- Source: Solar eclipse of March 19, 2007
A partial solar eclipse occurred at the Moon's ascending node of orbit on Monday, March 19, 2007, 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
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.
Eclipse season
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.
Related eclipses
= Eclipses in 2007
=A total lunar eclipse on March 3.
A partial solar eclipse on March 19.
A total lunar eclipse on August 28.
A partial solar eclipse on September 11.
= Metonic
=Preceded by: Solar eclipse of May 31, 2003
Followed by: Solar eclipse of January 4, 2011
= Tzolkinex
=Preceded by: Solar eclipse of February 5, 2000
Followed by: Solar eclipse of April 29, 2014
= Half-Saros
=Preceded by: Lunar eclipse of March 13, 1998
Followed by: Lunar eclipse of March 23, 2016
= Tritos
=Preceded by: Solar eclipse of April 17, 1996
Followed by: Solar eclipse of February 15, 2018
= Solar Saros 149
=Preceded by: Solar eclipse of March 7, 1989
Followed by: Solar eclipse of March 29, 2025
= Inex
=Preceded by: Solar eclipse of April 7, 1978
Followed by: Solar eclipse of February 27, 2036
= Triad
=Preceded by: Solar eclipse of May 18, 1920
Followed by: Solar eclipse of January 16, 2094
= 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.
= Saros 149
=This eclipse is a part of Saros series 149, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 21, 1664. It contains total eclipses from April 9, 2043 through October 2, 2331; hybrid eclipses from October 13, 2349 through November 3, 2385; and annular eclipses from November 15, 2403 through July 13, 2800. The series ends at member 71 as a partial eclipse on September 28, 2926. 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 will be produced by member 31 at 4 minutes, 10 seconds on July 17, 2205, and the longest duration of annularity will be produced by member 62 at 5 minutes, 6 seconds on June 21, 2764. All eclipses in this series occur at the Moon’s ascending node of orbit.
= 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.
= Tritos series
=This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
The partial solar eclipses on December 7, 2170 (part of Saros 164) and November 7, 2181 (part of Saros 165) are also a part of this series but are not included in the table below.
= Inex series
=This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
References
NASA graphics
NASA map
Besselian Elements – Partial Solar Eclipse of 2007 March 19
Photos:
Spaceweather.com eclipse gallery
NASA Astronomy Picture of the Day: Goa Silhouettes, from Goa India (22 March 2007)
NASA Astronomy Picture of the Day: Touran Sunrise, from Touran Wildlife Reserve in northeastern Iran (23 March 2007)
Solar Eclipse – 19th March 2007 Deepu George V Mananthavady, Wayanad, Kerala, India
Kozlovskiy, Aleksandr (28 March 2007). "Март — месяц затмений (глазами очевидца)" [March [2007] is the month of eclipses (through the eyes of an eyewitness)] (in Russian). Retrieved 6 December 2019.
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- Solar eclipse of March 19, 2007
- Solar eclipse of March 29, 2025
- Solar eclipse of March 29, 2006
- Solar eclipse of March 17, 1904
- Solar eclipse of March 20, 2015
- List of solar eclipses in the 20th century
- Solar eclipse of April 8, 2024
- March 2025 lunar eclipse
- List of solar eclipses visible from Russia
- Solar eclipse of March 19, 2072
