Solar eclipse of February 7, 2008
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse occurred at the Moon's ascending node of orbit on Thursday, February 7, 2008,[1][2] with a magnitude of 0.965. 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 7 days after apogee (on January 31, 2008, at 4:25 UTC) and 6.9 days before perigee (on February 14, 2008, at 1:00 UTC).[3]
The moon's apparent diameter was 1 arcminute, 17.8 arcseconds (77.8 arcseconds) smaller than the August 1, 2008 total solar eclipse.
Visibility
Centrality was visible from parts of Antarctica. A significant partial eclipse was visible over New Zealand and a minor partial eclipse was seen from southeastern Australia and much of Oceania.
For most solar eclipses the path of centrality moves eastwards. In this case the path moved west round Antarctica and then north.
Observations
The best land-based visibility outside of Antarctica was from New Zealand. Professional astronomer and eclipse-chaser Jay Pasachoff observed it from Nelson, New Zealand, 60% coverage, under perfect weather.[4][5]
Images
File:SE2008Feb07A.gif
Animated path
Gallery
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Partial from McMurdo, Antarctica, 3:23 UTC
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Eclipse projection in Christchurch, New Zealand
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 | 2008 February 07 at 01:39:34.7 UTC |
| Equatorial Conjunction | 2008 February 07 at 03:09:56.4 UTC |
| First Umbral External Contact | 2008 February 07 at 03:20:50.1 UTC |
| First Central Line | 2008 February 07 at 03:25:03.4 UTC |
| Greatest Duration | 2008 February 07 at 03:25:03.4 UTC |
| First Umbral Internal Contact | 2008 February 07 at 03:29:52.5 UTC |
| Ecliptic Conjunction | 2008 February 07 at 03:45:36.0 UTC |
| Greatest Eclipse | 2008 February 07 at 03:56:10.5 UTC |
| Last Umbral Internal Contact | 2008 February 07 at 04:23:01.0 UTC |
| Last Central Line | 2008 February 07 at 04:27:46.7 UTC |
| Last Umbral External Contact | 2008 February 07 at 04:31:56.6 UTC |
| Last Penumbral External Contact | 2008 February 07 at 06:12:58.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.96499 |
| Eclipse Obscuration | 0.93120 |
| Gamma | −0.95701 |
| Sun Right Ascension | 21h20m44.7s |
| Sun Declination | -15°30'56.2" |
| Sun Semi-Diameter | 16'13.1" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 21h22m15.3s |
| Moon Declination | -16°21'00.5" |
| Moon Semi-Diameter | 15'35.2" |
| Moon Equatorial Horizontal Parallax | 0°57'12.3" |
| ΔT | 65.4 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.
| February 7 Ascending node (new moon) |
February 21 Descending node (full moon) |
|---|---|
| File:SE2008Feb07A.png | File:Lunar eclipse chart close-08feb20.png |
| Annular solar eclipse Solar Saros 121 |
Total lunar eclipse Lunar Saros 133 |
Related eclipses
Eclipses in 2008
- An annular solar eclipse on February 7.
- A total lunar eclipse on February 21.
- A total solar eclipse on August 1.
- A partial lunar eclipse on August 16.
Metonic
- Preceded by: Solar eclipse of April 19, 2004
- Followed by: Solar eclipse of November 25, 2011
Tzolkinex
- Preceded by: Solar eclipse of December 25, 2000
- Followed by: Solar eclipse of March 20, 2015
Half-Saros
- Preceded by: Lunar eclipse of January 31, 1999
- Followed by: Lunar eclipse of February 11, 2017
Tritos
- Preceded by: Solar eclipse of March 9, 1997
- Followed by: Solar eclipse of January 6, 2019
Solar Saros 121
- Preceded by: Solar eclipse of January 26, 1990
- Followed by: Solar eclipse of February 17, 2026
Inex
- Preceded by: Solar eclipse of February 26, 1979
- Followed by: Solar eclipse of January 16, 2037
Triad
- Preceded by: Solar eclipse of April 8, 1921
- Followed by: Solar eclipse of December 7, 2094
Solar eclipses of 2008–2011
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 June 1, 2011 and November 25, 2011 occur in the next lunar year eclipse set.
Saros 121
Template:Solar Saros series 121
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.
| 21 eclipse events between July 1, 2000 and July 1, 2076 | ||||
|---|---|---|---|---|
| July 1–2 | April 19–20 | February 5–7 | November 24–25 | September 12–13 |
| 117 | 119 | 121 | 123 | 125 |
| File:SE2000Jul01P.png July 1, 2000 |
File:SE2004Apr19P.png April 19, 2004 |
File:SE2008Feb07A.png February 7, 2008 |
File:SE2011Nov25P.png November 25, 2011 |
File:SE2015Sep13P.png September 13, 2015 |
| 127 | 129 | 131 | 133 | 135 |
| File:SE2019Jul02T.png July 2, 2019 |
File:SE2023Apr20H.png April 20, 2023 |
File:SE2027Feb06A.png February 6, 2027 |
File:SE2030Nov25T.png November 25, 2030 |
File:SE2034Sep12A.png September 12, 2034 |
| 137 | 139 | 141 | 143 | 145 |
| File:SE2038Jul02A.png July 2, 2038 |
File:SE2042Apr20T.png April 20, 2042 |
File:SE2046Feb05A.png February 5, 2046 |
File:SE2049Nov25H.png November 25, 2049 |
File:SE2053Sep12T.png September 12, 2053 |
| 147 | 149 | 151 | 153 | 155 |
| File:SE2057Jul01A.png July 1, 2057 |
File:SE2061Apr20T.png April 20, 2061 |
File:SE2065Feb05P.png February 5, 2065 |
File:SE2068Nov24P.png November 24, 2068 |
File:SE2072Sep12T.png September 12, 2072 |
| 157 | ||||
| File:SE2076Jul01P.png July 1, 2076 | ||||
Tritos series
Template:Solar Tritos series 2008 February 7
Inex series
Template:Solar Inex series 2008 February 7
Notes
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- ↑ Script error: No such module "citation/CS1".
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- ↑ Script error: No such module "citation/CS1".
- ↑ Solar Eclipse in New Zealand Script error: No such module "webarchive"., meade4m.com: Advisor/Partner: Jay Pasachoff
- ↑ 2008 Annular Eclipse Professor Jay Pasachoff, Williams College--Hopkins Observatory
- ↑ Script error: No such module "citation/CS1".
- ↑ Script error: No such module "citation/CS1".
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- shadowandsubstance.com Annular Eclipse of the Sun animated for February 7, 2008
- Photos of solar eclipse around the world
- Animation: Partial solar eclipse from New Zealand [1]
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