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July 2009 lunar eclipse

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July 2009 lunar eclipse
Penumbral eclipse
The Moon grazed the southern penumbral shadow of the Earth.
DateJuly 7, 2009
Gamma−1.4915
Magnitude−0.9116
Saros cycle110 (71 of 72)
Penumbral121 minutes, 29 seconds
Contacts (UTC)
P18:37:51
Greatest9:38:36
P410:39:20

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, July 7, 2009,[1] with an umbral magnitude of −0.9116. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 8 hours before apogee (on July 7, 2009, at 17:40 UTC), the Moon's apparent diameter was smaller.[2] This eclipse entered only the southernmost tip of the penumbral shadow and thus was predicted to be very difficult to observe visually.[3]

This eclipse was the second of four lunar eclipses in 2009, with the others occurring on February 9 (penumbral), August 6 (penumbral), and December 31 (partial).

Visibility

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The eclipse was completely visible over eastern Australia and western North and South America, seen rising over western Australia and setting over eastern North and South America.[4]


Hourly motion shown right to left

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

Visibility map

Eclipse details

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Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[5]

July 7, 2009 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.15783
Umbral Magnitude −0.91159
Gamma −1.49158
Sun Right Ascension 07h06m54.1s
Sun Declination +22°32'55.2"
Sun Semi-Diameter 15'43.9"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 19h08m08.1s
Moon Declination -23°51'38.0"
Moon Semi-Diameter 14'42.6"
Moon Equatorial Horizontal Parallax 0°53'59.3"
ΔT 65.9 s

Eclipse season

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This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. The first and last eclipse in this sequence is separated by one synodic month.[6][7][8]

Eclipse season of July–August 2009
July 7
Ascending node (full moon)
July 22
Descending node (new moon)
August 6
Ascending node (full moon)
Penumbral lunar eclipse
Lunar Saros 110
Total solar eclipse
Solar Saros 136
Penumbral lunar eclipse
Lunar Saros 148
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Eclipses in 2009

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 110

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Inex

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Triad

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Lunar eclipses of 2009–2013

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This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[9]

The penumbral lunar eclipses on February 9, 2009 and August 6, 2009 occur in the previous lunar year eclipse set, and the lunar eclipses on April 25, 2013 (partial) and October 18, 2013 (penumbral) occur in the next lunar year eclipse set.

Lunar eclipse series sets from 2009 to 2013
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
110 2009 Jul 07
Penumbral
−1.4916 115
2009 Dec 31
Partial
0.9766
120
2010 Jun 26
Partial
−0.7091 125
2010 Dec 21
Total
0.3214
130
2011 Jun 15
Total
0.0897 135
2011 Dec 10
Total
−0.3882
140
2012 Jun 04
Partial
0.8248 145 2012 Nov 28
Penumbral
−1.0869
150 2013 May 25
Penumbral
1.5351

Saros 110

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This eclipse is a part of Saros series 110, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on May 28, 747 AD. It contains partial eclipses from August 23, 891 AD through April 18, 1288; total eclipses from April 29, 1306 through September 5, 1522; and a second set of partial eclipses from September 16, 1540 through April 22, 1883. The series ends at member 72 as a penumbral eclipse on July 18, 2027.

The longest duration of totality was produced by member 38 at 103 minutes, 8 seconds on July 3, 1414. All eclipses in this series occur at the Moon’s ascending node of orbit.[10]

Greatest First
The greatest eclipse of the series occurred on 1414 Jul 03, lasting 103 minutes, 8 seconds.[11] Penumbral Partial Total Central
747 May 28
891 Aug 23
1306 Apr 29
1360 May 31
Last
Central Total Partial Penumbral
1468 Aug 04
1522 Sep 05
1883 Apr 22
2027 Jul 18

Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

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 half saros).[12] This lunar eclipse is related to two partial solar eclipses of Solar Saros 117.

July 1, 2000 July 13, 2018

See also

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Notes

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  1. ^ "July 6–7, 2009 Penumbral Lunar Eclipse". timeanddate. Retrieved November 15, 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved November 15, 2024.
  3. ^ Sky&Telescope: "The moon skims through too little of the penumbra to be noticed even by the most intent observer." Archived February 2, 2009, at archive.today
  4. ^ "Penumbral Lunar Eclipse of 2009 Jul 07" (PDF). NASA. Retrieved November 15, 2024.
  5. ^ "Penumbral Lunar Eclipse of 2009 Jul 07". EclipseWise.com. Retrieved November 15, 2024.
  6. ^ (AFP) – 6 days ago. "AFP: Solar eclipse sparks tourism fever in China". Archived from the original on July 27, 2009. Retrieved July 22, 2009.{{cite web}}: CS1 maint: numeric names: authors list (link)
  7. ^ Wang, Hongjiang (July 22, 2009). "Scientists: China the best place to observe longest solar eclipse in 2,000 years_English_Xinhua". News.xinhuanet.com. Archived from the original on May 21, 2009. Retrieved July 22, 2009.
  8. ^ "Indian students on solar eclipse 'odyssey' to China – Yahoo! India News". In.news.yahoo.com. Archived from the original on July 29, 2009. Retrieved July 22, 2009.
  9. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved October 6, 2018.
  10. ^ "NASA - Catalog of Lunar Eclipses of Saros 110". eclipse.gsfc.nasa.gov.
  11. ^ Listing of Eclipses of series 110
  12. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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