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.
10 Mar, 0993 AD
max: 23:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.01; Saros 116)
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In this virtually non-existant eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow; although the eclipse lasted 26 minutes and 30 seconds, it was impossible to see in practice.
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22 Mar, 1011 AD
max: 07:48 UT
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 116)
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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 8% of the Moon's disc for 1 hour and 17 minutes, which was essentially impossible to see.
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1 Apr, 1029 AD
max: 15:45 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 116)
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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 17% of the Moon's disc for 1 hour and 48 minutes, which was essentially impossible to see.
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12 Apr, 1047 AD
max: 23:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.26; Saros 116)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 14 minutes, just 26% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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23 Apr, 1065 AD
max: 07:22 UT
Penumbral Lunar Eclipse
(penum. mag. 0.37; Saros 116)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 37 minutes, just 37% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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4 May, 1083 AD
max: 15:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 116)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 57 minutes, just 48% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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14 May, 1101 AD
max: 22:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.60; Saros 116)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 60% 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 16 minutes.
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26 May, 1119 AD
max: 06:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.73; Saros 116)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 73% 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 32 minutes.
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5 Jun, 1137 AD
max: 13:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.86; Saros 116)
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At maximum eclipse, 86% 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 48 minutes overall.
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16 Jun, 1155 AD
max: 21:06 UT
Partial Lunar Eclipse
(umbral mag. 0.05; Saros 116)
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A tiny bite out of the Moon may have been visible at maximum, though just 5% of the Moon was shadowed in a partial eclipse which lasted for 48 minutes and 54 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
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27 Jun, 1173 AD
max: 04:34 UT
Partial Lunar Eclipse
(umbral mag. 0.18; Saros 116)
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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 31 minutes, with just 18% of the Moon in shadow at maximum.
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8 Jul, 1191 AD
max: 12:03 UT
Partial Lunar Eclipse
(umbral mag. 0.31; Saros 116)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 31% of the Moon in shadow; the partial eclipse lasted for 1 hour and 57 minutes.
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18 Jul, 1209 AD
max: 19:35 UT
Partial Lunar Eclipse
(umbral mag. 0.44; Saros 116)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 44% of the Moon in shadow; the partial eclipse lasted for 2 hours and 16 minutes.
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30 Jul, 1227 AD
max: 03:11 UT
Partial Lunar Eclipse
(umbral mag. 0.56; Saros 116)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 56% of the Moon in shadow; the partial eclipse lasted for 2 hours and 31 minutes.
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9 Aug, 1245 AD
max: 10:52 UT
Partial Lunar Eclipse
(umbral mag. 0.67; Saros 116)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 42 minutes, with 67% of the Moon in darkness at maximum.
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20 Aug, 1263 AD
max: 18:37 UT
Partial Lunar Eclipse
(umbral mag. 0.77; Saros 116)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 52 minutes, with 77% of the Moon in darkness at maximum.
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31 Aug, 1281 AD
max: 02:29 UT
Partial Lunar Eclipse
(umbral mag. 0.86; Saros 116)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 59 minutes, with 86% of the Moon in darkness at maximum.
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11 Sep, 1299 AD
max: 10:28 UT
Partial Lunar Eclipse
(umbral mag. 0.94; Saros 116)
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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 5 minutes. With 94% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
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21 Sep, 1317 AD
max: 18:34 UT
Total Lunar Eclipse
(umbral mag. 1.01; Saros 116)
|
The Moon barely edged into total eclipse for just 17 minutes and 6 seconds. With the Moon just 1% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 9 minutes in total.
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3 Oct, 1335 AD
max: 02:47 UT
Total Lunar Eclipse
(umbral mag. 1.07; Saros 116)
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A shallow total eclipse saw the Moon in relative darkness for 39 minutes and 6 seconds. The Moon was 7% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 13 minutes in total.
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13 Oct, 1353 AD
max: 11:07 UT
Total Lunar Eclipse
(umbral mag. 1.11; Saros 116)
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A shallow total eclipse saw the Moon in relative darkness for 49 minutes and 18 seconds. The Moon was 11% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 15 minutes in total.
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24 Oct, 1371 AD
max: 19:34 UT
Total Lunar Eclipse
(umbral mag. 1.15; Saros 116)
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A shallow total eclipse saw the Moon in relative darkness for 55 minutes and 42 seconds. The Moon was 15% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 17 minutes in total.
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4 Nov, 1389 AD
max: 04:07 UT
Total Lunar Eclipse
(umbral mag. 1.17; Saros 116)
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A shallow total eclipse saw the Moon in relative darkness for 59 minutes and 36 seconds. The Moon was 17% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 19 minutes in total.
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15 Nov, 1407 AD
max: 12:45 UT
Total Lunar Eclipse
(umbral mag. 1.19; Saros 116)
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A shallow total eclipse saw the Moon in relative darkness for 1 hour and 2 minutes. The Moon was 19% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 20 minutes in total.
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25 Nov, 1425 AD
max: 21:27 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 116)
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A shallow total eclipse saw the Moon in relative darkness for 1 hour and 3 minutes. The Moon was 20% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 21 minutes in total.
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7 Dec, 1443 AD
max: 06:11 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 116)
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The Moon was plunged into darkness for 1 hour and 4 minutes, in a deep total eclipse which saw the Moon 20% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 21 minutes in total.
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17 Dec, 1461 AD
max: 14:56 UT
Total Lunar Eclipse
(umbral mag. 1.20; Saros 116)
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The Moon was plunged into darkness for 1 hour and 5 minutes, in a deep total eclipse which saw the Moon 20% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 22 minutes in total.
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28 Dec, 1479 AD
max: 23:39 UT
Total Lunar Eclipse
(umbral mag. 1.21; Saros 116)
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The Moon was plunged into darkness for 1 hour and 5 minutes, in a deep total eclipse which saw the Moon 21% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 23 minutes in total.
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8 Jan, 1498 AD
max: 08:22 UT
Total Lunar Eclipse
(umbral mag. 1.21; Saros 116)
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The Moon was plunged into darkness for 1 hour and 6 minutes, in a deep total eclipse which saw the Moon 21% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 23 minutes in total.
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19 Jan, 1516 AD
max: 16:59 UT
Total Lunar Eclipse
(umbral mag. 1.22; Saros 116)
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The Moon was plunged into darkness for 1 hour and 8 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 24 minutes in total.
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30 Jan, 1534 AD
max: 01:31 UT
Total Lunar Eclipse
(umbral mag. 1.24; Saros 116)
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The Moon was plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which saw the Moon 24% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 25 minutes in total.
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10 Feb, 1552 AD
max: 09:56 UT
Total Lunar Eclipse
(umbral mag. 1.27; Saros 116)
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The Moon was plunged into darkness for 1 hour and 14 minutes, in a deep total eclipse which saw the Moon 27% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 27 minutes in total.
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20 Feb, 1570 AD
max: 18:14 UT
Total Lunar Eclipse
(umbral mag. 1.31; Saros 116)
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The Moon was plunged into darkness for 1 hour and 18 minutes, in a deep total eclipse which saw the Moon 31% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 29 minutes in total.
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13 Mar, 1588 AD
max: 02:21 UT
Total Lunar Eclipse
(umbral mag. 1.36; Saros 116)
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The Moon was plunged into darkness for 1 hour and 23 minutes, in a deep total eclipse which saw the Moon 36% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 32 minutes in total.
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24 Mar, 1606 AD
max: 10:21 UT
Total Lunar Eclipse
(umbral mag. 1.42; Saros 116)
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The Moon was plunged into darkness for 1 hour and 28 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 34 minutes in total.
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3 Apr, 1624 AD
max: 18:10 UT
Total Lunar Eclipse
(umbral mag. 1.50; Saros 116)
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The Moon was plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which saw the Moon 50% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 37 minutes in total.
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15 Apr, 1642 AD
max: 01:51 UT
Total Lunar Eclipse
(umbral mag. 1.59; Saros 116)
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A dramatic total eclipse lasting 1 hour and 37 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 39 minutes in total.
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25 Apr, 1660 AD
max: 09:21 UT
Total Lunar Eclipse
(umbral mag. 1.69; Saros 116)
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A dramatic total eclipse lasting 1 hour and 41 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 41 minutes in total.
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6 May, 1678 AD
max: 16:44 UT
Total Lunar Eclipse
(umbral mag. 1.80; Saros 116)
|
A dramatic total eclipse lasting 1 hour and 43 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 43 minutes in total.
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16 May, 1696 AD
max: 23:58 UT
Total Lunar Eclipse
(umbral mag. 1.78; Saros 116)
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A dramatic total eclipse lasting 1 hour and 43 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 44 minutes in total.
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29 May, 1714 AD
max: 07:04 UT
Total Lunar Eclipse
(umbral mag. 1.65; Saros 116)
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A dramatic total eclipse lasting 1 hour and 40 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 43 minutes in total.
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8 Jun, 1732 AD
max: 14:06 UT
Total Lunar Eclipse
(umbral mag. 1.50; Saros 116)
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The Moon was plunged into darkness for 1 hour and 35 minutes, in a deep total eclipse which saw the Moon 50% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 41 minutes in total.
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19 Jun, 1750 AD
max: 21:02 UT
Total Lunar Eclipse
(umbral mag. 1.36; Saros 116)
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The Moon was plunged into darkness for 1 hour and 25 minutes, in a deep total eclipse which saw the Moon 36% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 38 minutes in total.
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30 Jun, 1768 AD
max: 03:56 UT
Total Lunar Eclipse
(umbral mag. 1.21; Saros 116)
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The Moon was plunged into darkness for 1 hour and 8 minutes, in a deep total eclipse which saw the Moon 21% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 33 minutes in total.
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11 Jul, 1786 AD
max: 10:47 UT
Total Lunar Eclipse
(umbral mag. 1.05; Saros 116)
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A shallow total eclipse saw the Moon in relative darkness for 36 minutes and 18 seconds. The Moon was 5% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 25 minutes in total.
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22 Jul, 1804 AD
max: 17:37 UT
Partial Lunar Eclipse
(umbral mag. 0.90; Saros 116)
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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 16 minutes. With 90% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
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3 Aug, 1822 AD
max: 00:29 UT
Partial Lunar Eclipse
(umbral mag. 0.75; Saros 116)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 4 minutes, with 75% of the Moon in darkness at maximum.
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13 Aug, 1840 AD
max: 07:23 UT
Partial Lunar Eclipse
(umbral mag. 0.61; Saros 116)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 50 minutes, with 61% of the Moon in darkness at maximum.
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24 Aug, 1858 AD
max: 14:20 UT
Partial Lunar Eclipse
(umbral mag. 0.47; Saros 116)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 47% of the Moon in shadow; the partial eclipse lasted for 2 hours and 33 minutes.
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3 Sep, 1876 AD
max: 21:22 UT
Partial Lunar Eclipse
(umbral mag. 0.34; Saros 116)
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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 14 minutes.
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15 Sep, 1894 AD
max: 04:31 UT
Partial Lunar Eclipse
(umbral mag. 0.23; Saros 116)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 23% of the Moon in shadow; the partial eclipse lasted for 1 hour and 51 minutes.
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26 Sep, 1912 AD
max: 11:44 UT
Partial Lunar Eclipse
(umbral mag. 0.12; Saros 116)
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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 22 minutes, with just 12% of the Moon in shadow at maximum.
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7 Oct, 1930 AD
max: 19:06 UT
Partial Lunar Eclipse
(umbral mag. 0.03; Saros 116)
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A tiny bite out of the Moon may have been visible at maximum, though just 3% of the Moon was shadowed in a partial eclipse which lasted for 38 minutes and 18 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
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18 Oct, 1948 AD
max: 02:35 UT
Penumbral Lunar Eclipse
(penum. mag. 1.01; Saros 116)
|
In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 40 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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29 Oct, 1966 AD
max: 10:12 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 116)
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At maximum eclipse, 95% 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 34 minutes overall.
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8 Nov, 1984 AD
max: 17:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 116)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 90% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 28 minutes.
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20 Nov, 2002 AD
23:34 on 19 Nov–03:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.86; Saros 116)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 86% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 24 minutes. The Moon was visible from the Americas, Europe, Africa, and most of Asia.
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30 Nov, 2020 AD
07:32–11:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 116)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 83% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 21 minutes. The Moon was visible from east Asia, Australia, and the Americas.
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11 Dec, 2038 AD
15:34–19:52 UT
Penumbral Lunar Eclipse
(penum. mag. 0.80; Saros 116)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 80% 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 19 minutes. The Moon will be visible from Europe, Africa, Asia, and north-western North America.
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22 Dec, 2056 AD
max: 01:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.79; Saros 116)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 79% 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 16 minutes.
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2 Jan, 2075 AD
max: 09:52 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 116)
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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 15 minutes.
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12 Jan, 2093 AD
max: 17:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 116)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 76% 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 13 minutes.
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25 Jan, 2111 AD
max: 01:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 116)
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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 11 minutes.
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4 Feb, 2129 AD
max: 09:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.71; Saros 116)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 71% 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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15 Feb, 2147 AD
max: 17:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 116)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 68% 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 3 minutes.
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26 Feb, 2165 AD
max: 01:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.64; Saros 116)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 64% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 57 minutes.
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9 Mar, 2183 AD
max: 09:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.60; Saros 116)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 49 minutes, just 60% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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20 Mar, 2201 AD
max: 16:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.53; Saros 116)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 38 minutes, just 53% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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1 Apr, 2219 AD
max: 00:10 UT
Penumbral Lunar Eclipse
(penum. mag. 0.46; Saros 116)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 24 minutes, just 46% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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11 Apr, 2237 AD
max: 07:21 UT
Penumbral Lunar Eclipse
(penum. mag. 0.37; Saros 116)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 4 minutes, just 37% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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22 Apr, 2255 AD
max: 14:26 UT
Penumbral Lunar Eclipse
(penum. mag. 0.27; Saros 116)
|
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 39 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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2 May, 2273 AD
max: 21:21 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros 116)
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In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 16% of the Moon's disc for 2 hours and 3 minutes, which will be essentially impossible to see.
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14 May, 2291 AD
max: 04:08 UT
Penumbral Lunar Eclipse
(penum. mag. 0.04; Saros 116)
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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 1 hour and 1 minute, which will be essentially impossible to see.
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