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! bgcolor=#e7dcc3 colspan=2|Total lunar eclipse<BR>July 27, 2018
! bgcolor=#e7dcc3 colspan=2|Total lunar eclipse<BR>July 27, 2018
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| align=center colspan=2|Ecliptic north up<BR>[[File:Lunar eclipse chart close-2018Jul27.png|250px]]<BR>The moon will pass through the center of the Earth's shadow.
| align=center colspan=2|Ecliptic north up<BR>[[File:Lunar eclipse chart close-2018Jul27.png|250px]]<BR>The moon will pass through the centre of the Earth's shadow.
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|align=center bgcolor=#c0d0e0| [[Saros cycle]] || 129 (38 of 71)
|align=center bgcolor=#c0d0e0| [[Saros cycle]] || 129 (38 of 71)

Revision as of 21:56, 14 July 2018

Total lunar eclipse
July 27, 2018
Ecliptic north up

The moon will pass through the centre of the Earth's shadow.
Saros cycle 129 (38 of 71)
Gamma +0.1168
Duration (hr:mn:sc)
Totality 1:42:57
Partial 3:54:32
Penumbral 6:13:48
Contacts (UTC)
P1 17:14:49
U1 18:24:27
U2 19:30:15
Greatest 20:21:44
U3 21:13:12
U4 22:19:00
P4 23:28:37

A total lunar eclipse will occur on July 27, 2018. The Moon will pass through the center of the Earth's shadow. This will be the first central lunar eclipse since June 15, 2011.

Since it will occur near apogee, this eclipse will also be the longest total lunar eclipse in the 21st century. Totality will last approximately 103 minutes.[1]

This eclipse will be the second total lunar eclipse in 2018, after the one in January.

Visibility

It will be completely visible over Eastern Africa, and Central Asia, seen rising over South America, Western Africa, and Europe, and setting over Eastern Asia, and Australia.


View of Earth from Moon at greatest eclipse

Visibility map

Background

A lunar eclipse occurs when the Moon passes within Earth's umbra (shadow). As the eclipse begins, Earth's shadow first darkens the Moon slightly. Then, the shadow begins to "cover" part of the Moon, turning it a dark red-brown color (typically – the color can vary based on atmospheric conditions). The Moon appears to be reddish because of Rayleigh scattering (the same effect that causes sunsets to appear reddish) and the refraction of that light by Earth's atmosphere into its umbra.[2]

The following simulation shows the approximate appearance of the Moon passing through Earth's shadow. The Moon's brightness is exaggerated within the umbral shadow. The northern portion of the Moon was closest to the center of the shadow, making it darkest, and most red in appearance.

Lunar year series

Lunar eclipse series sets from 2016–2020
Descending node   Ascending node
Saros Date Type
Viewing
Gamma Saros Date
Viewing
Type
Chart
Gamma
109 2016 Aug 18
Penumbral
1.56406 114
2017 Feb 11
Penumbral
−1.02548
119
2017 Aug 07
Partial
0.86690 124
2018 Jan 31
Total
−0.30143
129
2018 Jul 27
Total
0.11681 134
2019 Jan 21
Total
0.36842
139
2019 Jul 16
Partial
−0.64300 144
2020 Jan 10
Penumbral
1.07270
149 2020 Jul 05
Penumbral
−1.36387
Last set 2016 Sep 16 Last set 2016 Mar 23
Next set 2020 Jun 05 Next set 2020 Nov 30

Saros series

Lunar saros series 129, repeating every 18 years and 11 days, containing 71 events, has 11 total lunar eclipses. The first total lunar eclipse of this series was on May 24, 1910, and last will be on September 8, 2090. The longest occurrence of this series was on July 16, 2000 when totality lasted 106 minutes and 24.6 seconds.

Greatest First

The greatest eclipse of the series occurred on 2000 Jul 16, lasting 106 minutes.
Penumbral Partial Total Central
1351 Jun 10 1513 Sep 15 1910 May 24 1946 Jun 14
Last
Central Total Partial Penumbral
2036 Aug 7 2090 Sep 8 2469 Apr 26 2613 Jul 24
1901–2100
1910 May 24 1928 Jun 3 1946 Jun 14
1964 Jun 25 1982 Jul 6 2000 Jul 16
2018 Jul 27 2036 Aug 7 2054 Aug 18
2072 Aug 28 2090 Sep 8

See also

Notes

  1. ^ https://earth-chronicles.com/space/in-2018-the-longest-lunar-eclipse-will-take-place-in-100-years.html
  2. ^ Fred Espenak; Jean Meeus. "Visual Appearance of Lunar Eclipses". NASA. Retrieved April 13, 2014. {{cite web}}: Unknown parameter |last-author-amp= ignored (|name-list-style= suggested) (help)