Jump to content

September 1977 lunar eclipse

From Wikipedia, the free encyclopedia
September 1977 lunar eclipse
Penumbral eclipse
Date27 September 1977
Gamma1.07682
Magnitude0.90076
Saros cycle117 (50 of 72)
Penumbral257 minutes, 35.5 seconds
Contacts (UTC)
P106:20:28.6
Greatest08:29:19.4
P410:38:04.1

A penumbral lunar eclipse took place on Tuesday, September 27, 1977, the second of two lunar eclipses in 1977. At maximum eclipse, 90.076% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours, 17 minutes and 35.5 seconds overall. Occurring 6.2 days before apogee (Apogee on October 3, 1977), the Moon's apparent diameter was 2.2% smaller than average.[1]

Visibility

[edit]

It was completely visible over east in Asia, Australia, Pacific, North America and South America, seen rising over Asia, East China Sea and Australia and setting over the Atlantic and South America.

[edit]

Eclipses in 1977

[edit]

Lunar year series

[edit]
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

[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 solar eclipses of Solar Saros 124.

September 22, 1968 October 3, 1986

See also

[edit]

Notes

[edit]
  1. ^ Hermit Eclipse: Saros cycle 117
  2. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
[edit]