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.
13 May, 0971 AD
max: 03:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 114)
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In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 6% of the Moon's disc for 1 hour and 13 minutes, which was essentially impossible to see.
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23 May, 0989 AD
max: 10:26 UT
Penumbral Lunar Eclipse
(penum. mag. 0.19; Saros 114)
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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 2 hours and 9 minutes, which was essentially impossible to see.
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3 Jun, 1007 AD
max: 17:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.33; Saros 114)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 47 minutes, just 33% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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13 Jun, 1025 AD
max: 23:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.47; Saros 114)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 18 minutes, just 47% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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25 Jun, 1043 AD
max: 06:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 114)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 62% 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.
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5 Jul, 1061 AD
max: 13:19 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 114)
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This subtle penumbral 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 4 hours and 6 minutes.
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16 Jul, 1079 AD
max: 20:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.91; Saros 114)
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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 4 hours and 25 minutes overall.
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27 Jul, 1097 AD
max: 02:46 UT
Penumbral Lunar Eclipse
(penum. mag. 1.04; Saros 114)
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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. The penumbral phase lasted for 4 hours and 41 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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7 Aug, 1115 AD
max: 09:35 UT
Partial Lunar Eclipse
(umbral mag. 0.12; Saros 114)
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At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 21 minutes, with just 12% of the Moon in shadow at maximum.
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17 Aug, 1133 AD
max: 16:30 UT
Partial Lunar Eclipse
(umbral mag. 0.23; Saros 114)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 23% of the Moon in shadow; the partial eclipse lasted for 1 hour and 54 minutes.
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28 Aug, 1151 AD
max: 23:31 UT
Partial Lunar Eclipse
(umbral mag. 0.34; Saros 114)
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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 16 minutes.
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8 Sep, 1169 AD
max: 06:40 UT
Partial Lunar Eclipse
(umbral mag. 0.44; Saros 114)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 44% of the Moon in shadow; the partial eclipse lasted for 2 hours and 32 minutes.
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19 Sep, 1187 AD
max: 13:56 UT
Partial Lunar Eclipse
(umbral mag. 0.52; Saros 114)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 52% of the Moon in shadow; the partial eclipse lasted for 2 hours and 44 minutes.
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29 Sep, 1205 AD
max: 21:21 UT
Partial Lunar Eclipse
(umbral mag. 0.59; Saros 114)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 59% of the Moon in shadow; the partial eclipse lasted for 2 hours and 53 minutes.
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11 Oct, 1223 AD
max: 04:54 UT
Partial Lunar Eclipse
(umbral mag. 0.65; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours exactly, with 65% of the Moon in darkness at maximum.
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21 Oct, 1241 AD
max: 12:34 UT
Partial Lunar Eclipse
(umbral mag. 0.69; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 5 minutes, with 69% of the Moon in darkness at maximum.
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1 Nov, 1259 AD
max: 20:22 UT
Partial Lunar Eclipse
(umbral mag. 0.73; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 8 minutes, with 73% of the Moon in darkness at maximum.
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12 Nov, 1277 AD
max: 04:15 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 11 minutes, with 76% of the Moon in darkness at maximum.
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23 Nov, 1295 AD
max: 12:13 UT
Partial Lunar Eclipse
(umbral mag. 0.78; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 13 minutes, with 78% of the Moon in darkness at maximum.
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3 Dec, 1313 AD
max: 20:14 UT
Partial Lunar Eclipse
(umbral mag. 0.79; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 14 minutes, with 79% of the Moon in darkness at maximum.
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15 Dec, 1331 AD
max: 04:17 UT
Partial Lunar Eclipse
(umbral mag. 0.80; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 16 minutes, with 80% of the Moon in darkness at maximum.
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25 Dec, 1349 AD
max: 12:19 UT
Partial Lunar Eclipse
(umbral mag. 0.82; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 17 minutes, with 82% of the Moon in darkness at maximum.
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5 Jan, 1368 AD
max: 20:20 UT
Partial Lunar Eclipse
(umbral mag. 0.83; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 18 minutes, with 83% of the Moon in darkness at maximum.
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16 Jan, 1386 AD
max: 04:16 UT
Partial Lunar Eclipse
(umbral mag. 0.85; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 20 minutes, with 85% of the Moon in darkness at maximum.
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27 Jan, 1404 AD
max: 12:08 UT
Partial Lunar Eclipse
(umbral mag. 0.88; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 22 minutes, with 88% of the Moon in darkness at maximum.
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6 Feb, 1422 AD
max: 19:53 UT
Partial Lunar Eclipse
(umbral mag. 0.92; Saros 114)
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The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 25 minutes. With 92% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
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18 Feb, 1440 AD
max: 03:31 UT
Partial Lunar Eclipse
(umbral mag. 0.97; Saros 114)
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The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 29 minutes. With 97% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
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28 Feb, 1458 AD
max: 11:00 UT
Total Lunar Eclipse
(umbral mag. 1.04; Saros 114)
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The Moon barely edged into total eclipse for 31 minutes and 18 seconds. With the Moon just 4% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 33 minutes in total.
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10 Mar, 1476 AD
max: 18:21 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 114)
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A shallow total eclipse saw the Moon in relative darkness for 53 minutes and 54 seconds. The Moon was 11% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 37 minutes in total.
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22 Mar, 1494 AD
max: 01:33 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 114)
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The Moon was plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 42 minutes in total.
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1 Apr, 1512 AD
max: 08:37 UT
Total Lunar Eclipse
(umbral mag. 1.31; Saros 114)
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The Moon was plunged into darkness for 1 hour and 23 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. The partial eclipse lasted for 3 hours and 46 minutes in total.
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12 Apr, 1530 AD
max: 15:33 UT
Total Lunar Eclipse
(umbral mag. 1.43; Saros 114)
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The Moon was plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which saw the Moon 43% 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 50 minutes in total.
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22 Apr, 1548 AD
max: 22:22 UT
Total Lunar Eclipse
(umbral mag. 1.55; Saros 114)
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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. The partial eclipse lasted for 3 hours and 52 minutes in total.
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4 May, 1566 AD
max: 05:04 UT
Total Lunar Eclipse
(umbral mag. 1.69; Saros 114)
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A dramatic total eclipse lasting 1 hour and 45 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 54 minutes in total.
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24 May, 1584 AD
max: 11:43 UT
Total Lunar Eclipse
(umbral mag. 1.81; Saros 114)
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A dramatic total eclipse lasting 1 hour and 46 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 55 minutes in total.
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4 Jun, 1602 AD
max: 18:16 UT
Total Lunar Eclipse
(umbral mag. 1.66; Saros 114)
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A dramatic total eclipse lasting 1 hour and 44 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 53 minutes in total.
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15 Jun, 1620 AD
max: 00:49 UT
Total Lunar Eclipse
(umbral mag. 1.51; Saros 114)
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The Moon was plunged into darkness for 1 hour and 38 minutes, in a deep total eclipse which saw the Moon 51% 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 50 minutes in total.
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26 Jun, 1638 AD
max: 07:20 UT
Total Lunar Eclipse
(umbral mag. 1.35; Saros 114)
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The Moon was plunged into darkness for 1 hour and 27 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 45 minutes in total.
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6 Jul, 1656 AD
max: 13:54 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 114)
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The Moon was plunged into darkness for 1 hour and 9 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 39 minutes in total.
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17 Jul, 1674 AD
max: 20:29 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 114)
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The Moon barely edged into total eclipse for 35 minutes and 12 seconds. With the Moon just 5% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 30 minutes in total.
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28 Jul, 1692 AD
max: 03:10 UT
Partial Lunar Eclipse
(umbral mag. 0.90; Saros 114)
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The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 20 minutes. With 90% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
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9 Aug, 1710 AD
max: 09:55 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 7 minutes, with 76% of the Moon in darkness at maximum.
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19 Aug, 1728 AD
max: 16:48 UT
Partial Lunar Eclipse
(umbral mag. 0.63; Saros 114)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 54 minutes, with 63% of the Moon in darkness at maximum.
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30 Aug, 1746 AD
max: 23:48 UT
Partial Lunar Eclipse
(umbral mag. 0.51; Saros 114)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 51% of the Moon in shadow; the partial eclipse lasted for 2 hours and 39 minutes.
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10 Sep, 1764 AD
max: 06:58 UT
Partial Lunar Eclipse
(umbral mag. 0.40; Saros 114)
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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 23 minutes.
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21 Sep, 1782 AD
max: 14:17 UT
Partial Lunar Eclipse
(umbral mag. 0.30; Saros 114)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 30% of the Moon in shadow; the partial eclipse lasted for 2 hours and 6 minutes.
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2 Oct, 1800 AD
max: 21:46 UT
Partial Lunar Eclipse
(umbral mag. 0.22; Saros 114)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 22% of the Moon in shadow; the partial eclipse lasted for 1 hour and 48 minutes.
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14 Oct, 1818 AD
max: 05:25 UT
Partial Lunar Eclipse
(umbral mag. 0.15; Saros 114)
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At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 30 minutes, with just 15% of the Moon in shadow at maximum.
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24 Oct, 1836 AD
max: 13:14 UT
Partial Lunar Eclipse
(umbral mag. 0.10; Saros 114)
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A tiny bite out of the Moon may have been visible at maximum, though just 10% of the Moon was shadowed in a partial eclipse which lasted for 1 hour and 13 minutes. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
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4 Nov, 1854 AD
max: 21:12 UT
Partial Lunar Eclipse
(umbral mag. 0.05; Saros 114)
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A tiny bite out of the Moon may have been visible at maximum, though just 5% of the Moon was shadowed in a partial eclipse which lasted for 54 minutes and 18 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
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15 Nov, 1872 AD
max: 05:19 UT
Partial Lunar Eclipse
(umbral mag. 0.02; Saros 114)
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A tiny bite out of the Moon may have been visible at maximum, though just 2% of the Moon was shadowed in a partial eclipse which lasted for 35 minutes and 30 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
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26 Nov, 1890 AD
max: 13:33 UT
Partial Lunar Eclipse
(umbral mag. 0.00; Saros 114)
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While technically a partial eclipse, the Moon barely clipped the Earth's umbral shadow, which may have been very difficult to observe in practice; though a shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse. The partial eclipse lasted for 9 minutes and 48 seconds.
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7 Dec, 1908 AD
max: 21:55 UT
Penumbral Lunar Eclipse
(penum. mag. 1.03; Saros 114)
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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. The penumbral phase lasted for 4 hours and 30 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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19 Dec, 1926 AD
max: 06:19 UT
Penumbral Lunar Eclipse
(penum. mag. 1.03; Saros 114)
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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. The penumbral phase lasted for 4 hours and 28 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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29 Dec, 1944 AD
max: 14:49 UT
Penumbral Lunar Eclipse
(penum. mag. 1.02; Saros 114)
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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. The penumbral phase lasted for 4 hours and 27 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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9 Jan, 1963 AD
max: 23:19 UT
Penumbral Lunar Eclipse
(penum. mag. 1.02; Saros 114)
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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. The penumbral phase lasted for 4 hours and 25 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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20 Jan, 1981 AD
max: 07:49 UT
Penumbral Lunar Eclipse
(penum. mag. 1.01; Saros 114)
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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. The penumbral phase lasted for 4 hours and 24 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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31 Jan, 1999 AD
14:06–18:28 UT
Penumbral Lunar Eclipse
(penum. mag. 1.00; Saros 114)
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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. The penumbral phase lasted for 4 hours and 22 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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11 Feb, 2017 AD
22:34 on 10 Feb–02:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.99; Saros 114)
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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.
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22 Feb, 2035 AD
06:56–11:12 UT
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 114)
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At maximum eclipse, 97% 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 16 minutes overall, and will be visible from east Asia, Australia, New Zealand, and the Americas.
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4 Mar, 2053 AD
max: 17:20 UT
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros 114)
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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 11 minutes overall.
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16 Mar, 2071 AD
max: 01:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 114)
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At maximum eclipse, 89% 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.
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26 Mar, 2089 AD
max: 09:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 114)
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This subtle penumbral 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 3 hours and 58 minutes.
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7 Apr, 2107 AD
max: 17:26 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 114)
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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 49 minutes.
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18 Apr, 2125 AD
max: 01:14 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 114)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 69% 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.
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29 Apr, 2143 AD
max: 08:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.60; Saros 114)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 60% 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.
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9 May, 2161 AD
max: 16:32 UT
Penumbral Lunar Eclipse
(penum. mag. 0.50; Saros 114)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 8 minutes, just 50% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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21 May, 2179 AD
max: 00:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.40; Saros 114)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 48 minutes, just 40% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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31 May, 2197 AD
max: 07:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.28; Saros 114)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 22 minutes, just 28% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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12 Jun, 2215 AD
max: 14:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros 114)
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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 16% of the Moon's disc for 1 hour and 49 minutes, which will be essentially impossible to see.
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22 Jun, 2233 AD
max: 22:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.04; Saros 114)
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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 4% of the Moon's disc for 54 minutes and 48 seconds, which will be essentially impossible to see.
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