Jump to content

March 1980 lunar eclipse: Difference between revisions

From Wikipedia, the free encyclopedia
Content deleted Content added
No edit summary
Tag: Reverted
No edit summary
Tag: Reverted
Line 17: Line 17:
| next = July 1980
| 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. Occurring only 1.6 days before apogee (Apogee on Monday, March 3, 1980), the Moon's apparent diameter was 6.3% smaller than average.<ref>[http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=142 Hermit Eclipse: Saros cycle 142]</ref>
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. Occurring only 1.6 days before apogee (Apogee on Monday, March 3, 1980), the Moon's apparent diameter was 6.3% smaller than average. The Moon was 405,409.27 km (251,909.64 mi) making it a Micro Full Moon. Micro Full Moons are 12.4% smaller than Super Full Moons.<ref>[http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=142 Hermit Eclipse: Saros cycle 142]</ref>


== Visibility ==
== Visibility ==

Revision as of 22:12, 1 April 2023

March 1980 lunar eclipse
Penumbral eclipse
Date1 March 1980
Gamma1.22701
Magnitude0.65455
Saros cycle142 (16 of 74)
Penumbral238 minutes, 33.3 seconds
Contacts (UTC)
P118:45:54.9
Greatest20:45:13.1
P422:44:28.2

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. Occurring only 1.6 days before apogee (Apogee on Monday, March 3, 1980), the Moon's apparent diameter was 6.3% smaller than average. The Moon was 405,409.27 km (251,909.64 mi) making it a Micro Full Moon. Micro Full Moons are 12.4% smaller than Super Full Moons.[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.

Eclipses in 1980

Lunar year series

Lunar eclipse series sets from 1977–1980
Ascending node   Descending node
Saros Date
viewing
Type
chart
Gamma Saros Date
viewing
Type
chart
Gamma
112 1977 Apr 04
Partial
−0.91483 117 1977 Sep 27
Penumbral
1.07682
122 1978 Mar 24
Total
−0.21402 127 1978 Sep 16
Total
0.29510
132 1979 Mar 13
Partial
0.52537 137 1979 Sep 06
Total
−0.43050
142 1980 Mar 01
Penumbral
1.22701 147 1980 Aug 26
Penumbral
−1.16082
Last set 1976 May 13 Last set 1976 Nov 06
Next set 1981 Jan 20 Next set 1980 Jul 27

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.

February 25, 1971 March 7, 1989

See also

Notes

  1. ^ Hermit Eclipse: Saros cycle 142
  2. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros