Total eclipse | |||||||||||||||||
Date | 21 February 2008 | ||||||||||||||||
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Gamma | −0.39923 | ||||||||||||||||
Magnitude | 1.10618 | ||||||||||||||||
Saros cycle | 133 (26 of 71) | ||||||||||||||||
Totality | 49 minutes, 46 seconds | ||||||||||||||||
Partiality | 205 minutes, 28 seconds | ||||||||||||||||
Penumbral | 339 minutes, 3 seconds | ||||||||||||||||
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A total lunar eclipse occurred on February 20 and February 21, 2008. It was visible in the eastern evening sky on February 20 for all of North and South America, and on February 21 in the predawn western sky from most of Africa and Europe. Greatest Eclipse occurring on Thursday, February 21, 2008, at 03:26:03 UTC, totality lasting 49 minutes and 45.6 seconds.
Occurring 7.1 days after perigee (Perigee on February 14, 2008) and 6.9 days before apogee (Apogee on February 28, 2008), the Moon's apparent diameter was near the average diameter.
The total lunar eclipse was the first of the two lunar eclipses in 2008, with the second, the August 16, 2008 event being partial. [1] The next total lunar eclipse occurred on December 21, 2010. The tables below contain detailed predictions and additional information on the Total Lunar Eclipse of 21 February 2008.
The Moon's apparent diameter was 26.2 arcseconds larger than the August 16, 2008 partial lunar eclipse.
This is the second eclipse this season.
First eclipse this season: 7 February 2008 Annular Solar Eclipse
Date = 21 February 2008
The eclipse was visible in the eastern evening sky on February 20 for all of North and South America, and on February 21 in the predawn western sky from most of Africa and Europe.
These simulated views of the earth from the center of the moon during the lunar eclipse show where the eclipse is visible on earth. |
The penumbral eclipse began at 00:35 UTC (February 21), and ended at 6:17. A partial eclipse existed from 1:43 until 3:00, followed by 51 minutes of totality (3:00 - 3:51), and then partial again from 3:51 until 5:09. (For local times, see Timing.)
It is possible to mistake the appearance of partial eclipse as the Moon being in a different phase, but the shadow from the eclipse changes much more rapidly. [2]
The bright star Regulus of Leo and the planet Saturn were prominent very near the Moon during the total eclipse portion. Shortly before the eclipse began, Regulus was occulted by the Moon in parts of the far Southern Atlantic Ocean and Antarctica.
Lunar eclipse series sets from 2006–2009 | ||||||||
---|---|---|---|---|---|---|---|---|
Descending node | Ascending node | |||||||
Saros # and photo | Date Viewing | Type Chart | Gamma | Saros # and photo | Date Viewing | Type Chart | Gamma | |
113 | 2006 Mar 14 | penumbral | 1.0211 | 118 | 2006 Sep 7 | partial | −0.9262 | |
123 | 2007 Mar 03 | total | 0.3175 | 128 | 2007 Aug 28 | total | −0.2146 | |
133 | 2008 Feb 21 | total | −0.3992 | 138 | 2008 Aug 16 | partial | 0.5646 | |
143 | 2009 Feb 09 | penumbral | −1.0640 | 148 | 2009 Aug 06 | penumbral | 1.3572 | |
Last set | 2005 Apr 24 | Last set | 2005 Oct 17 | |||||
Next set | 2009 Dec 31 | Next set | 2009 Jul 07 |
This lunar eclipse is part of series 133 of the Saros cycle, which repeats every 18 years and 11 days. Series 133 runs from the year 1557 until 2819. The previous eclipse of this series occurred on February 9, 1990, and the next will occur on March 3, 2026.
It is the 6th of 21 total lunar eclipses in series 133. The first was on December 28, 1917. The last (21st) will be on August 3, 2278. The longest two occurrences of this series (14th and 15th) will last for a total of 1 hour and 42 minutes on May 18, 2152, and May 30, 2170. Solar saros 140 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Lunar saros series 133, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 54 umbral lunar eclipses (33 partial lunar eclipses and 21 total lunar eclipses).
Greatest | First | |||
---|---|---|---|---|
The greatest eclipse of the series will occur on 2170 May 30, lasting 102 minutes. | Penumbral | Partial | Total | Central |
1557 May 13 | 1683 Aug 07 | 1917 Dec 28 | 2098 Apr 15 | |
Last | ||||
Central | Total | Partial | Penumbral | |
2224 Jul 01 | 2278 Aug 03 | 2429 Dec 11 | 2754 Jun 26 |
There are 10 series events between 1901 and 2100, grouped into threes (called an exeligmos), each column with approximately the same viewing longitude on earth.
1917 Dec 28 | 1936 Jan 08 | 1954 Jan 19 | |||
1972 Jan 30 | 1990 Feb 09 | 2008 Feb 21 | |||
2026 Mar 03 | 2044 Mar 13 | 2062 Mar 25 | |||
2080 Apr 04 | 2098 Apr 15 | ||||
This is the fourth of five Metonic lunar eclipses.
The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the earth's shadow will in nearly the same location relative to the background stars.
Descending node | Ascending node | |||||
---|---|---|---|---|---|---|
Saros | Date | Type | Saros | Date | Type | |
103 | 1951 Feb 21.88 | Penumbral | 108 | 1951 Aug 17.13 | Penumbral | |
113 | 1970 Feb 21.35 | Partial | 118 | 1970 Aug 17.14 | Partial | |
123 | 1989 Feb 20.64 | Total | 128 | 1989 Aug 17.13 | Total | |
133 | 2008 Feb 21.14 | Total | 138 | 2008 Aug 16.88 | Partial | |
143 | 2027 Feb 20.96 | Penumbral | 148 | 2027 Aug 17.30 | Penumbral | |
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). [4] This lunar eclipse is related to two annular solar eclipses of Solar Saros 140.
February 16, 1999 | February 26, 2017 |
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The Moon entered the penumbral shadow at 0:36 UTC, and the umbral shadow at 1:43. Totality lasted for 50 minutes, between 3:01 and 3:51. The Moon left the umbra shadow at 5:09 and left the penumbra shadow at 6:16. [5]
Event | North and South America | Europe and Africa | ||||||||
---|---|---|---|---|---|---|---|---|---|---|
Evening of February 20th | Morning of February 21st | |||||||||
AKST (-9h) | PST (-8h) | MST (-7h) | CST (-6h) | EST (-5h) | AST (-4h) | GMT (0h) | CET (+1h) | EET (+2h) | ||
P1 | Penumbral began | Under Horizon | Under Horizon | Under Horizon | 18:36 | 19:36 | 20:36 | 0:36 | 1:36 | 2:36 |
U1 | Partial began | Under Horizon | Under Horizon | 18:43 | 19:43 | 20:43 | 21:43 | 1:43 | 2:43 | 3:43 |
U2 | Total began | Under Horizon | 19:01 | 20:01 | 21:01 | 22:01 | 23:01 | 3:01 | 4:01 | 5:01 |
Mid-eclipse | 18:26 | 19:26 | 20:26 | 21:26 | 22:26 | 23:26 | 3:26 | 4:26 | 5:26 | |
U3 | Total ended | 18:51 | 19:51 | 20:51 | 21:51 | 22:51 | 23:51 | 3:51 | 4:51 | Set |
U4 | Partial ended | 20:09 | 21:09 | 22:09 | 23:09 | 0:09 | 1:09 | 5:09 | Set | Set |
Eclipse observed from Sandim, Portugal. 41°02′22″N8°30′50″W / 41.03944°N 8.51389°W . | Eclipse observed from Regina, Saskatchewan. Each image is roughly taken 5 minutes apart. |
Images taken in 3-5 minute Intervals - from Bradley, Illinois. | Eclipse observed from Halton Hills, Ontario. From 01:47 to 03:15 UTC, each image is roughly taken 5min apart. |
Eclipse observed from Winnipeg, Manitoba | |
Lunar eclipse observed from Burlington, Ontario | |
Observed from Baltimore, Maryland, from 2:30 to 3:01 UTC. Lunar north is near left. |
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