June 2058 lunar eclipse

A total lunar eclipse will take place on June 6, 2058. The moon will pass through the center of the Earth's shadow.

The moon passes west to east (right to left) across the Earth's umbral shadow, shown in hourly intervals.

Visibility

Lunar year series
Lunar eclipse series sets from 2056-2060
Descending node   Ascending node
111 2056 Jun 27
 penumbral
 116 2056 Dec 22
 penumbral
121 2057 Jun 17
 partial
 126 2057 Dec 11
 partial
131 2058 Jun 06
 total
 136 2058 Nov 30
 total
141 2059 May 27
 partial
 146 2059 Nov 19
 partial
156 2060 Nov 08
 penumbral

Saros series

Lunar Saros series 131, has 72 lunar eclipses. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

This eclipse series began in AD 1427 with a partial eclipse at the southern edge of the Earth's shadow when the Moon was close to its descending node. Each successive Saros cycle, the Moon's orbital path is shifted northward with respect to the Earth's shadow, with the first total eclipse occurring in 1950. For the following 252 years, total eclipses occur, with the central eclipse being predicted to occur in 2078. The first partial eclipse after this is predicted to occur in the year 2220, and the final partial eclipse of the series will occur in 2707. The total lifetime of the lunar Saros series 131 is 1280 years. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Because of the ⅓ fraction of days in a Saros cycle, the visibility of each eclipse will differ for an observer at a given fixed locale. For the lunar Saros series 131, the first total eclipse of 1950 had its best visibility for viewers in Eastern Europe and the Middle East because mid-eclipse was at 20:44 UT. The following eclipse in the series occurred approximately 8 hours later in the day with mid-eclipse at 4:47 UT, and was best seen from North America and South America. The third total eclipse occurred approximately 8 hours later in the day than the second eclipse with mid-eclipse at 12:43 UT, and had its best visibility for viewers in the Western Pacific, East Asia, Australia and New Zealand. This cycle of visibility repeats from the initiation to termination of the series, with minor variations. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

Lunar Saros series 131, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 57 umbral lunar eclipses (42 partial lunar eclipses and 15 total lunar eclipses). Solar Saros 138 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 2094 Jun 28, lasting 102 minutes.[1]		 Penumbral Partial Total Central
1427 May 10 1553 July 25 1950 Apr 2 2022 May 16
Last
Central Total Partial Penumbral
2148 Jul 31 2202 Sep 3 2563 Apr 9 2707 Jul 7
1901–2100
1914 Mar 12 1932 Mar 22 1950 Apr 2
1968 Apr 13 1986 Apr 24 2004 May 4
2022 May 16 2040 May 26 2058 Jun 6
2076 Jun 17 2094 Jun 28

Tritos series

The tritos series repeats 31 days short of 11 years at alternating nodes. Sequential events have incremental Saros cycle indices.

This series produces 20 total eclipses between April 24, 1967 and August 11, 2185, only being partial on November 19, 2021.

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 40.

All events in this series shown (from 1000 to 2500 and beyond) 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

Half-Saros cycle

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 138.

May 31, 2049 June 11, 2067
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See also

Notes
  1. Listing of Eclipses of cycle 131
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros


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