March 1980 lunar eclipse explained

Type:penumbral
Date:1 March 1980
Axis:1.1060°
Gamma:1.22701
Magnitude:0.65455
Saros Ser:142
Saros No:16 of 74
Penumbral:238 minutes, 33.3 seconds
P1:18:45:54.9
Greatest:20:45:13.1
P4:22:44:28.2
Previous:September 1979
Next:July 1980

A penumbral lunar eclipse took place on Saturday, March 1, 1980, the first of three penumbral lunar eclipses in 1980. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 65.455% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 58 minutes and 33.3 seconds.[1]

Visibility

The penumbral eclipse was visible in northeast in North America, east in South America, Europe, Africa, Asia and Australia, seen rising over the Americas and setting over Asia and Australia.

Related lunar eclipses

Eclipses in 1980

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 149.

See also

Notes and References

  1. http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=142 Hermit Eclipse: Saros cycle 142
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros