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March 2025 lunar eclipse

Total lunar eclipse of 14 March 2025 From Wikipedia, the free encyclopedia

March 2025 lunar eclipse
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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]

Quick Facts Date, Gamma ...

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]

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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]

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Simulated view of earth from moon
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From moon, with IR clouds[6]
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Eclipse details

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

More information Parameter, Value ...

Eclipse season

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.

More information March 14Descending node (full moon), March 29Ascending node (new moon) ...
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Summarize
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Eclipses in 2025

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 123

Inex

Triad

Lunar eclipses of 2024–2027

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[8]

The penumbral lunar eclipse on July 18, 2027 occurs in the next lunar year eclipse set.

More information Lunar eclipse series sets from 2024 to 2027, Descending node ...

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)
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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.[9]

More information Greatest, First ...

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.

More information Series members 41–62 occur between 1801 and 2200: ...

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

More information Series members between 1801 and 2200 ...

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[11] Related to Solar Saros 130.

March 9, 2016 March 20, 2034
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See also

References

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