Lunar Eclipses in Saros Series 137

This page lists all the lunar eclipses in saros series 137. The series contains 78 eclipses, occurring over 1389 years.

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. Note that we only have mapping data for eclipses from year 1 AD, so any eclipses prior to that date will be missing. 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).
17 Dec, 1564 AD
max: 21:14 UT
Penumbral Lunar Eclipse
(penum. mag. 0.01; Saros 137)
In this virtually non-existant eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow; although the eclipse lasted 23 minutes exactly, it was impossible to see in practice.
8 Jan, 1583 AD
max: 05:52 UT
Penumbral Lunar Eclipse
(penum. mag. 0.02; Saros 137)
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 38 minutes and 24 seconds, which was essentially impossible to see.
18 Jan, 1601 AD
max: 14:30 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 137)
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 54 seconds, which was essentially impossible to see.
29 Jan, 1619 AD
max: 23:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.05; Saros 137)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 5% of the Moon's disc for 1 hour and 4 minutes, which was essentially impossible to see.
9 Feb, 1637 AD
max: 07:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 137)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 8% of the Moon's disc for 1 hour and 17 minutes, which was essentially impossible to see.
20 Feb, 1655 AD
max: 16:03 UT
Penumbral Lunar Eclipse
(penum. mag. 0.11; Saros 137)
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 32 minutes, which was essentially impossible to see.
3 Mar, 1673 AD
max: 00:23 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 137)
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 47 minutes, which was essentially impossible to see.
14 Mar, 1691 AD
max: 08:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros 137)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 4 minutes, just 21% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
25 Mar, 1709 AD
max: 16:43 UT
Penumbral Lunar Eclipse
(penum. mag. 0.27; Saros 137)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 20 minutes, just 27% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
6 Apr, 1727 AD
max: 00:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.35; Saros 137)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 37 minutes, just 35% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
16 Apr, 1745 AD
max: 08:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.44; Saros 137)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 54 minutes, just 44% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
27 Apr, 1763 AD
max: 16:20 UT
Penumbral Lunar Eclipse
(penum. mag. 0.54; Saros 137)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 10 minutes, just 54% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
8 May, 1781 AD
max: 00:00 UT
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 137)
This subtle penumbral eclipse 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 26 minutes.
19 May, 1799 AD
max: 07:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 137)
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 40 minutes.
30 May, 1817 AD
max: 15:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 137)
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 3 hours and 54 minutes overall.
10 Jun, 1835 AD
max: 22:35 UT
Partial Lunar Eclipse
(umbral mag. 0.07; Saros 137)
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 56 minutes and 48 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
21 Jun, 1853 AD
max: 06:01 UT
Partial Lunar Eclipse
(umbral mag. 0.21; Saros 137)
The Earth's shadow on the moon was clearly visible in this eclipse, with 21% of the Moon in shadow; the partial eclipse lasted for 1 hour and 37 minutes.
2 Jul, 1871 AD
max: 13:27 UT
Partial Lunar Eclipse
(umbral mag. 0.34; Saros 137)
The Earth's shadow on the moon was clearly visible in this eclipse, with 34% of the Moon in shadow; the partial eclipse lasted for 2 hours and 2 minutes.
12 Jul, 1889 AD
max: 20:53 UT
Partial Lunar Eclipse
(umbral mag. 0.48; Saros 137)
The Earth's shadow on the moon was clearly visible in this eclipse, with 48% of the Moon in shadow; the partial eclipse lasted for 2 hours and 22 minutes.
25 Jul, 1907 AD
max: 04:22 UT
Partial Lunar Eclipse
(umbral mag. 0.61; Saros 137)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 37 minutes, with 61% of the Moon in darkness at maximum.
4 Aug, 1925 AD
max: 11:52 UT
Partial Lunar Eclipse
(umbral mag. 0.75; Saros 137)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 49 minutes, with 75% of the Moon in darkness at maximum.
15 Aug, 1943 AD
max: 19:28 UT
Partial Lunar Eclipse
(umbral mag. 0.87; Saros 137)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 58 minutes, with 87% of the Moon in darkness at maximum.
26 Aug, 1961 AD
max: 03:08 UT
Partial Lunar Eclipse
(umbral mag. 0.99; Saros 137)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 6 minutes. With 99% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
6 Sep, 1979 AD
max: 10:54 UT
Total Lunar Eclipse
(umbral mag. 1.09; Saros 137)
A shallow total eclipse saw the Moon in relative darkness for 44 minutes and 24 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 12 minutes in total.
16 Sep, 1997 AD
max: 18:46 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 137)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 2 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 16 minutes in total.
28 Sep, 2015 AD
00:11–05:22 UT
Total Lunar Eclipse
(umbral mag. 1.28; Saros 137)
The Moon will be plunged into darkness for 1 hour and 12 minutes, in a deep total eclipse which will see 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 be stained a deep red colour for observers from the Americas, Europe and Africa. The partial eclipse will last for 3 hours and 20 minutes in total.
8 Oct, 2033 AD
08:18–13:31 UT
Total Lunar Eclipse
(umbral mag. 1.35; Saros 137)
The Moon will be plunged into darkness for 1 hour and 19 minutes, in a deep total eclipse which will see the Moon 35% 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 in east Asia, Australia, New Zealand, North and Central America, and north-western South America. The partial eclipse will last for 3 hours and 22 minutes in total.
19 Oct, 2051 AD
max: 19:10 UT
Total Lunar Eclipse
(umbral mag. 1.41; Saros 137)
The Moon will be plunged into darkness for 1 hour and 24 minutes, in a deep total eclipse which will see the Moon 41% 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.
30 Oct, 2069 AD
max: 03:32 UT
Total Lunar Eclipse
(umbral mag. 1.46; Saros 137)
The Moon will be plunged into darkness for 1 hour and 27 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 26 minutes in total.
10 Nov, 2087 AD
max: 12:02 UT
Total Lunar Eclipse
(umbral mag. 1.50; Saros 137)
The Moon will be plunged into darkness for 1 hour and 29 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 27 minutes in total.
21 Nov, 2105 AD
max: 20:38 UT
Total Lunar Eclipse
(umbral mag. 1.53; Saros 137)
The Moon will be plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 27 minutes in total.
3 Dec, 2123 AD
max: 05:19 UT
Total Lunar Eclipse
(umbral mag. 1.55; Saros 137)
The Moon will be plunged into darkness for 1 hour and 31 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 28 minutes in total.
13 Dec, 2141 AD
max: 14:05 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 137)
The Moon will be plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which will see the Moon 57% 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 28 minutes in total.
24 Dec, 2159 AD
max: 22:54 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 137)
The Moon will be plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which will see the Moon 57% 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 28 minutes in total.
4 Jan, 2178 AD
max: 07:43 UT
Total Lunar Eclipse
(umbral mag. 1.58; Saros 137)
The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see the Moon 58% 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 29 minutes in total.
15 Jan, 2196 AD
max: 16:34 UT
Total Lunar Eclipse
(umbral mag. 1.59; Saros 137)
The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see the Moon 59% 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 29 minutes in total.
27 Jan, 2214 AD
max: 01:22 UT
Total Lunar Eclipse
(umbral mag. 1.60; Saros 137)
A dramatic total eclipse lasting 1 hour and 34 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 30 minutes in total.
7 Feb, 2232 AD
max: 10:09 UT
Total Lunar Eclipse
(umbral mag. 1.61; Saros 137)
A dramatic total eclipse lasting 1 hour and 34 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 30 minutes in total.
17 Feb, 2250 AD
max: 18:49 UT
Total Lunar Eclipse
(umbral mag. 1.63; Saros 137)
A dramatic total eclipse lasting 1 hour and 35 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 31 minutes in total.
29 Feb, 2268 AD
max: 03:25 UT
Total Lunar Eclipse
(umbral mag. 1.66; Saros 137)
A dramatic total eclipse lasting 1 hour and 36 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 31 minutes in total.
11 Mar, 2286 AD
max: 11:53 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 137)
A dramatic total eclipse lasting 1 hour and 37 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.
22 Mar, 2304 AD
max: 20:14 UT
Total Lunar Eclipse
(umbral mag. 1.75; Saros 137)
A dramatic total eclipse lasting 1 hour and 38 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 33 minutes in total.
3 Apr, 2322 AD
max: 04:26 UT
Total Lunar Eclipse
(umbral mag. 1.81; Saros 137)
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 34 minutes in total.
13 Apr, 2340 AD
max: 12:31 UT
Total Lunar Eclipse
(umbral mag. 1.86; Saros 137)
A dramatic total eclipse lasting 1 hour and 40 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 35 minutes in total.
24 Apr, 2358 AD
max: 20:26 UT
Total Lunar Eclipse
(umbral mag. 1.77; Saros 137)
A dramatic total eclipse lasting 1 hour and 40 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 35 minutes in total.
5 May, 2376 AD
max: 04:13 UT
Total Lunar Eclipse
(umbral mag. 1.67; Saros 137)
A dramatic total eclipse lasting 1 hour and 38 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 34 minutes in total.
16 May, 2394 AD
max: 11:52 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 137)
The Moon will be plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which will see the Moon 57% 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 33 minutes in total.
26 May, 2412 AD
max: 19:25 UT
Total Lunar Eclipse
(umbral mag. 1.45; Saros 137)
The Moon will be plunged into darkness for 1 hour and 28 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 31 minutes in total.
7 Jun, 2430 AD
max: 02:50 UT
Total Lunar Eclipse
(umbral mag. 1.32; Saros 137)
The Moon will be plunged into darkness for 1 hour and 18 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 28 minutes in total.
17 Jun, 2448 AD
max: 10:09 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 137)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 3 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 23 minutes in total.
28 Jun, 2466 AD
max: 17:24 UT
Total Lunar Eclipse
(umbral mag. 1.04; Saros 137)
The Moon will barely edge into total eclipse for 32 minutes and 12 seconds. With the Moon just 4% 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 16 minutes in total.
9 Jul, 2484 AD
max: 00:37 UT
Partial Lunar Eclipse
(umbral mag. 0.90; Saros 137)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 8 minutes. With 90% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
21 Jul, 2502 AD
max: 07:46 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 137)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 57 minutes, with 76% of the Moon in darkness at maximum.
31 Jul, 2520 AD
max: 14:56 UT
Partial Lunar Eclipse
(umbral mag. 0.61; Saros 137)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 43 minutes, with 61% of the Moon in darkness at maximum.
11 Aug, 2538 AD
max: 22:06 UT
Partial Lunar Eclipse
(umbral mag. 0.47; Saros 137)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 47% of the Moon in shadow; the partial eclipse will last for 2 hours and 27 minutes.
22 Aug, 2556 AD
max: 05:19 UT
Partial Lunar Eclipse
(umbral mag. 0.33; Saros 137)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 33% of the Moon in shadow; the partial eclipse will last for 2 hours and 7 minutes.
2 Sep, 2574 AD
max: 12:33 UT
Partial Lunar Eclipse
(umbral mag. 0.20; Saros 137)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 20% of the Moon in shadow; the partial eclipse will last for 1 hour and 41 minutes.
12 Sep, 2592 AD
max: 19:53 UT
Partial Lunar Eclipse
(umbral mag. 0.08; Saros 137)
A tiny bite out of the Moon may be visible at maximum, though just 8% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 4 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
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, 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.
5 Oct, 2628 AD
max: 10:48 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 137)
At maximum eclipse, 88% 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 11 minutes overall.
16 Oct, 2646 AD
max: 18:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.80; Saros 137)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 80% 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 1 minute.
27 Oct, 2664 AD
max: 02:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 137)
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 53 minutes.
7 Nov, 2682 AD
max: 09:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.66; Saros 137)
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 45 minutes.
18 Nov, 2700 AD
max: 17:54 UT
Penumbral Lunar Eclipse
(penum. mag. 0.61; Saros 137)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 61% 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 38 minutes.
30 Nov, 2718 AD
max: 01:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.57; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 33 minutes, just 57% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
10 Dec, 2736 AD
max: 10:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.54; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 28 minutes, just 54% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
21 Dec, 2754 AD
max: 18:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.51; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 24 minutes, just 51% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
1 Jan, 2773 AD
max: 02:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 21 minutes, just 49% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
12 Jan, 2791 AD
max: 10:48 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 19 minutes, just 48% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
22 Jan, 2809 AD
max: 19:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.46; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 16 minutes, just 46% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
3 Feb, 2827 AD
max: 03:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.44; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 13 minutes, just 44% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
13 Feb, 2845 AD
max: 11:29 UT
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 9 minutes, just 42% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
24 Feb, 2863 AD
max: 19:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.39; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 3 minutes, just 39% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
7 Mar, 2881 AD
max: 03:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.35; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 55 minutes, just 35% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
18 Mar, 2899 AD
max: 11:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 43 minutes, just 30% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
29 Mar, 2917 AD
max: 19:08 UT
Penumbral Lunar Eclipse
(penum. mag. 0.24; Saros 137)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 27 minutes, just 24% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
10 Apr, 2935 AD
max: 02:42 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 137)
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 17% of the Moon's disc for 2 hours and 3 minutes, which will be essentially impossible to see.
20 Apr, 2953 AD
max: 10:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 137)
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 8% of the Moon's disc for 1 hour and 26 minutes, which will be essentially impossible to see.