Solar eclipse of April 29, 2014
An annular solar eclipse occurred at the Moon's descending node of orbit on Tuesday, April 29, 2014, with a magnitude of 0.9868. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus. An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The Moon's apparent diameter was near the average diameter because it occurred 6.2 days after perigee and 7.2 days before apogee.
This eclipse's gamma value was closer to 1 than any other eclipse from 2000 B.C. to 3000 A.D. This means the center of the Moon's shadow passed almost exactly at the surface of the Earth, barely missing the Antarctic continent by a few kilometers, but an annular eclipse was visible from a small part of Antarctica, and a partial eclipse was visible from parts of Antarctica and Australia.
Images
Animation of 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 | 2014 April 29 at 03:53:46.0 UTC |
| Equatorial Conjunction | 2014 April 29 at 05:38:58.2 UTC |
| First Umbral External Contact | 2014 April 29 at 05:58:45.6 UTC |
| Greatest Eclipse | 2014 April 29 at 06:04:32.9 UTC |
| Last Umbral Internal Contact | 2014 April 29 at 06:10:41.3 UTC |
| Ecliptic Conjunction | 2014 April 29 at 06:15:28.3 UTC |
| Last Penumbral External Contact | 2014 April 29 at 08:15:37.1 UTC |
| Parameter | Value |
| Eclipse Magnitude | 0.98679 |
| Eclipse Obscuration | - |
| Gamma | -0.99996 |
| Sun Right Ascension | 02h25m52.9s |
| Sun Declination | +14°26'54.2" |
| Sun Semi-Diameter | 15'52.9" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 02h26m46.0s |
| Moon Declination | +13°31'06.8" |
| Moon Semi-Diameter | 15'38.4" |
| Moon Equatorial Horizontal Parallax | 0°57'24.1" |
| ΔT | 67.3 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 15 Ascending node | April 29 Descending node |
| Total lunar eclipse Lunar Saros 122 | Annular solar eclipse Solar Saros 148 |
Related eclipses
Eclipses in 2014
- A total lunar eclipse on April 15.A non-central annular solar eclipse on April 29.
- A total lunar eclipse on October 8.
- A partial solar eclipse on October 23.
Metonic
- Preceded by: Solar eclipse of July 11, 2010
- Followed by: Solar eclipse of February 15, 2018
Tzolkinex
- Preceded by: Solar eclipse of March 19, 2007
- Followed by: Solar eclipse of June 10, 2021
Half-Saros
- Preceded by: Lunar eclipse of April 24, 2005
- Followed by: Lunar eclipse of May 5, 2023
Tritos
- Preceded by: Solar eclipse of May 31, 2003
- Followed by: Solar eclipse of March 29, 2025
Solar Saros 148
- Preceded by: Solar eclipse of April 17, 1996
- Followed by: Solar eclipse of May 9, 2032
Inex
- Preceded by: Solar eclipse of May 19, 1985
- Followed by: Solar eclipse of April 9, 2043
Triad
- Preceded by: Solar eclipse of June 29, 1927
- Followed by: Solar eclipse of February 28, 2101