March 2045 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Friday, March 3, 2045,[1] with an umbral magnitude of −0.0148. 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 1.8 days after perigee (on March 1, 2045, at 13:40 UTC), the Moon's apparent diameter will be larger.[2]

Visibility

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

File:Lunar eclipse from moon-2045Mar03.png File:Lunar eclipse chart close-2045Mar03.png

Eclipse details

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

March 3, 2045 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.96431
Umbral Magnitude −0.01482
Gamma −1.02738
Sun Right Ascension 22h57m49.1s
Sun Declination -06°37'35.6"
Sun Semi-Diameter 16'08.1"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 10h55m51.5s
Moon Declination +05°42'46.0"
Moon Semi-Diameter 16'28.7"
Moon Equatorial Horizontal Parallax 1°00'28.6"
ΔT 82.1 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 2045
February 16
Ascending node (new moon)
March 3
Descending node (full moon)
File:SE2045Feb16A.png File:Lunar eclipse chart close-2045Mar03.png
Annular solar eclipse
Solar Saros 131
Penumbral lunar eclipse
Lunar Saros 143

Related eclipses

Eclipses in 2045

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 143

Inex

Triad

Lunar eclipses of 2042–2045

Template:Lunar eclipse set 2042-2045

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 143

Template:Lunar Saros series 143

Tritos series

Template:Lunar Tritos series July 2001

Inex series

Template:Lunar Inex series March 2016

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two partial solar eclipses of Solar Saros 150.

February 27, 2036 March 9, 2054
File:SE2036Feb27P.png File:SE2054Mar09P.png

See also

Notes

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  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. ↑ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

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