Solar eclipse of December 24, 1992
Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse occurred at the Moon's ascending node of orbit between Wednesday, December 23 and Thursday, December 24, 1992,[1] with a magnitude of 0.8422. 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.
A partial eclipse was visible for parts of East Asia, Northeast Asia, and Alaska.
Images
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.[2]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1992 December 23 at 22:21:43.1 UTC |
| Greatest Eclipse | 1992 December 24 at 00:31:41.3 UTC |
| Ecliptic Conjunction | 1992 December 24 at 00:43:50.0 UTC |
| Equatorial Conjunction | 1992 December 24 at 00:46:08.3 UTC |
| Last Penumbral External Contact | 1992 December 24 at 02:41:38.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.84220 |
| Eclipse Obscuration | 0.77919 |
| Gamma | 1.07106 |
| Sun Right Ascension | 18h10m41.8s |
| Sun Declination | -23°25'00.8" |
| Sun Semi-Diameter | 16'15.6" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 18h10m11.4s |
| Moon Declination | -22°25'35.5" |
| Moon Semi-Diameter | 15'15.7" |
| Moon Equatorial Horizontal Parallax | 0°56'00.6" |
| ΔT | 59.1 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 9 Descending node (full moon) |
December 24 Ascending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-1992Dec09.png | File:SE1992Dec24P.png |
| Total lunar eclipse Lunar Saros 125 |
Partial solar eclipse Solar Saros 151 |
Related eclipses
Eclipses in 1992
- An annular solar eclipse on January 4.
- A partial lunar eclipse on June 15.
- A total solar eclipse on June 30.
- A total lunar eclipse on December 9.
- A partial solar eclipse on December 24.
Metonic
- Preceded by: Solar eclipse of March 7, 1989
- Followed by: Solar eclipse of October 12, 1996
Tzolkinex
- Preceded by: Solar eclipse of November 12, 1985
- Followed by: Solar eclipse of February 5, 2000
Half-Saros
- Preceded by: Lunar eclipse of December 20, 1983
- Followed by: Lunar eclipse of December 30, 2001
Tritos
- Preceded by: Solar eclipse of January 25, 1982
- Followed by: Solar eclipse of November 23, 2003
Solar Saros 151
- Preceded by: Solar eclipse of December 13, 1974
- Followed by: Solar eclipse of January 4, 2011
Inex
- Preceded by: Solar eclipse of January 14, 1964
- Followed by: Solar eclipse of December 4, 2021
Triad
- Preceded by: Solar eclipse of February 23, 1906
- Followed by: Solar eclipse of October 24, 2079
Solar eclipses of 1990–1992
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.[3]
| Solar eclipse series sets from 1990 to 1992 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 121 | January 26, 1990 File:SE1990Jan26A.png Annular |
−0.9457 | 126 File:1990.04 Pimennys (28866343838) (cropped).jpg Partial in Finland |
July 22, 1990 File:SE1990Jul22T.png Total |
0.7597 | |
| 131 | January 15, 1991 File:SE1991Jan15A.png Annular |
−0.2727 | 136 File:Eclipse CR 1991 a zoom.jpg Totality in Playas del Coco, Costa Rica |
July 11, 1991 File:SE1991Jul11T.png Total |
−0.0041 | |
| 141 | January 4, 1992 File:SE1992Jan04A.png Annular |
0.4091 | 146 | June 30, 1992 File:SE1992Jun30T.png Total |
−0.7512 | |
| 151 | December 24, 1992 File:SE1992Dec24P.png Partial |
1.0711 | ||||
Saros 151
Template:Solar Saros series 151
Metonic series
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 ascending node.
Tritos series
Template:Solar Tritos series 2003 November 23
Inex series
Template:Solar Inex series 2021 December 4
References
<templatestyles src="Reflist/styles.css" />
Script error: No such module "Check for unknown parameters".
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
Script error: No such module "Navbox". Script error: No such module "Side box".