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.
12 May, 1492 AD
max: 06:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 132)
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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 3% of the Moon's disc for 52 minutes exactly, which was essentially impossible to see.
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23 May, 1510 AD
max: 13:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 132)
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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 15% of the Moon's disc for 1 hour and 48 minutes, which was essentially impossible to see.
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2 Jun, 1528 AD
max: 20:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.28; Saros 132)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 25 minutes, just 28% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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14 Jun, 1546 AD
max: 03:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.41; Saros 132)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 54 minutes, just 41% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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24 Jun, 1564 AD
max: 11:00 UT
Penumbral Lunar Eclipse
(penum. mag. 0.54; Saros 132)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 19 minutes, just 54% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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5 Jul, 1582 AD
max: 18:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.67; Saros 132)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 67% 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.
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26 Jul, 1600 AD
max: 01:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.80; Saros 132)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 80% 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 58 minutes.
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6 Aug, 1618 AD
max: 08:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros 132)
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At maximum eclipse, 93% 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 14 minutes overall.
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16 Aug, 1636 AD
max: 15:28 UT
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 132)
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A tiny bite out of the Moon may have been visible at maximum, though just 4% of the Moon was shadowed in a partial eclipse which lasted for 47 minutes and 48 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
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27 Aug, 1654 AD
max: 22:43 UT
Partial Lunar Eclipse
(umbral mag. 0.15; Saros 132)
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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 29 minutes, with just 15% of the Moon in shadow at maximum.
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7 Sep, 1672 AD
max: 06:03 UT
Partial Lunar Eclipse
(umbral mag. 0.25; Saros 132)
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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 54 minutes.
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18 Sep, 1690 AD
max: 13:28 UT
Partial Lunar Eclipse
(umbral mag. 0.34; Saros 132)
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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 11 minutes.
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29 Sep, 1708 AD
max: 21:00 UT
Partial Lunar Eclipse
(umbral mag. 0.42; Saros 132)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 42% of the Moon in shadow; the partial eclipse lasted for 2 hours and 24 minutes.
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11 Oct, 1726 AD
max: 04:40 UT
Partial Lunar Eclipse
(umbral mag. 0.49; Saros 132)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 49% of the Moon in shadow; the partial eclipse lasted for 2 hours and 34 minutes.
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21 Oct, 1744 AD
max: 12:26 UT
Partial Lunar Eclipse
(umbral mag. 0.55; Saros 132)
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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 42 minutes.
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1 Nov, 1762 AD
max: 20:19 UT
Partial Lunar Eclipse
(umbral mag. 0.59; Saros 132)
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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 47 minutes.
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12 Nov, 1780 AD
max: 04:19 UT
Partial Lunar Eclipse
(umbral mag. 0.62; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 52 minutes, with 62% of the Moon in darkness at maximum.
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23 Nov, 1798 AD
max: 12:25 UT
Partial Lunar Eclipse
(umbral mag. 0.65; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 55 minutes, with 65% of the Moon in darkness at maximum.
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4 Dec, 1816 AD
max: 20:35 UT
Partial Lunar Eclipse
(umbral mag. 0.66; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 57 minutes, with 66% of the Moon in darkness at maximum.
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16 Dec, 1834 AD
max: 04:48 UT
Partial Lunar Eclipse
(umbral mag. 0.67; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 58 minutes, with 67% of the Moon in darkness at maximum.
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26 Dec, 1852 AD
max: 13:02 UT
Partial Lunar Eclipse
(umbral mag. 0.68; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 59 minutes, with 68% of the Moon in darkness at maximum.
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6 Jan, 1871 AD
max: 21:16 UT
Partial Lunar Eclipse
(umbral mag. 0.69; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 1 minute, with 69% of the Moon in darkness at maximum.
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17 Jan, 1889 AD
max: 05:29 UT
Partial Lunar Eclipse
(umbral mag. 0.70; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 2 minutes, with 70% of the Moon in darkness at maximum.
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29 Jan, 1907 AD
max: 13:37 UT
Partial Lunar Eclipse
(umbral mag. 0.71; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 4 minutes, with 71% of the Moon in darkness at maximum.
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8 Feb, 1925 AD
max: 21:41 UT
Partial Lunar Eclipse
(umbral mag. 0.73; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 6 minutes, with 73% of the Moon in darkness at maximum.
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20 Feb, 1943 AD
max: 05:37 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 9 minutes, with 76% of the Moon in darkness at maximum.
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2 Mar, 1961 AD
max: 13:28 UT
Partial Lunar Eclipse
(umbral mag. 0.80; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 13 minutes, with 80% of the Moon in darkness at maximum.
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13 Mar, 1979 AD
max: 21:08 UT
Partial Lunar Eclipse
(umbral mag. 0.85; Saros 132)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 18 minutes, with 85% of the Moon in darkness at maximum.
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24 Mar, 1997 AD
max: 04:39 UT
Partial Lunar Eclipse
(umbral mag. 0.92; Saros 132)
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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 23 minutes. With 92% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
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4 Apr, 2015 AD
09:01–14:58 UT
Total Lunar Eclipse
(umbral mag. 1.00; Saros 132)
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The Moon barely edged into total eclipse for a very brief 4 minutes and 42 seconds. With the Moon just barely inside the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing for observers from east Asia, Australia, and western North America. The partial eclipse lasted for 3 hours and 29 minutes in total and was visible from most of Asia, Australia, and the Americas.
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14 Apr, 2033 AD
16:11–22:13 UT
Total Lunar Eclipse
(umbral mag. 1.09; Saros 132)
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A shallow total eclipse will see the Moon in relative darkness for 49 minutes and 12 seconds. The Moon will be 9% of its diameter into the Earth's umbral shadow, and should be significantly darkened for viewers from Europe, Africa, most of Asia, and Australia. The partial eclipse will last for 3 hours and 35 minutes in total.
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26 Apr, 2051 AD
max: 02:14 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 132)
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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 41 minutes in total.
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6 May, 2069 AD
max: 09:07 UT
Total Lunar Eclipse
(umbral mag. 1.32; Saros 132)
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The Moon will be plunged into darkness for 1 hour and 24 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 46 minutes in total.
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17 May, 2087 AD
max: 15:52 UT
Total Lunar Eclipse
(umbral mag. 1.46; Saros 132)
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The Moon will be plunged into darkness for 1 hour and 35 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 51 minutes in total.
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28 May, 2105 AD
max: 22:30 UT
Total Lunar Eclipse
(umbral mag. 1.60; Saros 132)
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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 54 minutes in total.
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9 Jun, 2123 AD
max: 05:02 UT
Total Lunar Eclipse
(umbral mag. 1.75; Saros 132)
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A dramatic total eclipse lasting 1 hour and 46 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 56 minutes in total.
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19 Jun, 2141 AD
max: 11:29 UT
Total Lunar Eclipse
(umbral mag. 1.74; Saros 132)
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A dramatic total eclipse lasting 1 hour and 46 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 56 minutes in total.
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30 Jun, 2159 AD
max: 17:54 UT
Total Lunar Eclipse
(umbral mag. 1.58; Saros 132)
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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 54 minutes in total.
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11 Jul, 2177 AD
max: 00:18 UT
Total Lunar Eclipse
(umbral mag. 1.42; Saros 132)
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The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see the Moon 42% 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.
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22 Jul, 2195 AD
max: 06:41 UT
Total Lunar Eclipse
(umbral mag. 1.26; Saros 132)
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The Moon will be plunged into darkness for 1 hour and 17 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 45 minutes in total.
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2 Aug, 2213 AD
max: 13:08 UT
Total Lunar Eclipse
(umbral mag. 1.10; Saros 132)
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A shallow total eclipse will see the Moon in relative darkness for 50 minutes and 36 seconds. The Moon will be 10% 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.
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13 Aug, 2231 AD
max: 19:37 UT
Partial Lunar Eclipse
(umbral mag. 0.94; Saros 132)
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The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 27 minutes. With 94% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
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24 Aug, 2249 AD
max: 02:12 UT
Partial Lunar Eclipse
(umbral mag. 0.80; Saros 132)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 15 minutes, with 80% of the Moon in darkness at maximum.
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4 Sep, 2267 AD
max: 08:52 UT
Partial Lunar Eclipse
(umbral mag. 0.66; Saros 132)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 2 minutes, with 66% of the Moon in darkness at maximum.
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14 Sep, 2285 AD
max: 15:42 UT
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 132)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 54% of the Moon in shadow; the partial eclipse will last for 2 hours and 47 minutes.
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26 Sep, 2303 AD
max: 22:38 UT
Partial Lunar Eclipse
(umbral mag. 0.42; Saros 132)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 42% of the Moon in shadow; the partial eclipse will last for 2 hours and 31 minutes.
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7 Oct, 2321 AD
max: 05:45 UT
Partial Lunar Eclipse
(umbral mag. 0.32; Saros 132)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 32% of the Moon in shadow; the partial eclipse will last for 2 hours and 13 minutes.
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18 Oct, 2339 AD
max: 13:00 UT
Partial Lunar Eclipse
(umbral mag. 0.23; Saros 132)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 23% of the Moon in shadow; the partial eclipse will last for 1 hour and 55 minutes.
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28 Oct, 2357 AD
max: 20:26 UT
Partial Lunar Eclipse
(umbral mag. 0.16; Saros 132)
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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 16% of the Moon in shadow at maximum.
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9 Nov, 2375 AD
max: 04:00 UT
Partial Lunar Eclipse
(umbral mag. 0.10; Saros 132)
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At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 18 minutes, with just 10% of the Moon in shadow at maximum.
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19 Nov, 2393 AD
max: 11:43 UT
Partial Lunar Eclipse
(umbral mag. 0.06; Saros 132)
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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 57 minutes and 30 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
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30 Nov, 2411 AD
max: 19:34 UT
Partial Lunar Eclipse
(umbral mag. 0.02; Saros 132)
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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.
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11 Dec, 2429 AD
max: 03:32 UT
Penumbral Lunar Eclipse
(penum. mag. 1.09; Saros 132)
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In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 50 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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22 Dec, 2447 AD
max: 11:35 UT
Penumbral Lunar Eclipse
(penum. mag. 1.07; Saros 132)
|
In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 48 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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1 Jan, 2466 AD
max: 19:42 UT
Penumbral Lunar Eclipse
(penum. mag. 1.05; Saros 132)
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In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 46 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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13 Jan, 2484 AD
max: 03:51 UT
Penumbral Lunar Eclipse
(penum. mag. 1.04; Saros 132)
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In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 44 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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24 Jan, 2502 AD
max: 12:02 UT
Penumbral Lunar Eclipse
(penum. mag. 1.03; Saros 132)
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In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 42 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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4 Feb, 2520 AD
max: 20:10 UT
Penumbral Lunar Eclipse
(penum. mag. 1.02; Saros 132)
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In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 40 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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15 Feb, 2538 AD
max: 04:17 UT
Penumbral Lunar Eclipse
(penum. mag. 1.00; Saros 132)
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In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 37 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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26 Feb, 2556 AD
max: 12:19 UT
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 132)
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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 33 minutes overall.
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8 Mar, 2574 AD
max: 20:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.94; Saros 132)
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At maximum eclipse, 94% 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 28 minutes overall.
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19 Mar, 2592 AD
max: 04:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 132)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 89% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 4 hours and 21 minutes.
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31 Mar, 2610 AD
max: 11:52 UT
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 132)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 84% 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.
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10 Apr, 2628 AD
max: 19:29 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 132)
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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 4 hours and 4 minutes.
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22 Apr, 2646 AD
max: 02:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 132)
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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 52 minutes.
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2 May, 2664 AD
max: 10:22 UT
Penumbral Lunar Eclipse
(penum. mag. 0.60; Saros 132)
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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 37 minutes.
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13 May, 2682 AD
max: 17:39 UT
Penumbral Lunar Eclipse
(penum. mag. 0.50; Saros 132)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 19 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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25 May, 2700 AD
max: 00:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.39; Saros 132)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 57 minutes, just 39% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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5 Jun, 2718 AD
max: 07:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.27; Saros 132)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 29 minutes, just 27% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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15 Jun, 2736 AD
max: 15:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 132)
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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 15% of the Moon's disc for 1 hour and 52 minutes, which will be essentially impossible to see.
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26 Jun, 2754 AD
max: 22:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.02; Saros 132)
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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 2% of the Moon's disc for 45 minutes and 6 seconds, which will be essentially impossible to see.
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