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, 2581–2600 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).
20 Apr, 2581 AD
max: 06:30 UT
Penumbral Lunar Eclipse
(penum. mag. 0.98; Saros 131)
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 32 minutes overall. 		   
13 Oct, 2581 AD
max: 14:23 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 136)
The Moon will approach within 1% 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 exactly. 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. 		   
9 Apr, 2582 AD
max: 07:43 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 141)
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 42 minutes in total. 		   
3 Oct, 2582 AD
max: 06:58 UT
Total Lunar Eclipse
(umbral mag. 1.28; Saros 146)
The Moon will be plunged into darkness for 1 hour and 13 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. 		   
29 Mar, 2583 AD
max: 08:07 UT
Total Lunar Eclipse
(umbral mag. 1.12; Saros 151)
A shallow total eclipse will see the Moon in relative darkness for 53 minutes and 36 seconds. 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 33 minutes in total. 		   
22 Sep, 2583 AD
max: 21:27 UT
Total Lunar Eclipse
(umbral mag. 1.10; Saros 156)
A shallow total eclipse will see the Moon in relative darkness for 47 minutes and 54 seconds. The Moon will be 10% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 21 minutes in total. 		   
17 Mar, 2584 AD
max: 14:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 161)
At maximum eclipse, 90% 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 9 minutes overall. 		   
11 Sep, 2584 AD
max: 05:45 UT
Penumbral Lunar Eclipse
(penum. mag. 0.66; Saros 166)
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 50 minutes. 		   
5 Feb, 2585 AD
max: 17:09 UT
Partial Lunar Eclipse
(umbral mag. 0.11; Saros 133)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 12 minutes, with just 11% of the Moon in shadow at maximum. 		   
1 Aug, 2585 AD
max: 16:14 UT
Partial Lunar Eclipse
(umbral mag. 0.23; Saros 138)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 23% of the Moon in shadow; the partial eclipse will last for 1 hour and 53 minutes. 		   
26 Jan, 2586 AD
max: 08:35 UT
Total Lunar Eclipse
(umbral mag. 1.31; Saros 143)
The Moon will be plunged into darkness for 1 hour and 16 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 24 minutes in total. 		   
21 Jul, 2586 AD
max: 19:45 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 47 minutes in total. 		   
15 Jan, 2587 AD
max: 20:00 UT
Total Lunar Eclipse
(umbral mag. 1.10; Saros 153)
A shallow total eclipse will see the Moon in relative darkness for 49 minutes and 12 seconds. The Moon will be 10% 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. 		   
11 Jul, 2587 AD
max: 06:27 UT
Partial Lunar Eclipse
(umbral mag. 0.62; Saros 158)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 42 minutes, with 62% of the Moon in darkness at maximum. 		   
5 Jan, 2588 AD
max: 00:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 163)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 83% 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 21 minutes. 		   
31 May, 2588 AD
max: 15:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.78; Saros 130)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 78% 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 40 minutes. 		   
29 Jun, 2588 AD
max: 22:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.29; Saros 168)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 20 minutes, just 29% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
24 Nov, 2588 AD
max: 05:08 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 135)
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 59 minutes. 		   
21 May, 2589 AD
max: 07:14 UT
Total Lunar Eclipse
(umbral mag. 1.12; Saros 140)
A shallow total eclipse will see the Moon in relative darkness for 50 minutes and 30 seconds. 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 19 minutes in total. 		   
13 Nov, 2589 AD
max: 10:34 UT
Total Lunar Eclipse
(umbral mag. 1.01; Saros 145)
The Moon will barely edge into total eclipse for just 16 minutes and 53 seconds. With the Moon just 1% 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 18 minutes in total. 		   
10 May, 2590 AD
max: 17:05 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 150)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 6 minutes. The Moon will be 19% 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. 		   
2 Nov, 2590 AD
max: 23:08 UT
Total Lunar Eclipse
(umbral mag. 1.38; Saros 155)
The Moon will be plunged into darkness for 1 hour and 22 minutes, in a deep total eclipse which will see the Moon 38% 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. 		   
29 Apr, 2591 AD
max: 19:42 UT
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 160)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 84% 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 25 minutes. 		   
23 Oct, 2591 AD
max: 15:19 UT
Partial Lunar Eclipse
(umbral mag. 0.13; Saros 165)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 17 minutes, with just 13% of the Moon in shadow at maximum. 		   
19 Mar, 2592 AD
max: 04:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 132)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 89% 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 21 minutes. 		   
12 Sep, 2592 AD
max: 19:53 UT
Partial Lunar Eclipse
(umbral mag. 0.08; Saros 137)
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 4 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
8 Mar, 2593 AD
max: 12:26 UT
Total Lunar Eclipse
(umbral mag. 1.25; Saros 142)
The Moon will be plunged into darkness for 1 hour and 11 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 26 minutes in total. 		   
2 Sep, 2593 AD
max: 02:13 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 147)
The Moon will be plunged into darkness for 1 hour and 30 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 46 minutes in total. 		   
26 Feb, 2594 AD
max: 02:37 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 152)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 3 minutes. The Moon will be 20% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 17 minutes in total. 		   
22 Aug, 2594 AD
max: 03:02 UT
Partial Lunar Eclipse
(umbral mag. 0.86; Saros 157)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 21 minutes, with 86% of the Moon in darkness at maximum. 		   
15 Feb, 2595 AD
max: 18:27 UT
Penumbral Lunar Eclipse
(penum. mag. 0.94; Saros 162)
The Moon will approach within 4% 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 exactly. 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. 		   
12 Jul, 2595 AD
max: 17:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.19; Saros 129)
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 3 minutes, which will be essentially impossible to see. 		   
11 Aug, 2595 AD
max: 05:16 UT
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 167)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 37 minutes, just 58% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
6 Jan, 2596 AD
max: 16:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros 134)
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 23 minutes overall. 		   
1 Jul, 2596 AD
max: 06:08 UT
Partial Lunar Eclipse
(umbral mag. 0.69; Saros 139)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 47 minutes, with 69% of the Moon in darkness at maximum. 		   
25 Dec, 2596 AD
max: 18:52 UT
Total Lunar Eclipse
(umbral mag. 1.07; Saros 144)
A shallow total eclipse will see the Moon in relative darkness for 42 minutes and 18 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 34 minutes in total. 		   
20 Jun, 2597 AD
max: 22:53 UT
Total Lunar Eclipse
(umbral mag. 1.70; 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 31 minutes in total. 		   
14 Dec, 2597 AD
max: 18:00 UT
Total Lunar Eclipse
(umbral mag. 1.30; Saros 154)
The Moon will be plunged into darkness for 1 hour and 21 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 44 minutes in total. 		   
10 Jun, 2598 AD
max: 15:18 UT
Partial Lunar Eclipse
(umbral mag. 0.31; Saros 159)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 31% of the Moon in shadow; the partial eclipse will last for 1 hour and 59 minutes. 		   
3 Dec, 2598 AD
max: 21:34 UT
Partial Lunar Eclipse
(umbral mag. 0.08; Saros 164)
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 6 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. 		   
1 May, 2599 AD
max: 13:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 131)
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 21 minutes. 		   
24 Oct, 2599 AD
max: 22:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 136)
At maximum eclipse, 89% 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 53 minutes overall. 		   
20 Apr, 2600 AD
max: 14:53 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 141)
A shallow total eclipse will see the Moon in relative darkness for 53 minutes and 12 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 37 minutes in total. 		   
14 Oct, 2600 AD
max: 14:59 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 146)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 3 minutes. The Moon will be 20% 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.