August 2007 lunar eclipse

A total lunar eclipse occurred on 28 August 2007, lasting just over 90 minutes. The Moon entered the Earth's penumbra at 7:53:40 UTC. The first partial phase began in earnest at 8:51:16 UTC when the Moon entered the Earth's umbra. It exited the penumbra at 13:20:57 UTC.

Total Lunar Eclipse
28 August 2007

Viewed from Wollongong, Australia at 9:48 UTC, shortly before totality

The moon's path through the Earth's southern shadow.
Series (and member)128 (40 of 71)
Gamma-0.2145
Magnitude-1.481
Duration (hr:mn:sc)
Totality1:30:01
Partial3:32:12
Penumbral5:27:17
Contacts (UTC)
P17:53:40
U18:51:16
U29:52:21
Greatest10:37:21
U311:22:22
U412:23:28
P413:20:57

The Moon's hourly motion across the Earth's shadow in the constellation of Aquarius

It is a relatively rare central eclipse where the Moon passes in front of the center of the Earth's shadow. It was the last central lunar eclipse of Saros series 128 as well as the "longest and deepest lunar eclipse to be seen in 7 years". In the total lunar eclipse of 16 July 2000 the moon passed within two arc minutes of the center of the Earth's shadow. In comparison, this still very deep eclipse was off-center by over 12 minutes of arc.[1] The next total lunar eclipse of a longer duration was on 15 June 2011.

The lunar eclipse was the second one in 2007. The first one occurred on 3 March 2007.

Viewing

NASA chart of the eclipse

Viewing from Oceania is favoured for the eclipse, because at the moment of greatest eclipse (10:37:22 UTC), the Moon was at the zenith of French Polynesia. The Pacific regions of Canada and the continental United States (including all of Alaska) witnessed the whole event, along with most of eastern Australia, New Zealand and all the Pacific Island regions (except New Guinea), and the tip of the Chukchi Peninsula that includes the town of Uelen, Russia. The majority of the Americas observed an abbreviated eclipse, with moonset occurring at some time during the eclipse. Siberia, far eastern Russia, eastern South Asia, China, the rest of eastern and southeastern Asia, New Guinea, and the rest of Australia missed out on the beginning of the eclipse, because the eclipse occurred at or close to moonrise in those regions.[2]

Luzon (except Visayas and Mindanao) in the Philippines, particularly Metro Manila, missed the rare eclipse entirely, due to clouds in the area due to the rainy season, which saddened many eclipse watchers in the area, but the eclipse was sighted by other amateur astronomers in other parts of the country as the lunar eclipse seen in clear skies. The eclipse was also missed in New Guinea, especially Port Moresby because of clouds. Greenland, Europe (including western Russia), Africa, western Asia, western Central Asia, and western South Asia missed the eclipse completely.


This simulated view of the Earth from the center of the Moon during the lunar eclipse shows where the eclipse is visible on Earth.

Map

Relation to other lunar eclipses

Eclipses of 2007

This eclipse at the Moon's ascending node was the second of two lunar eclipses to occur in 2007. The first at the descending node was on 3 March 2007.

Lunar year series

Lunar eclipse series sets from 2006–2009
Descending node   Ascending node
Saros #
and photo
Date
Viewing
Type
Chart
Gamma Saros #
and photo
Date
Viewing
Type
Chart
Gamma
113
2006 Mar 14
penumbral
1.0211 118
2006 Sep 7
partial
−0.9262
123
2007 Mar 03
total
0.3175 128
2007 Aug 28
total
−0.2146
133
2008 Feb 21
total
−0.3992 138
2008 Aug 16
partial
0.5646
143
2009 Feb 09
penumbral
−1.0640 148
2009 Aug 06
penumbral
1.3572
Last set 2005 Apr 24 Last set 2005 Oct 17
Next set 2009 Dec 31 Next set 2009 Jul 07

Metonic cycle (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. 1988 Mar 03.675 – Partial (113)
  2. 2007 Mar 03.972 – Total (123)
  3. 2026 Mar 03.481 – Total (133)
  4. 2045 Mar 03.320 – Penumbral (143)
  1. 1988 Aug 27.461 – partial (118)
  2. 2007 Aug 28.442 – total (128)
  3. 2026 Aug 28.175 – partial (138)
  4. 2045 Aug 27.578 – penumbral (148)

Saros series

Lunar saros series 128, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 57 umbral eclipses (42 partial lunar eclipses and 15 total lunar eclipses). Solar Saros 135 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 occurred on 1953 Jul 26, lasting 108 minutes.[3]
Penumbral Partial Total Central
1304 Jun 18 1430 Sep 2 1845 May 21 1899 Jun 23
Last
Central Total Partial Penumbral
2007 Aug 28 2097 May 21 2440 May 17 2566 Aug 2
1901–2100
1917 Jul 4 1935 Jul 16 1953 Jul 26
1971 Aug 6 1989 Aug 17 2007 Aug 28
2025 Sep 7 2043 Sep 19 2061 Sep 29
2079 Oct 10 2097 Oct 21

Lunar Saros 128 contains 15 total lunar eclipses between 1845 and 2097 (in years 1845, 1863, 1881, 1899, 1917, 1935, 1953, 1971, 1989, 2007, 2025, 2043, 2061, 2079 and 2097). Solar Saros 135 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[4] This lunar eclipse is related to two annular solar eclipses of Solar Saros 135.

22 August 1998 1 September 2016
Collages

From the Oregon Coast.

From Swifts Creek, Australia.
(3 minute intervals)

From Bakersfield, California.

See also

Notes

  1. Visibility Map for Total Lunar Eclipse of 16 July 2000
  2. Visibility Map for Total Lunar Eclipse of 28 August 2007
  3. Listing of Eclipses of cycle 128
  4. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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