Lunar Eclipses in Saros Series 135

This page lists all the lunar eclipses in saros series 135 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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13 Apr, 1615 AD
Penumbral Lunar Eclipse
(penum. mag. 0.04; Saros 135)
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 55 minutes and 36 seconds, which was essentially impossible to see.
24 Apr, 1633 AD
Penumbral Lunar Eclipse
(penum. mag. 0.13; Saros 135)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 13% of the Moon's disc for 1 hour and 39 minutes, which was essentially impossible to see.
5 May, 1651 AD
Penumbral Lunar Eclipse
(penum. mag. 0.22; Saros 135)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 11 minutes, just 22% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
15 May, 1669 AD
Penumbral Lunar Eclipse
(penum. mag. 0.33; Saros 135)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 38 minutes, just 33% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
27 May, 1687 AD
Penumbral Lunar Eclipse
(penum. mag. 0.45; Saros 135)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 3 minutes, just 45% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
7 Jun, 1705 AD
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 135)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 25 minutes, just 58% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
18 Jun, 1723 AD
Penumbral Lunar Eclipse
(penum. mag. 0.71; Saros 135)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 71% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 45 minutes.
28 Jun, 1741 AD
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 135)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 84% 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 3 minutes.
10 Jul, 1759 AD
Penumbral Lunar Eclipse
(penum. mag. 0.98; Saros 135)
The Moon approached within 2% of the Earth's umbral shadow at maximum eclipse, with the overall eclipse lasting 4 hours and 20 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.
20 Jul, 1777 AD
Partial Lunar Eclipse
(umbral mag. 0.11; Saros 135)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 16 minutes, with just 11% of the Moon in shadow at maximum.
31 Jul, 1795 AD
Partial Lunar Eclipse
(umbral mag. 0.24; Saros 135)
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 50 minutes.
12 Aug, 1813 AD
Partial Lunar Eclipse
(umbral mag. 0.37; Saros 135)
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 15 minutes.
23 Aug, 1831 AD
Partial Lunar Eclipse
(umbral mag. 0.48; Saros 135)
The Earth's shadow on the moon was clearly visible in this eclipse, with 48% of the Moon in shadow; the partial eclipse lasted for 2 hours and 32 minutes.
2 Sep, 1849 AD
Partial Lunar Eclipse
(umbral mag. 0.59; Saros 135)
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 47 minutes.
14 Sep, 1867 AD
Partial Lunar Eclipse
(umbral mag. 0.70; Saros 135)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 58 minutes, with 70% of the Moon in darkness at maximum.
24 Sep, 1885 AD
Partial Lunar Eclipse
(umbral mag. 0.79; Saros 135)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 7 minutes, with 79% of the Moon in darkness at maximum.
6 Oct, 1903 AD
Partial Lunar Eclipse
(umbral mag. 0.87; Saros 135)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 14 minutes, with 87% of the Moon in darkness at maximum.
16 Oct, 1921 AD
Partial Lunar Eclipse
(umbral mag. 0.93; Saros 135)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 19 minutes. With 93% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
28 Oct, 1939 AD
Partial Lunar Eclipse
(umbral mag. 0.99; Saros 135)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 23 minutes. With 99% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
7 Nov, 1957 AD
Total Lunar Eclipse
(umbral mag. 1.03; Saros 135)
The Moon barely edged into total eclipse for 27 minutes and 54 seconds. With the Moon just 3% 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 27 minutes in total.
18 Nov, 1975 AD
Total Lunar Eclipse
(umbral mag. 1.06; Saros 135)
A shallow total eclipse saw the Moon in relative darkness for 40 minutes and 12 seconds. The Moon was 6% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 29 minutes in total.
29 Nov, 1993 AD
Total Lunar Eclipse
(umbral mag. 1.09; Saros 135)
A shallow total eclipse saw the Moon in relative darkness for 46 minutes and 42 seconds. The Moon was 9% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 31 minutes in total.
10 Dec, 2011 AD
Total Lunar Eclipse
(umbral mag. 1.11; Saros 135)
A shallow total eclipse saw the Moon in relative darkness for 51 minutes and 6 seconds. The Moon was 11% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers from North America (the beginning of the eclipse); eastern Asia and Australia; andmost of Europe and Africa (the end of the eclipse). The partial eclipse lasted for 3 hours and 32 minutes in total.
20 Dec, 2029 AD
(... 21 Dec UT)
Total Lunar Eclipse
(umbral mag. 1.12; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 53 minutes and 42 seconds. The Moon will be 12% of its diameter into the Earth's umbral shadow, and should be significantly darkened for viewers in eastern North and South America, all of Europe, Africa, and the Middle East, and most of Asia. The partial eclipse will last for 3 hours and 33 minutes in total.
1 Jan, 2048 AD
Total Lunar Eclipse
(umbral mag. 1.13; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 55 minutes and 54 seconds. The Moon will be 13% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 34 minutes in total.
11 Jan, 2066 AD
Total Lunar Eclipse
(umbral mag. 1.14; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 57 minutes and 54 seconds. The Moon will be 14% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 35 minutes in total.
22 Jan, 2084 AD
Total Lunar Eclipse
(umbral mag. 1.15; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 1 minute. The Moon will be 15% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 36 minutes in total.
3 Feb, 2102 AD
Total Lunar Eclipse
(umbral mag. 1.17; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 4 minutes. The Moon will be 17% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 38 minutes in total.
14 Feb, 2120 AD
Total Lunar Eclipse
(umbral mag. 1.20; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 8 minutes. The Moon will be 20% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 39 minutes in total.
24 Feb, 2138 AD
Total Lunar Eclipse
(umbral mag. 1.23; Saros 135)
The Moon will be plunged into darkness for 1 hour and 13 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 41 minutes in total.
7 Mar, 2156 AD
Total Lunar Eclipse
(umbral mag. 1.28; Saros 135)
The Moon will be plunged into darkness for 1 hour and 19 minutes, in a deep total eclipse which will see the Moon 28% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 44 minutes in total.
18 Mar, 2174 AD
Total Lunar Eclipse
(umbral mag. 1.34; Saros 135)
The Moon will be plunged into darkness for 1 hour and 25 minutes, in a deep total eclipse which will see the Moon 34% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 46 minutes in total.
28 Mar, 2192 AD
Total Lunar Eclipse
(umbral mag. 1.41; Saros 135)
The Moon will be plunged into darkness for 1 hour and 32 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 49 minutes in total.
10 Apr, 2210 AD
Total Lunar Eclipse
(umbral mag. 1.50; Saros 135)
The Moon will be plunged into darkness for 1 hour and 37 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 51 minutes in total.
20 Apr, 2228 AD
Total Lunar Eclipse
(umbral mag. 1.60; Saros 135)
A dramatic total eclipse lasting 1 hour and 42 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 54 minutes in total.
1 May, 2246 AD
Total Lunar Eclipse
(umbral mag. 1.71; Saros 135)
A dramatic total eclipse lasting 1 hour and 45 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 55 minutes in total.
12 May, 2264 AD
Total Lunar Eclipse
(umbral mag. 1.80; Saros 135)
A dramatic total eclipse lasting 1 hour and 46 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 56 minutes in total.
23 May, 2282 AD
Total Lunar Eclipse
(umbral mag. 1.66; Saros 135)
A dramatic total eclipse lasting 1 hour and 44 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 55 minutes in total.
3 Jun, 2300 AD
Total Lunar Eclipse
(umbral mag. 1.52; Saros 135)
The Moon will be plunged into darkness for 1 hour and 39 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 53 minutes in total.
14 Jun, 2318 AD
Total Lunar Eclipse
(umbral mag. 1.37; Saros 135)
The Moon will be plunged into darkness for 1 hour and 29 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 49 minutes in total.
25 Jun, 2336 AD
Total Lunar Eclipse
(umbral mag. 1.21; Saros 135)
The Moon will be plunged into darkness for 1 hour and 11 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 43 minutes in total.
6 Jul, 2354 AD
Total Lunar Eclipse
(umbral mag. 1.05; Saros 135)
A shallow total eclipse will see the Moon in relative darkness for 36 minutes and 42 seconds. The Moon will be 5% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 34 minutes in total.
16 Jul, 2372 AD
Partial Lunar Eclipse
(umbral mag. 0.89; Saros 135)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 23 minutes, with 89% of the Moon in darkness at maximum.
27 Jul, 2390 AD
Partial Lunar Eclipse
(umbral mag. 0.73; Saros 135)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 9 minutes, with 73% of the Moon in darkness at maximum.
7 Aug, 2408 AD
Partial Lunar Eclipse
(umbral mag. 0.57; Saros 135)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 57% of the Moon in shadow; the partial eclipse will last for 2 hours and 52 minutes.
18 Aug, 2426 AD
Partial Lunar Eclipse
(umbral mag. 0.43; Saros 135)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 43% of the Moon in shadow; the partial eclipse will last for 2 hours and 31 minutes.
28 Aug, 2444 AD
Partial Lunar Eclipse
(umbral mag. 0.29; Saros 135)
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 2 hours and 7 minutes.
9 Sep, 2462 AD
Partial Lunar Eclipse
(umbral mag. 0.16; Saros 135)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 35 minutes, with just 16% of the Moon in shadow at maximum.
19 Sep, 2480 AD
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 135)
A tiny bite out of the Moon may be visible at maximum, though just 4% of the Moon will be shadowed in a partial eclipse lasting for 46 minutes and 48 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
30 Sep, 2498 AD
Penumbral Lunar Eclipse
(penum. mag. 1.01; Saros 135)
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 42 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
11 Oct, 2516 AD
Penumbral Lunar Eclipse
(penum. mag. 0.91; Saros 135)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 91% 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 32 minutes.
23 Oct, 2534 AD
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 135)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 84% 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 22 minutes.
2 Nov, 2552 AD
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 135)
This subtle penumbral eclipse 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 13 minutes.
13 Nov, 2570 AD
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 135)
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 4 hours and 5 minutes.
24 Nov, 2588 AD
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 135)
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 59 minutes.
6 Dec, 2606 AD
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 135)
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 54 minutes.
16 Dec, 2624 AD
Penumbral Lunar Eclipse
(penum. mag. 0.63; Saros 135)
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 50 minutes.
28 Dec, 2642 AD
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 135)
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 47 minutes.
7 Jan, 2661 AD
Penumbral Lunar Eclipse
(penum. mag. 0.61; Saros 135)
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 45 minutes.
18 Jan, 2679 AD
Penumbral Lunar Eclipse
(penum. mag. 0.60; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 43 minutes, just 60% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
29 Jan, 2697 AD
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 40 minutes, just 59% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
10 Feb, 2715 AD
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 37 minutes, just 58% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
20 Feb, 2733 AD
Penumbral Lunar Eclipse
(penum. mag. 0.56; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 33 minutes, just 56% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
4 Mar, 2751 AD
Penumbral Lunar Eclipse
(penum. mag. 0.53; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 28 minutes, just 53% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
14 Mar, 2769 AD
Penumbral Lunar Eclipse
(penum. mag. 0.50; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 21 minutes, just 50% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
25 Mar, 2787 AD
Penumbral Lunar Eclipse
(penum. mag. 0.45; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 11 minutes, just 45% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
5 Apr, 2805 AD
Penumbral Lunar Eclipse
(penum. mag. 0.39; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 59 minutes, just 39% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
16 Apr, 2823 AD
Penumbral Lunar Eclipse
(penum. mag. 0.32; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 43 minutes, just 32% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
26 Apr, 2841 AD
Penumbral Lunar Eclipse
(penum. mag. 0.24; Saros 135)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 22 minutes, just 24% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
8 May, 2859 AD
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 135)
In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 15% of the Moon's disc for 1 hour and 53 minutes, which will be essentially impossible to see.
18 May, 2877 AD
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 135)
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 8 minutes, which will be essentially impossible to see.