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September 2042 lunar eclipse

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September 2042 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateSeptember 29, 2042
Gamma−1.0261
Magnitude−0.0011
Saros cycle118 (53 of 73)
Penumbral238 minutes, 32 seconds
Contacts (UTC)
P18:45:03
Greatest10:44:20
P412:43:35

A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Monday, September 29, 2042,[1] with an umbral magnitude of −0.0011. 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 only about 9 hours before perigee (on September 29, 2042, at 19:45 UTC), the Moon's apparent diameter will be larger.[2]

Earlier sources compute this as a 0.3% partial eclipse lasting under 12 minutes,[3] but newer calculations list it as a penumbral eclipse that never enters the umbral shadow.

Visibility

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The eclipse will be completely visible over eastern Australia, northeast Asia, and western North America, seen rising over east Asia and western Australia and setting over eastern North America and South America.[4]

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.[5]

September 29, 2042 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.95481
Umbral Magnitude −0.00105
Gamma −1.02617
Sun Right Ascension 12h23m37.3s
Sun Declination -02°33'13.4"
Sun Semi-Diameter 15'57.9"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 00h25m38.7s
Moon Declination +01°38'07.3"
Moon Semi-Diameter 16'42.1"
Moon Equatorial Horizontal Parallax 1°01'18.0"
ΔT 80.7 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of September–October 2042
September 29
Ascending node (full moon)
October 14
Descending node (new moon)
October 28
Ascending node (full moon)
Penumbral lunar eclipse
Lunar Saros 118
Annular solar eclipse
Solar Saros 144
Penumbral lunar eclipse
Lunar Saros 156
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Eclipses in 2042

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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 118

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Inex

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Triad

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Lunar eclipses of 2042–2045

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Lunar eclipse series sets from 2042-2045
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
113 2042 Apr 05
Penumbral
118 2042 Sep 29
Penumbral
123 2043 Mar 25
Total
128 2043 Sep 19
Total
133 2044 Mar 13
Total
138 2044 Sep 07
Total
143 2045 Mar 03
Penumbral
148 2045 Aug 27
Penumbral
Last set 2041 May 16 Last set 2042 Nov 08
Next set 2046 Jan 22 Next set 2046 Jul 18

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).[6] This lunar eclipse is related to two annular solar eclipses of Solar Saros 125.

September 23, 2033 October 4, 2051

See also

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References

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  1. ^ "September 28–29, 2042 Penumbral Lunar Eclipse". timeanddate. Retrieved 3 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 3 December 2024.
  3. ^ "Extremes of Lunar Eclipse from 1900 to 2100". www.hko.gov.hk.
  4. ^ "Penumbral Lunar Eclipse of 2042 Sep 29" (PDF). NASA. Retrieved 3 December 2024.
  5. ^ "Penumbral Lunar Eclipse of 2042 Sep 29". EclipseWise.com. Retrieved 3 December 2024.
  6. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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