June 2029 lunar eclipse

Total lunar eclipse
June 26, 2029
Ecliptic north up

The moon will pass through the center of the Earth's shadow.
Saros (and member) 130 (35 of 72)
Gamma +0.01240
Magnitude +1.84362
Duration (hr:mn:sc)
Totality 1:41:53
Partial 3:39:32
Penumbral 5:35:08
Contacts (UTC)
P1 0:34:34
U1 1:32:18
U2 2:31:18
Greatest 3:22:05
U3 4:13:01
U4 5:11:50
P4 6:09:42

A total lunar eclipse will take place between Monday and Tuesday, June 25-26, 2029. A central total eclipse lasting 1 hour and 41 minutes 53 seconds will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red color at maximum eclipse. It will be able to be seen from most of the Americas, Western Europe and Africa. The partial eclipse will last for 3 hours and 39 minutes 32 seconds in total.

The moon will pass through the center of the Earth's shadow. Totality will last 101 minutes 53 seconds, the maximum duration for Saros series 130.

With an umbral eclipse magnitude of 1.84362, this is the largest lunar eclipse of the 21st century. Gamma has a value of only 0.01240. Due to the Moon's relatively large size as seen from Earth and greater speed in its elliptical orbit, totality will not last over 106 minutes. This is the darkest and greatest total lunar eclipse in the 21st century.

Visibility

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It will be completely visible over South America, seen rising over North America, and setting over Africa and Europe.

 

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Lunar year series

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Lunar eclipse series sets from 2027–2031
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
110 2027 Jul 18
 
Penumbral
 
-1.57589 115 2028 Jan 12
 
Partial
 
0.98177
120 2028 Jul 06
 
Partial
 
-0.79040 125 2028 Dec 31
 
Total
 
0.32583
130 2029 Jun 26
 
Total
 
0.01240 135 2029 Dec 20
 
Total
 
-0.38110
140 2030 Jun 15
 
Partial
 
0.75346 145 2030 Dec 09
 
Penumbral
 
-1.07315
150 2031 Jun 05
 
Penumbral
 
1.47322
Last set 2027 Aug 17 Last set 2027 Feb 20
Next set 2031 May 07 Next set 2031 Oct 30

Metonic series

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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.

Ascending node Descending node
  1. 1991 Jun 27 - penumbral (110)
  2. 2010 Jun 26 - partial (120)
  3. 2029 Jun 26 - total (130)
  4. 2048 Jun 26 - partial (140)
  5. 2067 Jun 27 - penumbral (150)
  1. 1991 Dec 21 - partial (115)
  2. 2010 Dec 21 - total (125)
  3. 2029 Dec 20 - total (135)
  4. 2048 Dec 20 - partial (145)
   

Saros series

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Lunar saros series 130, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 56 umbral lunar eclipses (42 partial lunar eclipses and 14 total lunar eclipses). Solar Saros 137 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Greatest First
 
The greatest eclipse of the series will occur on 2029 Jun 26, lasting 102 minutes.[1]
Penumbral Partial Total Central
1416 Jun 10 1560 Sep 4 1921 Apr 22
 
1957 May 13
 
Last
Central Total Partial Penumbral
2083 Jul 29
 
2155 Sep 11 2552 May 10 2678 Jul 26
1901–2200
1903 Apr 12 1921 Apr 22 1939 May 3
           
1957 May 13 1975 May 25 1993 Jun 4
           
2011 Jun 15 2029 Jun 26 2047 Jul 7
           
2065 Jul 17 2083 Jul 29
       

Inex series

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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 40.

All events in this series shown (from 1000 to 2500) are central total lunar eclipses.

Inex series from 1000–2500 AD
Descending node Ascending node Descending node Ascending node
Saros Date Saros Date Saros Date Saros Date
95 1016 May 24 96 1045 May 3 97 1074 Apr 14 98 1103 Mar 25
99 1132 Mar 3 100 1161 Feb 12 101 1190 Jan 23 102 1219 Jan 2
103 1247 Dec 13 104 1276 Nov 23 105 1305 Nov 2 106 1334 Oct 13
107 1363 Sep 23 108 1392 Sep 2 109 1421 Aug 13 110 1450 Jul 24
111 1479 Jul 4 112 1508 Jun 13
 
113 1537 May 24 114 1566 May 4
115 1595 Apr 24 116 1624 Apr 3 117 1653 Mar 14 118 1682 Feb 21
119 1711 Feb 3 120 1740 Jan 13 121 1768 Dec 23 122 1797 Dec 4
123 1826 Nov 14 124 1855 Oct 25 125 1884 Oct 4 126 1913 Sep 15
 
127 1942 Aug 26
 
128 1971 Aug 6
 
129 2000 Jul 16
 
130 2029 Jun 26
 
131 2058 Jun 6
 
132 2087 May 17
 
133 2116 Apr 27 134 2145 Apr 7
135 2174 Mar 18 136 2203 Feb 26 137 2232 Feb 7 138 2261 Jan 17
139 2289 Dec 27 140 2318 Dec 9 141 2347 Nov 19 142 2376 Oct 28
143 2405 Oct 8 144 2434 Sep 18 145 2463 Aug 29 146 2492 Aug 8
 

Tritos

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Tzolkinex

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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).[2] This lunar eclipse is related to two annular solar eclipses of Solar Saros 137.

June 21, 2020 July 2, 2038
   

See also

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Notes

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  1. ^ Listing of Eclipses of cycle 130
  2. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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