December 1973 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A partial lunar eclipse occurred at the Moon’s descending node of orbit on Monday, December 10, 1973,[1] with an umbral magnitude of 0.1007. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in 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 only about 21 hours before perigee (on December 10, 1973, at 22:20 UTC), the Moon's apparent diameter was larger.[2]

This eclipse was the last of four lunar eclipses in 1973, with the others occurring on January 18 (penumbral), June 15 (penumbral), and July 15 (penumbral).

Visibility

The eclipse was completely visible over much of North and South America, Africa, Europe, and west and north Asia, seen rising over western North America and the eastern Pacific Ocean and setting over southeast Africa and much of Asia.[3]

File:Lunar eclipse from moon-1973Dec10.png File:Lunar eclipse chart close-1973Dec10.png

Eclipse details

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

December 10, 1973 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.07597
Umbral Magnitude 0.10069
Gamma 0.96441
Sun Right Ascension 17h07m12.8s
Sun Declination -22°53'16.9"
Sun Semi-Diameter 16'14.5"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 05h07m14.5s
Moon Declination +23°52'13.3"
Moon Semi-Diameter 16'39.2"
Moon Equatorial Horizontal Parallax 1°01'07.2"
ΔT 44.3 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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 1973
December 10
Descending node (full moon)
December 24
Ascending node (new moon)
File:Lunar eclipse chart close-1973Dec10.png File:SE1973Dec24A.png
Partial lunar eclipse
Lunar Saros 115
Annular solar eclipse
Solar Saros 141

Related eclipses

Eclipses in 1973

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 115

Inex

Triad

Lunar eclipses of 1973–1976

Template:Lunar eclipse set 1973-1976

Saros 115

Template:Lunar Saros series 115

Tritos series

Template:Lunar Tritos series September 2006

Inex series

Template:Lunar Inex series November 2002

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 partial solar eclipses of Solar Saros 122.

December 4, 1964 December 15, 1982
File:SE1964Dec04P.png File:SE1982Dec15P.png

See also

Notes

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

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External links

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