Solar eclipse of November 11, 1901
An annular solar eclipse occurred at the Moon's ascending node of orbit on Monday, November 11, 1901, with a magnitude of 0.9216. 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 4.5 hours before apogee, the Moon's apparent diameter was smaller.
Annularity was visible from the Italian island Sicily, the whole British Malta, Ottoman Tripolitania, Egypt, Ottoman Empire, Emirate of Jabal Shammar, Aden Protectorate, Muscat and Oman, British Raj, British Ceylon, Siam, French Indochina, Bombay Reef in the Paracel Islands, and Philippines. A partial eclipse was visible for parts of North Africa, East Africa, most of Asia, and Northern Australia.
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 | 1901 November 11 at 04:29:38.4 UTC |
| First Umbral External Contact | 1901 November 11 at 05:39:58.5 UTC |
| First Central Line | 1901 November 11 at 05:43:40.3 UTC |
| First Umbral Internal Contact | 1901 November 11 at 05:47:24.1 UTC |
| Equatorial Conjunction | 1901 November 11 at 07:17:59.6 UTC |
| Greatest Eclipse | 1901 November 11 at 07:28:20.9 UTC |
| Ecliptic Conjunction | 1901 November 11 at 07:34:04.9 UTC |
| Greatest Duration | 1901 November 11 at 07:34:34.5 UTC |
| Last Umbral Internal Contact | 1901 November 11 at 09:09:25.3 UTC |
| Last Central Line | 1901 November 11 at 09:13:09.0 UTC |
| Last Umbral External Contact | 1901 November 11 at 09:16:50.9 UTC |
| Last Penumbral External Contact | 1901 November 11 at 10:27:08.6 UTC |
| Parameter | Value |
| Eclipse Magnitude | 0.92156 |
| Eclipse Obscuration | 0.84926 |
| Gamma | 0.47576 |
| Sun Right Ascension | 15h03m02.2s |
| Sun Declination | -17°15'48.8" |
| Sun Semi-Diameter | 16'09.6" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 15h03m21.4s |
| Moon Declination | -16°50'38.2" |
| Moon Semi-Diameter | 14'41.8" |
| Moon Equatorial Horizontal Parallax | 0°53'56.3" |
| ΔT | -0.3 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.| October 27 Descending node | November 11 Ascending node |
| Partial lunar eclipse Lunar Saros 115 | Annular solar eclipse Solar Saros 141 |
Related eclipses
Eclipses in 1901
- A penumbral lunar eclipse on May 3.
- A total solar eclipse on May 18.
- A partial lunar eclipse on October 27.
- '''An annular solar eclipse on November 11.'''
Metonic
- Preceded by: Solar eclipse of January 22, 1898
- Followed by: Solar eclipse of August 30, 1905
Tzolkinex
- Preceded by: Solar eclipse of September 29, 1894
- Followed by: Solar eclipse of December 23, 1908
Half-Saros
- Preceded by: Lunar eclipse of November 4, 1892
- Followed by: Lunar eclipse of November 17, 1910
Tritos
- Preceded by: Solar eclipse of December 12, 1890
- Followed by: Solar eclipse of October 10, 1912
Solar Saros 141
- Preceded by: Solar eclipse of October 30, 1883
- Followed by: Solar eclipse of November 22, 1919
Inex
- Preceded by: Solar eclipse of November 30, 1872
- Followed by: Solar eclipse of October 21, 1930
Triad
- Preceded by: Solar eclipse of January 10, 1815
- Followed by: Solar eclipse of September 11, 1988