Lunar Eclipses in Saros Series 141

This page lists all the lunar eclipses in saros series 141. The series contains 72 eclipses, occurring over 1280 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).
25 Aug, 1608 AD
max: 19:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.01; Saros 141)
In this virtually non-existant eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow; although the eclipse lasted 21 minutes and 6 seconds, it was impossible to see in practice.
6 Sep, 1626 AD
max: 03:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.10; Saros 141)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 10% of the Moon's disc for 1 hour and 26 minutes, which was essentially impossible to see.
16 Sep, 1644 AD
max: 10:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.19; Saros 141)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 19% of the Moon's disc for 1 hour and 55 minutes, which was essentially impossible to see.
27 Sep, 1662 AD
max: 18:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.26; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 16 minutes, just 26% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
8 Oct, 1680 AD
max: 03:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.33; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 31 minutes, just 33% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
19 Oct, 1698 AD
max: 11:20 UT
Penumbral Lunar Eclipse
(penum. mag. 0.38; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 42 minutes, just 38% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
30 Oct, 1716 AD
max: 19:42 UT
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 50 minutes, just 42% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
11 Nov, 1734 AD
max: 04:10 UT
Penumbral Lunar Eclipse
(penum. mag. 0.45; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 56 minutes, just 45% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
21 Nov, 1752 AD
max: 12:43 UT
Penumbral Lunar Eclipse
(penum. mag. 0.47; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 1 minute, just 47% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
2 Dec, 1770 AD
max: 21:22 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 3 minutes, just 48% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
13 Dec, 1788 AD
max: 06:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 5 minutes, just 49% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
25 Dec, 1806 AD
max: 14:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 6 minutes, just 49% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
4 Jan, 1825 AD
max: 23:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 7 minutes, just 49% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
16 Jan, 1843 AD
max: 08:14 UT
Penumbral Lunar Eclipse
(penum. mag. 0.50; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 8 minutes, just 50% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
26 Jan, 1861 AD
max: 16:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.50; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 9 minutes, just 50% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
7 Feb, 1879 AD
max: 01:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.51; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 11 minutes, just 51% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
17 Feb, 1897 AD
max: 09:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.53; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 15 minutes, just 53% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
1 Mar, 1915 AD
max: 18:19 UT
Penumbral Lunar Eclipse
(penum. mag. 0.55; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 20 minutes, just 55% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
12 Mar, 1933 AD
max: 02:32 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 141)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 26 minutes, just 59% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
23 Mar, 1951 AD
max: 10:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.64; Saros 141)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 64% 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 34 minutes.
2 Apr, 1969 AD
max: 18:32 UT
Penumbral Lunar Eclipse
(penum. mag. 0.70; Saros 141)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 70% 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 44 minutes.
14 Apr, 1987 AD
max: 02:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.78; Saros 141)
This subtle penumbral eclipse 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 54 minutes.
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.
5 May, 2023 AD
15:14–19:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 141)
The Moon will approach within 5% of the Earth's umbral shadow at maximum eclipse, with the overall eclipse lasting 4 hours and 18 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 from most of Europe, Africa, Asia and Australia.
16 May, 2041 AD
max: 00:41 UT
Partial Lunar Eclipse
(umbral mag. 0.06; Saros 141)
A tiny bite out of the Moon may be visible at maximum, though just 6% of the Moon will be shadowed in a partial eclipse lasting for 58 minutes and 30 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
27 May, 2059 AD
max: 07:53 UT
Partial Lunar Eclipse
(umbral mag. 0.18; Saros 141)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 37 minutes, with just 18% of the Moon in shadow at maximum.
6 Jun, 2077 AD
max: 14:57 UT
Partial Lunar Eclipse
(umbral mag. 0.31; Saros 141)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 31% of the Moon in shadow; the partial eclipse will last for 2 hours and 5 minutes.
17 Jun, 2095 AD
max: 21:56 UT
Partial Lunar Eclipse
(umbral mag. 0.45; Saros 141)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 45% of the Moon in shadow; the partial eclipse will last for 2 hours and 27 minutes.
29 Jun, 2113 AD
max: 04:51 UT
Partial Lunar Eclipse
(umbral mag. 0.58; Saros 141)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 58% of the Moon in shadow; the partial eclipse will last for 2 hours and 45 minutes.
10 Jul, 2131 AD
max: 11:43 UT
Partial Lunar Eclipse
(umbral mag. 0.73; Saros 141)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours exactly, with 73% of the Moon in darkness at maximum.
20 Jul, 2149 AD
max: 18:32 UT
Partial Lunar Eclipse
(umbral mag. 0.87; Saros 141)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 13 minutes, with 87% of the Moon in darkness at maximum.
1 Aug, 2167 AD
max: 01:22 UT
Total Lunar Eclipse
(umbral mag. 1.01; Saros 141)
The Moon will barely edge into total eclipse for just 16 minutes and 36 seconds. With the Moon just 1% 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 24 minutes in total.
11 Aug, 2185 AD
max: 08:14 UT
Total Lunar Eclipse
(umbral mag. 1.15; Saros 141)
A shallow total eclipse will see the Moon in relative darkness for 59 minutes and 18 seconds. The Moon will be 15% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 32 minutes in total.
23 Aug, 2203 AD
max: 15:07 UT
Total Lunar Eclipse
(umbral mag. 1.28; Saros 141)
The Moon will be plunged into darkness for 1 hour and 18 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. The partial eclipse will last for 3 hours and 39 minutes in total.
2 Sep, 2221 AD
max: 22:05 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 141)
The Moon will be plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which will see the Moon 40% 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 44 minutes in total.
14 Sep, 2239 AD
max: 05:08 UT
Total Lunar Eclipse
(umbral mag. 1.52; Saros 141)
The Moon will be plunged into darkness for 1 hour and 37 minutes, in a deep total eclipse which will see the Moon 52% 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 47 minutes in total.
24 Sep, 2257 AD
max: 12:17 UT
Total Lunar Eclipse
(umbral mag. 1.62; Saros 141)
A dramatic total eclipse lasting 1 hour and 41 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 49 minutes in total.
5 Oct, 2275 AD
max: 19:33 UT
Total Lunar Eclipse
(umbral mag. 1.72; Saros 141)
A dramatic total eclipse lasting 1 hour and 44 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 51 minutes in total.
16 Oct, 2293 AD
max: 02:56 UT
Total Lunar Eclipse
(umbral mag. 1.80; Saros 141)
A dramatic total eclipse lasting 1 hour and 45 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 52 minutes in total.
28 Oct, 2311 AD
max: 10:27 UT
Total Lunar Eclipse
(umbral mag. 1.78; Saros 141)
A dramatic total eclipse lasting 1 hour and 45 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 52 minutes in total.
7 Nov, 2329 AD
max: 18:05 UT
Total Lunar Eclipse
(umbral mag. 1.71; Saros 141)
A dramatic total eclipse lasting 1 hour and 44 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 52 minutes in total.
19 Nov, 2347 AD
max: 01:50 UT
Total Lunar Eclipse
(umbral mag. 1.67; Saros 141)
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. The partial eclipse will last for 3 hours and 52 minutes in total.
29 Nov, 2365 AD
max: 09:41 UT
Total Lunar Eclipse
(umbral mag. 1.63; Saros 141)
A dramatic total eclipse lasting 1 hour and 42 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 52 minutes in total.
10 Dec, 2383 AD
max: 17:39 UT
Total Lunar Eclipse
(umbral mag. 1.60; Saros 141)
A dramatic total eclipse lasting 1 hour and 41 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 52 minutes in total.
21 Dec, 2401 AD
max: 01:38 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 141)
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 51 minutes in total.
1 Jan, 2420 AD
max: 09:42 UT
Total Lunar Eclipse
(umbral mag. 1.55; Saros 141)
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 51 minutes in total.
11 Jan, 2438 AD
max: 17:45 UT
Total Lunar Eclipse
(umbral mag. 1.54; Saros 141)
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 51 minutes in total.
23 Jan, 2456 AD
max: 01:48 UT
Total Lunar Eclipse
(umbral mag. 1.52; Saros 141)
The Moon will be plunged into darkness for 1 hour and 38 minutes, in a deep total eclipse which will see the Moon 52% 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 51 minutes in total.
2 Feb, 2474 AD
max: 09:48 UT
Total Lunar Eclipse
(umbral mag. 1.50; Saros 141)
The Moon will be plunged into darkness for 1 hour and 37 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 51 minutes in total.
13 Feb, 2492 AD
max: 17:45 UT
Total Lunar Eclipse
(umbral mag. 1.48; Saros 141)
The Moon will be plunged into darkness for 1 hour and 36 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 51 minutes in total.
25 Feb, 2510 AD
max: 01:36 UT
Total Lunar Eclipse
(umbral mag. 1.44; Saros 141)
The Moon will be plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 50 minutes in total.
7 Mar, 2528 AD
max: 09:20 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 141)
The Moon will be plunged into darkness for 1 hour and 31 minutes, in a deep total eclipse which will see the Moon 40% 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 49 minutes in total.
18 Mar, 2546 AD
max: 16:56 UT
Total Lunar Eclipse
(umbral mag. 1.35; Saros 141)
The Moon will be plunged into darkness for 1 hour and 26 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. The partial eclipse will last for 3 hours and 48 minutes in total.
29 Mar, 2564 AD
max: 00:24 UT
Total Lunar Eclipse
(umbral mag. 1.28; Saros 141)
The Moon will be plunged into darkness for 1 hour and 20 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. The partial eclipse will last for 3 hours and 45 minutes in total.
9 Apr, 2582 AD
max: 07:43 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 141)
The Moon will be plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which will see the Moon 20% 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 42 minutes in total.
20 Apr, 2600 AD
max: 14:53 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 141)
A shallow total eclipse will see the Moon in relative darkness for 53 minutes and 12 seconds. The Moon will be 11% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 37 minutes in total.
1 May, 2618 AD
max: 21:54 UT
Total Lunar Eclipse
(umbral mag. 1.00; Saros 141)
The Moon will barely edge into total eclipse for just 11 minutes and 36 seconds. With the Moon just barely inside 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 31 minutes in total.
12 May, 2636 AD
max: 04:48 UT
Partial Lunar Eclipse
(umbral mag. 0.89; Saros 141)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 23 minutes, with 89% of the Moon in darkness at maximum.
23 May, 2654 AD
max: 11:32 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 141)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 12 minutes, with 76% of the Moon in darkness at maximum.
2 Jun, 2672 AD
max: 18:12 UT
Partial Lunar Eclipse
(umbral mag. 0.62; Saros 141)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 58 minutes, with 62% of the Moon in darkness at maximum.
14 Jun, 2690 AD
max: 00:45 UT
Partial Lunar Eclipse
(umbral mag. 0.48; Saros 141)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 48% of the Moon in shadow; the partial eclipse will last for 2 hours and 39 minutes.
25 Jun, 2708 AD
max: 07:15 UT
Partial Lunar Eclipse
(umbral mag. 0.33; Saros 141)
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 15 minutes.
6 Jul, 2726 AD
max: 13:42 UT
Partial Lunar Eclipse
(umbral mag. 0.17; Saros 141)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 40 minutes, with just 17% of the Moon in shadow at maximum.
16 Jul, 2744 AD
max: 20:10 UT
Partial Lunar Eclipse
(umbral mag. 0.02; Saros 141)
A tiny bite out of the Moon may be visible at maximum, though just 2% of the Moon will be shadowed in a partial eclipse lasting for 34 minutes and 54 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
28 Jul, 2762 AD
max: 02:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros 141)
At maximum eclipse, 93% 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 33 minutes overall.
7 Aug, 2780 AD
max: 09:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.78; Saros 141)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 78% 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 14 minutes.
18 Aug, 2798 AD
max: 15:40 UT
Penumbral Lunar Eclipse
(penum. mag. 0.63; Saros 141)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 63% 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 51 minutes.
28 Aug, 2816 AD
max: 22:20 UT
Penumbral Lunar Eclipse
(penum. mag. 0.50; Saros 141)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 27 minutes, just 50% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
9 Sep, 2834 AD
max: 05:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.37; Saros 141)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 1 minute, just 37% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
19 Sep, 2852 AD
max: 11:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.25; Saros 141)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 31 minutes, just 25% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
30 Sep, 2870 AD
max: 19:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 141)
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 15% of the Moon's disc for 1 hour and 57 minutes, which will be essentially impossible to see.
11 Oct, 2888 AD
max: 02:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 141)
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 6% of the Moon's disc for 1 hour and 13 minutes, which will be essentially impossible to see.