February 1970 lunar eclipse explained

Type:partial
Date:21 February 1970
Axis:0.8698°
Gamma:0.96198
Magnitude:0.04639
Saros Ser:113
Saros No:61 of 71
Partiality:52 minutes, 42.4 seconds
Penumbral:298 minutes, 37.5 seconds
P1:06:00:45.3
U1:08:03:45.1
Greatest:08:30:03.4
U4:08:56:27.5
P4:10:59:22.8
Previous:September 1969
Next:August 1970

A partial lunar eclipse took place on Saturday, February 21, 1970. It was the first of two partial lunar eclipses in 1970, the other being on August 17 of the same year. A tiny bite out of the Moon may have been visible at maximum, though just 5% of the Moon was shadowed in a partial eclipse which lasted for 52 minutes and 42 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.

Occurring only 2.4 days after apogee (Apogee on Wednesday, February 18, 1970), the Moon's apparent diameter was 6% smaller than average. The Moon was only 404,163 km (251,135 mi) from the Earth's center.[1]

Visibility

It was completely visible over eastern Asia, Australia, Pacific, Americas, western Europe, seen rising over northwestern Pacific Ocean and setting over the north Atlantic Ocean.

Relation to other lunar eclipses

Metonic cycle

This is the third of five Metonic lunar eclipses.

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 total solar eclipses of Solar Saros 120.

See also

Notes and References

  1. http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=113 Saros series 113
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros