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, 1020–1001 BC

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).
23 Apr, 1020 BC
max: 20:03 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 44)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 88% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 28 minutes. 		   
17 Oct, 1020 BC
max: 17:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 49)
At maximum eclipse, 87% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 3 hours and 50 minutes overall. 		   
14 Mar, 1019 BC
max: 06:29 UT
Penumbral Lunar Eclipse
(penum. mag. 1.04; Saros 16)
In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 38 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. 		   
7 Sep, 1019 BC
max: 20:43 UT
Partial Lunar Eclipse
(umbral mag. 0.12; Saros 21)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 19 minutes, with just 12% of the Moon in shadow at maximum. 		   
3 Mar, 1018 BC
max: 14:56 UT
Total Lunar Eclipse
(umbral mag. 1.46; Saros 26)
The Moon was plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which saw the Moon 46% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 34 minutes in total. 		   
28 Aug, 1018 BC
max: 02:50 UT
Total Lunar Eclipse
(umbral mag. 1.39; Saros 31)
The Moon was plunged into darkness for 1 hour and 29 minutes, in a deep total eclipse which saw the Moon 39% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 45 minutes in total. 		   
21 Feb, 1017 BC
max: 05:26 UT
Partial Lunar Eclipse
(umbral mag. 0.96; Saros 36)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 5 minutes. With 96% of the Moon in shadow at maximum eclipse, this was quite a memorable event. 		   
16 Aug, 1017 BC
max: 03:15 UT
Partial Lunar Eclipse
(umbral mag. 0.92; Saros 41)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 25 minutes. With 92% of the Moon in shadow at maximum eclipse, this was quite a memorable event. 		   
11 Jan, 1016 BC
max: 11:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 8)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 17% of the Moon's disc for 1 hour and 51 minutes, which was essentially impossible to see. 		   
9 Feb, 1016 BC
max: 21:50 UT
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 46)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 65% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 25 minutes.
6 Jul, 1016 BC
max: 16:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.02; Saros 13)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 2% of the Moon's disc for 42 minutes and 18 seconds, which was essentially impossible to see. 		   
5 Aug, 1016 BC
max: 04:50 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 51)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 68% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 54 minutes.
31 Dec, 1016 BC
max: 21:53 UT
Partial Lunar Eclipse
(umbral mag. 0.31; Saros 18)
The Earth's shadow on the moon was clearly visible in this eclipse, with 31% of the Moon in shadow; the partial eclipse lasted for 2 hours and 5 minutes. 		   
26 Jun, 1015 BC
max: 04:30 UT
Partial Lunar Eclipse
(umbral mag. 0.52; Saros 23)
The Earth's shadow on the moon was clearly visible in this eclipse, with 52% of the Moon in shadow; the partial eclipse lasted for 2 hours and 29 minutes. 		   
21 Dec, 1015 BC
max: 00:44 UT
Total Lunar Eclipse
(umbral mag. 1.53; Saros 28)
The Moon was plunged into darkness for 1 hour and 38 minutes, in a deep total eclipse which saw the Moon 53% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 51 minutes in total. 		   
15 Jun, 1014 BC
max: 21:13 UT
Total Lunar Eclipse
(umbral mag. 1.87; Saros 33)
A dramatic total eclipse lasting 1 hour and 40 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 32 minutes in total. 		   
9 Dec, 1014 BC
max: 23:46 UT
Partial Lunar Eclipse
(umbral mag. 0.84; Saros 38)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 18 minutes, with 84% of the Moon in darkness at maximum. 		   
4 Jun, 1013 BC
max: 13:49 UT
Partial Lunar Eclipse
(umbral mag. 0.47; Saros 43)
The Earth's shadow on the moon was clearly visible in this eclipse, with 47% of the Moon in shadow; the partial eclipse lasted for 2 hours and 23 minutes. 		   
28 Nov, 1013 BC
max: 02:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 48)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 72% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 55 minutes. 		   
25 Apr, 1012 BC
max: 13:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.82; Saros 15)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 82% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 13 minutes. 		   
19 Oct, 1012 BC
max: 01:23 UT
Partial Lunar Eclipse
(umbral mag. 0.16; Saros 20)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 25 minutes, with just 16% of the Moon in shadow at maximum. 		   
14 Apr, 1011 BC
max: 15:46 UT
Total Lunar Eclipse
(umbral mag. 1.12; Saros 25)
A shallow total eclipse saw the Moon in relative darkness for 55 minutes and 24 seconds. The Moon was 12% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 38 minutes in total. 		   
8 Oct, 1011 BC
max: 17:14 UT
Total Lunar Eclipse
(umbral mag. 1.39; Saros 30)
The Moon was plunged into darkness for 1 hour and 22 minutes, in a deep total eclipse which saw the Moon 39% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 24 minutes in total. 		   
3 Apr, 1010 BC
max: 16:55 UT
Total Lunar Eclipse
(umbral mag. 1.14; Saros 35)
A shallow total eclipse saw the Moon in relative darkness for 58 minutes and 36 seconds. The Moon was 14% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 35 minutes in total. 		   
28 Sep, 1010 BC
max: 06:58 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 40)
The Moon barely edged into total eclipse for 32 minutes and 42 seconds. With the Moon just 5% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 17 minutes in total. 		   
22 Feb, 1009 BC
max: 13:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.02; Saros 7)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 2% of the Moon's disc for 36 minutes and 24 seconds, which was essentially impossible to see. 		   
22 Mar, 1009 BC
max: 23:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 45)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 84% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 1 minute.
16 Sep, 1009 BC
max: 14:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 50)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 69% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 55 minutes. 		   
11 Feb, 1008 BC
max: 05:11 UT
Partial Lunar Eclipse
(umbral mag. 0.38; Saros 17)
The Earth's shadow on the moon was clearly visible in this eclipse, with 38% of the Moon in shadow; the partial eclipse lasted for 2 hours and 8 minutes. 		   
6 Aug, 1008 BC
max: 22:32 UT
Penumbral Lunar Eclipse
(penum. mag. 1.05; Saros 22)
In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 49 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. 		   
31 Jan, 1007 BC
max: 21:12 UT
Total Lunar Eclipse
(umbral mag. 1.63; Saros 27)
A dramatic total eclipse lasting 1 hour and 36 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 32 minutes in total. 		   
27 Jul, 1007 BC
max: 01:49 UT
Total Lunar Eclipse
(umbral mag. 1.42; Saros 32)
The Moon was plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which saw the Moon 42% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 41 minutes in total. 		   
21 Jan, 1006 BC
max: 09:11 UT
Partial Lunar Eclipse
(umbral mag. 0.74; Saros 37)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 59 minutes, with 74% of the Moon in darkness at maximum. 		   
16 Jul, 1006 BC
max: 12:25 UT
Partial Lunar Eclipse
(umbral mag. 0.90; Saros 42)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 6 minutes. With 90% of the Moon in shadow at maximum eclipse, this was quite a memorable event. 		   
10 Jan, 1005 BC
max: 13:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros 47)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 12 minutes, just 42% of the Moon's disc was in partial shadow (with no part of it in complete shadow). 		   
5 Jun, 1005 BC
max: 21:42 UT
Penumbral Lunar Eclipse
(penum. mag. 0.51; Saros 14)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 2 minutes, just 51% of the Moon's disc was in partial shadow (with no part of it in complete shadow). 		   
5 Jul, 1005 BC
max: 04:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 52)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 12 minutes, just 58% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
29 Nov, 1005 BC
max: 18:33 UT
Penumbral Lunar Eclipse
(penum. mag. 1.08; Saros 19)
In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 49 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. 		   
26 May, 1004 BC
max: 13:28 UT
Partial Lunar Eclipse
(umbral mag. 0.85; Saros 24)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 3 minutes, with 85% of the Moon in darkness at maximum. 		   
18 Nov, 1004 BC
max: 23:24 UT
Total Lunar Eclipse
(umbral mag. 1.34; Saros 29)
The Moon was plunged into darkness for 1 hour and 22 minutes, in a deep total eclipse which saw the Moon 34% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 34 minutes in total. 		   
15 May, 1003 BC
max: 23:31 UT
Total Lunar Eclipse
(umbral mag. 1.44; Saros 34)
The Moon was plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which saw the Moon 44% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 43 minutes in total. 		   
8 Nov, 1003 BC
max: 11:19 UT
Total Lunar Eclipse
(umbral mag. 1.10; Saros 39)
A shallow total eclipse saw the Moon in relative darkness for 45 minutes exactly. The Moon was 10% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 14 minutes in total. 		   
5 May, 1002 BC
max: 02:32 UT
Penumbral Lunar Eclipse
(penum. mag. 1.03; Saros 44)
In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 46 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. 		   
29 Oct, 1002 BC
max: 02:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 49)
At maximum eclipse, 88% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 3 hours and 52 minutes overall. 		   
24 Mar, 1001 BC
max: 13:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros 16)
At maximum eclipse, 93% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 24 minutes overall. 		   
18 Sep, 1001 BC
max: 04:48 UT
Partial Lunar Eclipse
(umbral mag. 0.06; Saros 21)
A tiny bite out of the Moon may have been visible at maximum, though just 6% of the Moon was shadowed in a partial eclipse which lasted for 57 minutes and 54 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.