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, 1400–1381 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).
26 Mar, 1400 BC
max: 05:40 UT
Partial Lunar Eclipse
(umbral mag. 0.18; Saros 29)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 41 minutes, with just 18% of the Moon in shadow at maximum. 		   
19 Sep, 1400 BC
max: 14:25 UT
Partial Lunar Eclipse
(umbral mag. 0.30; Saros 34)
The Earth's shadow on the moon was clearly visible in this eclipse, with 30% of the Moon in shadow; the partial eclipse lasted for 1 hour and 57 minutes. 		   
13 Feb, 1399 BC
max: 21:44 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 1)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 76% 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 52 minutes. 		   
10 Aug, 1399 BC
max: 10:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 6)
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 55 minutes. 		   
3 Feb, 1398 BC
max: 11:21 UT
Total Lunar Eclipse
(umbral mag. 1.15; Saros 11)
A shallow total eclipse saw the Moon in relative darkness for 55 minutes and 42 seconds. The Moon was 15% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 16 minutes in total. 		   
30 Jul, 1398 BC
max: 11:55 UT
Partial Lunar Eclipse
(umbral mag. 0.92; Saros 16)
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. 		   
24 Jan, 1397 BC
max: 03:33 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 21)
The Moon was plunged into darkness for 1 hour and 17 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 22 minutes in total. 		   
18 Jul, 1397 BC
max: 13:03 UT
Total Lunar Eclipse
(umbral mag. 1.36; Saros 26)
The Moon was plunged into darkness for 1 hour and 26 minutes, in a deep total eclipse which saw the Moon 36% 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 44 minutes in total. 		   
12 Jan, 1396 BC
max: 17:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.99; Saros 31)
The Moon approached within 2% of the Earth's umbral shadow at maximum eclipse; 99% of the Moon's disc was partially shaded by the Earth, with the overall eclipse lasting 4 hours and 15 minutes. While less dramatic than a partial eclipse (as no part of the Moon was in complete shadow), a shading across the Moon should have been readily visible to observers. 		   
7 Jul, 1396 BC
max: 20:33 UT
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 36)
A tiny bite out of the Moon may have been visible at maximum, though just 4% of the Moon was shadowed in a partial eclipse which lasted for 43 minutes and 48 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse. 		   
3 Dec, 1396 BC
max: 07:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 3)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 74% 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 9 minutes. 		   
29 May, 1395 BC
max: 04:00 UT
Partial Lunar Eclipse
(umbral mag. 0.37; Saros 8)
The Earth's shadow on the moon was clearly visible in this eclipse, with 37% of the Moon in shadow; the partial eclipse lasted for 2 hours and 6 minutes. 		   
22 Nov, 1395 BC
max: 06:56 UT
Partial Lunar Eclipse
(umbral mag. 0.85; Saros 13)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 19 minutes, with 85% of the Moon in darkness at maximum. 		   
18 May, 1394 BC
max: 20:59 UT
Total Lunar Eclipse
(umbral mag. 1.71; Saros 18)
A dramatic total eclipse lasting 1 hour and 39 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 34 minutes in total. 		   
11 Nov, 1394 BC
max: 08:50 UT
Total Lunar Eclipse
(umbral mag. 1.50; Saros 23)
The Moon was plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 43 minutes in total. 		   
7 May, 1393 BC
max: 09:56 UT
Partial Lunar Eclipse
(umbral mag. 0.58; Saros 28)
The Earth's shadow on the moon was clearly visible in this eclipse, with 58% of the Moon in shadow; the partial eclipse lasted for 2 hours and 43 minutes. 		   
30 Oct, 1393 BC
max: 18:01 UT
Partial Lunar Eclipse
(umbral mag. 0.30; Saros 33)
The Earth's shadow on the moon was clearly visible in this eclipse, with 30% of the Moon in shadow; the partial eclipse lasted for 1 hour and 58 minutes. 		   
28 Mar, 1392 BC
max: 00:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.46; Saros 0)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 22 minutes, just 46% of the Moon's disc was in partial shadow (with no part of it in complete shadow). 		   
26 Apr, 1392 BC
max: 15:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.11; Saros 38)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 11% of the Moon's disc for 1 hour and 41 minutes, which was essentially impossible to see.
20 Sep, 1392 BC
max: 22:32 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 5)
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 28 minutes. 		   
20 Oct, 1392 BC
max: 08:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 43)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 15% of the Moon's disc for 1 hour and 42 minutes, which was essentially impossible to see.
17 Mar, 1391 BC
max: 01:34 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 10)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 9 minutes, with 76% of the Moon in darkness at maximum. 		   
10 Sep, 1391 BC
max: 13:03 UT
Partial Lunar Eclipse
(umbral mag. 0.91; Saros 15)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 7 minutes. With 91% of the Moon in shadow at maximum eclipse, this was quite a memorable event. 		   
6 Mar, 1390 BC
max: 07:20 UT
Total Lunar Eclipse
(umbral mag. 1.51; Saros 20)
The Moon was plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which saw the Moon 51% 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 39 minutes in total. 		   
30 Aug, 1390 BC
max: 21:51 UT
Total Lunar Eclipse
(umbral mag. 1.45; Saros 25)
The Moon was plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which saw the Moon 45% 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. 		   
23 Feb, 1389 BC
max: 20:01 UT
Partial Lunar Eclipse
(umbral mag. 0.22; Saros 30)
The Earth's shadow on the moon was clearly visible in this eclipse, with 22% of the Moon in shadow; the partial eclipse lasted for 1 hour and 41 minutes. 		   
18 Aug, 1389 BC
max: 23:47 UT
Partial Lunar Eclipse
(umbral mag. 0.07; Saros 35)
A tiny bite out of the Moon may have been visible at maximum, though just 7% of the Moon was shadowed in a partial eclipse which lasted for 1 hour and 4 minutes. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse. 		   
14 Jan, 1388 BC
max: 02:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 2)
At maximum eclipse, 92% 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 59 minutes overall. 		   
9 Jul, 1388 BC
max: 09:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 7)
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 56 minutes. 		   
3 Jan, 1387 BC
max: 15:30 UT
Total Lunar Eclipse
(umbral mag. 1.14; Saros 12)
A shallow total eclipse saw the Moon in relative darkness for 56 minutes and 24 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 25 minutes in total. 		   
28 Jun, 1387 BC
max: 19:30 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 17)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 3 minutes. The Moon was 19% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 24 minutes in total. 		   
23 Dec, 1387 BC
max: 21:05 UT
Total Lunar Eclipse
(umbral mag. 1.21; Saros 22)
The Moon was plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 39 minutes in total. 		   
18 Jun, 1386 BC
max: 11:04 UT
Total Lunar Eclipse
(umbral mag. 1.18; Saros 27)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 1 minute. The Moon was 18% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 17 minutes in total. 		   
12 Dec, 1386 BC
max: 20:42 UT
Penumbral Lunar Eclipse
(penum. mag. 1.04; Saros 32)
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 51 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. 		   
8 May, 1385 BC
max: 20:50 UT
Penumbral Lunar Eclipse
(penum. mag. 0.26; Saros -1)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 17 minutes, just 26% of the Moon's disc was in partial shadow (with no part of it in complete shadow). 		   
7 Jun, 1385 BC
max: 04:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.78; Saros 37)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 78% 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 41 minutes.
1 Nov, 1385 BC
max: 05:21 UT
Penumbral Lunar Eclipse
(penum. mag. 0.55; Saros 4)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 26 minutes, just 55% of the Moon's disc was in partial shadow (with no part of it in complete shadow). 		   
28 Apr, 1384 BC
max: 07:59 UT
Partial Lunar Eclipse
(umbral mag. 0.57; Saros 9)
The Earth's shadow on the moon was clearly visible in this eclipse, with 57% of the Moon in shadow; the partial eclipse lasted for 2 hours and 44 minutes. 		   
21 Oct, 1384 BC
max: 16:29 UT
Partial Lunar Eclipse
(umbral mag. 0.88; Saros 14)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 2 minutes, with 88% of the Moon in darkness at maximum. 		   
17 Apr, 1383 BC
max: 11:53 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 19)
A dramatic total eclipse lasting 1 hour and 45 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 55 minutes in total. 		   
11 Oct, 1383 BC
max: 07:54 UT
Total Lunar Eclipse
(umbral mag. 1.61; Saros 24)
A dramatic total eclipse lasting 1 hour and 34 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 28 minutes in total. 		   
6 Apr, 1382 BC
max: 12:22 UT
Partial Lunar Eclipse
(umbral mag. 0.32; Saros 29)
The Earth's shadow on the moon was clearly visible in this eclipse, with 32% of the Moon in shadow; the partial eclipse lasted for 2 hours and 13 minutes. 		   
30 Sep, 1382 BC
max: 22:56 UT
Partial Lunar Eclipse
(umbral mag. 0.32; Saros 34)
The Earth's shadow on the moon was clearly visible in this eclipse, with 32% of the Moon in shadow; the partial eclipse lasted for 2 hours and 1 minute. 		   
25 Feb, 1381 BC
max: 05:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 1)
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 41 minutes. 		   
25 Mar, 1381 BC
max: 16:50 UT
Penumbral Lunar Eclipse
(penum. mag. 0.07; Saros 39)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 7% of the Moon's disc for 1 hour and 19 minutes, which was essentially impossible to see.
20 Aug, 1381 BC
max: 18:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 6)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 42 minutes, just 59% of the Moon's disc was in partial shadow (with no part of it in complete shadow).