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{{Infobox lunar eclipse
{| class="wikitable" align=right width=240
| type = total
! bgcolor=#e7dcc3 colspan=2|Total Lunar Eclipse<br>November 8–9, 2003
| image = Lunar eclipse November 2003-TLR63.jpg
|-
|colspan=2|[[File:Lunar eclipse November 2003-TLR63.jpg|240px]]<BR>Totality from [[Minneapolis]], 1:16 UTC
| caption = Totality from [[Minneapolis]], 1:16 UTC
| date = 9 November 2003
|-
| gamma = -0.43193
|colspan=2|[[Image:Lunar eclipse chart close-03nov09.png|240px]]<br>The moon's path through the Earth's shadow
| magnitude = 1.01785
|-
| saros_ser = 126
|align=center bgcolor=#c0d0e0| [[Saros cycle|Series]]|| [[Lunar Saros 126|126]] (member 45 of 72)
| saros_no = 44 of 70
|-
| totality = 21 minutes, 58 seconds
|align=center bgcolor=#c0d0e0| Date || 9 November 2003
| partiality = 211 minutes, 26 seconds
|-
| penumbral = 363 minutes, 16 seconds
!align=center bgcolor=#c0b0e0 colspan=2| Duration (hr:mn:sc)
| p1 = 22:16:57 (8 November)
|-
| u1 = 23:32:50 (8 November)
|align=center bgcolor=#b0a0e0 | Totality || 21:58
| u2 = 01:07:34
|-
| greatest = 01:18:34
|align=center bgcolor=#c0a0e0 | Partial || 3:31:25
| u3 = 01:29:32
|-
| u4 = 03:04:16
|align=center bgcolor=#d0d0e0 | Penumbral || 6:03:09
| p4 = 04:20:12
|-
| previous = November 2003
!align=center bgcolor=#a0d0e0 colspan=2| Contacts
| next = October 2004
|-
}}
|align=center bgcolor=#d0d0e0 | P1 || 22:16:59 [[UTC]]
|-
|align=center bgcolor=#c0a0e0 | U1 || 23:32:50 UTC
|-
|align=center bgcolor=#b0a0e0 | U2 || 1:07:34 UTC
|-
|align=center bgcolor=#a0a0e0| Greatest || 1:18:34 UTC
|-
|align=center bgcolor=#b0a0e0 | U3 || 1:29:32 UTC
|-
|align=center bgcolor=#c0a0e0 | U4 || 3:04:15 UTC
|-
|align=center bgcolor=#d0d0e0 | P4 || 4:20:08 UTC
|-
|colspan=2|[[Image:Lunar eclipse chart-03nov09.png|240px]]<br>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 2003 lunar eclipse|May 16, 2003]]. It is the first total lunar eclipse of 21st century which happened in a [[micromoon]] day.
A '''total [[lunar eclipse]]''' took place on November 9, 2003, the second of two total lunar eclipses in 2003, the first being on [[May 2003 lunar eclipse|May 16, 2003]]. It is the first total lunar eclipse of 21st century which happened in a [[micromoon]] day.



Revision as of 14:38, 22 December 2020

November 2003 lunar eclipse
Total eclipse
Totality from Minneapolis, 1:16 UTC
Date9 November 2003
Gamma−0.43193
Magnitude1.01785
Saros cycle126 (44 of 70)
Totality21 minutes, 58 seconds
Partiality211 minutes, 26 seconds
Penumbral363 minutes, 16 seconds
Contacts (UTC)
P122:16:57 (8 November)
U123:32:50 (8 November)
U201:07:34
Greatest01:18:34
U301:29:32
U403:04:16
P404:20:12

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. It is the first total lunar eclipse of 21st century which happened in a micromoon day.

This was the last of 14 total lunar eclipses of Lunar Saros 126, which started on 19 June 1769 and ended on 9 November 2003.

Visibility

Relation to other lunar eclipses

Eclipses of 2003

Lunar year series

It is 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


Saros series

Lunar Saros series 126, repeating every 18 years and 11 days, has a total of 70 lunar eclipse events including 14 total lunar eclipses. Solar Saros 133 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

First Penumbral Lunar Eclipse: 1228 Jul 18

First Partial Lunar Eclipse: 1625 Mar 24

First Total Lunar Eclipse: 1769 Jun 19

First Central Lunar Eclipse: 1805 Jul 11

Greatest Eclipse of the Lunar Saros 126: 1859 Aug 13, lasting 106 minutes.

Last Central Lunar Eclipse: 1931 Sep 26

Last Total Lunar Eclipse: 2003 Nov 09

Last Partial Lunar Eclipse: 2346 Jun 05

Last Penumbral Lunar Eclipse: 2472 Aug 19

1901-2100

1913 Sep 15

1931 Sep 26

1949 Oct 07

1967 Oct 18

1985 Oct 28

2003 Nov 09

2021 Nov 19

2039 Nov 30

2057 Dec 11

2075 Dec 22

2094 Jan 01

Metonic series

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.

  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 total solar eclipses of Solar Saros 133.

November 3, 1994 November 13, 2012

See also

References

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