Solar eclipse of July 10, 1907
An annular solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, July 10, 1907, with a magnitude of 0.9456. 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. Occurring about 17 hours after apogee, the Moon's apparent diameter was smaller.
Annularity was visible from Chile, Bolivia, and Brazil. A partial eclipse was visible for most of South America and parts of southern Central America.
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.| Event | Time |
| First Penumbral External Contact | 1907 July 10 at 12:34:39.3 UTC |
| First Umbral External Contact | 1907 July 10 at 13:49:46.3 UTC |
| First Central Line | 1907 July 10 at 13:52:42.4 UTC |
| First Umbral Internal Contact | 1907 July 10 at 13:55:40.8 UTC |
| Ecliptic Conjunction | 1907 July 10 at 15:17:01.9 UTC |
| Greatest Duration | 1907 July 10 at 15:23:22.5 UTC |
| Greatest Eclipse | 1907 July 10 at 15:24:32.3 UTC |
| Equatorial Conjunction | 1907 July 10 at 15:26:36.7 UTC |
| Last Umbral Internal Contact | 1907 July 10 at 16:53:22.7 UTC |
| Last Central Line | 1907 July 10 at 16:56:20.7 UTC |
| Last Umbral External Contact | 1907 July 10 at 16:59:16.4 UTC |
| Last Penumbral External Contact | 1907 July 10 at 18:14:23.5 UTC |
| Parameter | Value |
| Eclipse Magnitude | 0.94562 |
| Eclipse Obscuration | 0.89421 |
| Gamma | −0.63126 |
| Sun Right Ascension | 07h14m35.6s |
| Sun Declination | +22°20'34.4" |
| Sun Semi-Diameter | 15'43.9" |
| Sun Equatorial Horizontal Parallax | 08.6" |
| Moon Right Ascension | 07h14m31.5s |
| Moon Declination | +21°46'36.5" |
| Moon Semi-Diameter | 14'42.3" |
| Moon Equatorial Horizontal Parallax | 0°53'58.2" |
| ΔT | 6.9 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.| July 10 Ascending node | July 25 Descending node |
| Annular solar eclipse Solar Saros 125 | Partial lunar eclipse Lunar Saros 137 |
Related eclipses
Eclipses in 1907
- A total solar eclipse on January 14.
- A partial lunar eclipse on January 29.An annular solar eclipse on July 10.
- A partial lunar eclipse on July 25.
Metonic
- Preceded by: Solar eclipse of September 21, 1903
- Followed by: Solar eclipse of April 28, 1911
Tzolkinex
- Preceded by: Solar eclipse of May 28, 1900
- Followed by: Solar eclipse of August 21, 1914
Half-Saros
- Preceded by: Lunar eclipse of July 3, 1898
- Followed by: Lunar eclipse of July 15, 1916
Tritos
- Preceded by: Solar eclipse of August 9, 1896
- Followed by: Solar eclipse of June 8, 1918
Solar Saros 125
- Preceded by: Solar eclipse of June 28, 1889
- Followed by: Solar eclipse of July 20, 1925
Inex
- Preceded by: Solar eclipse of July 29, 1878
- Followed by: Solar eclipse of June 19, 1936
Triad
- Preceded by: Solar eclipse of September 7, 1820
- Followed by: Solar eclipse of May 10, 1994