This catalog has a page for every lunar eclipse from 2000 BC to 3000 AD, 12,064 in all, shown in groups of 20 years at a time. You can go to any eclipse by selecting the milennium, century and 20-year period from the navigation tabs above; then click on an eclipse's date in the list below to to go its page.

You can see the solar eclipses or the combined eclipse catalog by clicking "Solar Eclipses" or "All Eclipses" in the top-right tabs.

Lunar Eclipses, 2041–2060 AD

The following chart shows the position where the Moon is directly overhead at the maximum times of the total (in blue) and partial (in red) lunar eclipses (penumbral eclipses are omitted). Each eclipse will be visible approximately from the half of the Earth centred on that point. Use the zoom controls on the left to zoom in and out; hover over a marker to see the area of visibility and summary information on that eclipse.

The interactive map is currently not available.

Note that eclipse dates are specified relative to UT. You have not selected a timezone for eclipse timings, so all times are shown in UT (essentially GMT).
16 May, 2041 AD
max: 00:41 UT
Partial Lunar Eclipse
(umbral mag. 0.06; Saros 141)
A tiny bite out of the Moon may be visible at maximum, though just 6% of the Moon will be shadowed in a partial eclipse lasting for 58 minutes and 30 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
8 Nov, 2041 AD
max: 04:33 UT
Partial Lunar Eclipse
(umbral mag. 0.17; Saros 146)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 30 minutes, with just 17% of the Moon in shadow at maximum. 		   
5 Apr, 2042 AD
max: 14:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 113)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 87% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 4 hours and 28 minutes. 		   
29 Sep, 2042 AD
max: 10:44 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 118)
The Moon will approach within 0% of the Earth's umbral shadow at maximum eclipse; 95% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 3 hours and 59 minutes. While less dramatic than a partial eclipse (as no part of the Moon will be in complete shadow), a shading across the Moon should be readily visible to observers. 		   
25 Mar, 2043 AD
max: 14:30 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 123)
A shallow total eclipse will see the Moon in relative darkness for 53 minutes and 24 seconds. The Moon will be 11% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 35 minutes in total. 		   
19 Sep, 2043 AD
max: 01:50 UT
Total Lunar Eclipse
(umbral mag. 1.26; Saros 128)
The Moon will be plunged into darkness for 1 hour and 12 minutes, in a deep total eclipse which will see the Moon 26% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 26 minutes in total. 		   
13 Mar, 2044 AD
max: 19:37 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 133)
The Moon will be plunged into darkness for 1 hour and 6 minutes, in a deep total eclipse which will see the Moon 20% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 29 minutes in total. 		   
7 Sep, 2044 AD
max: 11:19 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 138)
The Moon will barely edge into total eclipse for 33 minutes and 54 seconds. With the Moon just 5% of its diameter into the Earth's umbral shadow, the Moon may be quite bright, but even so, this should be worth seeing. The partial eclipse will last for 3 hours and 26 minutes in total. 		   
3 Mar, 2045 AD
max: 07:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 143)
The Moon will approach within 2% of the Earth's umbral shadow at maximum eclipse; 96% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 4 hours and 4 minutes. While less dramatic than a partial eclipse (as no part of the Moon will be in complete shadow), a shading across the Moon should be readily visible to observers. 		   
27 Aug, 2045 AD
max: 13:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 148)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 68% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 4 hours and 2 minutes. 		   
22 Jan, 2046 AD
max: 13:01 UT
Partial Lunar Eclipse
(umbral mag. 0.05; Saros 115)
A tiny bite out of the Moon may be visible at maximum, though just 5% of the Moon will be shadowed in a partial eclipse lasting for 50 minutes and 24 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
18 Jul, 2046 AD
max: 01:04 UT
Partial Lunar Eclipse
(umbral mag. 0.25; Saros 120)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 25% of the Moon in shadow; the partial eclipse will last for 1 hour and 55 minutes. 		   
12 Jan, 2047 AD
max: 01:24 UT
Total Lunar Eclipse
(umbral mag. 1.23; Saros 125)
The Moon will be plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which will see the Moon 23% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 29 minutes in total. 		   
7 Jul, 2047 AD
max: 10:34 UT
Total Lunar Eclipse
(umbral mag. 1.75; Saros 130)
A dramatic total eclipse lasting 1 hour and 41 minutes 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 colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 39 minutes in total. 		   
1 Jan, 2048 AD
max: 06:52 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 55 minutes and 54 seconds. The Moon will be 13% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 34 minutes in total. 		   
26 Jun, 2048 AD
max: 02:00 UT
Partial Lunar Eclipse
(umbral mag. 0.64; Saros 140)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 39 minutes, with 64% of the Moon in darkness at maximum. 		   
20 Dec, 2048 AD
max: 06:26 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 145)
At maximum eclipse, 96% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 4 hours and 42 minutes overall. 		   
17 May, 2049 AD
max: 11:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 112)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 76% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 44 minutes. 		   
15 Jun, 2049 AD
max: 19:12 UT
Penumbral Lunar Eclipse
(penum. mag. 0.25; Saros 150)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 12 minutes, just 25% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
9 Nov, 2049 AD
max: 15:50 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 117)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 68% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 46 minutes. 		   
6 May, 2050 AD
max: 22:30 UT
Total Lunar Eclipse
(umbral mag. 1.08; Saros 122)
A shallow total eclipse will see the Moon in relative darkness for 43 minutes and 12 seconds. The Moon will be 8% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 26 minutes in total. 		   
30 Oct, 2050 AD
max: 03:20 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 127)
A shallow total eclipse will see the Moon in relative darkness for 34 minutes and 30 seconds. The Moon will be 5% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 13 minutes in total. 		   
26 Apr, 2051 AD
max: 02:14 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 132)
The Moon will be plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which will see the Moon 20% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 41 minutes in total. 		   
19 Oct, 2051 AD
max: 19:10 UT
Total Lunar Eclipse
(umbral mag. 1.41; Saros 137)
The Moon will be plunged into darkness for 1 hour and 24 minutes, in a deep total eclipse which will see the Moon 41% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 24 minutes in total. 		   
14 Apr, 2052 AD
max: 02:16 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 142)
At maximum eclipse, 95% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 4 hours and 36 minutes overall. 		   
8 Oct, 2052 AD
max: 10:44 UT
Partial Lunar Eclipse
(umbral mag. 0.08; Saros 147)
A tiny bite out of the Moon may be visible at maximum, though just 8% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 3 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
4 Mar, 2053 AD
max: 17:20 UT
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros 114)
At maximum eclipse, 93% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 4 hours and 11 minutes overall. 		   
29 Aug, 2053 AD
max: 08:04 UT
Penumbral Lunar Eclipse
(penum. mag. 1.02; Saros 119)
In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 38 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see. 		   
22 Feb, 2054 AD
max: 06:49 UT
Total Lunar Eclipse
(umbral mag. 1.28; Saros 124)
The Moon will be plunged into darkness for 1 hour and 12 minutes, in a deep total eclipse which will see the Moon 28% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 21 minutes in total. 		   
18 Aug, 2054 AD
max: 09:24 UT
Total Lunar Eclipse
(umbral mag. 1.31; Saros 129)
The Moon will be plunged into darkness for 1 hour and 23 minutes, in a deep total eclipse which will see the Moon 31% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 47 minutes in total. 		   
11 Feb, 2055 AD
max: 22:44 UT
Total Lunar Eclipse
(umbral mag. 1.22; Saros 134)
The Moon will be plunged into darkness for 1 hour and 6 minutes, in a deep total eclipse which will see the Moon 22% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 18 minutes in total. 		   
7 Aug, 2055 AD
max: 10:51 UT
Partial Lunar Eclipse
(umbral mag. 0.96; Saros 139)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 23 minutes. With 96% of the Moon in shadow at maximum eclipse, this will be quite a memorable event. 		   
1 Feb, 2056 AD
max: 12:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.91; Saros 144)
At maximum eclipse, 91% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 4 hours and 7 minutes overall. 		   
27 Jun, 2056 AD
max: 10:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.31; Saros 111)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 30 minutes, just 31% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
26 Jul, 2056 AD
max: 18:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.64; Saros 149)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 64% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 34 minutes.
22 Dec, 2056 AD
max: 01:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.79; Saros 116)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 79% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 4 hours and 16 minutes. 		   
17 Jun, 2057 AD
max: 02:24 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 121)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 49 minutes, with 76% of the Moon in darkness at maximum. 		   
11 Dec, 2057 AD
max: 00:51 UT
Partial Lunar Eclipse
(umbral mag. 0.92; Saros 126)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 24 minutes. With 92% of the Moon in shadow at maximum eclipse, this will be quite a memorable event. 		   
6 Jun, 2058 AD
max: 19:13 UT
Total Lunar Eclipse
(umbral mag. 1.66; Saros 131)
A dramatic total eclipse lasting 1 hour and 37 minutes 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 colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 33 minutes in total. 		   
30 Nov, 2058 AD
max: 03:14 UT
Total Lunar Eclipse
(umbral mag. 1.43; Saros 136)
The Moon will be plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which will see the Moon 43% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 41 minutes in total. 		   
27 May, 2059 AD
max: 07:53 UT
Partial Lunar Eclipse
(umbral mag. 0.18; Saros 141)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 37 minutes, with just 18% of the Moon in shadow at maximum. 		   
19 Nov, 2059 AD
max: 12:59 UT
Partial Lunar Eclipse
(umbral mag. 0.21; Saros 146)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 21% of the Moon in shadow; the partial eclipse will last for 1 hour and 39 minutes. 		   
15 Apr, 2060 AD
max: 21:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 113)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 77% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 4 hours and 15 minutes. 		   
9 Oct, 2060 AD
max: 18:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 118)
At maximum eclipse, 88% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 3 hours and 51 minutes overall. 		   
8 Nov, 2060 AD
max: 04:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 156)
In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 3% of the Moon's disc for 43 minutes and 36 seconds, which will be essentially impossible to see.