Solar eclipse of December 12, 1909
| Partial eclipse | |
| Gamma | −1.2456 |
|---|---|
| Magnitude | 0.5424 |
| Maximum eclipse | |
| Coordinates | Lua error: callParserFunction: function "#coordinates" was not found. |
| Times (UTC) | |
| Greatest eclipse | 19:44:48 |
| References | |
| Saros | 150 (11 of 71) |
| Catalog # (SE5000) | 9303 |
A partial solar eclipse occurred at the Moon's descending node of orbit on Sunday, December 12, 1909,[1][2][3] with a magnitude of 0.5424. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
This event was visible as a partial solar eclipse across Antarctica and New Zealand.
Eclipse details
[edit | edit source]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.[4]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1909 December 12 at 17:56:19.6 UTC |
| Greatest Eclipse | 1909 December 12 at 19:44:48.1 UTC |
| Ecliptic Conjunction | 1909 December 12 at 19:58:40.0 UTC |
| Equatorial Conjunction | 1909 December 12 at 20:09:23.5 UTC |
| Last Penumbral External Contact | 1909 December 12 at 21:33:01.1 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.54243 |
| Eclipse Obscuration | 0.42921 |
| Gamma | –1.24559 |
| Sun Right Ascension | 17h17m14.6s |
| Sun Declination | -23°05'16.7" |
| Sun Semi-Diameter | 16'14.8" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 17h16m22.9s |
| Moon Declination | -24°13'34.7" |
| Moon Semi-Diameter | 15'12.2" |
| Moon Equatorial Horizontal Parallax | 0°55'47.8" |
| ΔT | 10.4 s |
Eclipse season
[edit | edit source]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.
| November 27 Ascending node (full moon) |
December 12 Descending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-1909Nov27.png | File:SE1909Dec12P.png |
| Penumbral lunar eclipse Lunar Saros 124 |
Annular solar eclipse Solar Saros 150 |
Related eclipses
[edit | edit source]Eclipses in 1909
[edit | edit source]- A total lunar eclipse on June 4.
- A hybrid solar eclipse on June 17.
- A total lunar eclipse on November 27.
- A partial solar eclipse on December 12.
Metonic
[edit | edit source]- Preceded by: Solar eclipse of February 23, 1906
- Followed by: Solar eclipse of September 30, 1913
Tzolkinex
[edit | edit source]- Preceded by: Solar eclipse of October 31, 1902
- Followed by: Solar eclipse of January 23, 1917
Half-Saros
[edit | edit source]- Preceded by: Lunar eclipse of December 6, 1900
- Followed by: Lunar eclipse of December 17, 1918
Tritos
[edit | edit source]- Preceded by: Solar eclipse of January 11, 1899
- Followed by: Solar eclipse of November 10, 1920
Solar Saros 150
[edit | edit source]- Preceded by: Solar eclipse of December 1, 1891
- Followed by: Solar eclipse of December 24, 1927
Inex
[edit | edit source]- Preceded by: Solar eclipse of December 31, 1880
- Followed by: Solar eclipse of November 21, 1938
Triad
[edit | edit source]- Preceded by: Solar eclipse of February 11, 1823
- Followed by: Solar eclipse of October 12, 1996
Solar eclipses of 1906–1909
[edit | edit source]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.[5]
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 150
[edit | edit source]This eclipse is a part of Saros series 150, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no hybrid or total eclipses in this set. The series ends at member 71 as a partial eclipse on September 29, 2991. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity will be produced by member 45 at 9 minutes, 58 seconds on December 19, 2522. All eclipses in this series occur at the Moon’s descending node of orbit.[6]
Metonic series
[edit | edit source]The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.
Tritos series
[edit | edit source]This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 1964 | ||||
|---|---|---|---|---|
| File:SE1811Sep17A.gif September 17, 1811 (Saros 141) |
File:SE1822Aug16T.gif August 16, 1822 (Saros 142) |
File:SE1833Jul17T.gif July 17, 1833 (Saros 143) |
File:SE1844Jun16P.gif June 16, 1844 (Saros 144) |
File:SE1855May16P.gif May 16, 1855 (Saros 145) |
| File:SE1866Apr15P.gif April 15, 1866 (Saros 146) |
File:SE1877Mar15P.gif March 15, 1877 (Saros 147) |
File:SE1888Feb11P.gif February 11, 1888 (Saros 148) |
File:SE1899Jan11P.gif January 11, 1899 (Saros 149) |
File:SE1909Dec12P.png December 12, 1909 (Saros 150) |
| File:SE1920Nov10P.png November 10, 1920 (Saros 151) |
File:SE1931Oct11P.png October 11, 1931 (Saros 152) |
File:SE1942Sep10P.png September 10, 1942 (Saros 153) |
File:SE1953Aug09P.png August 9, 1953 (Saros 154) |
File:SE1964Jul09P.png July 9, 1964 (Saros 155) |
Inex series
[edit | edit source]This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||
|---|---|---|
| File:SE1823Feb11P.gif February 11, 1823 (Saros 147) |
File:SE1852Jan21P.png January 21, 1852 (Saros 148) |
File:SE1880Dec31P.gif December 31, 1880 (Saros 149) |
| File:SE1909Dec12P.png December 12, 1909 (Saros 150) |
File:SE1938Nov21P.png November 21, 1938 (Saros 151) |
File:SE1967Nov02T.png November 2, 1967 (Saros 152) |
| File:SE1996Oct12P.png October 12, 1996 (Saros 153) |
File:SE2025Sep21P.png September 21, 2025 (Saros 154) |
File:SE2054Sep02P.png September 2, 2054 (Saros 155) |
| File:SE2083Aug13P.png August 13, 2083 (Saros 156) |
File:Saros157 04van70 SE2112Jul23P.jpg July 23, 2112 (Saros 157) |
File:Saros158 05van70 SE2141Jul03P.jpg July 3, 2141 (Saros 158) |
| File:Saros159 03van70 SE2170Jun14P.jpg June 14, 2170 (Saros 159) |
File:Saros160 02van71 SE2199May24P.jpg May 24, 2199 (Saros 160) |
|
References
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External links
[edit | edit source]- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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