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, 2541–2560 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).
13 Jan, 2541 AD
max: 16:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.91; Saros 162)
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 3 hours and 56 minutes overall. 		   
9 Jun, 2541 AD
max: 20:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 129)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 33 minutes, just 59% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
9 Jul, 2541 AD
max: 09:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 167)
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 12% of the Moon's disc for 1 hour and 46 minutes, which will be essentially impossible to see.
4 Dec, 2541 AD
max: 15:40 UT
Penumbral Lunar Eclipse
(penum. mag. 0.99; Saros 134)
At maximum eclipse, 99% 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 26 minutes overall. 		   
30 May, 2542 AD
max: 07:57 UT
Total Lunar Eclipse
(umbral mag. 1.07; Saros 139)
A shallow total eclipse will see the Moon in relative darkness for 39 minutes and 24 seconds. The Moon will be 7% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 16 minutes in total. 		   
23 Nov, 2542 AD
max: 19:09 UT
Total Lunar Eclipse
(umbral mag. 1.16; Saros 144)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 3 minutes. 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 38 minutes in total. 		   
20 May, 2543 AD
max: 00:03 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 149)
The Moon will be plunged into darkness for 1 hour and 18 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. 		   
12 Nov, 2543 AD
max: 18:33 UT
Total Lunar Eclipse
(umbral mag. 1.18; Saros 154)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 6 minutes. The Moon will be 18% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 40 minutes in total. 		   
8 May, 2544 AD
max: 16:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 159)
The Moon will approach within 2% 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 4 hours and 2 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. 		   
31 Oct, 2544 AD
max: 21:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.98; Saros 164)
At maximum eclipse, 98% 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 27 minutes overall. 		   
29 Mar, 2545 AD
max: 15:28 UT
Partial Lunar Eclipse
(umbral mag. 0.09; Saros 131)
A tiny bite out of the Moon may be visible at maximum, though just 9% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 10 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
21 Sep, 2545 AD
max: 22:28 UT
Partial Lunar Eclipse
(umbral mag. 0.16; Saros 136)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 26 minutes, with just 16% of the Moon in shadow at maximum. 		   
18 Mar, 2546 AD
max: 16:56 UT
Total Lunar Eclipse
(umbral mag. 1.35; Saros 141)
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 48 minutes in total. 		   
11 Sep, 2546 AD
max: 15:16 UT
Total Lunar Eclipse
(umbral mag. 1.49; Saros 146)
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 27 minutes in total. 		   
7 Mar, 2547 AD
max: 16:45 UT
Partial Lunar Eclipse
(umbral mag. 1.00; Saros 151)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 27 minutes. With 100% of the Moon in shadow at maximum eclipse, this will be quite a memorable event. 		   
1 Sep, 2547 AD
max: 06:28 UT
Partial Lunar Eclipse
(umbral mag. 0.89; Saros 156)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 6 minutes, with 89% of the Moon in darkness at maximum. 		   
24 Feb, 2548 AD
max: 22:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.82; Saros 161)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 82% 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 Jul, 2548 AD
max: 02:33 UT
Penumbral Lunar Eclipse
(penum. mag. 0.25; Saros 128)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 29 minutes, just 25% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
20 Aug, 2548 AD
max: 15:52 UT
Penumbral Lunar Eclipse
(penum. mag. 0.41; Saros 166)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 4 minutes, just 41% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
14 Jan, 2549 AD
max: 23:30 UT
Partial Lunar Eclipse
(umbral mag. 0.13; Saros 133)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 18 minutes, with just 13% of the Moon in shadow at maximum. 		   
11 Jul, 2549 AD
max: 03:22 UT
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 138)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 54% of the Moon in shadow; the partial eclipse will last for 2 hours and 48 minutes. 		   
4 Jan, 2550 AD
max: 15:02 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 143)
The Moon will be plunged into darkness for 1 hour and 18 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 24 minutes in total. 		   
30 Jun, 2550 AD
max: 06:10 UT
Total Lunar Eclipse
(umbral mag. 1.69; Saros 148)
A dramatic total eclipse lasting 1 hour and 43 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. 		   
25 Dec, 2550 AD
max: 03:02 UT
Total Lunar Eclipse
(umbral mag. 1.09; Saros 153)
A shallow total eclipse will see the Moon in relative darkness for 46 minutes and 6 seconds. The Moon will be 9% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 23 minutes in total. 		   
19 Jun, 2551 AD
max: 15:57 UT
Partial Lunar Eclipse
(umbral mag. 0.34; Saros 158)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 34% of the Moon in shadow; the partial eclipse will last for 2 hours and 5 minutes. 		   
14 Dec, 2551 AD
max: 08:03 UT
Penumbral Lunar Eclipse
(penum. mag. 0.80; Saros 163)
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 16 minutes. 		   
10 May, 2552 AD
max: 00:12 UT
Partial Lunar Eclipse
(umbral mag. 0.06; Saros 130)
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 50 minutes and 54 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
8 Jun, 2552 AD
max: 07:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.04; Saros 168)
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 4% of the Moon's disc for 53 minutes and 48 seconds, which will be essentially impossible to see.
2 Nov, 2552 AD
max: 13:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 135)
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 13 minutes. 		   
29 Apr, 2553 AD
max: 15:58 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 140)
The Moon will be plunged into darkness for 1 hour and 19 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 27 minutes in total. 		   
22 Oct, 2553 AD
max: 18:35 UT
Total Lunar Eclipse
(umbral mag. 1.12; Saros 145)
A shallow total eclipse will see the Moon in relative darkness for 52 minutes exactly. The Moon will be 12% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 25 minutes in total. 		   
19 Apr, 2554 AD
max: 02:23 UT
Partial Lunar Eclipse
(umbral mag. 0.99; Saros 150)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 21 minutes. With 99% of the Moon in shadow at maximum eclipse, this will be quite a memorable event. 		   
12 Oct, 2554 AD
max: 06:48 UT
Total Lunar Eclipse
(umbral mag. 1.25; Saros 155)
The Moon will be plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which will see the Moon 25% 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. 		   
8 Apr, 2555 AD
max: 05:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.66; Saros 160)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 66% 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 58 minutes. 		   
2 Sep, 2555 AD
max: 15:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 127)
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 6% of the Moon's disc for 1 hour and 6 minutes, which will be essentially impossible to see. 		   
1 Oct, 2555 AD
max: 23:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.94; Saros 165)
The Moon will approach within 1% of the Earth's umbral shadow at maximum eclipse; 94% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 3 hours and 57 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.
26 Feb, 2556 AD
max: 12:19 UT
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 132)
At maximum eclipse, 97% 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 33 minutes overall. 		   
22 Aug, 2556 AD
max: 05:19 UT
Partial Lunar Eclipse
(umbral mag. 0.33; Saros 137)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 33% of the Moon in shadow; the partial eclipse will last for 2 hours and 7 minutes. 		   
14 Feb, 2557 AD
max: 19:37 UT
Total Lunar Eclipse
(umbral mag. 1.30; Saros 142)
The Moon will be plunged into darkness for 1 hour and 17 minutes, in a deep total eclipse which will see the Moon 30% 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. 		   
11 Aug, 2557 AD
max: 12:43 UT
Total Lunar Eclipse
(umbral mag. 1.69; Saros 147)
A dramatic total eclipse lasting 1 hour and 44 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 51 minutes in total. 		   
4 Feb, 2558 AD
max: 09:12 UT
Total Lunar Eclipse
(umbral mag. 1.16; Saros 152)
A shallow total eclipse will see the Moon in relative darkness for 56 minutes and 18 seconds. 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 15 minutes in total. 		   
31 Jul, 2558 AD
max: 14:03 UT
Partial Lunar Eclipse
(umbral mag. 0.56; Saros 157)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 56% of the Moon in shadow; the partial eclipse will last for 2 hours and 50 minutes. 		   
25 Jan, 2559 AD
max: 00:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 162)
At maximum eclipse, 92% 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 57 minutes overall. 		   
21 Jun, 2559 AD
max: 03:44 UT
Penumbral Lunar Eclipse
(penum. mag. 0.46; Saros 129)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 10 minutes, just 46% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
20 Jul, 2559 AD
max: 15:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.28; Saros 167)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 35 minutes, just 28% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
15 Dec, 2559 AD
max: 23:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 134)
At maximum eclipse, 97% 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 25 minutes overall. 		   
9 Jun, 2560 AD
max: 15:23 UT
Partial Lunar Eclipse
(umbral mag. 0.95; Saros 139)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 8 minutes. With 95% of the Moon in shadow at maximum eclipse, this will be quite a memorable event. 		   
4 Dec, 2560 AD
max: 02:59 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 144)
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 37 minutes in total.