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, 2001–2020 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 Jan, 2001 AD
17:45–22:56 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 1 minute. The Moon was 19% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers over all of Europe, Africa, and Asia. The partial eclipse lasted for 3 hours and 16 minutes in total and was visible in parts of north-eastern North America and Australia.
5 Jul, 2001 AD
12:12–17:37 UT
Partial Lunar Eclipse
(umbral mag. 0.49; Saros 139)
The Earth's shadow on the moon was clearly visible in this eclipse, with 49% of the Moon in shadow; the partial eclipse lasted for 2 hours and 39 minutes and was visible over all of Australia, Indonesia, and south-east Asia.
30 Dec, 2001 AD
08:27–12:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 144)
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 4 minutes overall, and was visible from the Americas, Asia and Australasia.
26 May, 2002 AD
10:15–13:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 111)
This subtle penumbral eclipse 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 37 minutes. The Moon was visible from the western Americas, east Asia and Australasia.
24 Jun, 2002 AD
20:22–22:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros 149)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 9 minutes, just 21% of the Moon's disc was in partial shadow (with no part of it in complete shadow). The full Moon itself was visible from South America, Europe, Africa, south Asia, and Australia.
20 Nov, 2002 AD
23:34 on 19 Nov–03:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.86; Saros 116)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 86% 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. The Moon was visible from the Americas, Europe, Africa, and most of Asia.
16 May, 2003 AD
01:06–06:13 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 121)
A shallow total eclipse saw the Moon in relative darkness for 51 minutes and 24 seconds. The Moon was 13% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers over the Americas, Europe, and Africa. The partial eclipse lasted for 3 hours and 14 minutes in total.
9 Nov, 2003 AD
22:16 on 8 Nov–04:20 UT
Total Lunar Eclipse
(umbral mag. 1.02; Saros 126)
The Moon barely edged into total eclipse for 22 minutes exactly. 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 for observers over the Americas, Europe, Asia, and Africa. The partial eclipse lasted for 3 hours and 31 minutes in total.
4 May, 2004 AD
17:52–23:08 UT
Total Lunar Eclipse
(umbral mag. 1.30; Saros 131)
The Moon was plunged into darkness for 1 hour and 16 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour for observers over South America, Europe, Asia, Australia, and Africa. The partial eclipse lasted for 3 hours and 23 minutes in total.
28 Oct, 2004 AD
00:07–06:01 UT
Total Lunar Eclipse
(umbral mag. 1.31; Saros 136)
The Moon was plunged into darkness for 1 hour and 21 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour for observers over the Americas, Europe, Africa, and parts of Asia. The partial eclipse lasted for 3 hours and 39 minutes in total.
24 Apr, 2005 AD
07:52–11:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 141)
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 4 hours and 6 minutes overall, and was visible from east Asia, Australia, and the Americas.
17 Oct, 2005 AD
09:53–14:13 UT
Partial Lunar Eclipse
(umbral mag. 0.06; Saros 146)
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 56 minutes exactly and was visible over east Asia, Australasia, and most of North America. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
14 Mar, 2006 AD
21:23 on 14 Mar–02:11 on 15 Mar UT
Penumbral Lunar Eclipse
(penum. mag. 1.03; Saros 113)
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 to viewers over Asia (the beginning of the eclipse); Europe, Africa and west Asia (the whole eclipse); and the Americas barring western Canada and Alaska (the end of the eclipse). The penumbral phase lasted for 4 hours and 48 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
7 Sep, 2006 AD
16:44–20:58 UT
Partial Lunar Eclipse
(umbral mag. 0.18; Saros 118)
At maximum eclipse, a small bite out of the Moon should have been visible over Europe, Africa, Asia, and Australasia. The eclipse lasted for 1 hour and 31 minutes, with just 18% of the Moon in shadow at maximum.
3 Mar, 2007 AD
20:18 on 3 Mar–02:23 on 4 Mar UT
Total Lunar Eclipse
(umbral mag. 1.23; Saros 123)
The Moon was plunged into darkness for 1 hour and 13 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 for observers over the eastern Americas, Europe, Africa, and western Asia. The partial eclipse lasted for 3 hours and 41 minutes in total.
28 Aug, 2007 AD
07:53–13:20 UT
Total Lunar Eclipse
(umbral mag. 1.48; Saros 128)
The Moon was plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which saw the Moon 48% 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 for observers over the Americas, the Pacific, eastern Asia, and Australasia. The partial eclipse lasted for 3 hours and 32 minutes in total.
21 Feb, 2008 AD
00:36–06:15 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 133)
A shallow total eclipse saw the Moon in relative darkness for 49 minutes and 48 seconds. The Moon was 11% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers over the Americas, Europe, Africa, and western Asia. The partial eclipse lasted for 3 hours and 25 minutes in total.
16 Aug, 2008 AD
18:24–23:55 UT
Partial Lunar Eclipse
(umbral mag. 0.81; Saros 138)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 8 minutes, with 81% of the Moon in darkness at maximum. The eclipse was visible over most of Asia, Australasia, Europe, Africa, and south America.
9 Feb, 2009 AD
12:38–16:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 143)
At maximum eclipse, 90% 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, and was visible from eastern Europe and Africa, Asia, and most of North America.
7 Jul, 2009 AD
08:37–10:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros 110)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 16% of the Moon's disc for 2 hours and 2 minutes, which was essentially impossible to see. The full Moon itself was visible from the far East, Australia, the Pacific, South America, and most of North America.
6 Aug, 2009 AD
23:04 on 5 Aug–02:14 UT
Penumbral Lunar Eclipse
(penum. mag. 0.40; Saros 148)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 10 minutes, just 40% of the Moon's disc was in partial shadow (with no part of it in complete shadow). The full Moon itself was visible from south-east North America, South America, Europe, Africa, and west Asia.
31 Dec, 2009 AD
17:17–21:28 UT
Partial Lunar Eclipse
(umbral mag. 0.08; Saros 115)
A tiny bite out of the Moon may have been visible at maximum, though just 8% of the Moon was shadowed in a partial eclipse which lasted for 1 hour exactly and was visible over Asia, Australasia, Europe, and Africa. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
26 Jun, 2010 AD
08:57–14:19 UT
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 120)
The Earth's shadow on the moon was clearly visible in this eclipse, with 54% of the Moon in shadow; the partial eclipse lasted for 2 hours and 43 minutes and was visible over eastern Asia, Australasia, the Pacific, and (partially) the Americas.
21 Dec, 2010 AD
05:29–11:04 UT
Total Lunar Eclipse
(umbral mag. 1.26; Saros 125)
The Moon was plunged into darkness for 1 hour and 12 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 for observers over eastern Asia, Australasia, northwestern Europe and Africa, and the Americas. The partial eclipse lasted for 3 hours and 29 minutes in total.
15 Jun, 2011 AD
17:24–23:00 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 130)
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 from Europe, Africa, southern Asia, and Australia. The partial eclipse lasted for 3 hours and 39 minutes in total.
10 Dec, 2011 AD
11:33–17:29 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 135)
A shallow total eclipse saw the Moon in relative darkness for 51 minutes and 6 seconds. The Moon was 11% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers from North America (the beginning of the eclipse); eastern Asia and Australia; andmost of Europe and Africa (the end of the eclipse). The partial eclipse lasted for 3 hours and 32 minutes in total.
4 Jun, 2012 AD
08:48–13:18 UT
Partial Lunar Eclipse
(umbral mag. 0.37; Saros 140)
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 7 minutes and was visible from the Americas, the Pacific, south-east Asia and Australia.
28 Nov, 2012 AD
12:14–16:50 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 145)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 92% 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 36 minutes. The Moon was visible from North America (the beginning of the eclipse), Asia and Australia, and most of Europe and Africa (the end of the eclipse).
25 Apr, 2013 AD
18:03–22:11 UT
Partial Lunar Eclipse
(umbral mag. 0.01; Saros 112)
A tiny bite out of the Moon may have been visible at maximum, though just 1% of the Moon was shadowed in a partial eclipse which lasted for 27 minutes exactly and was visible from most of Asia, Australia, Europe and Africa. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
25 May, 2013 AD
03:53–04:26 UT
Penumbral Lunar Eclipse
(penum. mag. 0.02; Saros 150)
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 33 minutes and 36 seconds, which was essentially impossible to see. The full Moon itself was visible from the Americas, western Africa, and south-west Europe.
18 Oct, 2013 AD
21:50 on 18 Oct–01:49 on 19 Oct UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 117)
This subtle penumbral eclipse 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 59 minutes. The Moon was visible from the Americas (for the end), Europe, Africa, and most of Asia (the beginning of the eclipse will be visible in east Asia).
15 Apr, 2014 AD
04:53–10:37 UT
Total Lunar Eclipse
(umbral mag. 1.29; Saros 122)
The Moon was plunged into darkness for 1 hour and 18 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour for observers from the Americas. The partial eclipse lasted for 3 hours and 35 minutes in total.
8 Oct, 2014 AD
08:15–13:33 UT
Total Lunar Eclipse
(umbral mag. 1.17; Saros 127)
A shallow total eclipse saw the Moon in relative darkness for 58 minutes and 48 seconds. The Moon was 17% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers from east Asia and North America, with the beginning visible from most of South America. The partial eclipse lasted for 3 hours and 20 minutes in total.
4 Apr, 2015 AD
09:01–14:58 UT
Total Lunar Eclipse
(umbral mag. 1.00; Saros 132)
The Moon barely edged into total eclipse for a very brief 4 minutes and 42 seconds. With the Moon just barely inside the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing for observers from east Asia, Australia, and western North America. The partial eclipse lasted for 3 hours and 29 minutes in total and was visible from most of Asia, Australia, and the Americas.
28 Sep, 2015 AD
00:11–05:22 UT
Total Lunar Eclipse
(umbral mag. 1.28; Saros 137)
The Moon was plunged into darkness for 1 hour and 12 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour for observers from the Americas, Europe and Africa. The partial eclipse lasted for 3 hours and 20 minutes in total.
23 Mar, 2016 AD
09:39–13:54 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 142)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 77% 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 15 minutes. The Moon was visible from east Asia, Australia, and most of the Americas.
16 Sep, 2016 AD
16:54–20:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.91; Saros 147)
At maximum eclipse, 91% 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, and was visible from Europe, Afica, Asia and Australia.
11 Feb, 2017 AD
22:34 on 10 Feb–02:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.99; Saros 114)
The Moon approached within 4% 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 19 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 from the Americas, Europe, Africa, and most of Asia.
7 Aug, 2017 AD
15:50–20:50 UT
Partial Lunar Eclipse
(umbral mag. 0.25; Saros 119)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 25% of the Moon in shadow; the partial eclipse will last for 1 hour and 55 minutes and will be visible from Europe, Africa, most of Asia, and Australia.
31 Jan, 2018 AD
10:51–16:08 UT
Total Lunar Eclipse
(umbral mag. 1.32; Saros 124)
The Moon will be plunged into darkness for 1 hour and 16 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 for observers from Asia, Australia, and North America. The partial eclipse will last for 3 hours and 23 minutes in total.
27 Jul, 2018 AD
17:14–23:28 UT
Total Lunar Eclipse
(umbral mag. 1.61; Saros 129)
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 from Europe, Africa, Asia, and Australia. The partial eclipse will last for 3 hours and 55 minutes in total.
21 Jan, 2019 AD
02:36–07:48 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 134)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 2 minutes. The Moon will be 20% of its diameter into the Earth's umbral shadow, and should be significantly darkened for viewers from the Americas, Europe, and most of Africa. The partial eclipse will last for 3 hours and 17 minutes in total.
16 Jul, 2019 AD
18:43 on 16 Jul–00:17 on 17 Jul UT
Partial Lunar Eclipse
(umbral mag. 0.65; Saros 139)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 58 minutes, with 65% of the Moon in darkness at maximum. The eclipse will be visible from South America, Europe, Africa, south Asia, and Australia.
10 Jan, 2020 AD
17:07–21:12 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 144)
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 5 minutes overall, and will be visible from Africa, Europe, Asia, Alaska, and Australia.
5 Jun, 2020 AD
17:45–21:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.57; Saros 111)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 18 minutes, just 57% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). The full Moon itself will be visible from southern Europe, Africa, south Asia, and Australia.
5 Jul, 2020 AD
03:07–05:52 UT
Penumbral Lunar Eclipse
(penum. mag. 0.35; Saros 149)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 45 minutes, just 35% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). The full Moon itself will be visible from the Americas, south-west Europe, and western Africa.
30 Nov, 2020 AD
07:32–11:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 116)
This subtle penumbral eclipse 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. The Moon will be visible from east Asia, Australia, and the Americas.