Solar eclipse of March 19, 2007

Last updated
Solar eclipse of March 19, 2007
Solar Eclipse (3445953058) (cropped).jpg
From Jaipur, India at sunrise
SE2007Mar19P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0728
Magnitude 0.8756
Maximum eclipse
Coordinates 61°00′N55°30′E / 61°N 55.5°E / 61; 55.5
Times (UTC)
Greatest eclipse2:32:57
References
Saros 149 (20 of 71)
Catalog # (SE5000) 9523

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.

Contents

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

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
EventTime (UTC)
First Penumbral External Contact2007 March 19 at 00:39:26.5 UTC
Greatest Eclipse2007 March 19 at 02:32:57.5 UTC
Ecliptic Conjunction2007 March 19 at 02:43:39.1 UTC
Equatorial Conjunction2007 March 19 at 03:34:11.6 UTC
Last Penumbral External Contact2007 March 19 at 04:26:02.2 UTC
March 19, 2007 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.87558
Eclipse Obscuration0.85148
Gamma1.07277
Sun Right Ascension23h53m04.0s
Sun Declination-00°45'04.8"
Sun Semi-Diameter16'04.0"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension23h50m57.2s
Moon Declination+00°12'14.7"
Moon Semi-Diameter16'40.7"
Moon Equatorial Horizontal Parallax1°01'12.5"
ΔT65.2 s

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.

Eclipse season of March 2007
March 3
Descending node (full moon)
March 19
Ascending node (new moon)
Lunar eclipse chart close-07mar03.png SE2007Mar19P.png
Total lunar eclipse
Lunar Saros 123
Partial solar eclipse
Solar Saros 149

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
SarosMapGammaSarosMapGamma
119 April 19, 2004
SE2004Apr19P.png
Partial
−1.13345124 October 14, 2004
SE2004Oct14P.png
Partial
1.03481
129
Solar eclipse at sunset (2937676527) (cropped).jpg
Partial in Naiguatá, Venezuela
April 8, 2005
SE2005Apr08H.png
Hybrid
−0.34733134
Ecl-ann.jpg
Annularity in Madrid, Spain
October 3, 2005
SE2005Oct03A.png
Annular
0.33058
139
Diamondring-eclipse-March03-29-2006.jpg
Totality in Side, Turkey
March 29, 2006
SE2006Mar29T.png
Total
0.38433144
Helder da Rocha - Partial solar eclipse (by-sa).jpg
Partial in São Paulo, Brazil
September 22, 2006
SE2006Sep22A.png
Annular
−0.40624
149
Solar Eclipse (3445953058) (cropped).jpg
Partial in Jaipur, India
March 19, 2007
SE2007Mar19P.png
Partial
1.07277154
Eclipse solar 01 (1360685468) (cropped).jpg
Partial in Córdoba, Argentina
September 11, 2007
SE2007Sep11P.png
Partial
−1.12552

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. [6]

Series members 9–30 occur between 1801 and 2200:
91011
SE1808Nov18P.gif
November 18, 1808
SE1826Nov29P.gif
November 29, 1826
SE1844Dec09P.gif
December 9, 1844
121314
SE1862Dec21P.gif
December 21, 1862
SE1880Dec31P.gif
December 31, 1880
SE1899Jan11P.gif
January 11, 1899
151617
SE1917Jan23P.png
January 23, 1917
SE1935Feb03P.png
February 3, 1935
SE1953Feb14P.png
February 14, 1953
181920
SE1971Feb25P.png
February 25, 1971
SE1989Mar07P.png
March 7, 1989
SE2007Mar19P.png
March 19, 2007
212223
SE2025Mar29P.png
March 29, 2025
SE2043Apr09T.png
April 9, 2043
SE2061Apr20T.png
April 20, 2061
242526
SE2079May01T.png
May 1, 2079
SE2097May11T.png
May 11, 2097
SE2115May24T.png
May 24, 2115
272829
SE2133Jun03T.png
June 3, 2133
Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
SE2169Jun25T.png
June 25, 2169
30
Saros149 30van71 SE2187Jul06T.jpg
July 6, 2187

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 4–5October 23–24August 10–12May 30–31March 18–19
111113115117119
SE1935Jan05P.png
January 5, 1935
SE1942Aug12P.png
August 12, 1942
SE1946May30P.png
May 30, 1946
SE1950Mar18A.png
March 18, 1950
121123125127129
SE1954Jan05A.png
January 5, 1954
SE1957Oct23T.png
October 23, 1957
SE1961Aug11A.png
August 11, 1961
SE1965May30T.png
May 30, 1965
SE1969Mar18A.png
March 18, 1969
131133135137139
SE1973Jan04A.png
January 4, 1973
SE1976Oct23T.png
October 23, 1976
SE1980Aug10A.png
August 10, 1980
SE1984May30A.png
May 30, 1984
SE1988Mar18T.png
March 18, 1988
141143145147149
SE1992Jan04A.png
January 4, 1992
SE1995Oct24T.png
October 24, 1995
SE1999Aug11T.png
August 11, 1999
SE2003May31A.png
May 31, 2003
SE2007Mar19P.png
March 19, 2007
151153155
SE2011Jan04P.png
January 4, 2011
SE2014Oct23P.png
October 23, 2014
SE2018Aug11P.png
August 11, 2018

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.

Series members between 1801 and 2105
SE1810Sep28A.gif
September 28, 1810
(Saros 131)
SE1821Aug27A.gif
August 27, 1821
(Saros 132)
SE1832Jul27T.gif
July 27, 1832
(Saros 133)
SE1843Jun27H.gif
June 27, 1843
(Saros 134)
SE1854May26A.png
May 26, 1854
(Saros 135)
SE1865Apr25T.png
April 25, 1865
(Saros 136)
SE1876Mar25A.gif
March 25, 1876
(Saros 137)
SE1887Feb22A.png
February 22, 1887
(Saros 138)
SE1898Jan22T.png
January 22, 1898
(Saros 139)
SE1908Dec23H.png
December 23, 1908
(Saros 140)
SE1919Nov22A.png
November 22, 1919
(Saros 141)
SE1930Oct21T.png
October 21, 1930
(Saros 142)
SE1941Sep21T.png
September 21, 1941
(Saros 143)
SE1952Aug20A.png
August 20, 1952
(Saros 144)
SE1963Jul20T.png
July 20, 1963
(Saros 145)
SE1974Jun20T.png
June 20, 1974
(Saros 146)
SE1985May19P.png
May 19, 1985
(Saros 147)
SE1996Apr17P.png
April 17, 1996
(Saros 148)
SE2007Mar19P.png
March 19, 2007
(Saros 149)
SE2018Feb15P.png
February 15, 2018
(Saros 150)
SE2029Jan14P.png
January 14, 2029
(Saros 151)
SE2039Dec15T.png
December 15, 2039
(Saros 152)
SE2050Nov14P.png
November 14, 2050
(Saros 153)
SE2061Oct13A.png
October 13, 2061
(Saros 154)
SE2072Sep12T.png
September 12, 2072
(Saros 155)
SE2083Aug13P.png
August 13, 2083
(Saros 156)
SE2094Jul12P.png
July 12, 2094
(Saros 157)
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105
(Saros 158)

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.

Series members between 1801 and 2200
SE1804Aug05T.gif
August 5, 1804
(Saros 142)
SE1833Jul17T.gif
July 17, 1833
(Saros 143)
SE1862Jun27P.gif
June 27, 1862
(Saros 144)
SE1891Jun06A.gif
June 6, 1891
(Saros 145)
SE1920May18P.png
May 18, 1920
(Saros 146)
SE1949Apr28P.png
April 28, 1949
(Saros 147)
SE1978Apr07P.png
April 7, 1978
(Saros 148)
SE2007Mar19P.png
March 19, 2007
(Saros 149)
SE2036Feb27P.png
February 27, 2036
(Saros 150)
SE2065Feb05P.png
February 5, 2065
(Saros 151)
SE2094Jan16T.png
January 16, 2094
(Saros 152)
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
(Saros 153)
Saros154 14van71 SE2151Dec08A.jpg
December 8, 2151
(Saros 154)
Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
(Saros 155)

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of March 30, 2052</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, March 30, 2052, with a magnitude of 1.0466. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The path of totality will cross central Mexico and the southeastern states of the United States. Almost all of North America and the northern edge of South America will see a partial eclipse. It will be the 2nd total eclipse visible from the Florida Panhandle and southwest Georgia in 6.6 years. It will be the first total solar eclipse visible from Solar Saros 130 in 223 synodic months. It will be the last total solar eclipse visible in the United States until May 11, 2078.

<span class="mw-page-title-main">Solar eclipse of September 23, 2033</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Friday, September 23, 2033, with a magnitude of 0.689. 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.

<span class="mw-page-title-main">Solar eclipse of February 27, 2036</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Wednesday, February 27, 2036, with a magnitude of 0.6286. 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.

<span class="mw-page-title-main">Solar eclipse of August 21, 2036</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Thursday, August 21, 2036, with a magnitude of 0.8622. 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.

<span class="mw-page-title-main">Solar eclipse of February 25, 1971</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of orbit on Thursday, February 25, 1971, with a magnitude of 0.7872. 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.

<span class="mw-page-title-main">Solar eclipse of November 4, 2040</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, November 4, 2040, with a magnitude of 0.8074. 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.

<span class="mw-page-title-main">Solar eclipse of July 22, 2047</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Monday, July 22, 2047, with a magnitude of 0.3604. 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.

<span class="mw-page-title-main">Solar eclipse of November 14, 2050</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, November 14, 2050, with a magnitude of 0.8874. 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.

<span class="mw-page-title-main">Solar eclipse of January 16, 2075</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, January 16, 2075, with a magnitude of 1.0311. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of May 2, 2087</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, May 2, 2087, with a magnitude of 0.8011. 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.

<span class="mw-page-title-main">Solar eclipse of September 2, 2054</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, September 2, 2054, with a magnitude of 0.9793. 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.

<span class="mw-page-title-main">Solar eclipse of May 22, 2058</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, May 22, 2058, with a magnitude of 0.4141. 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.

<span class="mw-page-title-main">Solar eclipse of November 24, 2068</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Saturday, November 24, 2068, with a magnitude of 0.9109. 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.

<span class="mw-page-title-main">Solar eclipse of November 26, 2076</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Thursday, November 26, 2076, with a magnitude of 0.7315. 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.

<span class="mw-page-title-main">Solar eclipse of February 16, 2083</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, February 16, 2083, with a magnitude of 0.9433. 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.

<span class="mw-page-title-main">Solar eclipse of December 6, 2086</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Friday, December 6, 2086, with a magnitude of 0.9271. 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.

<span class="mw-page-title-main">Solar eclipse of April 1, 2098</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, April 1, 2098, with a magnitude of 0.7984. 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.

<span class="mw-page-title-main">Solar eclipse of October 26, 2087</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Sunday, October 26, 2087, with a magnitude of 0.4696. 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.

<span class="mw-page-title-main">Solar eclipse of March 31, 2090</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, March 31, 2090, with a magnitude of 0.7843. 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.

<span class="mw-page-title-main">Solar eclipse of September 10, 1942</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of orbit on Thursday, September 10, 1942, with a magnitude of 0.523. 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.

References

  1. "March 19, 2007 Partial Solar Eclipse". timeanddate. Retrieved 11 August 2024.
  2. "At a glance". The Daily Reporter. 2007-03-19. p. 2. Retrieved 2023-10-25 via Newspapers.com.
  3. "Southeast coast of India awakens to partial eclipse of the sun". The Toronto Star. 2007-03-20. p. 22. Retrieved 2023-10-25 via Newspapers.com.
  4. "Partial Solar Eclipse of 2007 Mar 19". EclipseWise.com. Retrieved 11 August 2024.
  5. 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.
  6. "NASA - Catalog of Solar Eclipses of Saros 149". eclipse.gsfc.nasa.gov.

Photos: