December 1946 lunar eclipse

December 1946 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateDecember 8, 1946
Gamma0.3864
Magnitude1.1639
Saros cycle134 (23 of 73)
Totality57 minutes, 15 seconds
Partiality194 minutes, 54 seconds
Penumbral309 minutes, 29 seconds
Contacts (UTC)
P115:13:16
U116:10:34
U217:19:23
Greatest17:48:01
U318:16:38
U419:25:28
P420:22:45

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, December 8, 1946,[1] with an umbral magnitude of 1.1639. 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 only about 6.5 hours before perigee (on December 9, 1946, at 0:15 UTC), the Moon's apparent diameter was larger.[2]

This lunar eclipse was the last of an almost tetrad, with the others being on June 25, 1945 (partial); December 19, 1945 (total); and June 14, 1946 (total).

Visibility

The eclipse was completely visible over central and eastern Europe, northeast Africa, Asia, and western Australia, seen rising over much of Africa and western Europe and setting over eastern Australia and northwestern North America.[3]

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

December 8, 1946 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.13370
Umbral Magnitude 1.16390
Gamma 0.38643
Sun Right Ascension 16h59m23.8s
Sun Declination -22°42'56.8"
Sun Semi-Diameter 16'14.4"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 04h59m03.0s
Moon Declination +23°06'12.2"
Moon Semi-Diameter 16'44.7"
Moon Equatorial Horizontal Parallax 1°01'27.3"
ΔT 27.8 s

Eclipse season

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 November–December 1946
November 23
Descending node (new moon)
December 8
Ascending node (full moon)
Partial solar eclipse
Solar Saros 122
Total lunar eclipse
Lunar Saros 134

Eclipses in 1946

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 134

Inex

Triad

Lunar eclipses of 1944–1947

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

Saros 134

It was part of Saros series 134.

Half-Saros cycle

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 141.

December 2, 1937 December 14, 1955

See also

Notes

  1. ^ "December 8–9, 1946 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 20 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 20 December 2024.
  3. ^ "Total Lunar Eclipse of 1946 Dec 08" (PDF). NASA. Retrieved 20 December 2024.
  4. ^ "Total Lunar Eclipse of 1946 Dec 08". EclipseWise.com. Retrieved 20 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros