Lunar Eclipses in Saros Series 117

This page lists all the lunar eclipses in saros series 117. The series contains 71 eclipses, occurring over 1262 years.

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.

Note that eclipse dates are specified relative to UT.
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3 Apr, 1094 AD
Penumbral Lunar Eclipse
(penum. mag. 0.04; Saros 117)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 4% of the Moon's disc for 1 hour exactly, which was essentially impossible to see.
14 Apr, 1112 AD
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros 117)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 14% of the Moon's disc for 1 hour and 51 minutes, which was essentially impossible to see.
25 Apr, 1130 AD
Penumbral Lunar Eclipse
(penum. mag. 0.25; Saros 117)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 27 minutes, just 25% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
5 May, 1148 AD
Penumbral Lunar Eclipse
(penum. mag. 0.38; Saros 117)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 58 minutes, just 38% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
16 May, 1166 AD
Penumbral Lunar Eclipse
(penum. mag. 0.51; Saros 117)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 25 minutes, just 51% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
27 May, 1184 AD
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 117)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 65% 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 49 minutes.
7 Jun, 1202 AD
Penumbral Lunar Eclipse
(penum. mag. 0.79; Saros 117)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 79% 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 10 minutes.
17 Jun, 1220 AD
Penumbral Lunar Eclipse
(penum. mag. 0.94; Saros 117)
At maximum eclipse, 94% 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 30 minutes overall.
29 Jun, 1238 AD
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 117)
A tiny bite out of the Moon may have been visible at maximum, though just 4% of the Moon was shadowed in a partial eclipse which lasted for 50 minutes and 42 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
9 Jul, 1256 AD
Partial Lunar Eclipse
(umbral mag. 0.19; Saros 117)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 43 minutes, with just 19% of the Moon in shadow at maximum.
20 Jul, 1274 AD
Partial Lunar Eclipse
(umbral mag. 0.33; Saros 117)
The Earth's shadow on the moon was clearly visible in this eclipse, with 33% of the Moon in shadow; the partial eclipse lasted for 2 hours and 14 minutes.
30 Jul, 1292 AD
Partial Lunar Eclipse
(umbral mag. 0.47; Saros 117)
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 36 minutes.
11 Aug, 1310 AD
Partial Lunar Eclipse
(umbral mag. 0.59; Saros 117)
The Earth's shadow on the moon was clearly visible in this eclipse, with 59% of the Moon in shadow; the partial eclipse lasted for 2 hours and 53 minutes.
21 Aug, 1328 AD
Partial Lunar Eclipse
(umbral mag. 0.71; Saros 117)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 6 minutes, with 71% of the Moon in darkness at maximum.
1 Sep, 1346 AD
Partial Lunar Eclipse
(umbral mag. 0.82; Saros 117)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 16 minutes, with 82% of the Moon in darkness at maximum.
11 Sep, 1364 AD
Partial Lunar Eclipse
(umbral mag. 0.92; Saros 117)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 24 minutes. With 92% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
23 Sep, 1382 AD
Partial Lunar Eclipse
(umbral mag. 1.00; Saros 117)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 30 minutes. With 100% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
3 Oct, 1400 AD
Total Lunar Eclipse
(umbral mag. 1.07; Saros 117)
A shallow total eclipse saw the Moon in relative darkness for 41 minutes and 42 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 34 minutes in total.
14 Oct, 1418 AD
Total Lunar Eclipse
(umbral mag. 1.12; Saros 117)
A shallow total eclipse saw the Moon in relative darkness for 56 minutes exactly. The Moon was 12% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 38 minutes in total.
25 Oct, 1436 AD
Total Lunar Eclipse
(umbral mag. 1.17; Saros 117)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 4 minutes. 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 40 minutes in total.
5 Nov, 1454 AD
Total Lunar Eclipse
(umbral mag. 1.20; Saros 117)
The Moon was plunged into darkness for 1 hour and 10 minutes, in a deep total eclipse which saw the Moon 20% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 42 minutes in total.
15 Nov, 1472 AD
Total Lunar Eclipse
(umbral mag. 1.23; Saros 117)
The Moon was plunged into darkness for 1 hour and 13 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 43 minutes in total.
27 Nov, 1490 AD
Total Lunar Eclipse
(umbral mag. 1.25; Saros 117)
The Moon was plunged into darkness for 1 hour and 16 minutes, in a deep total eclipse which saw the Moon 25% 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 44 minutes in total.
7 Dec, 1508 AD
Total Lunar Eclipse
(umbral mag. 1.26; Saros 117)
The Moon was plunged into darkness for 1 hour and 17 minutes, in a deep total eclipse which saw the Moon 26% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 44 minutes in total.
18 Dec, 1526 AD
Total Lunar Eclipse
(umbral mag. 1.28; Saros 117)
The Moon was plunged into darkness for 1 hour and 19 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 45 minutes in total.
29 Dec, 1544 AD
Total Lunar Eclipse
(umbral mag. 1.29; Saros 117)
The Moon was plunged into darkness for 1 hour and 21 minutes, in a deep total eclipse which saw the Moon 29% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 46 minutes in total.
9 Jan, 1563 AD
Total Lunar Eclipse
(umbral mag. 1.31; Saros 117)
The Moon was plunged into darkness for 1 hour and 23 minutes, in a deep total eclipse which saw the Moon 31% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 46 minutes in total.
19 Jan, 1581 AD
Total Lunar Eclipse
(umbral mag. 1.33; Saros 117)
The Moon was plunged into darkness for 1 hour and 25 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 47 minutes in total.
10 Feb, 1599 AD
Total Lunar Eclipse
(umbral mag. 1.37; Saros 117)
The Moon was plunged into darkness for 1 hour and 28 minutes, in a deep total eclipse which saw the Moon 37% 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 48 minutes in total.
20 Feb, 1617 AD
Total Lunar Eclipse
(umbral mag. 1.41; Saros 117)
The Moon was plunged into darkness for 1 hour and 31 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 49 minutes in total.
3 Mar, 1635 AD
Total Lunar Eclipse
(umbral mag. 1.47; Saros 117)
The Moon was plunged into darkness for 1 hour and 35 minutes, in a deep total eclipse which saw the Moon 47% 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 51 minutes in total.
14 Mar, 1653 AD
Total Lunar Eclipse
(umbral mag. 1.53; Saros 117)
The Moon was plunged into darkness for 1 hour and 39 minutes, in a deep total eclipse which saw the Moon 53% 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 52 minutes in total.
25 Mar, 1671 AD
Total Lunar Eclipse
(umbral mag. 1.62; Saros 117)
A dramatic total eclipse lasting 1 hour and 42 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 53 minutes in total.
4 Apr, 1689 AD
Total Lunar Eclipse
(umbral mag. 1.71; Saros 117)
A dramatic total eclipse lasting 1 hour and 45 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 54 minutes in total.
17 Apr, 1707 AD
Total Lunar Eclipse
(umbral mag. 1.82; Saros 117)
A dramatic total eclipse lasting 1 hour and 46 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 54 minutes in total.
27 Apr, 1725 AD
Total Lunar Eclipse
(umbral mag. 1.71; Saros 117)
A dramatic total eclipse lasting 1 hour and 45 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 54 minutes in total.
8 May, 1743 AD
Total Lunar Eclipse
(umbral mag. 1.58; Saros 117)
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 52 minutes in total.
18 May, 1761 AD
Total Lunar Eclipse
(umbral mag. 1.45; Saros 117)
The Moon was plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which saw the Moon 45% 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 49 minutes in total.
30 May, 1779 AD
Total Lunar Eclipse
(umbral mag. 1.31; Saros 117)
The Moon was plunged into darkness for 1 hour and 22 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 43 minutes in total.
9 Jun, 1797 AD
Total Lunar Eclipse
(umbral mag. 1.16; Saros 117)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 2 minutes. The Moon was 16% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 37 minutes in total.
21 Jun, 1815 AD
Total Lunar Eclipse
(umbral mag. 1.01; Saros 117)
The Moon barely edged into total eclipse for just 14 minutes and 42 seconds. With the Moon just barely inside the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 27 minutes in total.
2 Jul, 1833 AD
Partial Lunar Eclipse
(umbral mag. 0.86; Saros 117)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 16 minutes, with 86% of the Moon in darkness at maximum.
13 Jul, 1851 AD
Partial Lunar Eclipse
(umbral mag. 0.71; Saros 117)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 2 minutes, with 71% of the Moon in darkness at maximum.
23 Jul, 1869 AD
Partial Lunar Eclipse
(umbral mag. 0.56; Saros 117)
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 46 minutes.
3 Aug, 1887 AD
Partial Lunar Eclipse
(umbral mag. 0.42; Saros 117)
The Earth's shadow on the moon was clearly visible in this eclipse, with 42% of the Moon in shadow; the partial eclipse lasted for 2 hours and 26 minutes.
15 Aug, 1905 AD
Partial Lunar Eclipse
(umbral mag. 0.29; Saros 117)
The Earth's shadow on the moon was clearly visible in this eclipse, with 29% of the Moon in shadow; the partial eclipse lasted for 2 hours and 3 minutes.
26 Aug, 1923 AD
Partial Lunar Eclipse
(umbral mag. 0.16; Saros 117)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 34 minutes, with just 16% of the Moon in shadow at maximum.
5 Sep, 1941 AD
Partial Lunar Eclipse
(umbral mag. 0.05; Saros 117)
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 53 minutes and 24 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
17 Sep, 1959 AD
Penumbral Lunar Eclipse
(penum. mag. 0.99; Saros 117)
The Moon approached within 5% of the Earth's umbral shadow at maximum eclipse, with the overall eclipse lasting 4 hours and 28 minutes. While less dramatic than a partial eclipse (as no part of the Moon was in complete shadow), a shading across the Moon should have been readily visible to observers.
27 Sep, 1977 AD
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 117)
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 18 minutes overall.
8 Oct, 1995 AD
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 117)
This subtle penumbral eclipse 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 8 minutes.
18 Oct, 2013 AD
(... 19 Oct UT)
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 117)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 76% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 59 minutes. The Moon was visible from the Americas (for the end), Europe, Africa, and most of Asia (the beginning of the eclipse will be visible in east Asia).
30 Oct, 2031 AD
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 117)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 72% 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. The Moon will be visible in the Americas, eastern Asia and Australia, and western Europe and Africa.
9 Nov, 2049 AD
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 117)
This subtle penumbral eclipse 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 3 hours and 46 minutes.
21 Nov, 2067 AD
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 117)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 65% 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 42 minutes.
1 Dec, 2085 AD
Penumbral Lunar Eclipse
(penum. mag. 0.64; Saros 117)
This subtle penumbral eclipse 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 39 minutes.
13 Dec, 2103 AD
Penumbral Lunar Eclipse
(penum. mag. 0.63; Saros 117)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 63% 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.
24 Dec, 2121 AD
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 117)
This subtle penumbral eclipse 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 35 minutes.
4 Jan, 2140 AD
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 117)
This subtle penumbral eclipse 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 34 minutes.
14 Jan, 2158 AD
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 117)
This subtle penumbral eclipse 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 33 minutes.
26 Jan, 2176 AD
Penumbral Lunar Eclipse
(penum. mag. 0.61; Saros 117)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 61% 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 31 minutes.
5 Feb, 2194 AD
Penumbral Lunar Eclipse
(penum. mag. 0.60; Saros 117)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 60% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 29 minutes.
17 Feb, 2212 AD
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 117)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 25 minutes, just 59% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
28 Feb, 2230 AD
Penumbral Lunar Eclipse
(penum. mag. 0.56; Saros 117)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 21 minutes, just 56% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
10 Mar, 2248 AD
Penumbral Lunar Eclipse
(penum. mag. 0.53; Saros 117)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 14 minutes, just 53% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
21 Mar, 2266 AD
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 117)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 5 minutes, just 48% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
1 Apr, 2284 AD
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros 117)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 54 minutes, just 42% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
13 Apr, 2302 AD
Penumbral Lunar Eclipse
(penum. mag. 0.36; Saros 117)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 40 minutes, just 36% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
23 Apr, 2320 AD
Penumbral Lunar Eclipse
(penum. mag. 0.27; Saros 117)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 21 minutes, just 27% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
5 May, 2338 AD
Penumbral Lunar Eclipse
(penum. mag. 0.19; Saros 117)
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 1 hour and 57 minutes, which will be essentially impossible to see.
15 May, 2356 AD
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros 117)
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 20 minutes, which will be essentially impossible to see.