| Total Lunar Eclipse March 3-4, 2007 |
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|---|---|
The moon in the northern half of the Earth's shadow during totality. Taken at 23:29 UTC |
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The moon's path through the Earth's northern shadow. |
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| Series (and member) | 123 (57 of 73) |
| Duration (hr:mn:sc) | |
| Totality | 1:14:12 |
| Partial | 4:41:42 |
| Penumbral | 6:08:58 |
| Contacts | |
| P1 | 20:16:29 UTC |
| U1 | 21:30:04 UTC |
| U2 | 22:43:49 UTC |
| Greatest | 23:20:56 UTC |
| U3 | 23:58:01 UTC |
| U4 | 01:11:46 UTC |
| P4 | 02:25:27 UTC |
Eclipse across descending node in Leo |
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A total lunar eclipse took place on March 3, 2007, the first of two eclipses in 2007. The moon entered the penumbral shadow at 20:18 UTC, and the umbral shadow at 21:30 UTC. The total phase lasted between 22:44 UTC and 23:58 UTC with a distinctive brick-red shade (L=3 to L=4 on the Danjon scale). The moon left the umbra shadow at 01:11 UTC and left the penumbra shadow at 02:24 UTC 2007-03-04.[1] The second lunar eclipse of 2007 occurred on August 28.[2][3]
The previous lunar eclipse on September 7, 2006 was partial.
This eclipse is the first of two lunar eclipses to occur in 2007, the second being on 28 August 2007.
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The whole event was visible from Europe, Africa, parts of South America, and some areas of North America, Asia, and Western Australia. In North America, part of the event was visible at moonrise.
This simulated view of the earth from the center of the moon during the lunar eclipse shows where the eclipse is visible on earth. |
| Descending node | Ascending node | |||||
|---|---|---|---|---|---|---|
| Saros # and photo |
Date Viewing |
Type Chart |
Saros # and photo |
Date Viewing |
Type Chart |
|
| 113 |
2006 Mar 14 |
penumbral |
118 |
2006 Sep 7 |
partial |
|
| 123 |
2007 Mar 03 |
total |
128 |
2007 Aug 28 |
total |
|
| 133 |
2008 Feb 21 |
total |
138 |
2008 Aug 16 |
partial |
|
| 143 |
2009 Feb 9 |
penumbral |
148 |
2009 Aug 06 |
penumbral |
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| Last set | 2005 Apr 24 | Last set | 2005 Oct 17 | |||
| Next set | 2009 Dec 31 | Next set | 2009 Jul 07 | |||
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 be in nearly the same location relative to the background stars.
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Lunar saros series 123, repeating every 18 years and 11 days, has 25 total lunar eclipses. The first total lunar eclipse of this series was on July 16, 1628, and last will be on April 4, 2061. The two longest occurrence of this series were on September 20, 1736 and October 1, 1754 when totality lasted 106 minutes.[4]
It last occurred on February 20, 1989 and will next occur on March 14, 2025.
From Leeds, England. |
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From Degania A, Israel. |
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United Kingdom |
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Persian gulf |