February 1970 lunar eclipse

Summary

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.

February 1970 lunar eclipse
Partial eclipse
Date21 February 1970
Gamma0.96198
Magnitude0.04639
Saros cycle113 (61 of 71)
Partiality52 minutes, 42.4 seconds
Penumbral298 minutes, 37.5 seconds
Contacts (UTC)
P106:00:45.3
U108:03:45.1
Greatest08:30:03.4
U408:56:27.5
P410:59:22.8

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 edit

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 edit

Lunar year series edit

Lunar eclipse series sets from 1969–1973
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
108 1969 Aug 27
 
Penumbral
 
−1.54066 113 1970 Feb 21
 
Partial
 
0.96198
118 1970 Aug 17
 
Partial
 
−0.80534 123 1971 Feb 10
 
Total
 
0.27413
128 1971 Aug 6
 
Total
 
−0.07944 133 1972 Jan 30
 
Total
 
−0.42729
138 1972 Jul 26
 
Partial
 
0.71167 143 1973 Jan 18
 
Penumbral
 
−1.08446
148 1973 Jul 15
 
Penumbral
 
1.51782
Last set 1969 Sep 25 Last set 1969 Apr 2
Next set 1973 Jun 15 Next set 1973 Dec 10

Metonic cycle edit

This is the third of five Metonic lunar eclipses.

The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the Earth's shadow will in nearly the same location relative to the background stars.

Metonic lunar eclipse sets 1951–2027
Descending node   Ascending node
Saros Date Type Saros Date Type
103 1951 Feb 21.88 Penumbral 108 1951 Aug 17.13 Penumbral
   
113 1970 Feb 21.35 Partial 118 1970 Aug 17.14 Partial
   
123 1989 Feb 20.64 Total 128 1989 Aug 17.13 Total
   
133 2008 Feb 21.14 Total 138 2008 Aug 16.88 Partial
   
143 2027 Feb 20.96 Penumbral 148 2027 Aug 17.30 Penumbral
   

Half-Saros cycle edit

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.

February 15, 1961 February 26, 1979
   

See also edit

Notes edit

  1. ^ Saros series 113
  2. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

External links edit