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October 1986 lunar eclipse

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October 1986 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateOctober 17, 1986
Gamma0.3189
Magnitude1.2455
Saros cycle136 (18 of 72)
Totality73 minutes, 41 seconds
Partiality216 minutes, 48 seconds
Penumbral353 minutes, 12 seconds
Contacts (UTC)
P116:21:26
U117:29:33
U218:41:07
Greatest19:17:59
U319:54:48
U421:06:22
P422:14:38

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, October 17, 1986,[1] with an umbral magnitude of 1.2455. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 5.5 days before apogee (on October 23, 1986, at 6:35 UTC), the Moon's apparent diameter was smaller.[2]

This lunar eclipse was the last of a tetrad, with four total lunar eclipses in series, the others being on May 4, 1985; October 28, 1985; and April 24, 1986.

Visibility

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The eclipse was completely visible over east Africa, eastern Europe, and Asia, seen rising over northeastern North America, eastern South America, western Europe, and west Africa and setting over Australia, northeast Asia, and the western Pacific Ocean.[3]

Eclipse details

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Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

October 17, 1986 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.30082
Umbral Magnitude 1.24545
Gamma 0.31887
Sun Right Ascension 13h29m20.1s
Sun Declination -09°21'26.2"
Sun Semi-Diameter 16'03.1"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 01h28m47.0s
Moon Declination +09°37'14.9"
Moon Semi-Diameter 15'12.6"
Moon Equatorial Horizontal Parallax 0°55'49.1"
ΔT 55.2 s

Eclipse season

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This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of October 1986
October 3
Descending node (new moon)
October 17
Ascending node (full moon)
Hybrid solar eclipse
Solar Saros 124
Total lunar eclipse
Lunar Saros 136
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Eclipses in 1986

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 136

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Inex

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Triad

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Lunar eclipses of 1984–1987

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Lunar eclipse series sets from 1984–1987
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
111 1984 May 15
Penumbral
1.11308 116 1984 Nov 08
Penumbral
−1.08998
121 1985 May 04
Total
0.35197 126 1985 Oct 28
Total
−0.40218
131 1986 Apr 24
Total
−0.36826 136 1986 Oct 17
Total
0.31887
141 1987 Apr 14
Penumbral
−1.13641 146 1987 Oct 07
Penumbral
1.01890
Last set 1984 Jun 13 Last set 1983 Dec 20
Next set 1988 Mar 03 Next set 1988 Aug 27

Metonic series

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This eclipse is the third of four Metonic cycle lunar eclipses on the same date, October 17–18, each separated by 19 years:

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 1948–2005
Descending node   Ascending node
Saros Date Type Saros Date Type
111 1948 Apr 23 Partial 116 1948 Oct 18 Penumbral
121 1967 Apr 24 Total 126 1967 Oct 18 Total
131 1986 Apr 24 Total 136 1986 Oct 17 Total
141 2005 Apr 24 Penumbral 146 2005 Oct 17 Partial

Half-Saros cycle

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A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two total solar eclipses of Solar Saros 143.

October 12, 1977 October 24, 1995

See also

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Notes

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  1. ^ "October 17–18, 1986 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 6 January 2025.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 6 January 2025.
  3. ^ "Total Lunar Eclipse of 1986 Oct 17" (PDF). NASA. Retrieved 6 January 2025.
  4. ^ "Total Lunar Eclipse of 1986 Oct 17". EclipseWise.com. Retrieved 6 January 2025.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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