January 2018 lunar eclipse

A total lunar eclipse occurred on 31 January 2018. The Moon was near its perigee on 30 January and as such may be described as a "supermoon", when the Moon's distance from the Earth is less than 360,000 km (223,694 miles). The previous supermoon lunar eclipse was in September 2015.[1]

January 2018 lunar eclipse
Total eclipse
Totality as viewed from Lomita, California
Date31 January 2018
Gamma−0.3014
Magnitude1.3155
Saros cycle124 (49 of 74)
Totality76 minutes, 4 seconds
Partiality202 minutes, 44 seconds
Penumbral317 minutes, 12 seconds
Contacts (UTC)
P110:51:15
U111:48:27
U212:51:47
Greatest13:29:50
U314:07:51
U415:11:11
P416:08:27

During the total lunar eclipse of Wednesday, 31 January 2018, the Moon was 360,202 km (only 202 km to be a Super Full Moon) (223,819 mi) from the Earth. A blue moon occurs because there are 2 full moons in the same calendar month, or if there are 4 full moons in the same season (third of four is blue moon). As this supermoon was also a blue moon (the second full moon in a calendar month), it was referred to as a "super blue blood moon"; "blood" refers to the typical red color of the Moon during a total lunar eclipse. The 31 January, 2018 lunar event was called 'Trifecta'.[2] This coincidence last occurred on 30 December 1982 for the eastern hemisphere,[3] and otherwise before that on 31 March 1866.[4][5] The next occurrence will be on 31 January 2037, one metonic cycle (19 years) later.

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.[6]

The following simulation shows the approximate appearance of the Moon passing through Earth's shadow. The northern portion of the Moon is closest to the center of the shadow, making it darkest and reddest in appearance.

"Super blue blood moon"

This was a "supermoon", as the Moon was near to its closest distance to earth in its elliptical orbit, making it 7% larger in apparent diameter or 14% larger in area, than an average full moon. The previous supermoon lunar eclipse was the September 2015 lunar eclipse.[1]

The full moon of 31 January 2018 was the second full moon that calendar month (in most time zones), making it, under one definition of the term, a "blue moon".

Additionally referencing the orange or red "blood" colors that occur during a lunar eclipse, media sources described the event as a "super blue blood Moon".[7]

Characteristics

Visibility

The Pacific Ocean was turned toward the Moon at the time of the eclipse. Central and eastern Asia (including most of Siberia), Philippines, Indonesia, New Zealand and most of Australia got a good view of this moon show in the evening sky. For Western Asia, the Indian subcontinent, the Middle East and Eastern Europe, the eclipse was underway as the moon rose.[8]

Along the U.S. West Coast, the total phase began at 4:51 a.m. PST. The further east, the closer the start of the partial phases coincided with moonset. Along the U.S. Atlantic Seaboard, for instance, the Moon had only just begun to enter the darkest part of Earth's shadow, the umbra, at 6:48 a.m. EST when it disappeared from view below the west-northwest horizon. The duration of the total phase was 77 minutes, with the Moon tracking through the southern part of the Earth's shadow. During totality, the Moon's lower limb appeared brighter than the dark upper limb.[8]


Visibility map

Timing

Event timing by time zone
EclipseHSTAKSTPSTMSTCSTESTUTCMSKISTICTCSTJSTAEDTNZDT
Zone from UTC−10 h−9 h−8 h−7 h−6 h−5 h0 h+3 h+5½ h+7 h+8 h+9 h+11 h+13 h
Penumbral eclipse begins00:5101:5102:5103:5104:5105:5110:5113:5117:5118:5119:5121:5123:51
Partial eclipse begins01:4802:4803:4804:4805:4806:4811:4814:4817:1818:4819:4820:4822:4800:48
Total eclipse begins02:5203:5204:5205:5206:5212:5215:5218:2219:5220:5221:5223:5201:52
Mid-eclipse03:3004:3005:3006:3013:3016:3019:0020:3021:3022:3000:3002:30
Total eclipse ends04:0805:0806:0807:0814:0817:0819:3821:0822:0823:0801:0803:08
Partial eclipse ends05:1106:1107:1115:1118:1120:4122:1123:1100:1102:1104:11
Penumbral eclipse ends06:0807:0816:0819:0821:3823:0800:0801:0803:0805:08

North America

Asia and Middle East

Oceania

Eclipses of 2018

The January 2018 lunar eclipse is the first ascending node eclipse of the lunar eclipse series sets from 2016 to 2020. It is also part of Saros cycle 124.

Lunar eclipse series sets from 2016–2020
Descending node Ascending node
SarosDateType
Viewing
GammaSarosDate
Viewing
Type
Chart
Gamma
1092016 Aug 18
Penumbral
1.56406114
2017 Feb 11
Penumbral
−1.02548
119
2017 Aug 07
Partial
0.86690124
2018 Jan 31
Total
−0.30143
129
2018 Jul 27
Total
0.11681134
2019 Jan 21
Total
0.36842
139
2019 Jul 16
Partial
−0.64300144
2020 Jan 10
Penumbral
1.07270
1492020 Jul 05
Penumbral
−1.36387
Last set2016 Sep 16Last set2016 Mar 23
Next set2020 Jun 05Next set2020 Nov 30

A similar eclipse occurs on 31 January 2037, one metonic cycle of 19 years in the future.

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[9] This lunar eclipse is related to two annular solar eclipses of Solar Saros 131.

26 January 20096 February 2027

See also

References