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.
25 Sep, 1597 AD
max: 13:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros 140)
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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 9% of the Moon's disc for 1 hour and 27 minutes, which was essentially impossible to see.
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6 Oct, 1615 AD
max: 21:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 140)
|
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 17% of the Moon's disc for 1 hour and 58 minutes, which was essentially impossible to see.
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17 Oct, 1633 AD
max: 05:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.24; Saros 140)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 17 minutes, just 24% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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28 Oct, 1651 AD
max: 13:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 140)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 31 minutes, just 30% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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7 Nov, 1669 AD
max: 21:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.34; Saros 140)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 41 minutes, just 34% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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19 Nov, 1687 AD
max: 06:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.37; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 48 minutes, just 37% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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30 Nov, 1705 AD
max: 14:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.40; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 52 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 Dec, 1723 AD
max: 23:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros 140)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 55 minutes, just 42% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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22 Dec, 1741 AD
max: 08:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.43; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 57 minutes, just 43% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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2 Jan, 1760 AD
max: 16:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.44; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 59 minutes, just 44% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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13 Jan, 1778 AD
max: 01:29 UT
Penumbral Lunar Eclipse
(penum. mag. 0.45; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours exactly, just 45% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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24 Jan, 1796 AD
max: 10:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.47; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 2 minutes, just 47% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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4 Feb, 1814 AD
max: 18:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 5 minutes, just 48% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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16 Feb, 1832 AD
max: 03:20 UT
Penumbral Lunar Eclipse
(penum. mag. 0.51; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 8 minutes, just 51% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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26 Feb, 1850 AD
max: 11:48 UT
Penumbral Lunar Eclipse
(penum. mag. 0.54; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 13 minutes, just 54% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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8 Mar, 1868 AD
max: 20:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 140)
|
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 19 minutes, just 59% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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20 Mar, 1886 AD
max: 04:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.64; Saros 140)
|
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 64% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 26 minutes.
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31 Mar, 1904 AD
max: 12:32 UT
Penumbral Lunar Eclipse
(penum. mag. 0.70; Saros 140)
|
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 34 minutes.
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11 Apr, 1922 AD
max: 20:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.78; Saros 140)
|
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 43 minutes.
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22 Apr, 1940 AD
max: 04:26 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 140)
|
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 53 minutes overall.
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3 May, 1958 AD
max: 12:12 UT
Partial Lunar Eclipse
(umbral mag. 0.01; Saros 140)
|
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 21 minutes exactly.
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13 May, 1976 AD
max: 19:54 UT
Partial Lunar Eclipse
(umbral mag. 0.12; Saros 140)
|
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 15 minutes, with just 12% of the Moon in shadow at maximum.
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25 May, 1994 AD
max: 03:30 UT
Partial Lunar Eclipse
(umbral mag. 0.24; Saros 140)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 24% of the Moon in shadow; the partial eclipse lasted for 1 hour and 45 minutes.
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4 Jun, 2012 AD
08:48–13:18 UT
Partial Lunar Eclipse
(umbral mag. 0.37; Saros 140)
|
The Earth's shadow on the moon was clearly visible in this eclipse, with 37% of the Moon in shadow; the partial eclipse lasted for 2 hours and 7 minutes and was visible from the Americas, the Pacific, south-east Asia and Australia.
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15 Jun, 2030 AD
16:14–20:52 UT
Partial Lunar Eclipse
(umbral mag. 0.50; Saros 140)
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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 24 minutes and will be visible from most of Europe, Africa, Asia, and Australia.
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26 Jun, 2048 AD
max: 02:00 UT
Partial Lunar Eclipse
(umbral mag. 0.64; Saros 140)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 39 minutes, with 64% of the Moon in darkness at maximum.
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7 Jul, 2066 AD
max: 09:28 UT
Partial Lunar Eclipse
(umbral mag. 0.78; Saros 140)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 51 minutes, with 78% of the Moon in darkness at maximum.
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17 Jul, 2084 AD
max: 16:56 UT
Partial Lunar Eclipse
(umbral mag. 0.91; Saros 140)
|
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 1 minute. With 91% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
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30 Jul, 2102 AD
max: 00:25 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 140)
|
The Moon will barely edge into total eclipse for 31 minutes and 18 seconds. 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 10 minutes in total.
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9 Aug, 2120 AD
max: 07:57 UT
Total Lunar Eclipse
(umbral mag. 1.18; Saros 140)
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A shallow total eclipse will see the Moon in relative darkness for 59 minutes and 18 seconds. The Moon will be 18% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 16 minutes in total.
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20 Aug, 2138 AD
max: 15:33 UT
Total Lunar Eclipse
(umbral mag. 1.30; Saros 140)
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The Moon will be plunged into darkness for 1 hour and 14 minutes, in a deep total eclipse which will see the Moon 30% 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 21 minutes in total.
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30 Aug, 2156 AD
max: 23:14 UT
Total Lunar Eclipse
(umbral mag. 1.41; Saros 140)
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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 41% 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 25 minutes in total.
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11 Sep, 2174 AD
max: 07:01 UT
Total Lunar Eclipse
(umbral mag. 1.52; Saros 140)
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The Moon will be plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which will see the Moon 52% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 27 minutes in total.
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21 Sep, 2192 AD
max: 14:55 UT
Total Lunar Eclipse
(umbral mag. 1.62; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 34 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 29 minutes in total.
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3 Oct, 2210 AD
max: 22:56 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 37 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 30 minutes in total.
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14 Oct, 2228 AD
max: 07:04 UT
Total Lunar Eclipse
(umbral mag. 1.77; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 38 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 31 minutes in total.
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25 Oct, 2246 AD
max: 15:19 UT
Total Lunar Eclipse
(umbral mag. 1.83; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 39 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 31 minutes in total.
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4 Nov, 2264 AD
max: 23:42 UT
Total Lunar Eclipse
(umbral mag. 1.87; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 39 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 31 minutes in total.
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16 Nov, 2282 AD
max: 08:12 UT
Total Lunar Eclipse
(umbral mag. 1.83; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 38 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 31 minutes in total.
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27 Nov, 2300 AD
max: 16:48 UT
Total Lunar Eclipse
(umbral mag. 1.80; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 38 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 31 minutes in total.
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9 Dec, 2318 AD
max: 01:29 UT
Total Lunar Eclipse
(umbral mag. 1.77; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 38 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 31 minutes in total.
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19 Dec, 2336 AD
max: 10:15 UT
Total Lunar Eclipse
(umbral mag. 1.76; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 38 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 31 minutes in total.
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30 Dec, 2354 AD
max: 19:02 UT
Total Lunar Eclipse
(umbral mag. 1.74; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 38 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 31 minutes in total.
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10 Jan, 2373 AD
max: 03:51 UT
Total Lunar Eclipse
(umbral mag. 1.73; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 37 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 32 minutes in total.
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21 Jan, 2391 AD
max: 12:39 UT
Total Lunar Eclipse
(umbral mag. 1.72; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 37 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 32 minutes in total.
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31 Jan, 2409 AD
max: 21:26 UT
Total Lunar Eclipse
(umbral mag. 1.72; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 37 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 32 minutes in total.
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12 Feb, 2427 AD
max: 06:08 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 37 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 32 minutes in total.
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22 Feb, 2445 AD
max: 14:46 UT
Total Lunar Eclipse
(umbral mag. 1.68; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 37 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 32 minutes in total.
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5 Mar, 2463 AD
max: 23:17 UT
Total Lunar Eclipse
(umbral mag. 1.65; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 36 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 33 minutes in total.
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16 Mar, 2481 AD
max: 07:43 UT
Total Lunar Eclipse
(umbral mag. 1.61; Saros 140)
|
A dramatic total eclipse lasting 1 hour and 35 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 32 minutes in total.
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27 Mar, 2499 AD
max: 15:58 UT
Total Lunar Eclipse
(umbral mag. 1.55; Saros 140)
|
The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see the Moon 55% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 32 minutes in total.
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8 Apr, 2517 AD
max: 00:07 UT
Total Lunar Eclipse
(umbral mag. 1.49; Saros 140)
|
The Moon will be plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which will see the Moon 49% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 31 minutes in total.
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19 Apr, 2535 AD
max: 08:06 UT
Total Lunar Eclipse
(umbral mag. 1.41; Saros 140)
|
The Moon will be plunged into darkness for 1 hour and 26 minutes, in a deep total eclipse which will see the Moon 41% 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 30 minutes in total.
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29 Apr, 2553 AD
max: 15:58 UT
Total Lunar Eclipse
(umbral mag. 1.33; Saros 140)
|
The Moon will be plunged into darkness for 1 hour and 19 minutes, in a deep total eclipse which will see the Moon 33% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 27 minutes in total.
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10 May, 2571 AD
max: 23:39 UT
Total Lunar Eclipse
(umbral mag. 1.23; Saros 140)
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The Moon will be plunged into darkness for 1 hour and 8 minutes, in a deep total eclipse which will see the Moon 23% 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 24 minutes in total.
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21 May, 2589 AD
max: 07:14 UT
Total Lunar Eclipse
(umbral mag. 1.12; Saros 140)
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A shallow total eclipse will see the Moon in relative darkness for 50 minutes and 30 seconds. The Moon will be 12% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 19 minutes in total.
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2 Jun, 2607 AD
max: 14:41 UT
Partial Lunar Eclipse
(umbral mag. 0.99; Saros 140)
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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 13 minutes. With 99% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
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12 Jun, 2625 AD
max: 22:02 UT
Partial Lunar Eclipse
(umbral mag. 0.86; Saros 140)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 5 minutes, with 86% of the Moon in darkness at maximum.
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24 Jun, 2643 AD
max: 05:16 UT
Partial Lunar Eclipse
(umbral mag. 0.72; Saros 140)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 54 minutes, with 72% of the Moon in darkness at maximum.
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4 Jul, 2661 AD
max: 12:27 UT
Partial Lunar Eclipse
(umbral mag. 0.58; Saros 140)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 58% of the Moon in shadow; the partial eclipse will last for 2 hours and 40 minutes.
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15 Jul, 2679 AD
max: 19:35 UT
Partial Lunar Eclipse
(umbral mag. 0.44; Saros 140)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 44% of the Moon in shadow; the partial eclipse will last for 2 hours and 22 minutes.
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26 Jul, 2697 AD
max: 02:40 UT
Partial Lunar Eclipse
(umbral mag. 0.29; Saros 140)
|
The Earth's shadow on the moon will be clearly visible in this eclipse, with 29% of the Moon in shadow; the partial eclipse will last for 1 hour and 58 minutes.
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7 Aug, 2715 AD
max: 09:45 UT
Partial Lunar Eclipse
(umbral mag. 0.14; Saros 140)
|
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 25 minutes, with just 14% of the Moon in shadow at maximum.
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17 Aug, 2733 AD
max: 16:51 UT
Penumbral Lunar Eclipse
(penum. mag. 1.00; Saros 140)
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The Moon will approach within 0% of the Earth's umbral shadow at maximum eclipse; 100% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 4 hours and 21 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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28 Aug, 2751 AD
max: 23:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 140)
|
At maximum eclipse, 87% 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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8 Sep, 2769 AD
max: 07:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 140)
|
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 3 hours and 52 minutes.
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19 Sep, 2787 AD
max: 14:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 140)
|
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 62% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 36 minutes.
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29 Sep, 2805 AD
max: 21:45 UT
Penumbral Lunar Eclipse
(penum. mag. 0.51; Saros 140)
|
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 19 minutes, just 51% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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11 Oct, 2823 AD
max: 05:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.41; Saros 140)
|
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 2 minutes, just 41% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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21 Oct, 2841 AD
max: 12:45 UT
Penumbral Lunar Eclipse
(penum. mag. 0.33; Saros 140)
|
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 43 minutes, just 33% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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1 Nov, 2859 AD
max: 20:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.25; Saros 140)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 25 minutes, just 25% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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12 Nov, 2877 AD
max: 04:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.19; Saros 140)
|
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 19% of the Moon's disc for 2 hours and 7 minutes, which will be essentially impossible to see.
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23 Nov, 2895 AD
max: 12:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros 140)
|
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 14% of the Moon's disc for 1 hour and 49 minutes, which will be essentially impossible to see.
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4 Dec, 2913 AD
max: 20:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros 140)
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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 9% of the Moon's disc for 1 hour and 31 minutes, which will be essentially impossible to see.
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16 Dec, 2931 AD
max: 04:10 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 140)
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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 6% of the Moon's disc for 1 hour and 15 minutes, which will be essentially impossible to see.
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26 Dec, 2949 AD
max: 12:19 UT
Penumbral Lunar Eclipse
(penum. mag. 0.04; Saros 140)
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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 56 minutes and 54 seconds, which will be essentially impossible to see.
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6 Jan, 2968 AD
max: 20:30 UT
Penumbral Lunar Eclipse
(penum. mag. 0.01; Saros 140)
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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 1% of the Moon's disc for 36 minutes and 54 seconds, which will be essentially impossible to see.
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