en November 2040 lunar eclipse

November 2040 lunar eclipse
Total eclipse
	The Moon's hourly motion shown right to left
Date	November 18, 2040
Gamma	0.2361
Magnitude	1.3991
Saros cycle	136 (21 of 72)
Totality	87 minutes, 28 seconds
Partiality	220 minutes, 24 seconds
Penumbral	353 minutes, 36 seconds
P1
Contacts (UTC)
P1	16:07:52
U1	17:14:28
U2	18:20:46
Greatest	19:04:40
U3	19:48:34
U4	20:54:52
P4	22:01:28
	← May 2040 May 2041 →

A total lunar eclipse will occur at the Moon’s ascending node of orbit on Sunday, November 18, 2040,^[1] with an umbral magnitude of 1.3991. 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 5.7 days before apogee (on November 24, 2040, at 14:10 UTC), the Moon's apparent diameter will be smaller.^[2]

The southern limb of the Moon will pass through the center of the Earth's shadow. This is the second central lunar eclipse of Saros series 136, the first taking place on November 8, 2022.

Visibility

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

Eclipse details

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

November 18, 2040 Lunar Eclipse Parameters
Parameter	Value
Penumbral Magnitude	2.45427
Umbral Magnitude	1.39914
Gamma	0.23613
Sun Right Ascension	15h39m03.9s
Sun Declination	-19°29'49.7"
Sun Semi-Diameter	16'11.0"
Sun Equatorial Horizontal Parallax	08.9"
Moon Right Ascension	03h38m45.6s
Moon Declination	+19°42'23.6"
Moon Semi-Diameter	15'20.2"
Moon Equatorial Horizontal Parallax	0°56'17.3"
ΔT	79.6 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 November 2040
November 4 Descending node (new moon)	November 18 Ascending node (full moon)

Partial solar eclipse Solar Saros 124	Total lunar eclipse Lunar Saros 136

Related eclipses

Lunar eclipses of 2038–2042

Lunar eclipse series sets from 2038-2042
Saros	Date Viewing	Type Chart	Saros	Date Viewing	Type Chart
Descending node			Ascending node
111	2038 Jun 17	Penumbral	116	2038 Dec 11	Penumbral
121	2039 Jun 06	Partial	126	2039 Nov 30	Partial
131	2040 May 26	Total	136	2040 Nov 18	Total
141	2041 May 16	Partial	146	2041 Nov 08	Partial
			156	2042 Oct 28	Penumbral

Last set	2038 Jul 16		Last set	2038 Jan 21

Next set	2042 Apr 05		Next set	2042 Sep 29

Saros 136

This eclipse is a part of Saros cycle 136, and the second of the series that passes through the center of the Earth's shadow. The first central eclipse of this series will take place on 8 November 2022. The next occurrence will happen on 30 November 2058.

Metonic series

First eclipse: November 20, 2002.
Second eclipse: November 19, 2021.
Third eclipse: November 18, 2040.
Fourth eclipse: November 19, 2059.
Fifth eclipse: November 19, 2078.

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 annular solar eclipses of Solar Saros 143.