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November 2012 lunar eclipse

From Wikipedia, the free encyclopedia

Penumbral Lunar Eclipse
November 28, 2012

The northern parts of the Moon will perceptibly dim as the Moon passes through the Earth's penumbral shadow
Series (and member) 145 (11 of 71)
Gamma -1.0869
Duration (hr:mn:sc)
Penumbral 4:36:00
Contacts (UTC)
P1 12:14:59
Greatest 14:32:59
P4 16:50:59

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

A penumbral lunar eclipse occurred on 28 November 2012, the second of two lunar eclipses in 2012.

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Transcription

Visibility

NASA chart of the eclipse


A simulated view of the Earth from the center of the Moon at maximal eclipse

Map

Related eclipses

Eclipses of 2012

Lunar year (354 days)

This eclipse is the one of four 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.[citation needed]

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).[1] This lunar eclipse is related to two total solar eclipses of Solar Saros 152.

23 November 2003 4 December 2021

See also

References

  1. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

External links


This page was last edited on 7 October 2023, at 23:18
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