Total Lunar Eclipse November 8-9, 2003 |
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Totality from Oudenaarde, Belgium, 1:08 UTC |
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The moon's path through the Earth's shadow |
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Series | 126 (member 45 of 72) |
Duration (hr:mn:sc) | |
Totality | 24:32 |
Partial | 3:32:04 |
Penumbral | 6:06:48 |
Contacts | |
P1 | 22:15:10 UTC |
U1 | 23:32:30 UTC |
U2 | 1:06:17 UTC |
Greatest | 1:18:33 |
U3 | 1:30:48 UTC |
U4 | 3:04:34 UTC |
P4 | 4:21:58 UTC |
The moon's path across shadow in Aries. |
A total lunar eclipse took place on November 9, 2003, the second of two total lunar eclipses in 2003, the first being on May 16, 2003.
Contents |
1:00 UT (Just before totality) |
1:16 UT (Near greatest eclipse) |
1:35 UT (Just after of totality) |
From Minneapolis, Minnesota |
It is the second of four lunar year cycles, repeating every 354 days.
Descending node | Ascending node | |||||
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Saros Photo |
Date View |
Type Chart |
Saros Photo |
Date View |
Type Chart |
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111 | 2002 May 26 |
penumbral |
116 | 2002 Nov 20 |
penumbral |
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121 |
2003 May 16 |
total |
126 |
2003 Nov 09 |
total |
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131 |
2004 May 04 |
total |
136 |
2004 Oct 28 |
total |
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141 |
2005 Apr 24 |
penumbral |
146 | 2005 Oct 17 |
partial |
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Last set | 2002 Jun 24 | Last set | 2001 Dec 30 | |||
Next set | 2006 Mar 14 | Next set | 2006 Sep 7 |
This eclipse is the second of four Metonic cycle lunar eclipses on the same date, November 8-9, each separated by 19 years:
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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