March 1978 lunar eclipse explained

Type:total
Date:24 March 1978
Axis:0.2044°
Gamma:-0.21402
Magnitude:1.45179
Saros Ser:122
Saros No:54 of 75
Totality:90 minutes, 40.2 seconds
Partiality:218 minutes, 34.5 seconds
Penumbral:345 minutes, 2.2 seconds
P1:13:29:47.4
U1:14:33:05.8
U2:15:37:02.5
Greatest:16:22:21.7
U3:17:07:42.7
U4:18:11:40.3
P4:19:14:49.6
Previous:September 1977
Next:September 1978

A total lunar eclipse took place on Friday, March 24, 1978, the first of two total lunar eclipses in 1978. The moon passed through the center of the Earth's shadow. The Moon was plunged into darkness for 1 hour, 30 minutes and 40.2 seconds, in a deep total eclipse which saw the Moon 45.179% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours, 38 minutes and 34.5 seconds in total.[1]

This is the 54th member of Lunar Saros 122. The previous event is the March 1960 lunar eclipse. The next event is the April 1996 lunar eclipse.

Visibility

It was seen completely over Asia and Australia, and rising over Africa and Europe. It was seen setting over Pacific Ocean on the morning of Friday 24 March, 1978.

Related lunar eclipses

Eclipses in 1978

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 solar eclipses of Solar Saros 129.

See also

Notes and References

  1. http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=122 Hermit Eclipse: Saros cycle 122
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros