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== Visibility ==
== Visibility ==
The eclipse was visible over central Pacific, North America, South America, Atlantic, Europe, Africa and extreme southwestern Asia, seen rising over central Pacific and North America, and setting over Europe and Africa. In South America the entire eclipse was visible lasting just over 5 hours.


[[File:Lunar eclipse from moon-2003May16.png|320px]]
[[File:Lunar eclipse from moon-2003May16.png|320px]]

Revision as of 15:45, 6 April 2023

Total Lunar Eclipse
May 16, 2003

From Minneapolis, MN, 3:17 UTC

The moon's path through the Earth's shadow.
Series (and member) 121 (54 of 82)
Gamma 0.4123
Magnitude 1.12759
Duration (hr:mn:sc)
Totality 51:25
Partial 3:13:53
Penumbral 5:06:31
Contacts (UTC)
P1 1:06:53
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 Friday, May 16, 2003, the first of two total lunar eclipses in 2003, the other being on November 9, 2003. A shallow total eclipse saw the Moon in relative darkness for 52 minutes and 3.1 seconds. The Moon was 12.938% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 15 minutes and 3.1 seconds in total. Occurring only 0.5 days after perigee (Perigee on Thursday, May 15, 2003), the Moon's apparent diameter was 6.2% larger than average. At greatest eclipse the Moon was only 357,693 km (222,260 mi) from the Earth, making it a Super Full Moon.

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

The eclipse was visible over central Pacific, North America, South America, Atlantic, Europe, Africa and extreme southwestern Asia, seen rising over central Pacific and North America, and setting over Europe and Africa. In South America the entire eclipse was visible lasting just over 5 hours.

Relation to other lunar eclipses

This is the first eclipse this season.

Second eclipse this season: 31 May 2003 Annular Solar Eclipse

Eclipses of 2003

Lunar year series

It is also the second of four lunar year cycles, repeating every 354 days.

Lunar eclipse series sets from 2002–2005
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.

  1. 1984 May 15.19 - penumbral (111)
  2. 2003 May 16.15 - total (121)
  3. 2022 May 16.17 - total (131)
  4. 2041 May 16.03 - penumbral (141)
  1. 1984 Nov 08.75 - penumbral (116)
  2. 2003 Nov 09.05 - total (126)
  3. 2022 Nov 08.46 - total (136)
  4. 2041 Nov 08.19 - partial (146)
  5. 2060 Nov 08.17 - penumbral (156)

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

See also

References

  1. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros