Solar eclipse of September 21, 1903
Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, September 21, 1903,[1][2][3][4] with a magnitude of 1.0316. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.1 days after perigee (on September 19, 1904, at 2:00 UTC), the Moon's apparent diameter was larger.[5]
The path of totality crossed Antarctica and the south Indian Ocean. A partial eclipse was visible for parts of Southeast Africa, Southern Australia, New Zealand, and Antarctica.
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.[6]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1903 September 21 at 02:27:46.5 UTC |
| First Umbral External Contact | 1903 September 21 at 03:52:01.4 UTC |
| First Central Line | 1903 September 21 at 03:53:33.3 UTC |
| First Umbral Internal Contact | 1903 September 21 at 03:55:07.6 UTC |
| Ecliptic Conjunction | 1903 September 21 at 04:30:40.1 UTC |
| Greatest Duration | 1903 September 21 at 04:38:45.6 UTC |
| Greatest Eclipse | 1903 September 21 at 04:39:51.9 UTC |
| Equatorial Conjunction | 1903 September 21 at 05:10:23.8 UTC |
| Last Umbral Internal Contact | 1903 September 21 at 05:24:15.9 UTC |
| Last Central Line | 1903 September 21 at 05:25:48.2 UTC |
| Last Umbral External Contact | 1903 September 21 at 05:27:18.0 UTC |
| Last Penumbral External Contact | 1903 September 21 at 06:51:47.0 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.03156 |
| Eclipse Obscuration | 1.06411 |
| Gamma | −0.89674 |
| Sun Right Ascension | 11h49m03.6s |
| Sun Declination | +01°11'08.7" |
| Sun Semi-Diameter | 15'55.9" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 11h47m57.9s |
| Moon Declination | +00°20'09.1" |
| Moon Semi-Diameter | 16'19.2" |
| Moon Equatorial Horizontal Parallax | 0°59'53.7" |
| ΔT | 2.2 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| September 21 Ascending node (new moon) |
October 6 Descending node (full moon) |
|---|---|
| File:SE1903Sep21T.png | File:Lunar eclipse chart close-1903Oct06.png |
| Total solar eclipse Solar Saros 123 |
Partial lunar eclipse |
Related eclipses
Eclipses in 1903
- An annular solar eclipse on March 29.
- A partial lunar eclipse on April 12.
- A total solar eclipse on September 21.
- A partial lunar eclipse on October 6.
Metonic
- Preceded by: Solar eclipse of December 3, 1899
- Followed by: Solar eclipse of July 10, 1907
Tzolkinex
- Preceded by: Solar eclipse of August 9, 1896
- Followed by: Solar eclipse of November 2, 1910
Half-Saros
- Preceded by: Lunar eclipse of September 15, 1894
- Followed by: Lunar eclipse of September 26, 1912
Tritos
- Preceded by: Solar eclipse of October 20, 1892
- Followed by: Solar eclipse of August 21, 1914
Solar Saros 123
- Preceded by: Solar eclipse of September 8, 1885
- Followed by: Solar eclipse of October 1, 1921
Inex
- Preceded by: Solar eclipse of October 10, 1874
- Followed by: Solar eclipse of August 31, 1932
Triad
- Preceded by: Solar eclipse of November 19, 1816
- Followed by: Solar eclipse of July 22, 1990
Solar eclipses of 1902–1906
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[7]
The partial solar eclipses on May 7, 1902 and October 31, 1902 occur in the previous lunar year eclipse set, and the partial solar eclipse on July 21, 1906 occurs in the next lunar year eclipse set.
| Solar eclipse series sets from 1902 to 1906 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 108 | April 8, 1902 File:SE1902Apr08P.png Partial |
1.5024 | 113 | October 1, 1902 | ||
| 118 | March 29, 1903 File:SE1903Mar29A.png Annular |
0.8413 | 123 | September 21, 1903 File:SE1903Sep21T.png Total |
−0.8967 | |
| 128 | March 17, 1904 File:SE1904Mar17A.png Annular |
0.1299 | 133 | September 9, 1904 File:SE1904Sep09T.png Total |
−0.1625 | |
| 138 | March 6, 1905 File:SE1905Mar06A.png Annular |
−0.5768 | 143 File:PSM V68 D565 Sun corona of August 30 1905 taken with 40 foot camera.png |
August 30, 1905 File:SE1905Aug30T.png Total |
0.5708 | |
| 148 | February 23, 1906 File:SE1906Feb23P.png Partial |
−1.2479 | 153 | August 20, 1906 File:SE1906Aug20P.png Partial |
1.3731 | |
Saros 123
Template:Solar Saros series 123
Metonic series
Template:Solar Metonic series 1880–1964
Tritos series
Template:Solar Tritos series 2001 December 14
Inex series
Template:Solar Inex series 2019 July 2
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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