March 2026 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 Tuesday, March 3, 2026,[1] with an umbral magnitude of 1.1526. 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. The Moon's apparent diameter will be near the average diameter because it will occur 6.7 days after perigee (on February 24, 2026, at 18:15 UTC) and 6.9 days before apogee (on March 10, 2026, at 9:45 UTC).[2]

This lunar eclipse will be the third of an almost tetrad, with the others being on March 14, 2025 (total); September 8, 2025 (total); and August 28, 2026 (partial).

During the eclipse, the Moon will occult NGC 3423 over North America.[3]Template:Rp

Visibility

The eclipse will be completely visible over northeast Asia, northwestern North America, and the central Pacific Ocean, seen rising over much of Asia and Australia and setting over North and South America.[4]

File:Lunar eclipse from moon-2026Mar03.png File:Lunar eclipse chart close-2026Mar03.png

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.[5]

March 3, 2026 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.18580
Umbral Magnitude 1.15263
Gamma −0.37651
Sun Right Ascension 22h56m56.0s
Sun Declination -06°43'06.4"
Sun Semi-Diameter 16'08.0"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 10h56m15.0s
Moon Declination +06°24'05.3"
Moon Semi-Diameter 15'37.0"
Moon Equatorial Horizontal Parallax 0°57'18.7"
ΔT 72.1 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 February–March 2026
February 17
Ascending node (new moon)
March 3
Descending node (full moon)
File:SE2026Feb17A.png File:Lunar eclipse chart close-2026Mar03.png
Annular solar eclipse
Solar Saros 121
Total lunar eclipse
Lunar Saros 133

Related eclipses

Eclipses in 2026

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 133

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 be in nearly the same location relative to the background stars.

  1. 1988 Mar 03.675 – Partial (113)
  2. 2007 Mar 03.972 – Total (123)
  3. 2026 Mar 03.481 – Total (133)
  4. 2045 Mar 03.320 – Penumbral (143)
  1. 1988 Aug 27.461 – partial (118)
  2. 2007 Aug 28.442 – total (128)
  3. 2026 Aug 28.175 – partial (138)
  4. 2045 Aug 27.578 – penumbral (148)
File:Metonic lunar eclipse 1988-2045.png File:Metonic lunar eclipses 1988-2045.png

Saros 133

Template:Lunar Saros series 133

Tritos series

Template:Lunar Tritos series May 2004

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
1823 Jul 23
(Saros 126)
1852 Jul 01
(Saros 127)
1881 Jun 12
(Saros 128)
1910 May 24
(Saros 129)
1939 May 03
(Saros 130)
1968 Apr 13
(Saros 131)
File:Lunar eclipse chart close-1910May24.png File:Lunar eclipse from moon-1910May24.png File:Lunar eclipse chart close-1939May03.png File:Lunar eclipse from moon-1939May03.png File:Lunar eclipse chart close-1968Apr13.png File:Lunar eclipse from moon-1968Apr13.png
1997 Mar 24
(Saros 132)
2026 Mar 03
(Saros 133)
2055 Feb 11
(Saros 134)
File:Lunar eclipse chart close-1997Mar24.png File:Lunar eclipse from moon-1997Mar24.png File:Lunar eclipse chart close-2026Mar03.png File:Lunar eclipse from moon-2026Mar03.png File:Lunar eclipse chart close-2055Feb11.png File:Lunar eclipse from moon-2055Feb11.png
2084 Jan 22
(Saros 135)
2113 Jan 02
(Saros 136)
2141 Dec 13
(Saros 137)
File:Lunar eclipse chart close-2084Jan22.png File:Lunar eclipse from moon-2084Jan22.png
2170 Nov 23
(Saros 138)
2199 Nov 02
(Saros 139)

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two annular solar eclipses of Solar Saros 140.

February 26, 2017 March 9, 2035
File:SE2017Feb26A.png File:SE2035Mar09A.png

See also

References

  1. ↑ Script error: No such module "citation/CS1".
  2. ↑ Script error: No such module "citation/CS1".
  3. ↑ Script error: No such module "citation/CS1".
  4. ↑ Script error: No such module "citation/CS1".
  5. ↑ Script error: No such module "citation/CS1".
  6. ↑ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

External links

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