Lunar Eclipses in Saros Series 138

This page lists all the lunar eclipses in saros series 138 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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15 Oct, 1521 AD
Penumbral Lunar Eclipse
(penum. mag. 0.04; Saros 138)
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 53 minutes and 6 seconds, which was essentially impossible to see.
27 Oct, 1539 AD
Penumbral Lunar Eclipse
(penum. mag. 0.07; Saros 138)
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 12 minutes, which was essentially impossible to see.
6 Nov, 1557 AD
Penumbral Lunar Eclipse
(penum. mag. 0.10; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 10% of the Moon's disc for 1 hour and 24 minutes, which was essentially impossible to see.
18 Nov, 1575 AD
Penumbral Lunar Eclipse
(penum. mag. 0.11; Saros 138)
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 30 minutes, which was essentially impossible to see.
8 Dec, 1593 AD
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 12% of the Moon's disc for 1 hour and 33 minutes, which was essentially impossible to see.
19 Dec, 1611 AD
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 12% of the Moon's disc for 1 hour and 34 minutes, which was essentially impossible to see.
30 Dec, 1629 AD
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 12% of the Moon's disc for 1 hour and 35 minutes, which was essentially impossible to see.
10 Jan, 1648 AD
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 12% of the Moon's disc for 1 hour and 35 minutes, which was essentially impossible to see.
20 Jan, 1666 AD
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 12% of the Moon's disc for 1 hour and 37 minutes, which was essentially impossible to see.
1 Feb, 1684 AD
Penumbral Lunar Eclipse
(penum. mag. 0.13; Saros 138)
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 40 minutes, which was essentially impossible to see.
12 Feb, 1702 AD
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 15% of the Moon's disc for 1 hour and 45 minutes, which was essentially impossible to see.
23 Feb, 1720 AD
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 138)
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 52 minutes, which was essentially impossible to see.
6 Mar, 1738 AD
Penumbral Lunar Eclipse
(penum. mag. 0.20; Saros 138)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 20% of the Moon's disc for 2 hours and 2 minutes, which was essentially impossible to see.
16 Mar, 1756 AD
Penumbral Lunar Eclipse
(penum. mag. 0.24; Saros 138)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 15 minutes, just 24% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
27 Mar, 1774 AD
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 138)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 29 minutes, just 30% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
7 Apr, 1792 AD
Penumbral Lunar Eclipse
(penum. mag. 0.36; Saros 138)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 44 minutes, just 36% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
19 Apr, 1810 AD
Penumbral Lunar Eclipse
(penum. mag. 0.44; Saros 138)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 1 minute, just 44% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
29 Apr, 1828 AD
Penumbral Lunar Eclipse
(penum. mag. 0.53; Saros 138)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 17 minutes, just 53% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
11 May, 1846 AD
Penumbral Lunar Eclipse
(penum. mag. 0.64; Saros 138)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 64% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 34 minutes.
21 May, 1864 AD
Penumbral Lunar Eclipse
(penum. mag. 0.75; Saros 138)
This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 75% 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 51 minutes.
1 Jun, 1882 AD
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 138)
At maximum eclipse, 87% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 7 minutes overall.
13 Jun, 1900 AD
Penumbral Lunar Eclipse
(penum. mag. 1.00; Saros 138)
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 22 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
24 Jun, 1918 AD
Partial Lunar Eclipse
(umbral mag. 0.13; Saros 138)
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 13% of the Moon in shadow at maximum.
4 Jul, 1936 AD
Partial Lunar Eclipse
(umbral mag. 0.27; Saros 138)
The Earth's shadow on the moon was clearly visible in this eclipse, with 27% of the Moon in shadow; the partial eclipse lasted for 1 hour and 56 minutes.
16 Jul, 1954 AD
Partial Lunar Eclipse
(umbral mag. 0.41; Saros 138)
The Earth's shadow on the moon was clearly visible in this eclipse, with 41% of the Moon in shadow; the partial eclipse lasted for 2 hours and 21 minutes.
26 Jul, 1972 AD
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 138)
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 40 minutes.
6 Aug, 1990 AD
Partial Lunar Eclipse
(umbral mag. 0.68; Saros 138)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 56 minutes, with 68% of the Moon in darkness at maximum.
16 Aug, 2008 AD
Partial Lunar Eclipse
(umbral mag. 0.81; Saros 138)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 8 minutes, with 81% of the Moon in darkness at maximum. The eclipse was visible over most of Asia, Australasia, Europe, Africa, and south America.
28 Aug, 2026 AD
Partial Lunar Eclipse
(umbral mag. 0.93; Saros 138)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 18 minutes and visible from the Americas and western Europe and Africa. With 93% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
7 Sep, 2044 AD
Total Lunar Eclipse
(umbral mag. 1.05; Saros 138)
The Moon will barely edge into total eclipse for 33 minutes and 54 seconds. With the Moon just 5% of its diameter into the Earth's umbral shadow, the Moon may be quite bright, but even so, this should be worth seeing. The partial eclipse will last for 3 hours and 26 minutes in total.
18 Sep, 2062 AD
Total Lunar Eclipse
(umbral mag. 1.15; Saros 138)
A shallow total eclipse will see the Moon in relative darkness for 59 minutes and 30 seconds. 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 32 minutes in total.
29 Sep, 2080 AD
Total Lunar Eclipse
(umbral mag. 1.24; Saros 138)
The Moon will be plunged into darkness for 1 hour and 14 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 37 minutes in total.
10 Oct, 2098 AD
Total Lunar Eclipse
(umbral mag. 1.32; Saros 138)
The Moon will be plunged into darkness for 1 hour and 23 minutes, in a deep total eclipse which will see the Moon 32% 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.
21 Oct, 2116 AD
Total Lunar Eclipse
(umbral mag. 1.39; Saros 138)
The Moon will be plunged into darkness for 1 hour and 29 minutes, in a deep total eclipse which will see the Moon 39% 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.
2 Nov, 2134 AD
Total Lunar Eclipse
(umbral mag. 1.45; Saros 138)
The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 46 minutes in total.
12 Nov, 2152 AD
Total Lunar Eclipse
(umbral mag. 1.50; Saros 138)
The Moon will be plunged into darkness for 1 hour and 36 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 48 minutes in total.
23 Nov, 2170 AD
Total Lunar Eclipse
(umbral mag. 1.53; Saros 138)
The Moon will be plunged into darkness for 1 hour and 38 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 49 minutes in total.
4 Dec, 2188 AD
Total Lunar Eclipse
(umbral mag. 1.56; Saros 138)
A dramatic total eclipse lasting 1 hour and 39 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 50 minutes in total.
16 Dec, 2206 AD
Total Lunar Eclipse
(umbral mag. 1.58; Saros 138)
A dramatic total eclipse lasting 1 hour and 40 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 50 minutes in total.
26 Dec, 2224 AD
Total Lunar Eclipse
(umbral mag. 1.60; Saros 138)
A dramatic total eclipse lasting 1 hour and 41 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 51 minutes in total.
7 Jan, 2243 AD
Total Lunar Eclipse
(umbral mag. 1.61; Saros 138)
A dramatic total eclipse lasting 1 hour and 41 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 51 minutes in total.
17 Jan, 2261 AD
Total Lunar Eclipse
(umbral mag. 1.62; Saros 138)
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 52 minutes in total.
28 Jan, 2279 AD
Total Lunar Eclipse
(umbral mag. 1.64; Saros 138)
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 53 minutes in total.
8 Feb, 2297 AD
Total Lunar Eclipse
(umbral mag. 1.66; Saros 138)
A dramatic total eclipse lasting 1 hour and 43 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 53 minutes in total.
20 Feb, 2315 AD
Total Lunar Eclipse
(umbral mag. 1.69; Saros 138)
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 54 minutes in total.
2 Mar, 2333 AD
Total Lunar Eclipse
(umbral mag. 1.73; Saros 138)
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 54 minutes in total.
13 Mar, 2351 AD
Total Lunar Eclipse
(umbral mag. 1.77; Saros 138)
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.
24 Mar, 2369 AD
Total Lunar Eclipse
(umbral mag. 1.79; Saros 138)
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.
4 Apr, 2387 AD
Total Lunar Eclipse
(umbral mag. 1.72; Saros 138)
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.
14 Apr, 2405 AD
Total Lunar Eclipse
(umbral mag. 1.63; Saros 138)
A dramatic total eclipse lasting 1 hour and 43 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.
26 Apr, 2423 AD
Total Lunar Eclipse
(umbral mag. 1.53; Saros 138)
The Moon will be plunged into darkness for 1 hour and 39 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 53 minutes in total.
6 May, 2441 AD
Total Lunar Eclipse
(umbral mag. 1.41; Saros 138)
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 50 minutes in total.
17 May, 2459 AD
Total Lunar Eclipse
(umbral mag. 1.29; Saros 138)
The Moon will be plunged into darkness for 1 hour and 21 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 46 minutes in total.
28 May, 2477 AD
Total Lunar Eclipse
(umbral mag. 1.15; Saros 138)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 2 minutes. 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 40 minutes in total.
8 Jun, 2495 AD
Total Lunar Eclipse
(umbral mag. 1.01; Saros 138)
The Moon will barely edge into total eclipse for just 12 minutes and 54 seconds. With the Moon just barely inside the Earth's umbral shadow, the Moon may be quite bright, but even so, this should be worth seeing. The partial eclipse will last for 3 hours and 31 minutes in total.
19 Jun, 2513 AD
Partial Lunar Eclipse
(umbral mag. 0.85; Saros 138)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 20 minutes, with 85% of the Moon in darkness at maximum.
30 Jun, 2531 AD
Partial Lunar Eclipse
(umbral mag. 0.70; Saros 138)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 6 minutes, with 70% of the Moon in darkness at maximum.
11 Jul, 2549 AD
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 138)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 54% of the Moon in shadow; the partial eclipse will last for 2 hours and 48 minutes.
22 Jul, 2567 AD
Partial Lunar Eclipse
(umbral mag. 0.38; Saros 138)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 38% of the Moon in shadow; the partial eclipse will last for 2 hours and 24 minutes.
1 Aug, 2585 AD
Partial Lunar Eclipse
(umbral mag. 0.23; Saros 138)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 23% of the Moon in shadow; the partial eclipse will last for 1 hour and 53 minutes.
13 Aug, 2603 AD
Partial Lunar Eclipse
(umbral mag. 0.07; Saros 138)
A tiny bite out of the Moon may be visible at maximum, though just 7% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 7 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
24 Aug, 2621 AD
Penumbral Lunar Eclipse
(penum. mag. 1.00; Saros 138)
At maximum eclipse, 100% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 4 hours and 41 minutes overall.
4 Sep, 2639 AD
Penumbral Lunar Eclipse
(penum. mag. 0.86; Saros 138)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 86% 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 25 minutes.
14 Sep, 2657 AD
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 138)
This subtle penumbral eclipse 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 7 minutes.
26 Sep, 2675 AD
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 138)
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 50 minutes.
6 Oct, 2693 AD
Penumbral Lunar Eclipse
(penum. mag. 0.52; Saros 138)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 32 minutes, just 52% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
18 Oct, 2711 AD
Penumbral Lunar Eclipse
(penum. mag. 0.44; Saros 138)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 15 minutes, just 44% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
28 Oct, 2729 AD
Penumbral Lunar Eclipse
(penum. mag. 0.36; Saros 138)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 59 minutes, just 36% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
9 Nov, 2747 AD
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 138)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 44 minutes, just 30% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
19 Nov, 2765 AD
Penumbral Lunar Eclipse
(penum. mag. 0.26; Saros 138)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 32 minutes, just 26% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
30 Nov, 2783 AD
Penumbral Lunar Eclipse
(penum. mag. 0.22; Saros 138)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 21 minutes, just 22% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
11 Dec, 2801 AD
Penumbral Lunar Eclipse
(penum. mag. 0.20; Saros 138)
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 12 minutes, which will be essentially impossible to see.
22 Dec, 2819 AD
Penumbral Lunar Eclipse
(penum. mag. 0.18; Saros 138)
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 2 hours and 6 minutes, which will be essentially impossible to see.
1 Jan, 2838 AD
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 138)
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 17% of the Moon's disc for 2 hours and 2 minutes, which will be essentially impossible to see.
13 Jan, 2856 AD
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros 138)
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 59 minutes, which will be essentially impossible to see.
23 Jan, 2874 AD
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 138)
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 56 minutes, which will be essentially impossible to see.
3 Feb, 2892 AD
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 138)
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.
15 Feb, 2910 AD
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros 138)
In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 14% of the Moon's disc for 1 hour and 49 minutes, which will be essentially impossible to see.
26 Feb, 2928 AD
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 138)
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 41 minutes, which will be essentially impossible to see.
9 Mar, 2946 AD
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros 138)
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 30 minutes, which will be essentially impossible to see.
19 Mar, 2964 AD
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 138)
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 12 minutes, which will be essentially impossible to see.
30 Mar, 2982 AD
Penumbral Lunar Eclipse
(penum. mag. 0.02; Saros 138)
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 37 minutes and 36 seconds, which will be essentially impossible to see.