Lunar Eclipses in Saros Series 134

This page lists all the lunar eclipses in saros series 134. The series contains 72 eclipses, occurring over 1280 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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1 Apr, 1550 AD
Penumbral Lunar Eclipse
(penum. mag. 0.00; Saros 134)
In this virtually non-existant eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow; although the eclipse lasted 12 minutes and 54 seconds, it was impossible to see in practice.
11 Apr, 1568 AD
Penumbral Lunar Eclipse
(penum. mag. 0.10; Saros 134)
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 25 minutes, which was essentially impossible to see.
3 May, 1586 AD
Penumbral Lunar Eclipse
(penum. mag. 0.20; Saros 134)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 2 minutes, just 20% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
13 May, 1604 AD
Penumbral Lunar Eclipse
(penum. mag. 0.32; Saros 134)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 30 minutes, just 32% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
24 May, 1622 AD
Penumbral Lunar Eclipse
(penum. mag. 0.44; Saros 134)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 54 minutes, just 44% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
4 Jun, 1640 AD
Penumbral Lunar Eclipse
(penum. mag. 0.57; Saros 134)
This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 15 minutes, just 57% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
15 Jun, 1658 AD
Penumbral Lunar Eclipse
(penum. mag. 0.71; Saros 134)
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 33 minutes.
25 Jun, 1676 AD
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 134)
At maximum eclipse, 84% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 3 hours and 49 minutes overall.
7 Jul, 1694 AD
Partial Lunar Eclipse
(umbral mag. 0.03; Saros 134)
A tiny bite out of the Moon may have been visible at maximum, though just 3% of the Moon was shadowed in a partial eclipse which lasted for 39 minutes exactly. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
18 Jul, 1712 AD
Partial Lunar Eclipse
(umbral mag. 0.17; Saros 134)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 28 minutes, with just 17% of the Moon in shadow at maximum.
29 Jul, 1730 AD
Partial Lunar Eclipse
(umbral mag. 0.30; Saros 134)
The Earth's shadow on the moon was clearly visible in this eclipse, with 30% of the Moon in shadow; the partial eclipse lasted for 1 hour and 56 minutes.
8 Aug, 1748 AD
Partial Lunar Eclipse
(umbral mag. 0.43; Saros 134)
The Earth's shadow on the moon was clearly visible in this eclipse, with 43% of the Moon in shadow; the partial eclipse lasted for 2 hours and 15 minutes.
20 Aug, 1766 AD
Partial Lunar Eclipse
(umbral mag. 0.55; Saros 134)
The Earth's shadow on the moon was clearly visible in this eclipse, with 55% of the Moon in shadow; the partial eclipse lasted for 2 hours and 30 minutes.
30 Aug, 1784 AD
Partial Lunar Eclipse
(umbral mag. 0.66; Saros 134)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 41 minutes, with 66% of the Moon in darkness at maximum.
11 Sep, 1802 AD
Partial Lunar Eclipse
(umbral mag. 0.76; Saros 134)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 50 minutes, with 76% of the Moon in darkness at maximum.
22 Sep, 1820 AD
Partial Lunar Eclipse
(umbral mag. 0.85; Saros 134)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 57 minutes, with 85% of the Moon in darkness at maximum.
3 Oct, 1838 AD
Partial Lunar Eclipse
(umbral mag. 0.93; Saros 134)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 2 minutes. With 93% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
13 Oct, 1856 AD
Partial Lunar Eclipse
(umbral mag. 1.00; Saros 134)
The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 6 minutes. With 100% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
25 Oct, 1874 AD
Total Lunar Eclipse
(umbral mag. 1.05; Saros 134)
The Moon barely edged into total eclipse for 32 minutes and 42 seconds. With the Moon just 5% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 9 minutes in total.
4 Nov, 1892 AD
Total Lunar Eclipse
(umbral mag. 1.09; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 44 minutes and 6 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 12 minutes in total.
17 Nov, 1910 AD
Total Lunar Eclipse
(umbral mag. 1.12; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 50 minutes and 36 seconds. 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 13 minutes in total.
27 Nov, 1928 AD
Total Lunar Eclipse
(umbral mag. 1.15; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 54 minutes and 48 seconds. The Moon was 15% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 14 minutes in total.
8 Dec, 1946 AD
Total Lunar Eclipse
(umbral mag. 1.16; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 57 minutes and 18 seconds. 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 15 minutes in total.
19 Dec, 1964 AD
Total Lunar Eclipse
(umbral mag. 1.17; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 58 minutes and 54 seconds. The Moon was 17% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 16 minutes in total.
30 Dec, 1982 AD
Total Lunar Eclipse
(umbral mag. 1.18; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 1 hour exactly. The Moon was 18% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 16 minutes in total.
9 Jan, 2001 AD
Total Lunar Eclipse
(umbral mag. 1.19; Saros 134)
A shallow total eclipse saw the Moon in relative darkness for 1 hour and 1 minute. The Moon was 19% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers over all of Europe, Africa, and Asia. The partial eclipse lasted for 3 hours and 16 minutes in total and was visible in parts of north-eastern North America and Australia.
21 Jan, 2019 AD
Total Lunar Eclipse
(umbral mag. 1.20; Saros 134)
A shallow total eclipse will see the Moon in relative darkness for 1 hour and 2 minutes. The Moon will be 20% of its diameter into the Earth's umbral shadow, and should be significantly darkened for viewers from the Americas, Europe, and most of Africa. The partial eclipse will last for 3 hours and 17 minutes in total.
31 Jan, 2037 AD
Total Lunar Eclipse
(umbral mag. 1.21; Saros 134)
The Moon will be plunged into darkness for 1 hour and 4 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 for observers in north and west North America, most of Asia, Australia and New Zealand. The partial eclipse will last for 3 hours and 18 minutes in total.
11 Feb, 2055 AD
Total Lunar Eclipse
(umbral mag. 1.22; Saros 134)
The Moon will be plunged into darkness for 1 hour and 6 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 18 minutes in total.
22 Feb, 2073 AD
Total Lunar Eclipse
(umbral mag. 1.25; Saros 134)
The Moon will be plunged into darkness for 1 hour and 9 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 20 minutes in total.
5 Mar, 2091 AD
Total Lunar Eclipse
(umbral mag. 1.28; Saros 134)
The Moon will be plunged into darkness for 1 hour and 13 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 21 minutes in total.
17 Mar, 2109 AD
Total Lunar Eclipse
(umbral mag. 1.33; Saros 134)
The Moon will be plunged into darkness for 1 hour and 18 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 23 minutes in total.
28 Mar, 2127 AD
Total Lunar Eclipse
(umbral mag. 1.38; Saros 134)
The Moon will be plunged into darkness for 1 hour and 22 minutes, in a deep total eclipse which will see the Moon 38% 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 26 minutes in total.
7 Apr, 2145 AD
Total Lunar Eclipse
(umbral mag. 1.46; Saros 134)
The Moon will be plunged into darkness for 1 hour and 27 minutes, in a deep total eclipse which will see the Moon 46% 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 28 minutes in total.
19 Apr, 2163 AD
Total Lunar Eclipse
(umbral mag. 1.53; Saros 134)
The Moon will be plunged into darkness for 1 hour and 32 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 30 minutes in total.
29 Apr, 2181 AD
Total Lunar Eclipse
(umbral mag. 1.63; Saros 134)
A dramatic total eclipse lasting 1 hour and 36 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 32 minutes in total.
10 May, 2199 AD
Total Lunar Eclipse
(umbral mag. 1.73; Saros 134)
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 34 minutes in total.
21 May, 2217 AD
Total Lunar Eclipse
(umbral mag. 1.84; Saros 134)
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 35 minutes in total.
2 Jun, 2235 AD
Total Lunar Eclipse
(umbral mag. 1.78; Saros 134)
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 36 minutes in total.
12 Jun, 2253 AD
Total Lunar Eclipse
(umbral mag. 1.65; Saros 134)
A dramatic total eclipse lasting 1 hour and 38 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 35 minutes in total.
23 Jun, 2271 AD
Total Lunar Eclipse
(umbral mag. 1.52; Saros 134)
The Moon will be plunged into darkness for 1 hour and 32 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 33 minutes in total.
4 Jul, 2289 AD
Total Lunar Eclipse
(umbral mag. 1.38; Saros 134)
The Moon will be plunged into darkness for 1 hour and 23 minutes, in a deep total eclipse which will see the Moon 38% 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 30 minutes in total.
16 Jul, 2307 AD
Total Lunar Eclipse
(umbral mag. 1.23; Saros 134)
The Moon will be plunged into darkness for 1 hour and 9 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 25 minutes in total.
26 Jul, 2325 AD
Total Lunar Eclipse
(umbral mag. 1.09; Saros 134)
A shallow total eclipse will see the Moon in relative darkness for 45 minutes exactly. The Moon will be 9% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 19 minutes in total.
7 Aug, 2343 AD
Partial Lunar Eclipse
(umbral mag. 0.95; Saros 134)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 11 minutes. With 95% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
17 Aug, 2361 AD
Partial Lunar Eclipse
(umbral mag. 0.81; Saros 134)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 1 minute, with 81% of the Moon in darkness at maximum.
28 Aug, 2379 AD
Partial Lunar Eclipse
(umbral mag. 0.68; Saros 134)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 50 minutes, with 68% of the Moon in darkness at maximum.
8 Sep, 2397 AD
Partial Lunar Eclipse
(umbral mag. 0.56; Saros 134)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 56% of the Moon in shadow; the partial eclipse will last for 2 hours and 37 minutes.
19 Sep, 2415 AD
Partial Lunar Eclipse
(umbral mag. 0.44; Saros 134)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 44% of the Moon in shadow; the partial eclipse will last for 2 hours and 23 minutes.
29 Sep, 2433 AD
Partial Lunar Eclipse
(umbral mag. 0.34; Saros 134)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 34% of the Moon in shadow; the partial eclipse will last for 2 hours and 7 minutes.
10 Oct, 2451 AD
Partial Lunar Eclipse
(umbral mag. 0.24; Saros 134)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 24% of the Moon in shadow; the partial eclipse will last for 1 hour and 50 minutes.
21 Oct, 2469 AD
Partial Lunar Eclipse
(umbral mag. 0.16; Saros 134)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 31 minutes, with just 16% of the Moon in shadow at maximum.
1 Nov, 2487 AD
Partial Lunar Eclipse
(umbral mag. 0.09; Saros 134)
A tiny bite out of the Moon may be visible at maximum, though just 9% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 9 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
12 Nov, 2505 AD
Partial Lunar Eclipse
(umbral mag. 0.03; Saros 134)
A tiny bite out of the Moon may be visible at maximum, though just 3% of the Moon will be shadowed in a partial eclipse lasting for 40 minutes and 18 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
24 Nov, 2523 AD
Penumbral Lunar Eclipse
(penum. mag. 1.02; Saros 134)
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 28 minutes in all, though for most of it, the eclipse will be extremely difficult or impossible to see.
4 Dec, 2541 AD
Penumbral Lunar Eclipse
(penum. mag. 0.99; Saros 134)
At maximum eclipse, 99% 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 26 minutes overall.
15 Dec, 2559 AD
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 134)
At maximum eclipse, 97% 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 25 minutes overall.
26 Dec, 2577 AD
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 134)
At maximum eclipse, 95% 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 24 minutes overall.
6 Jan, 2596 AD
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros 134)
At maximum eclipse, 93% 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 23 minutes overall.
18 Jan, 2614 AD
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 134)
At maximum eclipse, 92% 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 22 minutes overall.
29 Jan, 2632 AD
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 134)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 90% 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 21 minutes.
8 Feb, 2650 AD
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 134)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 88% 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 20 minutes.
20 Feb, 2668 AD
Penumbral Lunar Eclipse
(penum. mag. 0.86; Saros 134)
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 17 minutes.
2 Mar, 2686 AD
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 134)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 83% 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.
13 Mar, 2704 AD
Penumbral Lunar Eclipse
(penum. mag. 0.78; Saros 134)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 78% 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 9 minutes.
25 Mar, 2722 AD
Penumbral Lunar Eclipse
(penum. mag. 0.73; Saros 134)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 73% 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 2 minutes.
4 Apr, 2740 AD
Penumbral Lunar Eclipse
(penum. mag. 0.66; Saros 134)
This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 66% 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.
15 Apr, 2758 AD
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 134)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 40 minutes, just 58% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
26 Apr, 2776 AD
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 134)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 24 minutes, just 48% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
7 May, 2794 AD
Penumbral Lunar Eclipse
(penum. mag. 0.38; Saros 134)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 2 minutes, just 38% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
17 May, 2812 AD
Penumbral Lunar Eclipse
(penum. mag. 0.26; Saros 134)
This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 33 minutes, just 26% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
28 May, 2830 AD
Penumbral Lunar Eclipse
(penum. mag. 0.13; Saros 134)
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 13% of the Moon's disc for 1 hour and 50 minutes, which will be essentially impossible to see.