Penumbral eclipse | |||||||||
Date | January 10, 2020 | ||||||||
---|---|---|---|---|---|---|---|---|---|
Gamma | 1.0726 | ||||||||
Magnitude | −0.1146 | ||||||||
Saros cycle | 144 (16 of 71) | ||||||||
Penumbral | 244 minutes, 34 seconds | ||||||||
| |||||||||
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, January 10, 2020,[1] with an umbral magnitude of −0.1146. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 2.8 days before perigee (on January 13, 2020, at 15:20 UTC), the Moon's apparent diameter was larger.[2]
This eclipse was the first of four penumbral lunar eclipses in 2020, with the others occurring on June 5, July 5, and November 30.
The eclipse was completely visible over east Africa, Europe, and Asia, seen rising over the west Africa and northern North America and setting over Australia and the central Pacific Ocean.[3]
Visibility map |
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]
Parameter | Value |
---|---|
Penumbral Magnitude | 0.89692 |
Umbral Magnitude | −0.11460 |
Gamma | 1.07270 |
Sun Right Ascension | 19h26m32.0s |
Sun Declination | -21°56'49.6" |
Sun Semi-Diameter | 16'15.9" |
Sun Equatorial Horizontal Parallax | 08.9" |
Moon Right Ascension | 07h26m45.8s |
Moon Declination | +23°00'02.8" |
Moon Semi-Diameter | 16'04.8" |
Moon Equatorial Horizontal Parallax | 0°59'00.8" |
ΔT | 69.5 s |
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.
December 26 Descending node (new moon) |
January 10 Ascending node (full moon) |
---|---|
Annular solar eclipse Solar Saros 132 |
Penumbral lunar eclipse Lunar Saros 144 |
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 |
It is part of Saros cycle 144.
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 partial solar eclipses of Solar Saros 151.
January 4, 2011 | January 14, 2029 |
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