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December 1936 lunar eclipse

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December 1936 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateDecember 28, 1936
Gamma−1.0971
Magnitude−0.1550
Saros cycle143 (14 of 73)
Penumbral235 minutes, 31 seconds
Contacts (UTC)
P11:50:57
Greatest3:48:45
P45:46:28

A penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Monday, December 28, 1936,[1] with an umbral magnitude of −0.1550. 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 2.3 days after perigee (on December 25, 1936, at 20:45 UTC), the Moon's apparent diameter was larger.[2]

Visibility

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The eclipse was completely visible over North and South America, west Africa, and Europe, seen rising over the central Pacific Ocean and setting over central Africa, east Africa, west Asia, and central Asia.[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]

December 28, 1936 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.84510
Umbral Magnitude −0.15495
Gamma −1.09705
Sun Right Ascension 18h27m15.3s
Sun Declination -23°17'57.2"
Sun Semi-Diameter 16'16.0"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 06h26m34.6s
Moon Declination +22°13'08.7"
Moon Semi-Diameter 16'15.9"
Moon Equatorial Horizontal Parallax 0°59'41.6"
ΔT 23.9 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 December 1936
December 13
Ascending node (new moon)
December 28
Descending node (full moon)
Annular solar eclipse
Solar Saros 131
Penumbral lunar eclipse
Lunar Saros 143
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Eclipses in 1936

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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 143

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Inex

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Triad

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Lunar eclipses of 1933–1936

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Lunar eclipse series sets from 1933–1936
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
103 1933 Feb 10
Penumbral
108 1933 Aug 05
Penumbral
113 1934 Jan 30
Partial
118 1934 Jul 26
Partial
123 1935 Jan 19
Total
128 1935 Jul 16
Total
133 1936 Jan 08
Total
138 1936 Jul 04
Partial
143 1936 Dec 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 partial solar eclipses of Solar Saros 150.

December 24, 1927 January 3, 1946

See also

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Notes

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  1. ^ "December 27–28, 1936 Penumbral Lunar Eclipse". timeanddate. Retrieved 17 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 17 December 2024.
  3. ^ "Penumbral Lunar Eclipse of 1936 Dec 28" (PDF). NASA. Retrieved 17 December 2024.
  4. ^ "Penumbral Lunar Eclipse of 1936 Dec 28". EclipseWise.com. Retrieved 17 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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