File:SE1942Aug12P.png
August 12, 1942
File:SE1946May30P.png
May 30, 1946
File:SE1950Mar18A.png
March 18, 1950
121 123 125 127 129
File:SE1954Jan05A.png
January 5, 1954
File:SE1957Oct23T.png
October 23, 1957
File:SE1961Aug11A.png
August 11, 1961
File:SE1965May30T.png
May 30, 1965
File:SE1969Mar18A.png
March 18, 1969
131 133 135 137 139
File:SE1973Jan04A.png
January 4, 1973
File:SE1976Oct23T.png
October 23, 1976
File:SE1980Aug10A.png
August 10, 1980
File:SE1984May30A.png
May 30, 1984
File:SE1988Mar18T.png
March 18, 1988
141 143 145 147 149
File:SE1992Jan04A.png
January 4, 1992
File:SE1995Oct24T.png
October 24, 1995
File:SE1999Aug11T.png
August 11, 1999
File:SE2003May31A.png
May 31, 2003
File:SE2007Mar19P.png
March 19, 2007
151 153 155
File:SE2011Jan04P.png
January 4, 2011
File:SE2014Oct23P.png
October 23, 2014
File:SE2018Aug11P.png
August 11, 2018

Tritos series

Template:Solar Tritos series 2000 February 5

Inex series

Template:Solar Inex series 2011 January 4

Notes

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  4. Eclipses during 2011 NASA
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References

External links

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