An annular solar eclipse occurred at the Moon's ascending node of orbit between Friday, July 9 and Saturday, July 10, 1926,[1] with a magnitude of 0.968. 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 (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 4.3 days before apogee (on July 14, 1926, at 5:50 UTC), the Moon's apparent diameter was smaller.[2]
Annularity was visible from the islands of Pulo Anna and Merir in Japan's South Seas Mandate (now in Palau) and Wake Island on July 10 (Saturday), and Midway Atoll on July 9 (Friday). A partial eclipse was visible for parts of Northeast Asia, northern Oceania, Hawaii, southern North America, and Central America.
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.[3]
| First Penumbral External Contact | 1926 July 09 at 20:05:21.4 UTC | |
| First Umbral External Contact | 1926 July 09 at 21:08:43.5 UTC | |
| First Central Line | 1926 July 09 at 21:10:16.8 UTC | |
| First Umbral Internal Contact | 1926 July 09 at 21:11:50.1 UTC | |
| First Penumbral Internal Contact | 1926 July 09 at 22:15:23.2 UTC | |
| Equatorial Conjunction | 1926 July 09 at 23:05:52.4 UTC | |
| Greatest Eclipse | 1926 July 09 at 23:06:02.0 UTC | |
| Ecliptic Conjunction | 1926 July 09 at 23:06:39.5 UTC | |
| Greatest Duration | 1926 July 09 at 23:08:37.8 UTC | |
| Last Penumbral Internal Contact | 1926 July 09 at 23:56:40.1 UTC | |
| Last Umbral Internal Contact | 1926 July 10 at 01:00:12.3 UTC | |
| Last Central Line | 1926 July 10 at 01:01:48.0 UTC | |
| Last Umbral External Contact | 1926 July 10 at 01:03:23.6 UTC | |
| Last Penumbral External Contact | 1926 July 10 at 02:06:47.9 UTC |
| Eclipse Magnitude | 0.96799 | |
| Eclipse Obscuration | 0.93701 | |
| Gamma | 0.05379 | |
| Sun Right Ascension | 07h13m29.8s | |
| Sun Declination | +22°22'23.4" | |
| Sun Semi-Diameter | 15'43.9" | |
| Sun Equatorial Horizontal Parallax | 08.6" | |
| Moon Right Ascension | 07h13m30.1s | |
| Moon Declination | +22°25'20.5" | |
| Moon Semi-Diameter | 14'59.8" | |
| Moon Equatorial Horizontal Parallax | 0°55'02.2" | |
| ΔT | 24.2 s |
See also: Eclipse cycle. 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. The first and last eclipse in this sequence is separated by one synodic month.