March 2026 lunar eclipse

{{Short description|Total lunar eclipse of 2 March 2026}}

{{Infobox lunar eclipse

| type = total

| image = Lunar eclipse chart close-2026Mar03.png

| caption = The Moon's hourly motion shown right to left

| date = March 3, 2026

| gamma = −0.3765

| magnitude = 1.1526

| saros_ser = 133

| saros_no = 27 of 71

| totality = 58 minutes, 19 seconds

| partiality = 207 minutes, 10 seconds

| penumbral = 338 minutes, 37 seconds

| p1 = 8:44:22

| u1 = 9:50:00

| u2 = 11:04:26

| greatest = 11:33:37

| u3 = 12:02:45

| u4 = 13:17:10

| p4 = 14:22:59

| previous = September 2025

| next = August 2026

}}

A total lunar eclipse will occur at the Moon’s descending node of orbit on Tuesday, March 3, 2026,{{cite web|title=March 2–3, 2026 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/2026-march-3|publisher=timeanddate|access-date=19 November 2024}} 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).{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2026&n=136|publisher=timeanddate|access-date=19 November 2024}}

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.{{cite book |date=2002 |first=Jan |last=Meeus |chapter=Occultations of deep-sky objects during a total lunar eclipse |pages=157-162 |title=More Mathematical Astronomy Morsels |isbn=0943396743 |url=https://falakmu.id/khgt/dokumen/More%20mathematical%20astronomy%20morsels%20(Jean%20Meeus)%20(Z-Library).pdf}}{{rp|161}}

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.{{cite web|title=Total Lunar Eclipse of 2026 Mar 03|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2026Mar03T.pdf|publisher=NASA|access-date=19 November 2024}}

class=wikitable

|300px 300px

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.{{cite web|title=Total Lunar Eclipse of 2026 Mar 03|url=https://eclipsewise.com/lunar/LEprime/2001-2100/LE2026Mar03Tprime.html|publisher=EclipseWise.com|access-date=19 November 2024}}

class="wikitable" align="{{{align|left}}}" style="margin:{{#ifeq:{{{align}}}|right|0 0 0.5em 1em|0 1em 0.5em 0}}"

|+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

{{clear}}

Eclipse season

{{See also|Eclipse cycle}}

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.

class="wikitable"

|+ Eclipse season of February–March 2026

! February 17
Ascending node (new moon)
!! March 3
Descending node (full moon)

200px200px
align=center

| 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 =

{{Lunar eclipse set 2024-2027}}

= Metonic series =

{{Metonic lunar eclipse 1988-2045}}

= Saros 133 =

{{Lunar Saros series 133}}

= Tritos series =

{{Lunar Tritos series May 2004}}

= Inex series =

{{Lunar Inex series March 2026}}

= Half-Saros cycle =

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros This lunar eclipse is related to two annular solar eclipses of Solar Saros 140.

class=wikitable

!February 26, 2017

!March 9, 2035

240px

|240px

See also

References