March 2053 lunar eclipse

A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Tuesday, March 4, 2053,[1] with an umbral magnitude of −0.0796. 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 4.1 days after perigee (on February 28, 2053, at 15:30 UTC), the Moon's apparent diameter will be larger.[2]

March 2053 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateMarch 4, 2053
Gamma−1.0530
Magnitude−0.0796
Saros cycle114 (61 of 71)
Penumbral251 minutes, 5 seconds
Contacts (UTC)
P115:14:56
Greatest17:20:31
P419:26:01

Visibility

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The eclipse will be completely visible over Asia and Australia, seen rising over Africa and Europe and setting over northwestern North America and the central Pacific Ocean.[3]

   

Eclipse details

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Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

March 4, 2053 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.93338
Umbral Magnitude −0.07963
Gamma −1.05310
Sun Right Ascension 23h03m14.8s
Sun Declination -06°03'47.9"
Sun Semi-Diameter 16'07.7"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 11h02m02.1s
Moon Declination +05°04'58.9"
Moon Semi-Diameter 15'55.3"
Moon Equatorial Horizontal Parallax 0°58'26.0"
ΔT 87.2 s

Eclipse season

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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.

Eclipse season of March 2053
March 4
Ascending node (full moon)
March 20
Descending node (new moon)
   
Penumbral lunar eclipse
Lunar Saros 114
Annular solar eclipse
Solar Saros 140
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Eclipses in 2053

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 114

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Inex

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Triad

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Lunar eclipses of 2053–2056

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Lunar eclipse series sets from 2053–2056
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
114 2053 Mar 04
 
Penumbral
 
119 2053 Aug 29
Penumbral
 
124 2054 Feb 22
 
Total
 
129 2054 Aug 18
 
Total
 
134 2055 Feb 11
 
Total
 
139 2055 Aug 07
 
Partial
 
144 2056 Feb 01
 
Penumbral
 
149 2056 Jul 26
 
Partial
 
Last set 2052 Apr 14 Last set 2052 Oct 08
Next set 2056 Dec 22 Next set 2056 Jun 27

Half-Saros cycle

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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 total solar eclipses of Solar Saros 121.

February 28, 2044 March 11, 2062
   

See also

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  1. ^ "March 4–5, 2053 Penumbral Lunar Eclipse". timeanddate. Retrieved 12 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 12 December 2024.
  3. ^ "Partial Lunar Eclipse of 2053 Mar 04" (PDF). NASA. Retrieved 12 December 2024.
  4. ^ "Penumbral Lunar Eclipse of 2053 Mar 04". EclipseWise.com. Retrieved 12 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros