May 2003 lunar eclipse: Difference between revisions
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{{Metonic lunar eclipse 1984-2041}} |
{{Metonic lunar eclipse 1984-2041}} |
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=== Half-Saros cycle=== |
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A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a [[Saros_(astronomy)#Relationship_between_lunar_and_solar_saros_.28sar.29|half saros]]).<ref>Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, ''The half-saros''</ref> This lunar eclipse is related to two annular solar eclipses of [[Solar Saros 128]]. |
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![[Solar eclipse of May 10, 1994|May 10, 1994]] |
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![[Solar eclipse of May 20, 2012|May 20, 2012]] |
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== See also == |
== See also == |
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*[[List of lunar eclipses]] and [[List of 21st-century lunar eclipses]] |
*[[List of lunar eclipses]] and [[List of 21st-century lunar eclipses]] |
Revision as of 10:39, 12 December 2018
Total Lunar Eclipse May 15, 2003 | |
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From Minneapolis, Minnesota, 3:17 UTC | |
The moon's path through the Earth's shadow. | |
Series (and member) | 121 (51 of 82) |
Duration (hr:mn:sc) | |
Totality | 51:25 |
Partial | 3:13:54 |
Penumbral | 5:06:31 |
Contacts | |
P1 | 1:06:53 UTC |
U1 | 2:03:11 |
U2 | 3:14:26 |
Greatest | 3:40:09 |
U3 | 4:05:51 |
U4 | 5:17:05 |
P4 | 6:13:24 |
The moon's path across the Earth's shadow near its descending node in Libra. |
A total lunar eclipse took place on May 16, 2003, the first of two total lunar eclipses in 2003, the other being on November 9, 2003.
This lunar eclipse is first of a tetrad, four total lunar eclipses in series. The previous series was in 1985 and 1986, starting with a May 1985 lunar eclipse. The next one was in 2014 and 2015, starting with the April 15, 2014 lunar eclipse.
Visibility
Gallery
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From Minneapolis, Minnesota, 3:35 UTC, wide angle, near greatest eclipse
Relation to other lunar eclipses
Saros series
It is a member of Saros cycle 121.
Lunar year series
It is also the second of four lunar year cycles, repeating every 354 days.
Lunar eclipse series sets from 2002–2005 | ||||||||
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Descending node | Ascending node | |||||||
Saros Photo |
Date View |
Type Chart |
Gamma | Saros Photo |
Date View |
Type Chart |
Gamma | |
111 | 2002 May 26 |
penumbral |
1.1759 | 116 | 2002 Nov 20 |
penumbral |
−1.1127 | |
121 |
2003 May 16 |
total |
0.4123 | 126 |
2003 Nov 09 |
total |
−0.4319 | |
131 |
2004 May 04 |
total |
−0.3132 | 136 |
2004 Oct 28 |
total |
0.2846 | |
141 | 2005 Apr 24 |
penumbral |
−1.0885 | 146 |
2005 Oct 17 |
partial |
0.9796 | |
Last set | 2002 Jun 24 | Last set | 2001 Dec 30 | |||||
Next set | 2006 Mar 14 | Next set | 2006 Sep 07 |
Metonic series
This eclipse is the second of four Metonic cycle lunar eclipses on the same date, May 15–16, 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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Half-Saros cycle
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[1] This lunar eclipse is related to two annular solar eclipses of Solar Saros 128.
May 10, 1994 | May 20, 2012 |
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See also
- List of lunar eclipses and List of 21st-century lunar eclipses
- November 2003 lunar eclipse
- October 2004 lunar eclipse
- May 2004 lunar eclipse
External links
- Saros cycle 121
- 2003 May 16 chart: Eclipse Predictions by Fred Espenak, NASA/GSFC
- NASA Saros series 121
- Lunar Eclipse Gallery
- Pictures of the May 15-16 Lunar Eclipse
- Prof. Druckmüller's eclipse photography site. Czech Republic
- ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros