August 1988 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, August 27, 1988,[1] with an umbral magnitude of 0.2916. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. 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. Occurring only about 7 hours before perigee (on August 17, 1988, at 17:50 UTC), the Moon's apparent diameter was larger.[2]

Visibility

The eclipse was completely visible over eastern Australia, western North America, and much of the Pacific Ocean, seen rising over western Australia and the eastern half of Asia and setting over much of North America and South America.[3]

File:Lunar eclipse from moon-1988Aug27.png File:Lunar eclipse chart close-1988Aug27.png

Eclipse details

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

August 27, 1988 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.23803
Umbral Magnitude 0.29159
Gamma −0.86816
Sun Right Ascension 10h25m02.1s
Sun Declination +09°54'10.9"
Sun Semi-Diameter 15'50.0"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 22h26m40.4s
Moon Declination -10°41'41.3"
Moon Semi-Diameter 16'43.7"
Moon Equatorial Horizontal Parallax 1°01'23.7"
ΔT 56.1 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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 August–September 1988
August 27
Ascending node (full moon)
September 11
Descending node (new moon)
File:Lunar eclipse chart close-1988Aug27.png File:SE1988Sep11A.png
Partial lunar eclipse
Lunar Saros 118
Annular solar eclipse
Solar Saros 144

Related eclipses

Eclipses in 1988

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 118

Inex

Triad

Lunar eclipses of 1988–1991

Template:Lunar eclipse set 1988-1991

Metonic series

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 be in nearly the same location relative to the background stars.

  1. 1988 Mar 03.675 – Partial (113)
  2. 2007 Mar 03.972 – Total (123)
  3. 2026 Mar 03.481 – Total (133)
  4. 2045 Mar 03.320 – Penumbral (143)
  1. 1988 Aug 27.461 – partial (118)
  2. 2007 Aug 28.442 – total (128)
  3. 2026 Aug 28.175 – partial (138)
  4. 2045 Aug 27.578 – penumbral (148)
File:Metonic lunar eclipse 1988-2045.png File:Metonic lunar eclipses 1988-2045.png

Saros 118

Template:Lunar Saros series 118

Tritos series

Template:Lunar Tritos series June 2010

Inex series

Template:Lunar Inex series August 2017

Half-Saros cycle

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 solar eclipses of Solar Saros 125.

August 22, 1979 September 2, 1997
File:SE1979Aug22A.png File:SE1997Sep02P.png

See also

Notes

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  1. Script error: No such module "citation/CS1".
  2. Script error: No such module "citation/CS1".
  3. Script error: No such module "citation/CS1".
  4. Script error: No such module "citation/CS1".
  5. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

Template:Lunar eclipses