January 2084 lunar eclipse

January 2084 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateJanuary 22, 2084
Gamma−0.3610
Magnitude1.1531
Saros cycle135 (27 of 71)
Totality60 minutes, 32 seconds
Partiality216 minutes, 16 seconds
Penumbral362 minutes, 0 seconds
Contacts (UTC)
P120:09:13
U121:22:08
U222:39:59
Greatest23:10:14
U323:40:31
U40:58:23
P42:11:13
July 2084 →

A total lunar eclipse will occur at the Moon’s descending node of orbit on Saturday, January 22, 2084,[1] with an umbral magnitude of 1.1531. 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 days after apogee (on January 18, 2084, at 23:50 UTC), the Moon's apparent diameter will be smaller.[2]

This lunar eclipse will be the third of an almost tetrad, with the others being on February 2, 2083 (total); July 29, 2083 (total); and July 17, 2084 (partial).

Visibility

The eclipse will be completely visible over Africa, Europe, and west and central Asia, seen rising over North and South America and setting over south and east Asia and western 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]

January 22, 2084 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.24251
Umbral Magnitude 1.15312
Gamma −0.36098
Sun Right Ascension 20h20m36.4s
Sun Declination -19°30'37.0"
Sun Semi-Diameter 16'15.1"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 08h20m09.1s
Moon Declination +19°11'55.7"
Moon Semi-Diameter 14'55.1"
Moon Equatorial Horizontal Parallax 0°54'45.0"
ΔT 111.5 s

Eclipse season

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 January 2084
January 7
Ascending node (new moon)
January 22
Descending node (full moon)
Partial solar eclipse
Solar Saros 123
Total lunar eclipse
Lunar Saros 135

Eclipses in 2084

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 135

Inex

Triad

Lunar eclipses of 2082–2085

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 eclipses on June 8, 2085 and December 1, 2085 occur in the next lunar year eclipse set.

Lunar eclipse series sets from 2082 to 2085
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
115 2082 Feb 13
Partial
1.0101 120 2082 Aug 08
Penumbral
−1.0203
125 2083 Feb 02
Total
0.3463 130 2083 Jul 29
Total
−0.2143
135 2084 Jan 22
Total
−0.3610 140 2084 Jul 17
Partial
0.5312
145 2085 Jan 10
Penumbral
−1.0453 150 2085 Jul 07
Penumbral
1.2694

Inex series

The inex series repeats eclipses 20 days short of 29 years, repeating on average every 10571.95 days. This period is equal to 358 lunations (synodic months) and 388.5 draconic months. Saros series increment by one on successive Inex events and repeat at alternate ascending and descending lunar nodes.

This period is 383.6734 anomalistic months (the period of the Moon's elliptical orbital precession). Despite the average 0.05 time-of-day shift between subsequent events, the variation of the Moon in its elliptical orbit at each event causes the actual eclipse time to vary significantly. It is a part of Lunar Inex series 35.

Series events from 1500–2500
Descending node Ascending node Descending node Ascending node
Saros Date
Chart
Saros Date
Chart
Saros Date
Chart
Saros Date
Chart
115 1505 Feb 18
116 1534 Jan 30
117 1563 Jan 9 118 1591 Dec 30
119 1620 Dec 9 120 1649 Nov 19 121 1678 Oct 29 122 1707 Oct 11
123 1736 Sep 20 124 1765 Aug 30 125 1794 Aug 11 126 1823 Jul 23
127 1852 Jul 1 128 1881 Jun 12 129 1910 May 24
130 1939 May 3
131 1968 Apr 13
132 1997 Mar 24
133 2026 Mar 3
134 2055 Feb 11
135 2084 Jan 22
136 2113 Jan 2 137 2141 Dec 13 138 2170 Nov 23
139 2199 Nov 2 140 2228 Oct 14 141 2257 Sep 24 142 2286 Sep 3
143 2315 Aug 16 144 2344 Jul 26 145 2373 Jul 5 146 2402 Jun 16
147 2431 May 27 148 2460 May 5
149 2489 Apr 16

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two total solar eclipses of Solar Saros 142.

January 16, 2075 January 27, 2093

See also

Notes

  1. ^ "January 22–23, 2084 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 14 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 December 2024.
  3. ^ "Total Lunar Eclipse of 2084 Jan 22" (PDF). NASA. Retrieved 14 December 2024.
  4. ^ "Total Lunar Eclipse of 2084 Jan 22". EclipseWise.com. Retrieved 14 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. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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