October 2033 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A total lunar eclipse will occur at the Moon’s descending node of orbit on Saturday, October 8, 2033,[1] with an umbral magnitude of 1.3508. 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 only about 3 hours after perigee (on October 8, 2033, at 8:15 UTC), the Moon's apparent diameter will be larger.[2]

This lunar eclipse is the last of a tetrad, with four total lunar eclipses in series, the others being on April 25, 2032; October 18, 2032; and April 14, 2033.

This will also be a supermoon, the first supermoon lunar eclipse by all definitions since May 26, 2021, unlike May 16 in 2022, which was defined by only some as taking place during a supermoon.

Visibility

The eclipse will be completely visible over northeast Asia, eastern Australia, western North America and the Pacific Ocean, seen rising over most of Asia and western Australia and setting over eastern North America and South America.[3]

File:Lunar eclipse from moon-2033Oct08.png File:Lunar eclipse chart close-2033Oct08.png

Eclipse details

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

October 8, 2033 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.30682
Umbral Magnitude 1.35080
Gamma −0.28888
Sun Right Ascension 12h57m01.9s
Sun Declination -06°05'34.4"
Sun Semi-Diameter 16'00.5"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 00h57m22.8s
Moon Declination +05°48'36.0"
Moon Semi-Diameter 16'44.6"
Moon Equatorial Horizontal Parallax 1°01'27.1"
ΔT 75.8 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 September–October 2033
September 23
Ascending node (new moon)
October 8
Descending node (full moon)
File:SE2033Sep23P.png File:Lunar eclipse chart close-2033Oct08.png
Partial solar eclipse
Solar Saros 125
Total lunar eclipse
Lunar Saros 137

Related eclipses

Eclipses in 2033

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 137

Inex

Triad

Lunar eclipses of 2031–2034

Template:Lunar eclipse set 2031-2034

Saros 137

Template:Lunar Saros series 137

Tritos series

Template:Lunar Tritos series January 2001

Inex series

Template:Lunar Inex series October 2004

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 total solar eclipses of Solar Saros 144.

October 2, 2024 October 14, 2042
File:SE2024Oct02A.png File:SE2042Oct14A.png

See also

Notes

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

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External links

Template:Lunar eclipses