May 2004 lunar eclipse

Total Lunar Eclipse 4-5 May 2004
Haifa, Israel
The moon's path through the Earth's shadow.
Series (and member)	131 (33 of 72)
Gamma	-0.3132
Magnitude	1.3035
Duration (hr:mn:sc)
Totality	1:15:28
Partial	3:23:12
Penumbral	5:15:43
Contacts (UTC)
P1	17:52:54
U1	18:48:38
U2	19:52:29
Greatest	20:30:13
U3	21:07:57
U4	22:11:50
P4	23:08:03
The moon's hourly motion across the Earth's shadow in the constellation of Libra.

A total lunar eclipse took place on Tuesday 4 May 2004, the first of two total lunar eclipses in 2004, the second being on 28 October 2004.

Visibility

It was visible throughout most of Europe and Asia, eastern Africa, Indian Ocean and western South America including the Pacific Ocean. The eclipse seen in eastern Asia before sunrise and western South America after sunset. The eclipse was seen over and the Philippines at dawn. Mid Eclipse was visible during moonset in Eastern Australia.

Related lunar eclipses

Eclipse season

This is the second eclipse this season.

First eclipse this season: 19 April 2004 Partial Solar Eclipse

Eclipses of 2004

Lunar year series

It is the third 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 131, has 72 lunar eclipses. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

This eclipse series began in AD 1427 with a partial eclipse at the southern edge of the Earth's shadow when the Moon was close to its descending node. Each successive Saros cycle, the Moon's orbital path is shifted northward with respect to the Earth's shadow, with the first total eclipse occurring in 1950. For the following 252 years, total eclipses occur, with the central eclipse being predicted to occur in 2078. The first partial eclipse after this is predicted to occur in the year 2220, and the final partial eclipse of the series will occur in 2707. The total lifetime of the lunar Saros series 131 is 1280 years. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Because of the ⅓ fraction of days in a Saros cycle, the visibility of each eclipse will differ for an observer at a given fixed locale. For the lunar Saros series 131, the first total eclipse of 1950 had its best visibility for viewers in Eastern Europe and the Middle East because mid-eclipse was at 20:44 UT. The following eclipse in the series occurred approximately 8 hours later in the day with mid-eclipse at 4:47 UT, and was best seen from North America and South America. The third total eclipse occurred approximately 8 hours later in the day than the second eclipse with mid-eclipse at 12:43 UT, and had its best visibility for viewers in the Western Pacific, East Asia, Australia and New Zealand. This cycle of visibility repeats from the initiation to termination of the series, with minor variations. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Lunar Saros series 131, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 57 umbral lunar eclipses (42 partial lunar eclipses and 15 total lunar eclipses). Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Greatest	First
The greatest eclipse of the series will occur on 2094 Jun 28, lasting 102 minutes.^[1]	Penumbral	Partial	Total	Central
	1427 May 10	1553 July 25	1950 Apr 2	2022 May 16
	Last
	Central	Total	Partial	Penumbral
	2148 Jul 31	2202 Sep 3	2563 Apr 9	2707 Jul 7

Metonic series

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 in nearly the same location relative to the background stars.

Metonic events: May 4 and October 28
Descending node	Ascending node
1966 May 4 - Penumbral (111) 1985 May 4 - Total (121) 2004 May 4 - Total (131) 2023 May 5 - Penumbral (141)	1966 Oct 29 - Penumbral (116) 1985 Oct 28 - Total (126) 2004 Oct 28 - Total (136) 2023 Oct 28 - Partial (146) 2042 Oct 28 - Penumbral (156)

Tritos series

Preceded: Lunar eclipse of 4 June 1993

Followed: Lunar eclipse of 5 April 2015

Tzolkinex

Preceded: Lunar eclipse of 24 March 1997

Followed: Lunar eclipse of 15 June 2011

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).^[2] This lunar eclipse is related to two annular solar eclipses of Solar Saros 138.

29 April 1995	10 May 2013

Notes

^ Listing of Eclipses of cycle 131
^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

External links

NASA
- 2004 May 04 chart: Eclipse Predictions by Fred Espenak, NASA/GSFC
[1] APOD 2004 May 6, A Lunar Eclipse Mosaic, from Greece
[2] APOD 2004 May 8, Good Morning Sydney, Sydney Australia
Photos Archived 2009-02-28 at the Wayback Machine
Spaceweather.com: Lunar eclipse gallery

This lunar eclipse-related article is a stub. You can help Wikipedia by expanding it.

[1] Listing of Eclipses of cycle 131

[2] Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

[1]

[2]

1914 Mar 12	1932 Mar 22	1950 Apr 2

1968 Apr 13	1986 Apr 24	2004 May 4

2022 May 16	2040 May 26	2058 Jun 6

2076 Jun 17	2094 Jun 28