March 2044 lunar eclipse

March 2044 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateMarch 13, 2044
Gamma−0.3496
Magnitude1.2050
Saros cycle133 (28 of 71)
Totality66 minutes, 25 seconds
Partiality209 minutes, 5 seconds
Penumbral338 minutes, 23 seconds
Contacts (UTC)
P116:47:56
U117:52:31
U219:03:51
Greatest19:37:05
U320:10:16
U421:21:35
P422:26:19

A total lunar eclipse will occur at the Moon’s descending node of orbit on Sunday, March 13, 2044,[1] with an umbral magnitude of 1.2050. 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. Occurring about 6.2 days after perigee (on March 7, 2044, at 15:30 UTC), the Moon's apparent diameter will be larger.[2]

This lunar eclipse is the third of a tetrad, with four total lunar eclipses in series, the others being on March 25, 2043; September 19, 2043; and September 7, 2044.

Visibility

The eclipse will be completely visible over east Africa, eastern Europe, and much of Asia, seen rising over west Africa, western Europe, and eastern South America and setting over northeast Asia and Australia.[3]

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

March 13, 2044 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.23223
Umbral Magnitude 1.20503
Gamma −0.34957
Sun Right Ascension 23h37m30.3s
Sun Declination -02°25'56.9"
Sun Semi-Diameter 16'05.4"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 11h36m51.3s
Moon Declination +02°08'22.5"
Moon Semi-Diameter 15'39.8"
Moon Equatorial Horizontal Parallax 0°57'29.1"
ΔT 81.5 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 February–March 2044
February 28
Ascending node (new moon)
 March 13
Descending node (full moon)
Annular solar eclipse
Solar Saros 121		 Total lunar eclipse
Lunar Saros 133

Eclipses in 2044

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 133

Inex

Triad

Lunar eclipses of 2042–2045

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.[5]

The penumbral lunar eclipse on October 28, 2042 occurs in the previous lunar year eclipse set.

Lunar eclipse series sets from 2042 to 2045
Descending node   Ascending node
Saros Date
Viewing 		Type
Chart 		Gamma Saros Date
Viewing 		Type
Chart 		Gamma
113 2042 Apr 05
 Penumbral
 1.1080 118 2042 Sep 29
 Penumbral
 −1.0261
123 2043 Mar 25
 Total
 0.3849 128 2043 Sep 19
 Total
 −0.3316
133 2044 Mar 13
 Total
 −0.3496 138 2044 Sep 07
 Total
 0.4318
143 2045 Mar 03
 Penumbral
 −1.0274 148 2045 Aug 27
 Penumbral
 1.2060

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)

Saros 133

This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 71 events. The series started with a penumbral lunar eclipse on May 13, 1557. It contains partial eclipses from August 7, 1683 through December 17, 1899; total eclipses from December 28, 1917 through August 3, 2278; and a second set of partial eclipses from August 14, 2296 through March 11, 2639. The series ends at member 71 as a penumbral eclipse on June 29, 2819.

The longest duration of totality will be produced by member 35 at 101 minutes, 41 seconds on May 30, 2170. All eclipses in this series occur at the Moon’s descending node of orbit.[6]

Greatest First
The greatest eclipse of the series will occur on 2170 May 30, lasting 101 minutes, 41 seconds.[7] Penumbral Partial Total Central
1557 May 13
 1683 Aug 07
 1917 Dec 28
 2098 Apr 15
Last
Central Total Partial Penumbral
2224 Jul 01
 2278 Aug 03
 2639 Mar 11
 2819 Jun 29

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

The tritos series repeats 31 days short of 11 years at alternating nodes. Sequential events have incremental Saros cycle indices.

This series produces 23 total eclipses between June 22, 1880 and August 9, 2120.

Tritos eclipse series (subset 1901–2100)
Ascending node   Descending node
Saros Date
Viewing 		Type
chart 		Saros Date
Viewing 		Type
chart
120 1902 Apr 22
 Total
 121 1913 Mar 22
 Total
122 1924 Feb 20
 Total
 123 1935 Jan 19
 Total
124 1945 Dec 19
 Total
 125 1956 Nov 18
 Total
126 1967 Oct 18
 Total
 127 1978 Sep 16
 Total
128 1989 Aug 17
 Total
 129 2000 Jul 16
 Total
130 2011 Jun 15
 Total
 131 2022 May 16
 Total
132 2033 Apr 14
 Total
 133 2044 Mar 13
 Total
134 2055 Feb 11
 Total
 135 2066 Jan 11
 Total
136 2076 Dec 10
 Total
 137 2087 Nov 10
 Total
138 2098 Oct 10
 Total

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[8] This lunar eclipse is related to two annular solar eclipses of Solar Saros 140.

March 9, 2035 March 20, 2053

See also

References

  1. ^ "March 13–14, 2044 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 3 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 3 December 2024.
  3. ^ "Total Lunar Eclipse of 2044 Mar 13" (PDF). NASA. Retrieved 3 December 2024.
  4. ^ "Total Lunar Eclipse of 2044 Mar 13". EclipseWise.com. Retrieved 3 December 2024.
  5. ^ 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.
  6. ^ "NASA - Catalog of Lunar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.
  7. ^ Listing of Eclipses of series 133
  8. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros


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