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January 1936 lunar eclipse

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January 1936 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateJanuary 8, 1936
Gamma−0.4429
Magnitude1.0173
Saros cycle133 (22 of 71)
Totality20 minutes, 48 seconds
Partiality202 minutes, 31 seconds
Penumbral342 minutes, 5 seconds
Contacts (UTC)
P115:18:34
U116:28:17
U217:59:09
Greatest18:09:34
U318:19:56
U419:50:48
P421:00:40

A total lunar eclipse occurred at the Moon’s descending node of orbit on Wednesday, January 8, 1936,[1] with an umbral magnitude of 1.0173. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 6.2 days before apogee (on January 14, 1936, at 23:50 UTC), the Moon's apparent diameter was smaller.[2]

Visibility

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The eclipse was completely visible over eastern Europe, Asia, and western Australia, seen rising over Africa andwestern Europe and setting over eastern Australia, 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]

January 8, 1936 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.07396
Umbral Magnitude 1.01725
Gamma −0.44288
Sun Right Ascension 19h15m02.9s
Sun Declination -22°19'38.2"
Sun Semi-Diameter 16'15.9"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 07h14m38.5s
Moon Declination +21°55'15.9"
Moon Semi-Diameter 15'23.6"
Moon Equatorial Horizontal Parallax 0°56'29.6"
ΔT 23.8 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 1935–January 1936
December 25
Ascending node (new moon)
January 8
Descending node (full moon)
Annular solar eclipse
Solar Saros 121
Total lunar eclipse
Lunar Saros 133
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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 133

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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 annular solar eclipses of Solar Saros 140.

January 3, 1927 January 14, 1945

See also

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Notes

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  1. ^ "January 8–9, 1936 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 17 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 17 December 2024.
  3. ^ "Total Lunar Eclipse of 1936 Jan 08" (PDF). NASA. Retrieved 17 December 2024.
  4. ^ "Total Lunar Eclipse of 1936 Jan 08". EclipseWise.com. Retrieved 17 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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