December 1983 lunar eclipse explained

Type:penumbral
Date:20 December 1983
Axis:1.0625°
Gamma:1.07468
Magnitude:0.88903
Saros Ser:144
Saros No:14 of 71
Penumbral:242 minutes, 20.6 seconds
P1:23:47:55.9 (19 Dec)
Greatest:01:49:03.3
P4:03:50:16.5
Previous:June 1983
Next:May 1984

A penumbral lunar eclipse took place on Tuesday, December 20, 1983, the second of two lunar eclipses in 1983. At the maximum eclipse, 89% of the Moon's disk was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 2 minutes overall.[1]

Related lunar eclipses

Eclipses in 1983

Saros cycle

Lunar Saros series 144, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 20 total lunar eclipses.

First Penumbral Lunar Eclipse: 1749 Jul 29

First Partial Lunar Eclipse: 2146 Mar 28

First Total Lunar Eclipse: 2308 Jul 04

First Central Lunar Eclipse: 2362 Aug 06

Greatest Eclipse of the Lunar Saros 144: 2416 Sep 07

Last Central Lunar Eclipse: 2488 Oct 20

Last Total Lunar Eclipse: 2651 Jan 28

Last Partial Lunar Eclipse: 2867 Jun 08

Last Penumbral Lunar Eclipse: 3011 Sep 04

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[2] This lunar eclipse is related to two partial solar eclipses of Solar Saros 151.

Tzolkinex

See also

Notes and References

  1. http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=144 Hermit Eclipse: Saros cycle 144
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros