Solar eclipse of April 19, 2004
A partial solar eclipse occurred at the Moon's ascending node of orbit on Monday, April 19, 2004, with a magnitude of 0.7367. 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.
The eclipse was largely visible over the south Atlantic Ocean and north shores of Antarctica, most prominently the Antarctic Peninsula. The eclipse could also be seen in southern Africa at sunset. Considering the magnitude and the solar altitude, South Africa was the best place to observe this eclipse. In Cape Town, the Sun was about 40% obscured, while in Pretoria the Sun was 29% obscured. Further north, the eclipse remained visible up to Angola, the southern Democratic Republic of the Congo and Tanzania.
Images
Animated eclipse pathEclipse 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.| Event | Time |
| First Penumbral External Contact | 2004 April 19 at 11:30:59.6 UTC |
| Equatorial Conjunction | 2004 April 19 at 12:30:29.4 UTC |
| Ecliptic Conjunction | 2004 April 19 at 13:22:15.9 UTC |
| Greatest Eclipse | 2004 April 19 at 13:35:05.3 UTC |
| Last Penumbral External Contact | 2004 April 19 at 15:39:41.1 UTC |
| Parameter | Value |
| Eclipse Magnitude | 0.73674 |
| Eclipse Obscuration | 0.65501 |
| Gamma | −1.13345 |
| Sun Right Ascension | 01h50m58.6s |
| Sun Declination | +11°24'41.2" |
| Sun Semi-Diameter | 15'55.2" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 01h52m50.5s |
| Moon Declination | +10°28'42.9" |
| Moon Semi-Diameter | 15'01.7" |
| Moon Equatorial Horizontal Parallax | 0°55'09.3" |
| ΔT | 64.6 s |
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months 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.| April 19 Ascending node | May 4 Descending node |
| Partial solar eclipse Solar Saros 119 | Total lunar eclipse Lunar Saros 131 |
Related eclipses
Eclipses in 2004
A partial solar eclipse on April 19.- A total lunar eclipse on May 4.
- A partial solar eclipse on October 14.
- A total lunar eclipse on October 28.
Metonic
- Preceded by: Solar eclipse of July 1, 2000
- Followed by: Solar eclipse of February 7, 2008
Tzolkinex
- Preceded by: Solar eclipse of March 9, 1997
- Followed by: Solar eclipse of June 1, 2011
Half-Saros
- Preceded by: Lunar eclipse of April 15, 1995
- Followed by: Lunar eclipse of April 25, 2013
Tritos
- Preceded by: Solar eclipse of May 21, 1993
- Followed by: Solar eclipse of March 20, 2015
Solar Saros 119
- Preceded by: Solar eclipse of April 9, 1986
- Followed by: Solar eclipse of April 30, 2022
Inex
- Preceded by: Solar eclipse of May 11, 1975
- Followed by: Solar eclipse of March 30, 2033
Triad
- Preceded by: Solar eclipse of June 19, 1917
- Followed by: Solar eclipse of February 18, 2091