Solar eclipse of March 19, 2007

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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 Monday, March 19, 2007,[1][2][3] with a magnitude of 0.8756. 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 partial eclipse was visible from India at sunrise, across Asia and eastern part of European Russia, and ending near sunset over northern Alaska. The greatest eclipse was on north of Perm Krai, Russia.

Visibility

File:SE2007Mar19P.gif

Images

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.[4]

March 19, 2007 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2007 March 19 at 00:39:26.5 UTC
Greatest Eclipse 2007 March 19 at 02:32:57.5 UTC
Ecliptic Conjunction 2007 March 19 at 02:43:39.1 UTC
Equatorial Conjunction 2007 March 19 at 03:34:11.6 UTC
Last Penumbral External Contact 2007 March 19 at 04:26:02.2 UTC
March 19, 2007 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.87558
Eclipse Obscuration 0.85148
Gamma 1.07277
Sun Right Ascension 23h53m04.0s
Sun Declination -00°45'04.8"
Sun Semi-Diameter 16'04.0"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 23h50m57.2s
Moon Declination +00°12'14.7"
Moon Semi-Diameter 16'40.7"
Moon Equatorial Horizontal Parallax 1°01'12.5"
ΔT 65.2 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 March 2007
March 3
Descending node (full moon)
 March 19
Ascending node (new moon)
File:Lunar eclipse chart close-07mar03.png File:SE2007Mar19P.png
Total lunar eclipse
Lunar Saros 123		 Partial solar eclipse
Solar Saros 149

Related eclipses

Eclipses in 2007

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 149

Inex

Triad

Solar eclipses of 2004–2007

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.[5]

Solar eclipse series sets from 2004 to 2007
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 April 19, 2004
File:SE2004Apr19P.png
Partial 		−1.13345 124 October 14, 2004
File:SE2004Oct14P.png
Partial 		1.03481
129
File:Solar eclipse at sunset (2937676527) (cropped).jpg
Partial in Naiguatá, Venezuela 		April 8, 2005
File:SE2005Apr08H.png
Hybrid 		−0.34733 134
File:Ecl-ann.jpg
Annularity in Madrid, Spain 		October 3, 2005
File:SE2005Oct03A.png
Annular 		0.33058
139
File:Diamondring-eclipse-March03-29-2006.jpg
Totality in Side, Turkey 		March 29, 2006
File:SE2006Mar29T.png
Total 		0.38433 144
File:Helder da Rocha - Partial solar eclipse (by-sa).jpg
Partial in São Paulo, Brazil 		September 22, 2006
File:SE2006Sep22A.png
Annular 		−0.40624
149
File:Solar Eclipse (3445953058) (cropped).jpg
Partial in Jaipur, India 		March 19, 2007
File:SE2007Mar19P.png
Partial 		1.07277 154
File:Eclipse solar 01 (1360685468) (cropped).jpg
Partial in Córdoba, Argentina 		September 11, 2007
File:SE2007Sep11P.png
Partial 		−1.12552

Saros 149

Template:Solar Saros series 149

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 2007 March 19

Inex series

Template:Solar Inex series 2007 March 19

References

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  5. ↑ Script error: No such module "citation/CS1".

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Photos:

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