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.
29 Jul, 1749 AD
max: 16:30 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 144)
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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 8 minutes, which was essentially impossible to see.
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10 Aug, 1767 AD
max: 00:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.18; Saros 144)
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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 18% of the Moon's disc for 1 hour and 53 minutes, which was essentially impossible to see.
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20 Aug, 1785 AD
max: 07:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 144)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 23 minutes, just 30% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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1 Sep, 1803 AD
max: 15:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.40; Saros 144)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 45 minutes, just 40% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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11 Sep, 1821 AD
max: 23:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.50; Saros 144)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 3 minutes, just 50% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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23 Sep, 1839 AD
max: 06:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 144)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 17 minutes, just 58% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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3 Oct, 1857 AD
max: 14:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.66; Saros 144)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 66% 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 28 minutes.
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14 Oct, 1875 AD
max: 23:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 144)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 72% 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 38 minutes.
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25 Oct, 1893 AD
max: 07:16 UT
Penumbral Lunar Eclipse
(penum. mag. 0.78; Saros 144)
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This subtle penumbral 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 45 minutes.
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6 Nov, 1911 AD
max: 15:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.82; Saros 144)
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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 3 hours and 51 minutes.
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17 Nov, 1929 AD
max: 00:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.85; Saros 144)
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At maximum eclipse, 85% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 3 hours and 55 minutes overall.
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28 Nov, 1947 AD
max: 08:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 144)
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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 3 hours and 58 minutes overall.
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8 Dec, 1965 AD
max: 17:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 144)
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At maximum eclipse, 88% 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 1 minute overall.
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20 Dec, 1983 AD
max: 01:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 144)
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At maximum eclipse, 89% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 2 minutes overall.
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30 Dec, 2001 AD
08:27–12:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 144)
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At maximum eclipse, 89% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 4 minutes overall, and was visible from the Americas, Asia and Australasia.
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10 Jan, 2020 AD
17:07–21:12 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 144)
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At maximum eclipse, 90% 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 5 minutes overall, and was visible from Africa, Europe, Asia, Alaska, and Australia.
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21 Jan, 2038 AD
01:45–05:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 144)
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At maximum eclipse, 90% 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 6 minutes overall, and will be visible from the Americas, Europe, Africa, and western Asia.
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1 Feb, 2056 AD
max: 12:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.91; Saros 144)
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At maximum eclipse, 91% 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 7 minutes overall.
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11 Feb, 2074 AD
max: 20:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 144)
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At maximum eclipse, 92% 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 10 minutes overall.
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23 Feb, 2092 AD
max: 05:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.94; Saros 144)
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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 12 minutes overall.
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6 Mar, 2110 AD
max: 13:33 UT
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 144)
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The Moon will approach within 5% of the Earth's umbral shadow at maximum eclipse; 97% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 4 hours and 16 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.
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16 Mar, 2128 AD
max: 21:41 UT
Penumbral Lunar Eclipse
(penum. mag. 1.01; Saros 144)
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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 21 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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28 Mar, 2146 AD
max: 05:39 UT
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 144)
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A tiny bite out of the Moon may be visible at maximum, though just 4% of the Moon will be shadowed in a partial eclipse lasting for 48 minutes and 36 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
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7 Apr, 2164 AD
max: 13:28 UT
Partial Lunar Eclipse
(umbral mag. 0.11; Saros 144)
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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 16 minutes, with just 11% of the Moon in shadow at maximum.
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18 Apr, 2182 AD
max: 21:07 UT
Partial Lunar Eclipse
(umbral mag. 0.19; Saros 144)
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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 38 minutes, with just 19% of the Moon in shadow at maximum.
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30 Apr, 2200 AD
max: 04:37 UT
Partial Lunar Eclipse
(umbral mag. 0.28; Saros 144)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 28% of the Moon in shadow; the partial eclipse will last for 1 hour and 59 minutes.
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11 May, 2218 AD
max: 11:57 UT
Partial Lunar Eclipse
(umbral mag. 0.38; Saros 144)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 38% of the Moon in shadow; the partial eclipse will last for 2 hours and 17 minutes.
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21 May, 2236 AD
max: 19:09 UT
Partial Lunar Eclipse
(umbral mag. 0.50; Saros 144)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 50% of the Moon in shadow; the partial eclipse will last for 2 hours and 34 minutes.
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2 Jun, 2254 AD
max: 02:14 UT
Partial Lunar Eclipse
(umbral mag. 0.62; Saros 144)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 50 minutes, with 62% of the Moon in darkness at maximum.
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12 Jun, 2272 AD
max: 09:13 UT
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 144)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 3 minutes, with 76% of the Moon in darkness at maximum.
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23 Jun, 2290 AD
max: 16:06 UT
Partial Lunar Eclipse
(umbral mag. 0.90; Saros 144)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 15 minutes, with 90% of the Moon in darkness at maximum.
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4 Jul, 2308 AD
max: 22:55 UT
Total Lunar Eclipse
(umbral mag. 1.04; Saros 144)
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The Moon will barely edge into total eclipse for 31 minutes and 54 seconds. With the Moon just 4% of its diameter into the Earth's umbral shadow, the Moon may be quite bright, but even so, this should be worth seeing. The partial eclipse will last for 3 hours and 26 minutes in total.
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16 Jul, 2326 AD
max: 05:41 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 144)
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A shallow total eclipse will see the Moon in relative darkness for 1 hour and 6 minutes. The Moon will be 19% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 34 minutes in total.
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26 Jul, 2344 AD
max: 12:26 UT
Total Lunar Eclipse
(umbral mag. 1.34; Saros 144)
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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 34% 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 Aug, 2362 AD
max: 19:11 UT
Total Lunar Eclipse
(umbral mag. 1.48; Saros 144)
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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 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 46 minutes in total.
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17 Aug, 2380 AD
max: 01:59 UT
Total Lunar Eclipse
(umbral mag. 1.62; Saros 144)
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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 49 minutes in total.
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28 Aug, 2398 AD
max: 08:48 UT
Total Lunar Eclipse
(umbral mag. 1.76; Saros 144)
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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 51 minutes in total.
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7 Sep, 2416 AD
max: 15:43 UT
Total Lunar Eclipse
(umbral mag. 1.78; Saros 144)
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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.
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18 Sep, 2434 AD
max: 22:42 UT
Total Lunar Eclipse
(umbral mag. 1.65; Saros 144)
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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 51 minutes in total.
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29 Sep, 2452 AD
max: 05:49 UT
Total Lunar Eclipse
(umbral mag. 1.54; Saros 144)
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The Moon will be plunged into darkness for 1 hour and 39 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 50 minutes in total.
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10 Oct, 2470 AD
max: 13:01 UT
Total Lunar Eclipse
(umbral mag. 1.44; Saros 144)
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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 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 48 minutes in total.
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20 Oct, 2488 AD
max: 20:22 UT
Total Lunar Eclipse
(umbral mag. 1.35; Saros 144)
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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 45 minutes in total.
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2 Nov, 2506 AD
max: 03:50 UT
Total Lunar Eclipse
(umbral mag. 1.28; Saros 144)
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The Moon will be plunged into darkness for 1 hour and 19 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 43 minutes in total.
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12 Nov, 2524 AD
max: 11:26 UT
Total Lunar Eclipse
(umbral mag. 1.22; Saros 144)
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The Moon will be plunged into darkness for 1 hour and 11 minutes, in a deep total eclipse which will see the Moon 22% 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 40 minutes in total.
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23 Nov, 2542 AD
max: 19:09 UT
Total Lunar Eclipse
(umbral mag. 1.16; Saros 144)
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A shallow total eclipse will see the Moon in relative darkness for 1 hour and 3 minutes. The Moon will be 16% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 38 minutes in total.
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4 Dec, 2560 AD
max: 02:59 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 144)
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A shallow total eclipse will see the Moon in relative darkness for 55 minutes and 54 seconds. The Moon will be 13% 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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15 Dec, 2578 AD
max: 10:54 UT
Total Lunar Eclipse
(umbral mag. 1.09; Saros 144)
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A shallow total eclipse will see the Moon in relative darkness for 48 minutes and 48 seconds. The Moon will be 9% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 35 minutes in total.
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25 Dec, 2596 AD
max: 18:52 UT
Total Lunar Eclipse
(umbral mag. 1.07; Saros 144)
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A shallow total eclipse will see the Moon in relative darkness for 42 minutes and 18 seconds. The Moon will be 7% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 34 minutes in total.
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7 Jan, 2615 AD
max: 02:53 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 144)
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The Moon will barely edge into total eclipse for 36 minutes exactly. With the Moon just 5% 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 33 minutes in total.
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17 Jan, 2633 AD
max: 10:56 UT
Total Lunar Eclipse
(umbral mag. 1.03; Saros 144)
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The Moon will barely edge into total eclipse for 29 minutes and 54 seconds. With the Moon just 3% 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 32 minutes in total.
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28 Jan, 2651 AD
max: 18:56 UT
Total Lunar Eclipse
(umbral mag. 1.02; Saros 144)
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The Moon will barely edge into total eclipse for 20 minutes and 12 seconds. With the Moon just 2% 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 31 minutes in total.
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8 Feb, 2669 AD
max: 02:55 UT
Partial Lunar Eclipse
(umbral mag. 1.00; Saros 144)
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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 30 minutes. With 100% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
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19 Feb, 2687 AD
max: 10:48 UT
Partial Lunar Eclipse
(umbral mag. 0.97; Saros 144)
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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 28 minutes. With 97% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
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2 Mar, 2705 AD
max: 18:37 UT
Partial Lunar Eclipse
(umbral mag. 0.94; Saros 144)
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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 26 minutes. With 94% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
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14 Mar, 2723 AD
max: 02:17 UT
Partial Lunar Eclipse
(umbral mag. 0.89; Saros 144)
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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.
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24 Mar, 2741 AD
max: 09:52 UT
Partial Lunar Eclipse
(umbral mag. 0.84; Saros 144)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 19 minutes, with 84% of the Moon in darkness at maximum.
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4 Apr, 2759 AD
max: 17:16 UT
Partial Lunar Eclipse
(umbral mag. 0.77; Saros 144)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 13 minutes, with 77% of the Moon in darkness at maximum.
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15 Apr, 2777 AD
max: 00:33 UT
Partial Lunar Eclipse
(umbral mag. 0.69; Saros 144)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 5 minutes, with 69% of the Moon in darkness at maximum.
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26 Apr, 2795 AD
max: 07:41 UT
Partial Lunar Eclipse
(umbral mag. 0.60; Saros 144)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 60% of the Moon in shadow; the partial eclipse will last for 2 hours and 55 minutes.
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6 May, 2813 AD
max: 14:41 UT
Partial Lunar Eclipse
(umbral mag. 0.50; Saros 144)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 50% of the Moon in shadow; the partial eclipse will last for 2 hours and 42 minutes.
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17 May, 2831 AD
max: 21:33 UT
Partial Lunar Eclipse
(umbral mag. 0.38; Saros 144)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 38% of the Moon in shadow; the partial eclipse will last for 2 hours and 24 minutes.
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28 May, 2849 AD
max: 04:18 UT
Partial Lunar Eclipse
(umbral mag. 0.25; Saros 144)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 25% of the Moon in shadow; the partial eclipse will last for 2 hours exactly.
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8 Jun, 2867 AD
max: 10:58 UT
Partial Lunar Eclipse
(umbral mag. 0.12; Saros 144)
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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 24 minutes, with just 12% of the Moon in shadow at maximum.
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18 Jun, 2885 AD
max: 17:33 UT
Penumbral Lunar Eclipse
(penum. mag. 1.04; Saros 144)
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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 47 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
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1 Jul, 2903 AD
max: 00:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 144)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 90% 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 29 minutes.
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11 Jul, 2921 AD
max: 06:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 144)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 74% 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 8 minutes.
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22 Jul, 2939 AD
max: 13:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 144)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 44 minutes, just 59% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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1 Aug, 2957 AD
max: 19:35 UT
Penumbral Lunar Eclipse
(penum. mag. 0.44; Saros 144)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 16 minutes, just 44% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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13 Aug, 2975 AD
max: 02:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.29; Saros 144)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 42 minutes, just 29% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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23 Aug, 2993 AD
max: 08:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 144)
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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 58 minutes, which will be essentially impossible to see.
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