Penumbral lunar eclipse
25 May 2013

The Moon barely grazes the northern penumbral shadow of the Earth.
Saros (and member)150 (1 of 71)
Gamma1.5350
Duration (hr:mn:sc)
Penumbral0:33:34
Contacts (UTC)
P13:53:15
Greatest4:09:58
P44:26:49

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

A penumbral lunar eclipse took place on 24–25 May 2013, the second of three lunar eclipses in 2013. It was visually imperceptible due to the small entry into the penumbral shadow.

This event marked the beginning of Saros series 150.

Visibility

NASA chart of the eclipse


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

Map

Eclipses of 2013

Lunar year (354 days)

This eclipse is the 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

Saros series

This is the first lunar eclipse of Saros series 150.[1] The next occurrence will also be a penumbral eclipse on 5 June 2031. Solar Saros 157 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Partial eclipses in series 150 will occur between 20 August 2157 and past the year 3000. Total eclipses will occur between 29 April 2572 and 28 August 2770.

See also

Notes and references

  1. "Saros Series of Lunar Eclipses".
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