Lunar Eclipses in Saros Series 120

This page lists all the lunar eclipses in saros series 120 which are in our database.

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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16 Oct, 1000 AD
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 120)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 3% of the Moon's disc for 47 minutes and 6 seconds, which was essentially impossible to see.
27 Oct, 1018 AD
Penumbral Lunar Eclipse
(penum. mag. 0.05; Saros 120)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 5% of the Moon's disc for 1 hour and 5 minutes, which was essentially impossible to see.
6 Nov, 1036 AD
Penumbral Lunar Eclipse
(penum. mag. 0.07; Saros 120)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 7% of the Moon's disc for 1 hour and 15 minutes, which was essentially impossible to see.
18 Nov, 1054 AD
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 120)
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 20 minutes, which was essentially impossible to see.
28 Nov, 1072 AD
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 120)
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 22 minutes, which was essentially impossible to see.
9 Dec, 1090 AD
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 120)
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 22 minutes, which was essentially impossible to see.
20 Dec, 1108 AD
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 120)
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 22 minutes, which was essentially impossible to see.
31 Dec, 1126 AD
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 120)
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 21 minutes, which was essentially impossible to see.
10 Jan, 1145 AD
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 120)
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 24 minutes, which was essentially impossible to see.
22 Jan, 1163 AD
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros 120)
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 29 minutes, which was essentially impossible to see.
1 Feb, 1181 AD
Penumbral Lunar Eclipse
(penum. mag. 0.11; Saros 120)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 11% of the Moon's disc for 1 hour and 38 minutes, which was essentially impossible to see.
12 Feb, 1199 AD
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros 120)
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 49 minutes, which was essentially impossible to see.
23 Feb, 1217 AD
Penumbral Lunar Eclipse
(penum. mag. 0.18; Saros 120)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 18% of the Moon's disc for 2 hours and 4 minutes, which was essentially impossible to see.
6 Mar, 1235 AD
Penumbral Lunar Eclipse
(penum. mag. 0.23; Saros 120)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 20 minutes, just 23% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
16 Mar, 1253 AD
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 120)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 39 minutes, just 30% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
28 Mar, 1271 AD
Penumbral Lunar Eclipse
(penum. mag. 0.38; Saros 120)
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).
7 Apr, 1289 AD
Penumbral Lunar Eclipse
(penum. mag. 0.47; Saros 120)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 18 minutes, just 47% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
18 Apr, 1307 AD
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 120)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 37 minutes, just 58% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
29 Apr, 1325 AD
Penumbral Lunar Eclipse
(penum. mag. 0.70; Saros 120)
This subtle penumbral eclipse 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 56 minutes.
10 May, 1343 AD
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 120)
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 15 minutes.
20 May, 1361 AD
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 120)
At maximum eclipse, 96% 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 32 minutes overall.
31 May, 1379 AD
Partial Lunar Eclipse
(umbral mag. 0.06; Saros 120)
A tiny bite out of the Moon may have been visible at maximum, though just 6% of the Moon was shadowed in a partial eclipse which lasted for 58 minutes and 48 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
11 Jun, 1397 AD
Partial Lunar Eclipse
(umbral mag. 0.21; Saros 120)
The Earth's shadow on the moon was clearly visible in this eclipse, with 21% of the Moon in shadow; the partial eclipse lasted for 1 hour and 48 minutes.
22 Jun, 1415 AD
Partial Lunar Eclipse
(umbral mag. 0.36; Saros 120)
The Earth's shadow on the moon was clearly visible in this eclipse, with 36% of the Moon in shadow; the partial eclipse lasted for 2 hours and 19 minutes.
2 Jul, 1433 AD
Partial Lunar Eclipse
(umbral mag. 0.51; Saros 120)
The Earth's shadow on the moon was clearly visible in this eclipse, with 51% of the Moon in shadow; the partial eclipse lasted for 2 hours and 42 minutes.
14 Jul, 1451 AD
Partial Lunar Eclipse
(umbral mag. 0.66; Saros 120)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours exactly, with 66% of the Moon in darkness at maximum.
24 Jul, 1469 AD
Partial Lunar Eclipse
(umbral mag. 0.81; Saros 120)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 15 minutes, with 81% of the Moon in darkness at maximum.
4 Aug, 1487 AD
Partial Lunar Eclipse
(umbral mag. 0.95; Saros 120)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 26 minutes. With 95% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
14 Aug, 1505 AD
Total Lunar Eclipse
(umbral mag. 1.08; Saros 120)
A shallow total eclipse saw the Moon in relative darkness for 44 minutes and 42 seconds. The Moon was 8% 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.
26 Aug, 1523 AD
Total Lunar Eclipse
(umbral mag. 1.20; Saros 120)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 9 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 41 minutes in total.
5 Sep, 1541 AD
Total Lunar Eclipse
(umbral mag. 1.31; Saros 120)
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.
16 Sep, 1559 AD
Total Lunar Eclipse
(umbral mag. 1.40; Saros 120)
The Moon was plunged into darkness for 1 hour and 31 minutes, in a deep total eclipse which saw the Moon 40% 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.
27 Sep, 1577 AD
Total Lunar Eclipse
(umbral mag. 1.49; Saros 120)
The Moon was plunged into darkness for 1 hour and 37 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 52 minutes in total.
18 Oct, 1595 AD
Total Lunar Eclipse
(umbral mag. 1.56; Saros 120)
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 53 minutes in total.
28 Oct, 1613 AD
Total Lunar Eclipse
(umbral mag. 1.61; Saros 120)
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 54 minutes in total.
8 Nov, 1631 AD
Total Lunar Eclipse
(umbral mag. 1.66; Saros 120)
A dramatic total eclipse lasting 1 hour and 44 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 55 minutes in total.
19 Nov, 1649 AD
Total Lunar Eclipse
(umbral mag. 1.70; Saros 120)
A dramatic total eclipse lasting 1 hour and 44 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 55 minutes in total.
30 Nov, 1667 AD
Total Lunar Eclipse
(umbral mag. 1.72; Saros 120)
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 55 minutes in total.
10 Dec, 1685 AD
Total Lunar Eclipse
(umbral mag. 1.74; Saros 120)
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 55 minutes in total.
23 Dec, 1703 AD
Total Lunar Eclipse
(umbral mag. 1.76; Saros 120)
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 55 minutes in total.
2 Jan, 1722 AD
Total Lunar Eclipse
(umbral mag. 1.77; Saros 120)
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 55 minutes in total.
13 Jan, 1740 AD
Total Lunar Eclipse
(umbral mag. 1.79; Saros 120)
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 55 minutes in total.
24 Jan, 1758 AD
Total Lunar Eclipse
(umbral mag. 1.81; Saros 120)
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 55 minutes in total.
4 Feb, 1776 AD
Total Lunar Eclipse
(umbral mag. 1.79; Saros 120)
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 55 minutes in total.
14 Feb, 1794 AD
Total Lunar Eclipse
(umbral mag. 1.76; Saros 120)
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 55 minutes in total.
27 Feb, 1812 AD
Total Lunar Eclipse
(umbral mag. 1.71; Saros 120)
A dramatic total eclipse lasting 1 hour and 44 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.
9 Mar, 1830 AD
Total Lunar Eclipse
(umbral mag. 1.66; Saros 120)
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 53 minutes in total.
19 Mar, 1848 AD
Total Lunar Eclipse
(umbral mag. 1.60; Saros 120)
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.
31 Mar, 1866 AD
Total Lunar Eclipse
(umbral mag. 1.52; Saros 120)
The Moon was plunged into darkness for 1 hour and 38 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 51 minutes in total.
10 Apr, 1884 AD
Total Lunar Eclipse
(umbral mag. 1.43; Saros 120)
The Moon was plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which saw the Moon 43% 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.
22 Apr, 1902 AD
Total Lunar Eclipse
(umbral mag. 1.33; Saros 120)
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 45 minutes in total.
3 May, 1920 AD
Total Lunar Eclipse
(umbral mag. 1.22; Saros 120)
The Moon was plunged into darkness for 1 hour and 12 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 40 minutes in total.
14 May, 1938 AD
Total Lunar Eclipse
(umbral mag. 1.10; Saros 120)
A shallow total eclipse saw the Moon in relative darkness for 49 minutes and 24 seconds. The Moon was 10% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 33 minutes in total.
24 May, 1956 AD
Partial Lunar Eclipse
(umbral mag. 0.96; Saros 120)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 25 minutes. With 96% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
4 Jun, 1974 AD
Partial Lunar Eclipse
(umbral mag. 0.83; Saros 120)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 14 minutes, with 83% of the Moon in darkness at maximum.
15 Jun, 1992 AD
Partial Lunar Eclipse
(umbral mag. 0.68; Saros 120)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours exactly, with 68% of the Moon in darkness at maximum.
26 Jun, 2010 AD
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 120)
The Earth's shadow on the moon was clearly visible in this eclipse, with 54% of the Moon in shadow; the partial eclipse lasted for 2 hours and 43 minutes and was visible over eastern Asia, Australasia, the Pacific, and (partially) the Americas.
6 Jul, 2028 AD
Partial Lunar Eclipse
(umbral mag. 0.39; Saros 120)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 39% of the Moon in shadow; the partial eclipse will last for 2 hours and 22 minutes and will be visible from most of Africa, south and east Europe, Asia, and Australia.
18 Jul, 2046 AD
Partial Lunar Eclipse
(umbral mag. 0.25; Saros 120)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 25% of the Moon in shadow; the partial eclipse will last for 1 hour and 55 minutes.
28 Jul, 2064 AD
Partial Lunar Eclipse
(umbral mag. 0.10; Saros 120)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 16 minutes, with just 10% of the Moon in shadow at maximum.
8 Aug, 2082 AD
Penumbral Lunar Eclipse
(penum. mag. 1.00; Saros 120)
In a rare total penumbral eclipse, the entire Moon will be partially shaded by the Earth (though none of it will be in complete shadow), and the shading across the Moon should be quite visible at maximum eclipse. The penumbral phase will last for 4 hours and 30 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
19 Aug, 2100 AD
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 120)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 87% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 4 hours and 14 minutes.
31 Aug, 2118 AD
Penumbral Lunar Eclipse
(penum. mag. 0.75; Saros 120)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 75% 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 59 minutes.
10 Sep, 2136 AD
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 120)
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.
21 Sep, 2154 AD
Penumbral Lunar Eclipse
(penum. mag. 0.55; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 27 minutes, just 55% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
2 Oct, 2172 AD
Penumbral Lunar Eclipse
(penum. mag. 0.47; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 11 minutes, just 47% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
13 Oct, 2190 AD
Penumbral Lunar Eclipse
(penum. mag. 0.40; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 57 minutes, just 40% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
24 Oct, 2208 AD
Penumbral Lunar Eclipse
(penum. mag. 0.34; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 44 minutes, just 34% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
5 Nov, 2226 AD
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 34 minutes, just 30% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
15 Nov, 2244 AD
Penumbral Lunar Eclipse
(penum. mag. 0.27; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 25 minutes, just 27% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
26 Nov, 2262 AD
Penumbral Lunar Eclipse
(penum. mag. 0.24; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 18 minutes, just 24% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
7 Dec, 2280 AD
Penumbral Lunar Eclipse
(penum. mag. 0.23; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 14 minutes, just 23% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
18 Dec, 2298 AD
Penumbral Lunar Eclipse
(penum. mag. 0.22; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 11 minutes, just 22% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
29 Dec, 2316 AD
Penumbral Lunar Eclipse
(penum. mag. 0.22; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 10 minutes, just 22% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
10 Jan, 2335 AD
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 9 minutes, just 21% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
20 Jan, 2353 AD
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 8 minutes, just 21% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
31 Jan, 2371 AD
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros 120)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 6 minutes, just 21% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
11 Feb, 2389 AD
Penumbral Lunar Eclipse
(penum. mag. 0.20; Saros 120)
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 20% of the Moon's disc for 2 hours and 3 minutes, which will be essentially impossible to see.
22 Feb, 2407 AD
Penumbral Lunar Eclipse
(penum. mag. 0.18; Saros 120)
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 18% of the Moon's disc for 1 hour and 58 minutes, which will be essentially impossible to see.
4 Mar, 2425 AD
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros 120)
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 1 hour and 50 minutes, which will be essentially impossible to see.
16 Mar, 2443 AD
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 120)
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 12% of the Moon's disc for 1 hour and 37 minutes, which will be essentially impossible to see.
26 Mar, 2461 AD
Penumbral Lunar Eclipse
(penum. mag. 0.08; Saros 120)
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 8% of the Moon's disc for 1 hour and 17 minutes, which will be essentially impossible to see.
7 Apr, 2479 AD
Penumbral Lunar Eclipse
(penum. mag. 0.02; Saros 120)
In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 2% of the Moon's disc for 41 minutes and 6 seconds, which will be essentially impossible to see.