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January 2046 lunar eclipse

January 2046 lunar eclipse
Partial eclipse
The Moon's hourly motion shown right to left
DateJanuary 22, 2046
Gamma0.9885
Magnitude0.0550
Saros cycle115 (59 of 72)
Partiality50 minutes, 23 seconds
Penumbral250 minutes, 1 second
Contacts (UTC)
P110:56:07
U112:35:59
Greatest13:01:07
U413:26:22
P415:06:08

A partial lunar eclipse will occur at the Moon’s descending node of orbit on Monday, January 22, 2046,[1] with an umbral magnitude of 0.0550. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in 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 1.1 days before perigee (on January 23, 2046, at 14:00 UTC), the Moon's apparent diameter will be larger.[2]

Visibility

The eclipse will be completely visible over Australia, east and north Asia, and northwestern North America, seen rising over eastern Europe and west, central, and south Asia and setting over much of North America.[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, 2046 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.03650
Umbral Magnitude 0.05499
Gamma 0.98859
Sun Right Ascension 20h19m45.5s
Sun Declination -19°33'42.8"
Sun Semi-Diameter 16'15.1"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 08h21m07.9s
Moon Declination +20°30'34.8"
Moon Semi-Diameter 16'33.4"
Moon Equatorial Horizontal Parallax 1°00'46.0"
ΔT 82.6 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–February 2046
January 22
Descending node (full moon)
February 5
Ascending node (new moon)
Partial lunar eclipse
Lunar Saros 115
Annular solar eclipse
Solar Saros 141

Eclipses in 2046

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 115

Inex

Triad

Lunar eclipses of 2046–2049

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 May 17, 2049 and November 9, 2049 occur in the next lunar year eclipse set.

Lunar eclipse series sets from 2046 to 2049
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
115 2046 Jan 22
Partial
0.9885 120 2046 Jul 18
Partial
−0.8691
125 2047 Jan 12
Total
0.3317 130 2047 Jul 07
Total
−0.0636
135 2048 Jan 01
Total
−0.3745 140 2048 Jun 26
Partial
0.6796
145 2048 Dec 20
Penumbral
−1.0624 150 2049 Jun 15
Penumbral
1.4068

Saros 115

This eclipse is a part of Saros series 115, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on April 21, 1000. It contains partial eclipses from July 6, 1126 through September 30, 1270; total eclipses from October 11, 1288 through July 20, 1739; and a second set of partial eclipses from July 30, 1757 through February 13, 2082. The series ends at member 72 as a penumbral eclipse on June 13, 2280.

The longest duration of totality was produced by member 36 at 99 minutes, 47 seconds on May 15, 1631. All eclipses in this series occur at the Moon’s descending node of orbit.[6]

Greatest First
The greatest eclipse of the series occurred on 1631 May 15, lasting 99 minutes, 47 seconds.[7] Penumbral Partial Total Central
1000 Apr 21
1126 Jul 06
1288 Oct 11
1541 Mar 12
Last
Central Total Partial Penumbral
1685 Jun 16
1739 Jul 20
2082 Feb 13
2280 Jun 13

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

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1904 and 2200
1904 Mar 02
(Saros 102)
1915 Jan 31
(Saros 103)
1969 Aug 27
(Saros 108)
1980 Jul 27
(Saros 109)
1991 Jun 27
(Saros 110)
2002 May 26
(Saros 111)
2013 Apr 25
(Saros 112)
2024 Mar 25
(Saros 113)
2035 Feb 22
(Saros 114)
2046 Jan 22
(Saros 115)
2056 Dec 22
(Saros 116)
2067 Nov 21
(Saros 117)
2078 Oct 21
(Saros 118)
2089 Sep 19
(Saros 119)
2100 Aug 19
(Saros 120)
2111 Jul 21
(Saros 121)
2122 Jun 20
(Saros 122)
2133 May 19
(Saros 123)
2144 Apr 18
(Saros 124)
2155 Mar 19
(Saros 125)
2166 Feb 15
(Saros 126)
2177 Jan 14
(Saros 127)
2187 Dec 15
(Saros 128)
2198 Nov 13
(Saros 129)

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 partial solar eclipses of Solar Saros 122.

January 16, 2037 January 27, 2055

See also

Notes

  1. ^ "January 22–23, 2046 Partial Lunar Eclipse". timeanddate. Retrieved 6 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 6 December 2024.
  3. ^ "Partial Lunar Eclipse of 2046 Jan 22" (PDF). NASA. Retrieved 6 December 2024.
  4. ^ "Partial Lunar Eclipse of 2046 Jan 22". EclipseWise.com. Retrieved 6 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 115". eclipse.gsfc.nasa.gov.
  7. ^ Listing of Eclipses of series 115
  8. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros