December 1965 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, December 8, 1965,[1] with an umbral magnitude of −0.1200. 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 2.5 days before perigee (on December 11, 1965, at 6:00 UTC), the Moon's apparent diameter was larger.[2]

Visibility

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

File:Lunar eclipse from moon-1965Dec08.png File:Lunar eclipse chart close-1965Dec08.png

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, 1965 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.88203
Umbral Magnitude −0.12004
Gamma 1.07748
Sun Right Ascension 17h00m58.1s
Sun Declination -22°45'04.3"
Sun Semi-Diameter 16'14.4"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 05h00m02.9s
Moon Declination +23°47'53.1"
Moon Semi-Diameter 16'12.3"
Moon Equatorial Horizontal Parallax 0°59'28.5"
ΔT 36.5 s

Eclipse season

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Eclipse season of November–December 1965
November 23
Descending node (new moon)
December 8
Ascending node (full moon)
File:SE1965Nov23A.png File:Lunar eclipse chart close-1965Dec08.png
Annular solar eclipse
Solar Saros 132
Penumbral lunar eclipse
Lunar Saros 144

Related eclipses

Eclipses in 1965

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 144

Inex

Triad

Lunar eclipses of 1962–1965

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[5]

The penumbral lunar eclipses on February 19, 1962 and August 15, 1962 occur in the previous lunar year eclipse set.

Lunar eclipse series sets from 1962 to 1965
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
109 1962 Jul 17
File:Lunar eclipse from moon-1962Jul17.png
Penumbral
File:Lunar eclipse chart close-1962Jul17.png
1.3371 114 1963 Jan 09
File:Lunar eclipse from moon-1963Jan09.png
Penumbral
File:Lunar eclipse chart close-1963Jan09.png
−1.0128
119 1963 Jul 06
File:Lunar eclipse from moon-1963Jul06.png
Partial
File:Lunar eclipse chart close-1963Jul06.png
0.6197 124 1963 Dec 30
File:Lunar eclipse from moon-1963Dec30.png
Total
File:Lunar eclipse chart close-1963Dec30.png
−0.2889
129 1964 Jun 25
File:Lunar eclipse from moon-1964Jun25.png
Total
File:Lunar eclipse chart close-1964Jun25.png
−0.1461 134 1964 Dec 19
File:Lunar eclipse from moon-1964Dec19.png
Total
File:Lunar eclipse chart close-1964Dec19.png
0.3801
139 1965 Jun 14
File:Lunar eclipse from moon-1965Jun14.png
Partial
File:Lunar eclipse chart close-1965Jun14.png
−0.9006 144 1965 Dec 08
File:Lunar eclipse from moon-1965Dec08.png
Penumbral
File:Lunar eclipse chart close-1965Dec08.png
1.0775

Saros 144

Template:Lunar Saros series 144

Tritos series

Template:Lunar Tritos series August 2009

Inex series

Template:Lunar Inex series October 2023

Half-Saros cycle

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 partial solar eclipses of Solar Saros 151.

December 2, 1956 December 13, 1974
File:SE1956Dec02P.png File:SE1974Dec13P.png

See also

Notes

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  6. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

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