April 2005 lunar eclipse
penumbral
DateApril 24, 2005
Gamma−1.0885
Magnitude−0.1417
Saros ser141
Saros no23 of 73
Penumbral245 minutes, 38 seconds
P 17:52:06
Greatest9:54:51
P 411:57:44
PreviousOctober 2004
NextOctober 2005

A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, April 24, 2005,[1] with an umbral magnitude of −0.1417. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 about 4.9 days before perigee (on April 29, 2005, at 6:10 UTC), the Moon's apparent diameter was larger.[2]

Visibility

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


Hourly motion shown right to left

The Moon's hourly motion across the Earth's shadow in the constellation of Virgo.

Visibility map

Eclipse details

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

April 24, 2005 Lunar Eclipse Parameters
ParameterValue
Penumbral Magnitude0.86693
Umbral Magnitude−0.14165
Gamma−1.08851
Sun Right Ascension02h08m13.9s
Sun Declination+12°57'36.8"
Sun Semi-Diameter15'54.1"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension14h06m23.1s
Moon Declination-13°54'32.8"
Moon Semi-Diameter15'46.0"
Moon Equatorial Horizontal Parallax0°57'51.7"
ΔT64.7 s

Eclipse season

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 April 2005
April 8
Ascending node (new moon)
April 24
Descending node (full moon)
Hybrid solar eclipse
Solar Saros 129
Penumbral lunar eclipse
Lunar Saros 141

Eclipses in 2005

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 141

Inex

Triad

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 148.

April 17, 1996April 29, 2014

See also

References

  1. ^ "April 23–24, 2005 Penumbral Lunar Eclipse". timeanddate. Retrieved 13 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 13 November 2024.
  3. ^ "Penumbral Lunar Eclipse of 2005 Apr 24". NASA. Retrieved 13 November 2024.
  4. ^ "Penumbral Lunar Eclipse of 2005 Apr 24". EclipseWise.com. Retrieved 13 November 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros