March 2025 lunar eclipse

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Template:Short description Script error: No such module "Unsubst". Template:Infobox lunar eclipse

A total lunar eclipse occurred at the Moon's descending node of orbit on Friday, March 14, 2025,[1] with an umbral magnitude of 1.1804. 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 total 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 3.3 days before apogee (on March 17, 2025, at 12:35 UTC), the Moon's apparent diameter was smaller.[2]

This lunar eclipse was the first of an almost tetrad, with the others being on September 8, 2025 (total); March 3, 2026 (total); and August 28, 2026 (partial).

This eclipse was seen from the surface of the Moon by Firefly Aerospace's Blue Ghost Mission 1 lander, which captured images of the ring of light around the Earth as the Sun passed behind it and the red glow on the Moon's surface.[3][4]

Visibility

The eclipse was completely visible over North America and South America, seen rising over Australia and northeast Asia and setting over Africa and Europe.[5]

File:Lunar eclipse from moon-2025Mar14.png
Simulated view of earth from moon
File:Lunar-eclipse-from-moon-earth-3-14-2025.png
From moon, with IR clouds[6]
File:Lunar eclipse chart close-2025Mar14.png

Gallery

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.[7]

March 14, 2025 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.26146
Umbral Magnitude 1.18038
Gamma 0.34846
Sun Right Ascension 23h37m46.0s
Sun Declination -02°24'16.8"
Sun Semi-Diameter 16'05.2"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 11h38m23.0s
Moon Declination +02°40'54.6"
Moon Semi-Diameter 14'52.8"
Moon Equatorial Horizontal Parallax 0°54'36.8"
ΔT 71.7 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. Each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each calendar year and part of a third may occur. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of March 2025
March 14
Descending node (full moon)
March 29
Ascending node (new moon)
File:Lunar eclipse chart close-2025Mar14.png File:SE2025Mar29P.png
Total lunar eclipse
Lunar Saros 123
Partial solar eclipse
Solar Saros 149

Related eclipses

Eclipses in 2025

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 123

Inex

Triad

Lunar eclipses of 2024–2027

Template:Lunar eclipse set 2024-2027

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 in nearly the same location relative to the background stars.

  1. 2006 Mar 14.99 - penumbral (113)
  2. 2025 Mar 14.29 - total (123)
  3. 2044 Mar 13.82 - total (133)
  4. 2063 Mar 14.67- partial (143)
  1. 2006 Sep 07.79 - partial (118)
  2. 2025 Sep 07.76 - total (128)
  3. 2044 Sep 07.47 - partial (138)
  4. 2063 Sep 07.86 - penumbral (148)
File:Metonic lunar eclipses 2006-2063A.png

Saros 123

This eclipse is a part of Saros series 123, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on August 16, 1087. It contains partial eclipses from May 2, 1520 through July 6, 1610; total eclipses from July 16, 1628 through April 4, 2061; and a second set of partial eclipses from April 16, 2079 through July 2, 2205. The series ends at member 72 as a penumbral eclipse on October 8, 2367.

The longest duration of totality was produced by member 37 at 105 minutes, 58 seconds on September 20, 1736. All eclipses in this series occur at the Moon’s descending node of orbit.[8]

Greatest First
The greatest eclipse of the series occurred on 1736 Sep 20, lasting 105 minutes, 58 seconds.[9] Penumbral Partial Total Central
1087 Aug 16
1520 May 02
1628 Jul 16
1682 Aug 18
Last
Central Total Partial Penumbral
1953 Jan 29
File:Lunar eclipse chart close-1953Jan29.png
2061 Apr 04
2205 Jul 02
2367 Oct 08

Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

Tritos series

Template:Lunar Tritos series May 2003

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[10] Related to Solar Saros 130.

March 9, 2016 March 20, 2034
File:SE2016Mar09T.png File:SE2034Mar20T.png

See also

References

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  9. Listing of Eclipses of series 123
  10. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

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Template:Lunar eclipses Template:Portal bar