March 2024 lunar eclipse

March 2024 lunar eclipse
Penumbral eclipse
From Richmond, Virginia, 7:18 UTC
DateMarch 25, 2024
Gamma1.0609
Magnitude−0.1304
Saros cycle113 (64 of 71)
Penumbral279 minutes, 9 seconds
Contacts (UTC)
P104:53:11
Greatest07:12:45
P409:32:18

A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Monday, March 25, 2024,[1] with an umbral magnitude of −0.1304. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. 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. Occurring about 2.2 days after apogee (on March 23, 2024, at 11:45 UTC), the Moon's apparent diameter was smaller.[2]

This was the deepest penumbral eclipse overall since May 5, 2023, and the deepest for North and South America since February 11, 2017.[3]

Visibility

The eclipse was completely visible over North and South America, seen rising over eastern Australia and northeast Asia and setting over west Africa and western Europe.[4]

Eclipse details

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

March 25, 2024 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.95767
Umbral Magnitude −0.13044
Gamma 1.06098
Sun Right Ascension 00h18m49.9s
Sun Declination +02°02'16.6"
Sun Semi-Diameter 16'02.2"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 12h20m41.3s
Moon Declination -01°12'05.6"
Moon Semi-Diameter 14'44.3"
Moon Equatorial Horizontal Parallax 0°54'05.4"
ΔT 71.2 s

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.

Eclipse season of March–April 2024
March 25
Descending node (full moon)
 April 8
Ascending node (new moon)
Penumbral lunar eclipse
Lunar Saros 113		 Total solar eclipse
Solar Saros 139

Eclipses in 2024

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 113

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.[6]

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

Lunar eclipse series sets from 2024 to 2027
Descending node   Ascending node
Saros Date
Viewing 		Type
Chart 		Gamma Saros Date
Viewing 		Type
Chart 		Gamma
113
 2024 Mar 25
 Penumbral
 1.0610 118
 2024 Sep 18
 Partial
 −0.9792
123 2025 Mar 14
 Total
 0.3485 128 2025 Sep 07
 Total
 −0.2752
133 2026 Mar 03
 Total
 −0.3765 138 2026 Aug 28
 Partial
 0.4964
143 2027 Feb 20
 Penumbral
 −1.0480 148 2027 Aug 17
 Penumbral
 1.2797

Saros 113

This eclipse is a part of Saros series 113, repeating every 18 years, 11 days, and containing 71 events. The series started with a penumbral lunar eclipse on April 29, 888 AD. It contains partial eclipses from July 14, 1014 through March 10, 1411; total eclipses from March 20, 1429 through August 7, 1645; and a second set of partial eclipses from August 18, 1663 through February 21, 1970. The series ends at member 71 as a penumbral eclipse on June 10, 2150.

The longest duration of totality was produced by member 38 at 103 minutes, 6 seconds on June 5, 1555. All eclipses in this series occur at the Moon’s descending node of orbit.[7]

Greatest First
The greatest eclipse of the series occurred on 1555 Jun 05, lasting 103 minutes, 6 seconds.[8] Penumbral Partial Total Central
888 Apr 29
 1014 Jul 14
 1429 Mar 20
 1483 Apr 22
Last
Central Total Partial Penumbral
1609 Jul 16
 1645 Aug 07
 1970 Feb 21
 2150 Jun 10

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.

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[9] This lunar eclipse is related to two total solar eclipses of Solar Saros 120.

March 20, 2015 March 30, 2033

See also

References

  1. ^ "March 24–25, 2024 Penumbral Lunar Eclipse". timeanddate. Retrieved 18 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 18 November 2024.
  3. ^ Hermit Eclipse: Saros cycle 113
  4. ^ "Penumbral Lunar Eclipse of 2024 Mar 25" (PDF). NASA. Retrieved 18 November 2024.
  5. ^ "Penumbral Lunar Eclipse of 2024 Mar 25". EclipseWise.com. Retrieved 18 November 2024.
  6. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  7. ^ "NASA - Catalog of Lunar Eclipses of Saros 113". eclipse.gsfc.nasa.gov.
  8. ^ Listing of Eclipses of series 113
  9. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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