October 2013 lunar eclipse

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Template:Short description Script error: No such module "Unsubst". Template:Infobox lunar eclipse A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Friday, 18 October 2013,[1] with an umbral magnitude of −0.2706. 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. The Moon's apparent diameter was near the average diameter because it occurred 8.2 days after perigee (on 10 October 2013, at 19:15 UTC) and 6.9 days before apogee (on 25 October 2013, at 10:25 UTC).[2]

Visibility

The eclipse was completely visible over Africa, Europe, eastern South America, and west Asia, seen rising over western South America and North America and setting over south and east Asia.[3]

File:Lunar eclipse from moon-2013Oct18.png File:Lunar eclipse chart close-2013Oct18.png
File:Visibility Lunar Eclipse 2013-10-18.png
Visibility map

Images

File:2013-10-18 Lunar Eclipse Sketch.png
NASA chart of the eclipse

Gallery

Eclipse details

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

18 October 2013 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.76603
Umbral Magnitude −0.27064
Gamma 1.15082
Sun Right Ascension 13h35m31.9s
Sun Declination -09°57'14.9"
Sun Semi-Diameter 16'03.4"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 01h34m19.6s
Moon Declination +11°00'12.1"
Moon Semi-Diameter 15'29.3"
Moon Equatorial Horizontal Parallax 0°56'50.7"
ΔT 67.2 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 October–November 2013
October 18
Descending node (full moon)
November 3
Ascending node (new moon)
File:Lunar eclipse chart close-2013Oct18.png File:SE2013Nov03H.png
Penumbral lunar eclipse
Lunar Saros 117
Hybrid solar eclipse
Solar Saros 143

Related eclipses

Eclipses in 2013

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 117

Inex

Triad

Lunar eclipses of 2013–2016

Template:Lunar eclipse set 2013-2016

Saros 117

Template:Lunar Saros series 117

Tritos series

Template:Lunar Tritos series November 2002

Inex series

Template:Lunar Inex series October 2013

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 partial solar eclipses of Solar Saros 124.

October 14, 2004 October 25, 2022
File:SE2004Oct14P.png File:SE2022Oct25P.png

See also

References

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  5. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

Script error: No such module "Side box". Template:Lunar eclipses