August 1952 lunar eclipse explained

Type:partial
Date:August 5, 1952
Gamma:-0.7383
Magnitude:0.5317
Saros Ser:118
Saros No:48 of 74
Partiality:147 minutes and 10 seconds
Penumbral:278 minutes and 22 seconds
P1:17:28:13
U1:18:33:49
Greatest:19:47:55
U4:21:01:00
P4:22:06:35
Previous:February 1952
Next:January 1953

A partial lunar eclipse took place on Tuesday, August 5, 1952. The Earth's shadow on the Moon was clearly visible in this eclipse, with 53.2% of the Moon in shadow; the partial eclipse lasted for 2 hours and 27 minutes. The Moon's apparent diameter was larger and Supermoon because the eclipse occurred only 45 minutes before perigee.[1]

Visibility

The partial eclipse was visible from Europe, Africa, Asia, and Australia, seen rising over eastern South America and Atlantic, and setting over Pacific.

Related 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 annular solar eclipses of Solar Saros 125.

See also

Notes and References

  1. http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=118 Hermit Eclipse: Saros cycle 118
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros