August 1980 lunar eclipse explained

Type:penumbral
Date:26 August 1980
Axis:1.1682°
Gamma:-1.16082
Magnitude:0.70891
Saros Ser:147
Saros No:7 of 71
Penumbral:214 minutes, 26.0 seconds
P1:01:43:19.5
Greatest:03:30:29.5
P4:05:17:45.5
Previous:July 1980
Next:January 1981

A penumbral lunar eclipse took place at the Moon's descending node of the orbit on Tuesday, August 26, 1980, the last of three penumbral lunar eclipses in 1980 with a penumbral magnitude of 0.70891. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70.891% 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, 34 minutes and 26 seconds.[1]

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 154.

See also

Notes and References

  1. http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=147 Hermit Eclipse: Saros cycle 147
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros