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, 1540–1521 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).
14 Mar, 1540 BC
max: 01:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros -2)
At maximum eclipse, 89% 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 7 minutes overall.
   
7 Sep, 1540 BC
max: 15:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 3)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 89% 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 24 minutes.
   
3 Mar, 1539 BC
max: 14:56 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 8)
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 23 minutes in total.
   
27 Aug, 1539 BC
max: 15:57 UT
Total Lunar Eclipse
(umbral mag. 1.09; Saros 13)
A shallow total eclipse saw the Moon in relative darkness for 47 minutes and 36 seconds. The Moon was 9% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 36 minutes in total.
   
21 Feb, 1538 BC
max: 07:32 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 18)
A shallow total eclipse saw the Moon in relative darkness for 51 minutes and 36 seconds. The Moon was 13% 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.
   
16 Aug, 1538 BC
max: 16:31 UT
Total Lunar Eclipse
(umbral mag. 1.22; Saros 23)
The Moon was plunged into darkness for 1 hour and 12 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 39 minutes in total.
   
10 Feb, 1537 BC
max: 22:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 28)
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 3 hours and 46 minutes.
   
4 Aug, 1537 BC
max: 23:23 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 33)
At maximum eclipse, 95% 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 14 minutes overall.
   
31 Dec, 1537 BC
max: 14:17 UT
Partial Lunar Eclipse
(umbral mag. 0.03; Saros 0)
A tiny bite out of the Moon may have been visible at maximum, though just 3% of the Moon was shadowed in a partial eclipse which lasted for 43 minutes and 18 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
26 Jun, 1536 BC
max: 05:44 UT
Partial Lunar Eclipse
(umbral mag. 0.37; Saros 5)
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.
   
20 Dec, 1536 BC
max: 13:35 UT
Total Lunar Eclipse
(umbral mag. 1.27; Saros 10)
The Moon was plunged into darkness for 1 hour and 18 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 44 minutes in total.
   
15 Jun, 1535 BC
max: 22:38 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 15)
A dramatic total eclipse lasting 1 hour and 38 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.
   
9 Dec, 1535 BC
max: 15:14 UT
Total Lunar Eclipse
(umbral mag. 1.10; Saros 20)
A shallow total eclipse saw the Moon in relative darkness for 47 minutes and 54 seconds. 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 28 minutes in total.
   
5 Jun, 1534 BC
max: 11:41 UT
Partial Lunar Eclipse
(umbral mag. 0.59; Saros 25)
The Earth's shadow on the moon was clearly visible in this eclipse, with 59% of the Moon in shadow; the partial eclipse lasted for 2 hours and 44 minutes.
   
29 Nov, 1534 BC
max: 00:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 30)
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 4 hours and 6 minutes overall.
   
25 Apr, 1533 BC
max: 03:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros -3)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 28 minutes, just 49% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
24 May, 1533 BC
max: 17:43 UT
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 35)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 12% of the Moon's disc for 1 hour and 45 minutes, which was essentially impossible to see.
19 Oct, 1533 BC
max: 03:43 UT
Partial Lunar Eclipse
(umbral mag. 0.03; Saros 2)
A tiny bite out of the Moon may have been visible at maximum, though just 3% of the Moon was shadowed in a partial eclipse which lasted for 38 minutes exactly. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
14 Apr, 1532 BC
max: 04:12 UT
Partial Lunar Eclipse
(umbral mag. 0.83; Saros 7)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 15 minutes, with 83% of the Moon in darkness at maximum.
   
8 Oct, 1532 BC
max: 18:05 UT
Total Lunar Eclipse
(umbral mag. 1.22; Saros 12)
The Moon was plunged into darkness for 1 hour and 6 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 24 minutes in total.
   
3 Apr, 1531 BC
max: 10:05 UT
Total Lunar Eclipse
(umbral mag. 1.42; Saros 17)
The Moon was plunged into darkness for 1 hour and 29 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 37 minutes in total.
   
28 Sep, 1531 BC
max: 02:52 UT
Total Lunar Eclipse
(umbral mag. 1.15; Saros 22)
A shallow total eclipse saw the Moon in relative darkness for 1 hour exactly. 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 32 minutes in total.
   
23 Mar, 1530 BC
max: 22:56 UT
Partial Lunar Eclipse
(umbral mag. 0.11; Saros 27)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 11 minutes, with just 11% of the Moon in shadow at maximum.
   
17 Sep, 1530 BC
max: 04:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 32)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 90% 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 33 minutes.
   
12 Feb, 1529 BC
max: 07:14 UT
Partial Lunar Eclipse
(umbral mag. 0.20; Saros -1)
The Earth's shadow on the moon was clearly visible in this eclipse, with 20% of the Moon in shadow; the partial eclipse lasted for 1 hour and 36 minutes.
   
6 Aug, 1529 BC
max: 12:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 4)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 83% 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.
   
31 Jan, 1528 BC
max: 20:31 UT
Total Lunar Eclipse
(umbral mag. 1.45; Saros 9)
The Moon was plunged into darkness for 1 hour and 30 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 36 minutes in total.
   
26 Jul, 1528 BC
max: 22:01 UT
Total Lunar Eclipse
(umbral mag. 1.26; Saros 14)
The Moon was plunged into darkness for 1 hour and 13 minutes, in a deep total eclipse which saw the Moon 26% 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 27 minutes in total.
   
21 Jan, 1527 BC
max: 02:51 UT
Partial Lunar Eclipse
(umbral mag. 0.86; Saros 19)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 17 minutes, with 86% of the Moon in darkness at maximum.
   
16 Jul, 1527 BC
max: 13:10 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 24)
A shallow total eclipse saw the Moon in relative darkness for 51 minutes and 48 seconds. The Moon was 13% 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.
   
10 Jan, 1526 BC
max: 02:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 29)
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 59 minutes.
   
6 Jun, 1526 BC
max: 22:29 UT
Penumbral Lunar Eclipse
(penum. mag. 0.26; Saros -4)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 18 minutes, just 26% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
6 Jul, 1526 BC
max: 06:08 UT
Penumbral Lunar Eclipse
(penum. mag. 0.75; Saros 34)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 75% 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 38 minutes.
30 Nov, 1526 BC
max: 11:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 1)
At maximum eclipse, 95% 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 21 minutes overall.
   
26 May, 1525 BC
max: 09:48 UT
Partial Lunar Eclipse
(umbral mag. 0.57; Saros 6)
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.
   
18 Nov, 1525 BC
max: 22:22 UT
Total Lunar Eclipse
(umbral mag. 1.26; Saros 11)
The Moon was plunged into darkness for 1 hour and 11 minutes, in a deep total eclipse which saw the Moon 26% 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 23 minutes in total.
   
15 May, 1524 BC
max: 13:55 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 16)
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.
   
8 Nov, 1524 BC
max: 13:30 UT
Total Lunar Eclipse
(umbral mag. 1.25; Saros 21)
The Moon was plunged into darkness for 1 hour and 8 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 18 minutes in total.
   
4 May, 1523 BC
max: 14:34 UT
Partial Lunar Eclipse
(umbral mag. 0.30; Saros 26)
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 2 hours and 8 minutes.
   
29 Oct, 1523 BC
max: 04:27 UT
Penumbral Lunar Eclipse
(penum. mag. 0.98; Saros 31)
The Moon approached within 2% of the Earth's umbral shadow at maximum eclipse; 98% of the Moon's disc was partially shaded by the Earth, with the overall eclipse lasting 4 hours and 9 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.
   
25 Mar, 1522 BC
max: 08:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.79; Saros -2)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 79% 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.
   
23 Apr, 1522 BC
max: 19:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 36)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 3% of the Moon's disc for 50 minutes and 24 seconds, which was essentially impossible to see.
18 Sep, 1522 BC
max: 22:54 UT
Penumbral Lunar Eclipse
(penum. mag. 0.85; Saros 3)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 85% 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 19 minutes.
   
13 Mar, 1521 BC
max: 22:49 UT
Total Lunar Eclipse
(umbral mag. 1.23; Saros 8)
The Moon was plunged into darkness for 1 hour and 7 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 20 minutes in total.
   
6 Sep, 1521 BC
max: 23:24 UT
Total Lunar Eclipse
(umbral mag. 1.02; Saros 13)
The Moon barely edged into total eclipse for 22 minutes and 24 seconds. With the Moon just 2% 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 32 minutes in total.