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July 1944 lunar eclipse

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July 1944 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateJuly 6, 1944
Gamma1.2597
Magnitude−0.4398
Saros cycle109 (69 of 73)
Penumbral192 minutes, 43 seconds
Contacts (UTC)
P13:03:18
Greatest4:39:34
P46:16:01

A penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Thursday, July 6, 1944,[1] with an umbral magnitude of −0.4398. 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 July 8, 1944, at 23:40 UTC), the Moon's apparent diameter was larger.[2]

This eclipse was the second of four penumbral lunar eclipses in 1944, with the others occurring on February 9, August 4, and December 29.

Visibility

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The eclipse was completely visible over much of North America, South America, and Antarctica, seen rising over northwestern North America and the central Pacific Ocean and setting over western Europe and Africa.[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]

July 6, 1944 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.53278
Umbral Magnitude −0.43977
Gamma 1.25971
Sun Right Ascension 07h00m41.1s
Sun Declination +22°42'44.2"
Sun Semi-Diameter 15'43.9"
Sun Equatorial Horizontal Parallax 08.6"
Moon Right Ascension 19h00m38.4s
Moon Declination -21°27'57.6"
Moon Semi-Diameter 16'10.5"
Moon Equatorial Horizontal Parallax 0°59'21.8"
ΔT 26.6 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 July–August 1944
July 6
Descending node (full moon)
July 20
Ascending node (new moon)
August 4
Descending node (full moon)
Penumbral lunar eclipse
Lunar Saros 109
Annular solar eclipse
Solar Saros 135
Penumbral lunar eclipse
Lunar Saros 147
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Eclipses in 1944

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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 109

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Inex

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Triad

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Lunar eclipses of 1944–1947

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Lunar eclipse series sets from 1944–1947
Descending node   Ascending node
Saros Date
viewing
Type
chart
Saros Date
viewing
Type
chart
109 1944 Jul 06
Penumbral
114 1944 Dec 29
Penumbral
119 1945 Jun 25
Partial
124 1945 Dec 19
Total
129 1946 Jun 14
Total
134 1946 Dec 08
Total
139 1947 Jun 03
Partial
144 1947 Nov 28
Penumbral

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 116.

June 30, 1935 July 11, 1953

See also

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Notes

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  1. ^ "July 5–6, 1944 Penumbral Lunar Eclipse". timeanddate. Retrieved 19 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 19 December 2024.
  3. ^ "Penumbral Lunar Eclipse of 1944 Jul 06" (PDF). NASA. Retrieved 19 December 2024.
  4. ^ "Penumbral Lunar Eclipse of 1944 Jul 06". EclipseWise.com. Retrieved 19 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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