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June 2012 lunar eclipse

June 2012 lunar eclipse
Partial eclipse
Totality as viewed from Brisbane, Australia, 11:06 UTC
DateJune 4, 2012
Gamma0.8248
Magnitude0.3718
Saros cycle140 (25 of 80)
Partiality126 minutes, 35 seconds
Penumbral270 minutes, 2 seconds
Contacts (UTC)
P18:48:11
U19:59:53
Greatest11:03:12
U412:06:28
P413:18:13

A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, June 4, 2012,[1] with an umbral magnitude of 0.3718. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in 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 1.1 days before perigee (on June 3, 2012, at 9:15 UTC), the Moon's apparent diameter was larger.[2]

Visibility

The eclipse was completely visible over Australia, Antarctica, and the Pacific Ocean, seen rising over east Asia and setting over North and South America.[3]


Hourly motion shown right to left

The Moon's hourly motion across the Earth's shadow in the constellation of Ophiuchus (north of Scorpius).

Visibility map

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

June 4, 2012 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.31975
Umbral Magnitude 0.37184
Gamma 0.82480
Sun Right Ascension 04h51m33.3s
Sun Declination +22°30'16.0"
Sun Semi-Diameter 15'45.9"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 16h51m37.6s
Moon Declination -21°39'56.2"
Moon Semi-Diameter 16'37.9"
Moon Equatorial Horizontal Parallax 1°01'02.3"
ΔT 66.8 s

Eclipse season

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.

Eclipse season of May–June 2012
May 20
Descending node (new moon)
June 4
Ascending node (full moon)
Annular solar eclipse
Solar Saros 128
Partial lunar eclipse
Lunar Saros 140

Eclipses in 2012

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 140

Inex

Triad

Lunar eclipses of 2009–2013

This eclipse was one of five lunar eclipses in a short-lived series. The lunar year series repeats after 12 lunations or 354 days (Shifting back about 10 days in sequential years). Because of the date shift, the Earth's shadow will be about 11 degrees west in sequential events.

Lunar eclipse series sets from 2009–2013
Ascending node   Descending node
Saros #
Photo
Date
Viewing
Type
chart
Gamma Saros #
Photo
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
Last set 2009 Aug 06 Last set 2009 Feb 9
Next set 2013 Apr 25 Next set 2013 Oct 18

Half-Saros cycle

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 two annular solar eclipses of Solar Saros 147.

May 31, 2003 June 10, 2021

See also

References

  1. ^ "June 3–4, 2012 Partial Lunar Eclipse". timeanddate. Retrieved 15 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 15 November 2024.
  3. ^ "Partial Lunar Eclipse of 2012 Jun 04" (PDF). NASA. Retrieved 15 November 2024.
  4. ^ "Partial Lunar Eclipse of 2012 Jun 04". EclipseWise.com. Retrieved 15 November 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros


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