Solar eclipse of July 10, 1907
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, July 10, 1907,[1][2][3][4] 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 (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 17 hours after apogee (on July 9, 1907, at 22:20 UTC), the Moon's apparent diameter was smaller.[5]
Annularity was visible from Chile, Bolivia (including its capital Sucre), 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.[6]
| Event | Time (UTC) |
|---|---|
| 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
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.
| July 10 Ascending node (new moon) |
July 25 Descending node (full moon) |
|---|---|
| File:SE1907Jul10A.png | File:Lunar eclipse chart close-1907Jul25.png |
| 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
Solar eclipses of 1906–1909
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 February 23, 1906 and August 20, 1906 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 1906 to 1909 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 115 | July 21, 1906 File:SE1906Jul21P.png Partial |
−1.3637 | 120 | January 14, 1907 File:SE1907Jan14T.png Total |
0.8628 | |
| 125 | July 10, 1907 File:SE1907Jul10A.png Annular |
−0.6313 | 130 | January 3, 1908 File:SE1908Jan03T.png Total |
0.1934 | |
| 135 | June 28, 1908 File:SE1908Jun28A.png Annular |
0.1389 | 140 | December 23, 1908 File:SE1908Dec23H.png Hybrid |
−0.4985 | |
| 145 | June 17, 1909 File:SE1909Jun17H.png Hybrid |
0.8957 | 150 | December 12, 1909 File:SE1909Dec12P.png Partial |
−1.2456 | |
Saros 125
Template:Solar Saros series 125
Metonic series
Template:Solar Metonic series 1880–1964
Tritos series
Template:Solar Tritos series 2005 October 3
Inex series
Template:Solar Inex series 2023 April 20
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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