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October 2052 lunar eclipse

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October 2052 lunar eclipse
Partial eclipse
The Moon's hourly motion shown right to left
DateOctober 8, 2052
Gamma−0.9726
Magnitude0.0821
Saros cycle147 (10 of 70)
Partiality63 minutes, 16 seconds
Penumbral256 minutes, 37 seconds
Contacts (UTC)
P18:36:02
U110:12:46
Greatest10:44:19
U411:16:02
P412:52:38

A partial lunar eclipse will occur at the Moon’s descending node of orbit on Tuesday, October 8, 2052,[1] with an umbral magnitude of 0.0821. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in 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 2.1 days before perigee (on October 10, 2052, at 11:35 UTC), the Moon's apparent diameter will be larger.[2]

Visibility

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The eclipse will be completely visible over northeast Asia, eastern Australia, and western North America, seen rising over east and south Asia and western Australia and setting over eastern North America and much of South America.[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]

October 8, 2052 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.06533
Umbral Magnitude 0.08320
Gamma −0.97270
Sun Right Ascension 12h58m28.0s
Sun Declination -06°14'27.6"
Sun Semi-Diameter 16'00.5"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 00h59m36.6s
Moon Declination +05°18'49.9"
Moon Semi-Diameter 16'18.0"
Moon Equatorial Horizontal Parallax 0°59'49.3"
ΔT 86.9 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 September–October 2052
September 22
Ascending node (new moon)
October 8
Descending node (full moon)
Annular solar eclipse
Solar Saros 135
Partial lunar eclipse
Lunar Saros 147
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Eclipses in 2052

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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 147

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Inex

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Triad

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Lunar eclipses of 2049–2052

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Lunar eclipse series sets from 2049-2052
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
112 2049 May 17
Penumbral
117 2049 Nov 09
Penumbral
122 2050 May 06
Total
127 2050 Oct 30
Total
132 2051 Apr 26
Total
137 2051 Oct 19
Total
142 2052 Apr 14
Penumbral
147 2052 Oct 08
Partial
Last set 2049 Jun 15 Last set 2048 Dec 20
Next set 2053 Mar 04 Next set 2053 Aug 29

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 154.

October 3, 2043 October 13, 2061

See also

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Notes

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  1. ^ "October 7–8, 2052 Partial 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 2052 Oct 08" (PDF). NASA. Retrieved 12 December 2024.
  4. ^ "Partial Lunar Eclipse of 2052 Oct 08". EclipseWise.com. Retrieved 12 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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