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January 2048 lunar eclipse

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January 2048 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateJanuary 1, 2048
Gamma−0.3745
Magnitude1.1297
Saros cycle135 (25 of 71)
Totality55 minutes, 56 seconds
Partiality214 minutes, 16 seconds
Penumbral359 minutes, 26 seconds
Contacts (UTC)
P13:52:39
U15:05:17
U26:24:27
Greatest6:52:24
U37:20:23
U48:39:33
P49:52:05

A total lunar eclipse will occur at the Moon’s descending node of orbit on Wednesday, January 1, 2048,[1] with an umbral magnitude of 1.1297. 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 4.4 days after apogee (on December 27, 2047, at 21:50 UTC), the Moon's apparent diameter will be smaller.[2]

This will be the first recorded lunar eclipse to be visible on New Year's Day for nearly all of Earth's timezones. The next such eclipse will occur in 2094.

Visibility

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

Eclipse details

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

January 1, 2048 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.21576
Umbral Magnitude 1.12966
Gamma −0.37456
Sun Right Ascension 18h45m45.0s
Sun Declination -23°01'00.1"
Sun Semi-Diameter 16'15.9"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 06h45m29.1s
Moon Declination +22°40'44.8"
Moon Semi-Diameter 14'58.6"
Moon Equatorial Horizontal Parallax 0°54'57.7"
ΔT 83.8 s

Eclipse season

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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 December 2047–January 2048
December 16
Ascending node (new moon)
January 1
Descending node (full moon)
Partial solar eclipse
Solar Saros 123
Total lunar eclipse
Lunar Saros 135
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Eclipses in 2048

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 135

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Inex

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Triad

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Lunar eclipses of 2046–2049

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Lunar eclipse series sets from 2046-2049
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
115 2046 Jan 22
Partial
120 2046 Jul 18
Partial
125 2047 Jan 12
Total
130 2047 Jul 07
Total
135 2048 Jan 01
Total
140 2048 Jun 26
Partial
145 2048 Dec 20
Penumbral
150 2049 Jun 15
Penumbral
Last set 2045 Aug 27 Last set 2045 Mar 03
Next set 2049 Nov 09 Next set 2049 May 17

Half-Saros cycle

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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 total solar eclipses of Solar Saros 142.

December 26, 2038 January 5, 2057

See also

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References

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  1. ^ "December 31, 2047–January 1, 2048 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 11 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 11 December 2024.
  3. ^ "Total Lunar Eclipse of 2048 Jan 01" (PDF). NASA. Retrieved 11 December 2024.
  4. ^ "Total Lunar Eclipse of 2048 Jan 01". EclipseWise.com. Retrieved 11 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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