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June 2002 lunar eclipse

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June 2002 lunar eclipse
Penumbral eclipse
Hourly motion shown right to left
DateJune 24, 2002
Gamma−1.4439
Magnitude−0.791
Saros cycle149 (2 of 72)
Penumbral129 minutes, 5 seconds
Contacts (UTC)
P120:22:28
Greatest21:27:09
P422:31:33

A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Monday, June 24, 2002,[1] with an umbral magnitude of −0.791. 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 about 6.7 days after perigee (on June 19, 2002, at 3:30 UTC), the Moon's apparent diameter was larger.[2]

Visibility

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The eclipse was completely visible over Africa, Europe, west and central Asia, and Antarctica, seen rising over much of South America and setting over much of east Asia and Australia.[3]


The moon's hourly motion across the Earth's shadow in the constellation of Scorpius.

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.[4]

June 24, 2002 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.21095
Umbral Magnitude −0.79099
Gamma −1.44399
Sun Right Ascension 06h13m52.0s
Sun Declination +23°24'03.8"
Sun Semi-Diameter 15'44.2"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 18h13m25.9s
Moon Declination -24°47'04.8"
Moon Semi-Diameter 15'42.3"
Moon Equatorial Horizontal Parallax 0°57'38.4"
ΔT 64.3 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.

Eclipse season of May–June 2002
May 26
Descending node (full moon)
June 10
Ascending node (new moon)
June 24
Descending node (full moon)
Penumbral lunar eclipse
Lunar Saros 111
Annular solar eclipse
Solar Saros 137
Penumbral lunar eclipse
Lunar Saros 149
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Eclipses in 2002

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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 149

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Inex

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Triad

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Lunar eclipses of 1998–2002

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Lunar eclipse series sets from 1998–2002
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
109 1998 Aug 08
penumbral
1.4876 114 1999 Jan 31
penumbral
−1.0190
119 1999 Jul 28
partial
0.7863 124
2000 Jan 21
total
−0.2957
129 2000 Jul 16
total
0.0302 134
2001 Jan 09
total
0.3720
139 2001 Jul 05
partial
−0.7287 144 2001 Dec 30
penumbral
1.0732
149 2002 Jun 24
penumbral
−1.4440
Last set 1998 Sep 06 Last set 1998 Mar 13
Next set 2002 May 26 Next set 2002 Nov 20

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).[5] This lunar eclipse is related to one partial solar eclipse of Solar Saros 156.

July 1, 2011

See also

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References

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  1. ^ "June 24–25, 2002 Penumbral Lunar Eclipse". timeanddate. Retrieved 12 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 12 November 2024.
  3. ^ "Penumbral Lunar Eclipse of 2002 Jun 24" (PDF). NASA. Retrieved 12 November 2024.
  4. ^ "Penumbral Lunar Eclipse of 2002 Jun 24". EclipseWise.com. Retrieved 12 November 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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