February 2035 lunar eclipse

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February 2035 lunar eclipse
Penumbral eclipse
File:Lunar eclipse chart close-2035Feb22.png
The Moon's hourly motion shown right to left
DateFebruary 22, 2035
Gamma−1.0357
Magnitude−0.0523
Saros cycle114 (60 of 71)
Penumbral255 minutes, 42 seconds
Contacts (UTC)
P16:58:21
Greatest9:06:12
P411:14:03

A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Thursday, February 22, 2035,[1] with an umbral magnitude of −0.0523. 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 4.3 days after perigee (on February 18, 2035, at 0:40 UTC), the Moon's apparent diameter will be larger.[2]

Visibility

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The eclipse will be completely visible over northeast Asia and North America, seen rising over east Asia and Australia and setting over South America.[3]

File:Lunar eclipse from moon-2035Feb22.png File:Lunar eclipse chart close-2035Feb22.png

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]

February 22, 2035 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.96629
Umbral Magnitude −0.05232
Gamma −1.03672
Sun Right Ascension 22h21m54.2s
Sun Declination -10°11'53.9"
Sun Semi-Diameter 16'10.2"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 10h20m48.3s
Moon Declination +09°13'43.5"
Moon Semi-Diameter 15'52.5"
Moon Equatorial Horizontal Parallax 0°58'15.8"
ΔT 76.5 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 February–March 2035
February 22
Ascending node (full moon)
March 9
Descending node (new moon)
File:Lunar eclipse chart close-2035Feb22.png File:SE2035Mar09A.png
Penumbral lunar eclipse
Lunar Saros 114
Annular solar eclipse
Solar Saros 140
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Eclipses in 2035

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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 114

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Triad

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Lunar eclipses of 2035–2038

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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 17, 2038 and December 11, 2038 occur in the next lunar year eclipse set.

Lunar eclipse series sets from 2035 to 2038
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
114 2035 Feb 22
File:Lunar eclipse from moon-2035Feb22.png
Penumbral
File:Lunar eclipse chart close-2035Feb22.png
−1.0357 119 2035 Aug 19
File:Lunar eclipse from moon-2035Aug19.png
Partial
File:Lunar eclipse chart close-2035Aug19.png
0.9433
124 2036 Feb 11
File:Lunar eclipse from moon-2036Feb11.png
Total
File:Lunar eclipse chart close-2036Feb11.png
−0.3110 129 2036 Aug 07
File:Lunar eclipse from moon-2036Aug07.png
Total
File:Lunar eclipse chart close-2036Aug07.png
0.2004
134 2037 Jan 31
File:Lunar eclipse from moon-2037Jan31.png
Total
File:Lunar eclipse chart close-2037Jan31.png
0.3619 139 2037 Jul 27
File:Lunar eclipse from moon-2037Jul27.png
Partial
File:Lunar eclipse chart close-2037Jul27.png
−0.5582
144 2038 Jan 21
File:Lunar eclipse from moon-2038Jan21.png
Penumbral
File:Lunar eclipse chart close-2038Jan21.png
1.0710 149 2038 Jul 16
File:Lunar eclipse from moon-2038Jul16.png
Penumbral
File:Lunar eclipse chart close-2038Jul16.png
−1.2837

Saros 114

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This eclipse is a part of Saros series 114, repeating every 18 years, 11 days, and containing 71 events. The series started with a penumbral lunar eclipse on May 13, 971 AD. It contains partial eclipses from August 7, 1115 through February 18, 1440; total eclipses from February 28, 1458 through July 17, 1674; and a second set of partial eclipses from July 28, 1692 through November 26, 1890. The series ends at member 71 as a penumbral eclipse on June 22, 2233.

The longest duration of totality was produced by member 35 at 106 minutes, 5 seconds on May 24, 1584. All eclipses in this series occur at the Moon’s ascending node of orbit.[6]

Greatest First
The greatest eclipse of the series occurred on 1584 May 24, lasting 106 minutes, 5 seconds.[7] Penumbral Partial Total Central
971 May 13
1115 Aug 07
1458 Feb 28
1530 Apr 12
Last
Central Total Partial Penumbral
1638 Jun 26
1674 Jul 17
1890 Nov 26
2233 Jun 22

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

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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)
File:Lunar eclipse chart close-1904Mar02.png File:Lunar eclipse from moon-1904Mar02.png File:Lunar eclipse chart close-1915Jan31.png File:Lunar eclipse from moon-1915Jan31.png
1969 Aug 27
(Saros 108)
1980 Jul 27
(Saros 109)
1991 Jun 27
(Saros 110)
2002 May 26
(Saros 111)
File:Lunar eclipse chart close-1969Aug27.png File:Lunar eclipse from moon-1969Aug27.png File:Lunar eclipse chart close-1980Jul27.png File:Lunar eclipse from moon-1980Jul27.png File:Lunar eclipse chart close-1991Jun27.png File:Lunar eclipse from moon-1991Jun27.png File:Lunar eclipse chart close-2002May26.png File:Lunar eclipse from moon-2002May26.png
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)
File:Lunar eclipse chart close-2013Apr25.png File:Lunar eclipse from moon-2013Apr25.png File:Lunar eclipse chart close-2024Mar25.png File:Lunar eclipse from moon-2024Mar25.png File:Lunar eclipse chart close-2035Feb22.png File:Lunar eclipse from moon-2035Feb22.png File:Lunar eclipse chart close-2046Jan22.png File:Lunar eclipse from moon-2046Jan22.png File:Lunar eclipse chart close-2056Dec22.png File:Lunar eclipse from moon-2056Dec22.png
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)
File:Lunar eclipse chart close-2067Nov21.png File:Lunar eclipse from moon-2067Nov21.png
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)

Inex series

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This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
1803 Aug 03
(Saros 106)
1832 Jul 12
(Saros 107)
1861 Jun 22
(Saros 108)
1890 Jun 03
(Saros 109)
1919 May 15
(Saros 110)
1948 Apr 23
(Saros 111)
File:Lunar eclipse chart close-1919May15.png File:Lunar eclipse from moon-1919May15.png File:Lunar eclipse chart close-1948Apr23.png File:Lunar eclipse from moon-1948Apr23.png
1977 Apr 04
(Saros 112)
2006 Mar 14
(Saros 113)
2035 Feb 22
(Saros 114)
File:Lunar eclipse chart close-1977Apr04.png File:Lunar eclipse from moon-1977Apr04.png File:Lunar eclipse chart close-06mar14.png File:Lunar eclipse from moon-2006Mar14.png File:Lunar eclipse chart close-2035Feb22.png File:Lunar eclipse from moon-2035Feb22.png
2064 Feb 02
(Saros 115)
2093 Jan 12
(Saros 116)
2121 Dec 24
(Saros 117)
2150 Dec 04
(Saros 118)
2179 Nov 14
(Saros 119)

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).[8] This lunar eclipse is related to two total solar eclipses of Solar Saros 121.

February 17, 2026 February 28, 2044
File:SE2026Feb17A.png File:SE2044Feb28A.png

See also

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Notes

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  1. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  2. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  3. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  4. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  5. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  6. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  7. ^ Listing of Eclipses of series 114
  8. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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