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, 2601–2620 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.

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).
9 Apr, 2601 AD
max: 15:38 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 151)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 7 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 37 minutes in total.
4 Oct, 2601 AD
max: 05:04 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 156)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 4 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 26 minutes in total.
29 Mar, 2602 AD
max: 22:29 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 161)
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 14 minutes overall.
23 Sep, 2602 AD
max: 12:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 166)
This subtle penumbral eclipse 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 7 minutes.
18 Feb, 2603 AD
max: 01:54 UT
Partial Lunar Eclipse
(umbral mag. 0.10; Saros 133)
A tiny bite out of the Moon may be visible at maximum, though just 10% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 7 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
13 Aug, 2603 AD
max: 22:45 UT
Partial Lunar Eclipse
(umbral mag. 0.07; Saros 138)
A tiny bite out of the Moon may be visible at maximum, though just 7% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 7 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
7 Feb, 2604 AD
max: 17:18 UT
Total Lunar Eclipse
(umbral mag. 1.29; Saros 143)
The Moon will be plunged into darkness for 1 hour and 15 minutes, in a deep total eclipse which will see the Moon 29% 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.
2 Aug, 2604 AD
max: 02:38 UT
Total Lunar Eclipse
(umbral mag. 1.55; Saros 148)
The Moon will be plunged into darkness for 1 hour and 38 minutes, in a deep total eclipse which will see the Moon 55% 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.
27 Jan, 2605 AD
max: 04:26 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 153)
A shallow total eclipse will see the Moon in relative darkness for 51 minutes and 6 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 26 minutes in total.
22 Jul, 2605 AD
max: 13:43 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 158)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 55 minutes, with 76% of the Moon in darkness at maximum.
16 Jan, 2606 AD
max: 08:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 163)
This subtle penumbral eclipse 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 24 minutes.
12 Jun, 2606 AD
max: 23:14 UT
Penumbral Lunar Eclipse
(penum. mag. 0.66; Saros 130)
This subtle penumbral eclipse 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 24 minutes.
12 Jul, 2606 AD
max: 05:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros 168)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 47 minutes, just 42% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
6 Dec, 2606 AD
max: 13:03 UT
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 135)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 65% 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 54 minutes.
2 Jun, 2607 AD
max: 14:41 UT
Partial Lunar Eclipse
(umbral mag. 0.99; Saros 140)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 13 minutes. With 99% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
25 Nov, 2607 AD
max: 18:47 UT
Partial Lunar Eclipse
(umbral mag. 0.98; Saros 145)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 15 minutes. With 98% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
22 May, 2608 AD
max: 00:12 UT
Total Lunar Eclipse
(umbral mag. 1.31; Saros 150)
The Moon will be plunged into darkness for 1 hour and 21 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 39 minutes in total.
14 Nov, 2608 AD
max: 07:31 UT
Total Lunar Eclipse
(umbral mag. 1.43; Saros 155)
The Moon will be plunged into darkness for 1 hour and 25 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 27 minutes in total.
11 May, 2609 AD
max: 02:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 160)
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 38 minutes overall.
3 Nov, 2609 AD
max: 23:36 UT
Partial Lunar Eclipse
(umbral mag. 0.19; Saros 165)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 32 minutes, with just 19% of the Moon in shadow at maximum.
31 Mar, 2610 AD
max: 11:52 UT
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 132)
This subtle penumbral eclipse 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 14 minutes.
25 Sep, 2610 AD
max: 03:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.98; Saros 137)
The Moon will approach within 4% of the Earth's umbral shadow at maximum eclipse; 98% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 4 hours and 20 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.
20 Mar, 2611 AD
max: 20:41 UT
Total Lunar Eclipse
(umbral mag. 1.22; Saros 142)
The Moon will be plunged into darkness for 1 hour and 7 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 24 minutes in total.
14 Sep, 2611 AD
max: 09:04 UT
Total Lunar Eclipse
(umbral mag. 1.27; Saros 147)
The Moon will be plunged into darkness for 1 hour and 18 minutes, in a deep total eclipse which will see the Moon 27% 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.
9 Mar, 2612 AD
max: 11:12 UT
Total Lunar Eclipse
(umbral mag. 1.23; Saros 152)
The Moon will be plunged into darkness for 1 hour and 7 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 18 minutes in total.
2 Sep, 2612 AD
max: 09:39 UT
Total Lunar Eclipse
(umbral mag. 1.01; Saros 157)
The Moon will barely edge into total eclipse for just 12 minutes exactly. With the Moon just barely inside 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.
27 Feb, 2613 AD
max: 03:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 162)
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 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.
24 Jul, 2613 AD
max: 00:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; 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 6% of the Moon's disc for 1 hour and 8 minutes, which will be essentially impossible to see.
22 Aug, 2613 AD
max: 12:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 167)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 72% 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.
18 Jan, 2614 AD
max: 00:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 134)
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 4 hours and 22 minutes overall.
13 Jul, 2614 AD
max: 13:29 UT
Partial Lunar Eclipse
(umbral mag. 0.56; Saros 139)
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 33 minutes.
7 Jan, 2615 AD
max: 02:53 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 144)
The Moon will barely edge into total eclipse for 36 minutes exactly. 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 33 minutes in total.
3 Jul, 2615 AD
max: 06:24 UT
Total Lunar Eclipse
(umbral mag. 1.83; Saros 149)
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 32 minutes in total.
27 Dec, 2615 AD
max: 02:00 UT
Total Lunar Eclipse
(umbral mag. 1.32; Saros 154)
The Moon will be plunged into darkness for 1 hour and 23 minutes, in a deep total eclipse which will see the Moon 32% 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.
21 Jun, 2616 AD
max: 22:41 UT
Partial Lunar Eclipse
(umbral mag. 0.43; Saros 159)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 43% of the Moon in shadow; the partial eclipse will last for 2 hours and 19 minutes.
15 Dec, 2616 AD
max: 05:52 UT
Partial Lunar Eclipse
(umbral mag. 0.11; Saros 164)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 16 minutes, with just 11% of the Moon in shadow at maximum.
12 May, 2617 AD
max: 20:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 131)
This subtle penumbral eclipse 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 4 hours and 6 minutes.
5 Nov, 2617 AD
max: 06:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 136)
At maximum eclipse, 84% 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 47 minutes overall.
1 May, 2618 AD
max: 21:54 UT
Total Lunar Eclipse
(umbral mag. 1.00; Saros 141)
The Moon will barely edge into total eclipse for just 11 minutes and 36 seconds. With the Moon just barely inside 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.
25 Oct, 2618 AD
max: 23:08 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 146)
A shallow total eclipse will see the Moon in relative darkness for 51 minutes and 30 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 15 minutes in total.
20 Apr, 2619 AD
max: 23:00 UT
Total Lunar Eclipse
(umbral mag. 1.29; Saros 151)
The Moon will be plunged into darkness for 1 hour and 19 minutes, in a deep total eclipse which will see the Moon 29% 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 40 minutes in total.
15 Oct, 2619 AD
max: 12:48 UT
Total Lunar Eclipse
(umbral mag. 1.27; Saros 156)
The Moon will be plunged into darkness for 1 hour and 15 minutes, in a deep total eclipse which will see the Moon 27% 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 30 minutes in total.
9 Apr, 2620 AD
max: 06:25 UT
Partial Lunar Eclipse
(umbral mag. 0.01; Saros 161)
A tiny bite out of the Moon may be visible at maximum, though just 1% of the Moon will be shadowed in a partial eclipse lasting for 26 minutes exactly. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
3 Oct, 2620 AD
max: 20:00 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 166)
This subtle penumbral eclipse 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 22 minutes.