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, 2641–2660 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).
17 Feb, 2641 AD
max: 21:10 UT
Total Lunar Eclipse
(umbral mag. 1.14; Saros 153)
A shallow total eclipse will see the Moon in relative darkness for 56 minutes and 42 seconds. The Moon will be 14% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 28 minutes in total. 		   
13 Aug, 2641 AD
max: 04:23 UT
Total Lunar Eclipse
(umbral mag. 1.04; Saros 158)
The Moon will barely edge into total eclipse for 30 minutes and 36 seconds. With the Moon just 4% 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 13 minutes in total. 		   
7 Feb, 2642 AD
max: 00:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 163)
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. 		   
4 Jul, 2642 AD
max: 14:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.40; Saros 130)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 43 minutes, just 40% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
2 Aug, 2642 AD
max: 20:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 168)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 69% 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 27 minutes.
28 Dec, 2642 AD
max: 05:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 135)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 62% 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 47 minutes. 		   
24 Jun, 2643 AD
max: 05:16 UT
Partial Lunar Eclipse
(umbral mag. 0.72; Saros 140)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 54 minutes, with 72% of the Moon in darkness at maximum. 		   
17 Dec, 2643 AD
max: 11:33 UT
Partial Lunar Eclipse
(umbral mag. 0.93; Saros 145)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 12 minutes. With 93% of the Moon in shadow at maximum eclipse, this will be quite a memorable event. 		   
12 Jun, 2644 AD
max: 14:04 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 150)
A dramatic total eclipse lasting 1 hour and 39 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 48 minutes in total. 		   
6 Dec, 2644 AD
max: 00:37 UT
Total Lunar Eclipse
(umbral mag. 1.49; Saros 155)
The Moon will be plunged into darkness for 1 hour and 29 minutes, in a deep total eclipse which will see the Moon 49% 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 28 minutes in total. 		   
1 Jun, 2645 AD
max: 16:04 UT
Partial Lunar Eclipse
(umbral mag. 0.14; Saros 160)
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 14% of the Moon in shadow at maximum. 		   
25 Nov, 2645 AD
max: 16:32 UT
Partial Lunar Eclipse
(umbral mag. 0.26; Saros 165)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 26% of the Moon in shadow; the partial eclipse will last for 1 hour and 48 minutes. 		   
22 Apr, 2646 AD
max: 02:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 132)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 69% 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 52 minutes. 		   
16 Oct, 2646 AD
max: 18:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.80; Saros 137)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 80% 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 1 minute. 		   
11 Apr, 2647 AD
max: 12:52 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 142)
A shallow total eclipse will see the Moon in relative darkness for 48 minutes and 30 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 18 minutes in total. 		   
5 Oct, 2647 AD
max: 23:06 UT
Total Lunar Eclipse
(umbral mag. 1.04; Saros 147)
The Moon will barely edge into total eclipse for 31 minutes and 18 seconds. With the Moon just 4% 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 31 minutes in total. 		   
31 Mar, 2648 AD
max: 04:02 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 152)
The Moon will be plunged into darkness for 1 hour and 17 minutes, in a deep total eclipse which will see the Moon 33% 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 22 minutes in total. 		   
23 Sep, 2648 AD
max: 23:13 UT
Total Lunar Eclipse
(umbral mag. 1.26; Saros 157)
The Moon will be plunged into darkness for 1 hour and 17 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 44 minutes in total. 		   
20 Mar, 2649 AD
max: 20:05 UT
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 162)
A tiny bite out of the Moon may be visible at maximum, though just 4% of the Moon will be shadowed in a partial eclipse lasting for 44 minutes and 42 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
13 Sep, 2649 AD
max: 02:08 UT
Penumbral Lunar Eclipse
(penum. mag. 0.99; Saros 167)
The Moon will approach within 5% of the Earth's umbral shadow at maximum eclipse; 99% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 4 hours and 29 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. 		   
8 Feb, 2650 AD
max: 17:33 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 134)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 88% 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 20 minutes. 		   
4 Aug, 2650 AD
max: 04:15 UT
Partial Lunar Eclipse
(umbral mag. 0.30; Saros 139)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 30% of the Moon in shadow; the partial eclipse will last for 1 hour and 56 minutes. 		   
28 Jan, 2651 AD
max: 18:56 UT
Total Lunar Eclipse
(umbral mag. 1.02; Saros 144)
The Moon will barely edge into total eclipse for 20 minutes and 12 seconds. With the Moon just 2% 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 31 minutes in total. 		   
24 Jul, 2651 AD
max: 21:19 UT
Total Lunar Eclipse
(umbral mag. 1.67; Saros 149)
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 30 minutes in total. 		   
17 Jan, 2652 AD
max: 18:11 UT
Total Lunar Eclipse
(umbral mag. 1.35; Saros 154)
The Moon will be plunged into darkness for 1 hour and 26 minutes, in a deep total eclipse which will see the Moon 35% 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 45 minutes in total. 		   
13 Jul, 2652 AD
max: 13:15 UT
Partial Lunar Eclipse
(umbral mag. 0.70; Saros 159)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 49 minutes, with 70% of the Moon in darkness at maximum. 		   
5 Jan, 2653 AD
max: 22:42 UT
Partial Lunar Eclipse
(umbral mag. 0.15; Saros 164)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 28 minutes, with just 15% of the Moon in shadow at maximum. 		   
3 Jun, 2653 AD
max: 10:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 131)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 25 minutes, just 49% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
2 Jul, 2653 AD
max: 23:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.19; Saros 169)
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 19% of the Moon's disc for 2 hours and 7 minutes, which will be essentially impossible to see.
26 Nov, 2653 AD
max: 23:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 136)
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 38 minutes. 		   
26 Dec, 2653 AD
max: 10:23 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 174)
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 47 minutes and 30 seconds, which will be essentially impossible to see.
23 May, 2654 AD
max: 11:32 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 141)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 12 minutes, with 76% of the Moon in darkness at maximum. 		   
16 Nov, 2654 AD
max: 15:46 UT
Total Lunar Eclipse
(umbral mag. 1.02; Saros 146)
The Moon will barely edge into total eclipse for just 18 minutes and 30 seconds. With the Moon just 2% 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 9 minutes in total. 		   
12 May, 2655 AD
max: 13:25 UT
Total Lunar Eclipse
(umbral mag. 1.50; Saros 151)
The Moon will be plunged into darkness for 1 hour and 36 minutes, in a deep total eclipse which will see the Moon 50% 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 46 minutes in total. 		   
6 Nov, 2655 AD
max: 04:36 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 156)
The Moon will be plunged into darkness for 1 hour and 26 minutes, in a deep total eclipse which will see the Moon 40% 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 35 minutes in total. 		   
30 Apr, 2656 AD
max: 21:55 UT
Partial Lunar Eclipse
(umbral mag. 0.20; Saros 161)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 38 minutes, with just 20% of the Moon in shadow at maximum. 		   
25 Oct, 2656 AD
max: 10:41 UT
Penumbral Lunar Eclipse
(penum. mag. 1.04; Saros 166)
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 43 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see. 		   
22 Mar, 2657 AD
max: 03:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 133)
The Moon will approach within 0% 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 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. 		   
14 Sep, 2657 AD
max: 18:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 138)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 74% 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 7 minutes. 		   
11 Mar, 2658 AD
max: 19:00 UT
Total Lunar Eclipse
(umbral mag. 1.21; Saros 143)
The Moon will be plunged into darkness for 1 hour and 6 minutes, in a deep total eclipse which will see the Moon 21% 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 22 minutes in total. 		   
3 Sep, 2658 AD
max: 23:40 UT
Total Lunar Eclipse
(umbral mag. 1.14; Saros 148)
A shallow total eclipse will see the Moon in relative darkness for 57 minutes and 42 seconds. The Moon will be 14% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 28 minutes in total. 		   
1 Mar, 2659 AD
max: 05:24 UT
Total Lunar Eclipse
(umbral mag. 1.16; Saros 153)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 1 minute. The Moon will be 16% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 30 minutes in total. 		   
24 Aug, 2659 AD
max: 11:48 UT
Total Lunar Eclipse
(umbral mag. 1.17; Saros 158)
A shallow total eclipse will see the Moon in relative darkness for 59 minutes and 54 seconds. The Moon will be 17% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 20 minutes in total. 		   
18 Feb, 2660 AD
max: 08:22 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 163)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 90% 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 31 minutes. 		   
14 Jul, 2660 AD
max: 21:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.27; Saros 130)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 15 minutes, just 27% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
13 Aug, 2660 AD
max: 04:26 UT
Penumbral Lunar Eclipse
(penum. mag. 0.81; Saros 168)
At maximum eclipse, 81% 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 43 minutes overall.