Solar eclipse of January 3, 1927
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse occurred at the Moon's descending node of orbit between Monday, January 3 and Tuesday, January 4, 1927,[1] with a magnitude of 0.9995. 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. The Moon's apparent diameter was near the average diameter because it occurred 8.6 days after apogee (on December 26, 1926, at 7:10 UTC) and 3.3 days before perigee (on January 7, 1927, at 3:00 UTC).[2]
Annularity was visible from New Zealand on January 4 (Tuesday), and Chile, Argentina, Uruguay and southern Brazil on January 3 (Monday). A partial eclipse was visible for parts of Oceania, Antarctica, and South America.
Observations
File:Eclipse solar - Buenos Aires - 1927.jpg
View of the eclipse from Buenos Aires
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.[3]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1927 January 3 at 17:44:12.4 UTC |
| First Umbral External Contact | 1927 January 3 at 18:48:36.9 UTC |
| First Central Line | 1927 January 3 at 18:49:09.7 UTC |
| Greatest Duration | 1927 January 3 at 18:49:09.7 UTC |
| First Umbral Internal Contact | 1927 January 3 at 18:49:42.5 UTC |
| Greatest Eclipse | 1927 January 3 at 20:22:53.1 UTC |
| Equatorial Conjunction | 1927 January 3 at 20:23:09.7 UTC |
| Ecliptic Conjunction | 1927 January 3 at 20:28:11.0 UTC |
| Last Umbral Internal Contact | 1927 January 3 at 21:56:05.6 UTC |
| Last Central Line | 1927 January 3 at 21:56:35.8 UTC |
| Last Umbral External Contact | 1927 January 3 at 21:57:05.9 UTC |
| Last Penumbral External Contact | 1927 January 3 at 23:01:27.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.99947 |
| Eclipse Obscuration | 0.99894 |
| Gamma | −0.49559 |
| Sun Right Ascension | 18h54m14.6s |
| Sun Declination | -22°51'45.8" |
| Sun Semi-Diameter | 16'15.9" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 18h54m13.9s |
| Moon Declination | -23°20'50.4" |
| Moon Semi-Diameter | 16'01.7" |
| Moon Equatorial Horizontal Parallax | 0°58'49.4" |
| ΔT | 24.5 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.
| December 19 Ascending node (full moon) |
January 3 Descending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-1926Dec19.png | File:SE1927Jan03A.png |
| Penumbral lunar eclipse Lunar Saros 114 |
Annular solar eclipse Solar Saros 140 |
Related eclipses
Eclipses in 1927
- An annular solar eclipse on January 3.
- A total lunar eclipse on June 15.
- A total solar eclipse on June 29.
- A total lunar eclipse on December 8.
- A partial solar eclipse on December 24.
Metonic
- Preceded by: Solar eclipse of March 17, 1923
- Followed by: Solar eclipse of October 21, 1930
Tzolkinex
- Preceded by: Solar eclipse of November 22, 1919
- Followed by: Solar eclipse of February 14, 1934
Half-Saros
- Preceded by: Lunar eclipse of December 28, 1917
- Followed by: Lunar eclipse of January 8, 1936
Tritos
- Preceded by: Solar eclipse of February 3, 1916
- Followed by: Solar eclipse of December 2, 1937
Solar Saros 140
- Preceded by: Solar eclipse of December 23, 1908
- Followed by: Solar eclipse of January 14, 1945
Inex
- Preceded by: Solar eclipse of January 22, 1898
- Followed by: Solar eclipse of December 14, 1955
Triad
- Preceded by: Solar eclipse of March 4, 1840
- Followed by: Solar eclipse of November 3, 2013
Solar eclipses of 1924–1928
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.[4]
The partial solar eclipses on March 5, 1924 and August 30, 1924 occur in the previous lunar year eclipse set, and the solar eclipses on May 19, 1928 and November 12, 1928 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 1924 to 1928 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 115 | July 31, 1924 File:SE1924Jul31P.png Partial |
−1.4459 | 120 | January 24, 1925 File:SE1925Jan24T.png Total |
0.8661 | |
| 125 | July 20, 1925 File:SE1925Jul20A.png Annular |
−0.7193 | 130 File:Solar eclipse of 1926-01-14, John A. Miller.jpg Totality in Sumatra, Indonesia |
January 14, 1926 File:SE1926Jan14T.png Total |
0.1973 | |
| 135 | July 9, 1926 File:SE1926Jul09A.png Annular |
0.0538 | 140 | January 3, 1927 File:SE1927Jan03A.png Annular |
−0.4956 | |
| 145 | June 29, 1927 File:SE1927Jun29T.png Total |
0.8163 | 150 | December 24, 1927 File:SE1927Dec24P.png Partial |
−1.2416 | |
| 155 | June 17, 1928 File:SE1928Jun17P.png Partial |
1.5107 | ||||
Saros 140
Template:Solar Saros series 140
Metonic series
Template:Solar Metonic series 1866–1953
Tritos series
Template:Solar Tritos series 2003 May 31
Inex series
Template:Solar Inex series 2013 November 3
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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