Solar eclipse of October 14, 2004

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Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse occurred at the Moon's descending node of orbit between Wednesday, October 13 and Thursday, October 14, 2004,[1][2][3] with a magnitude of 0.9282. 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.

A partial eclipse was visible for parts of eastern Russia, Mongolia, northeastern China, Korea, Japan, Hawaii, and western Alaska.

Images

File:SE2004Oct14P.gif
Animated path

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]

October 14, 2004 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2004 October 14 at 00:55:42.4 UTC
Equatorial Conjunction 2004 October 14 at 02:01:31.9 UTC
Ecliptic Conjunction 2004 October 14 at 02:49:19.6 UTC
Greatest Eclipse 2004 October 14 at 03:00:23.0 UTC
Last Penumbral External Contact 2004 October 14 at 05:05:22.2 UTC
October 14, 2004 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.92826
Eclipse Obscuration 0.90617
Gamma 1.03481
Sun Right Ascension 13h18m00.5s
Sun Declination -08°14'10.7"
Sun Semi-Diameter 16'02.2"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 13h19m53.4s
Moon Declination -07°20'43.5"
Moon Semi-Diameter 15'55.4"
Moon Equatorial Horizontal Parallax 0°58'26.4"
ΔT 64.6 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 October 2004
October 14
Descending node (new moon)
October 28
Ascending node (full moon)
File:SE2004Oct14P.png File:Lunar eclipse chart close-04oct28.png
Partial solar eclipse
Solar Saros 124
Total lunar eclipse
Lunar Saros 136

Related eclipses

Eclipses in 2004

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 124

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 124

Template:Solar Saros series 124

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 descending node.

21 eclipse events between May 21, 1993 and May 20, 2069
May 20–21 March 9 December 25–26 October 13–14 August 1–2
118 120 122 124 126
File:SE1993May21P.png
May 21, 1993
File:SE1997Mar09T.png
March 9, 1997
File:SE2000Dec25P.png
December 25, 2000
File:SE2004Oct14P.png
October 14, 2004
File:SE2008Aug01T.png
August 1, 2008
128 130 132 134 136
File:SE2012May20A.png
May 20, 2012
File:SE2016Mar09T.png
March 9, 2016
File:SE2019Dec26A.png
December 26, 2019
File:SE2023Oct14A.png
October 14, 2023
File:SE2027Aug02T.png
August 2, 2027
138 140 142 144 146
File:SE2031May21A.png
May 21, 2031
File:SE2035Mar09A.png
March 9, 2035
File:SE2038Dec26T.png
December 26, 2038
File:SE2042Oct14A.png
October 14, 2042
File:SE2046Aug02T.png
August 2, 2046
148 150 152 154 156
File:SE2050May20H.png
May 20, 2050
File:SE2054Mar09P.png
March 9, 2054
File:SE2057Dec26T.png
December 26, 2057
File:SE2061Oct13A.png
October 13, 2061
File:SE2065Aug02P.png
August 2, 2065
158
File:SE2069May20P.png
May 20, 2069

Tritos series

Template:Solar Tritos series 2004 October 14

Inex series

Template:Solar Inex series 2004 October 14

References

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External links

Photos:

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