Lunar Eclipses in Saros Series 118

This page lists all the lunar eclipses in saros series 118. The series contains 73 eclipses, occurring over 1298 years.

This series is partnered with solar Saros series 125.

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.

The interactive map is currently not available.

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).
2 Mar, 1105 AD
max: 16:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 118)
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 56 minutes and 18 seconds, which was essentially impossible to see.
   
13 Mar, 1123 AD
max: 23:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.11; Saros 118)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 11% of the Moon's disc for 1 hour and 41 minutes, which was essentially impossible to see.
   
24 Mar, 1141 AD
max: 06:50 UT
Penumbral Lunar Eclipse
(penum. mag. 0.20; Saros 118)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 14 minutes, just 20% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
4 Apr, 1159 AD
max: 14:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.31; Saros 118)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 43 minutes, just 31% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
14 Apr, 1177 AD
max: 21:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros 118)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 8 minutes, just 42% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
26 Apr, 1195 AD
max: 04:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.54; Saros 118)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 30 minutes, just 54% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
6 May, 1213 AD
max: 11:03 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 118)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 68% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 51 minutes.
   
17 May, 1231 AD
max: 17:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.82; Saros 118)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 82% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 9 minutes.
   
28 May, 1249 AD
max: 00:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 118)
At maximum eclipse, 97% 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 25 minutes overall.
   
8 Jun, 1267 AD
max: 07:35 UT
Partial Lunar Eclipse
(umbral mag. 0.09; Saros 118)
A tiny bite out of the Moon may have been visible at maximum, though just 9% of the Moon was shadowed in a partial eclipse which lasted for 1 hour and 11 minutes. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
18 Jun, 1285 AD
max: 14:27 UT
Partial Lunar Eclipse
(umbral mag. 0.25; Saros 118)
The Earth's shadow on the moon was clearly visible in this eclipse, with 25% of the Moon in shadow; the partial eclipse lasted for 1 hour and 53 minutes.
   
29 Jun, 1303 AD
max: 21:20 UT
Partial Lunar Eclipse
(umbral mag. 0.40; Saros 118)
The Earth's shadow on the moon was clearly visible in this eclipse, with 40% of the Moon in shadow; the partial eclipse lasted for 2 hours and 20 minutes.
   
10 Jul, 1321 AD
max: 04:17 UT
Partial Lunar Eclipse
(umbral mag. 0.55; Saros 118)
The Earth's shadow on the moon was clearly visible in this eclipse, with 55% of the Moon in shadow; the partial eclipse lasted for 2 hours and 40 minutes.
   
21 Jul, 1339 AD
max: 11:19 UT
Partial Lunar Eclipse
(umbral mag. 0.69; Saros 118)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 55 minutes, with 69% of the Moon in darkness at maximum.
   
31 Jul, 1357 AD
max: 18:29 UT
Partial Lunar Eclipse
(umbral mag. 0.82; Saros 118)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 6 minutes, with 82% of the Moon in darkness at maximum.
   
12 Aug, 1375 AD
max: 01:44 UT
Partial Lunar Eclipse
(umbral mag. 0.95; Saros 118)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 15 minutes. With 95% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
   
22 Aug, 1393 AD
max: 09:09 UT
Total Lunar Eclipse
(umbral mag. 1.07; Saros 118)
A shallow total eclipse saw the Moon in relative darkness for 39 minutes and 12 seconds. The Moon was 7% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 21 minutes in total.
   
2 Sep, 1411 AD
max: 16:43 UT
Total Lunar Eclipse
(umbral mag. 1.17; Saros 118)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 1 minute. The Moon was 17% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 26 minutes in total.
   
13 Sep, 1429 AD
max: 00:25 UT
Total Lunar Eclipse
(umbral mag. 1.26; Saros 118)
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 29 minutes in total.
   
24 Sep, 1447 AD
max: 08:18 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 118)
The Moon was plunged into darkness for 1 hour and 21 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 31 minutes in total.
   
4 Oct, 1465 AD
max: 16:20 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 118)
The Moon was plunged into darkness for 1 hour and 26 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
16 Oct, 1483 AD
max: 00:32 UT
Total Lunar Eclipse
(umbral mag. 1.45; Saros 118)
The Moon was plunged into darkness for 1 hour and 29 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 34 minutes in total.
   
26 Oct, 1501 AD
max: 08:51 UT
Total Lunar Eclipse
(umbral mag. 1.49; Saros 118)
The Moon was plunged into darkness for 1 hour and 31 minutes, in a deep total eclipse which saw the Moon 49% 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 34 minutes in total.
   
6 Nov, 1519 AD
max: 17:19 UT
Total Lunar Eclipse
(umbral mag. 1.52; Saros 118)
The Moon was plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 34 minutes in total.
   
17 Nov, 1537 AD
max: 01:53 UT
Total Lunar Eclipse
(umbral mag. 1.54; Saros 118)
The Moon was plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which saw the Moon 54% 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 34 minutes in total.
   
28 Nov, 1555 AD
max: 10:32 UT
Total Lunar Eclipse
(umbral mag. 1.55; Saros 118)
The Moon was plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 34 minutes in total.
   
8 Dec, 1573 AD
max: 19:14 UT
Total Lunar Eclipse
(umbral mag. 1.56; Saros 118)
The Moon was plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which saw the Moon 56% 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 33 minutes in total.
   
30 Dec, 1591 AD
max: 03:58 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 118)
The Moon was plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
9 Jan, 1610 AD
max: 12:42 UT
Total Lunar Eclipse
(umbral mag. 1.58; Saros 118)
The Moon was plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
20 Jan, 1628 AD
max: 21:26 UT
Total Lunar Eclipse
(umbral mag. 1.59; Saros 118)
A dramatic total eclipse lasting 1 hour and 34 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 32 minutes in total.
   
31 Jan, 1646 AD
max: 06:06 UT
Total Lunar Eclipse
(umbral mag. 1.60; Saros 118)
A dramatic total eclipse lasting 1 hour and 35 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 32 minutes in total.
   
11 Feb, 1664 AD
max: 14:42 UT
Total Lunar Eclipse
(umbral mag. 1.63; Saros 118)
A dramatic total eclipse lasting 1 hour and 35 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 32 minutes in total.
   
21 Feb, 1682 AD
max: 23:12 UT
Total Lunar Eclipse
(umbral mag. 1.66; Saros 118)
A dramatic total eclipse lasting 1 hour and 36 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 33 minutes in total.
   
5 Mar, 1700 AD
max: 07:37 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 118)
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 33 minutes in total.
   
16 Mar, 1718 AD
max: 15:54 UT
Total Lunar Eclipse
(umbral mag. 1.76; Saros 118)
A dramatic total eclipse lasting 1 hour and 39 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
27 Mar, 1736 AD
max: 00:05 UT
Total Lunar Eclipse
(umbral mag. 1.82; Saros 118)
A dramatic total eclipse lasting 1 hour and 39 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
7 Apr, 1754 AD
max: 08:07 UT
Total Lunar Eclipse
(umbral mag. 1.85; Saros 118)
A dramatic total eclipse lasting 1 hour and 39 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
17 Apr, 1772 AD
max: 16:04 UT
Total Lunar Eclipse
(umbral mag. 1.77; Saros 118)
A dramatic total eclipse lasting 1 hour and 39 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 32 minutes in total.
   
28 Apr, 1790 AD
max: 23:53 UT
Total Lunar Eclipse
(umbral mag. 1.67; Saros 118)
A dramatic total eclipse lasting 1 hour and 37 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 31 minutes in total.
   
10 May, 1808 AD
max: 07:38 UT
Total Lunar Eclipse
(umbral mag. 1.56; Saros 118)
The Moon was plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which saw the Moon 56% 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 29 minutes in total.
   
21 May, 1826 AD
max: 15:15 UT
Total Lunar Eclipse
(umbral mag. 1.45; Saros 118)
The Moon was plunged into darkness for 1 hour and 27 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 26 minutes in total.
   
31 May, 1844 AD
max: 22:50 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 118)
The Moon was plunged into darkness for 1 hour and 17 minutes, in a deep total eclipse which saw the Moon 33% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 22 minutes in total.
   
12 Jun, 1862 AD
max: 06:20 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 118)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 2 minutes. The Moon was 20% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 17 minutes in total.
   
22 Jun, 1880 AD
max: 13:50 UT
Total Lunar Eclipse
(umbral mag. 1.06; Saros 118)
A shallow total eclipse saw the Moon in relative darkness for 37 minutes and 12 seconds. The Moon was 6% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 11 minutes in total.
   
3 Jul, 1898 AD
max: 21:17 UT
Partial Lunar Eclipse
(umbral mag. 0.93; Saros 118)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 2 minutes. With 93% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
   
15 Jul, 1916 AD
max: 04:45 UT
Partial Lunar Eclipse
(umbral mag. 0.79; Saros 118)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 53 minutes, with 79% of the Moon in darkness at maximum.
   
26 Jul, 1934 AD
max: 12:15 UT
Partial Lunar Eclipse
(umbral mag. 0.66; Saros 118)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 41 minutes, with 66% of the Moon in darkness at maximum.
   
5 Aug, 1952 AD
max: 19:47 UT
Partial Lunar Eclipse
(umbral mag. 0.53; Saros 118)
The Earth's shadow on the moon was clearly visible in this eclipse, with 53% of the Moon in shadow; the partial eclipse lasted for 2 hours and 27 minutes.
   
17 Aug, 1970 AD
max: 03:23 UT
Partial Lunar Eclipse
(umbral mag. 0.41; Saros 118)
The Earth's shadow on the moon was clearly visible in this eclipse, with 41% of the Moon in shadow; the partial eclipse lasted for 2 hours and 11 minutes.
   
27 Aug, 1988 AD
max: 11:04 UT
Partial Lunar Eclipse
(umbral mag. 0.29; Saros 118)
The Earth's shadow on the moon was clearly visible in this eclipse, with 29% of the Moon in shadow; the partial eclipse lasted for 1 hour and 53 minutes.
   
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.
   
18 Sep, 2024 AD
00:41–04:47 UT
Partial Lunar Eclipse
(umbral mag. 0.08; Saros 118)
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 3 minutes and visible across the Americas, Africa, Europe, and the Middle East. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
   
29 Sep, 2042 AD
max: 10:44 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 118)
The Moon will approach within 0% of the Earth's umbral shadow at maximum eclipse; 95% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 3 hours and 59 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.
   
9 Oct, 2060 AD
max: 18:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 118)
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 3 hours and 51 minutes overall.
   
21 Oct, 2078 AD
max: 03:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.82; Saros 118)
At maximum eclipse, 82% 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 3 hours and 45 minutes overall.
   
31 Oct, 2096 AD
max: 11:27 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 118)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 77% 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 39 minutes.
   
12 Nov, 2114 AD
max: 19:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.73; Saros 118)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 73% 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 35 minutes.
   
23 Nov, 2132 AD
max: 04:30 UT
Penumbral Lunar Eclipse
(penum. mag. 0.70; Saros 118)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 70% 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 31 minutes.
   
4 Dec, 2150 AD
max: 13:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.67; Saros 118)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 67% 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 29 minutes.
   
14 Dec, 2168 AD
max: 21:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.66; Saros 118)
This subtle penumbral 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 27 minutes.
   
26 Dec, 2186 AD
max: 06:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.64; Saros 118)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 64% 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 26 minutes.
   
6 Jan, 2205 AD
max: 15:27 UT
Penumbral Lunar Eclipse
(penum. mag. 0.63; Saros 118)
This subtle penumbral 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 25 minutes.
   
18 Jan, 2223 AD
max: 00:14 UT
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 118)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 62% 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 24 minutes.
   
28 Jan, 2241 AD
max: 08:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.61; Saros 118)
This subtle penumbral 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 22 minutes.
   
8 Feb, 2259 AD
max: 17:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 118)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 20 minutes, just 59% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
19 Feb, 2277 AD
max: 02:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.57; Saros 118)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 17 minutes, just 57% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
2 Mar, 2295 AD
max: 10:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.53; Saros 118)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 12 minutes, just 53% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
13 Mar, 2313 AD
max: 19:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 118)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 5 minutes, just 49% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
25 Mar, 2331 AD
max: 03:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.43; Saros 118)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 56 minutes, just 43% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
4 Apr, 2349 AD
max: 11:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.37; Saros 118)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 43 minutes, just 37% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
15 Apr, 2367 AD
max: 19:33 UT
Penumbral Lunar Eclipse
(penum. mag. 0.29; Saros 118)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 26 minutes, just 29% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
26 Apr, 2385 AD
max: 03:22 UT
Penumbral Lunar Eclipse
(penum. mag. 0.20; Saros 118)
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 20% of the Moon's disc for 2 hours and 2 minutes, which will be essentially impossible to see.
   
7 May, 2403 AD
max: 11:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros 118)
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 9% of the Moon's disc for 1 hour and 25 minutes, which will be essentially impossible to see.