Lunar Eclipses in Saros Series 162

This page lists all the lunar eclipses in saros series 162 which are in our database. Note that the end of this series is not included in our database, so the list below only covers the earlier part of the series.

This series is partnered with solar Saros series 169.

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.

The interactive map is currently not available.

Note that eclipse dates are specified relative to UT. You have not selected a timezone for eclipse timings, so all times are shown in UT (essentially GMT).
12 Aug, 2288 AD
max: 20:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros 162)
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 18 minutes, which will be essentially impossible to see.
   
25 Aug, 2306 AD
max: 03:41 UT
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros 162)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 1 hour and 59 minutes, just 21% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
4 Sep, 2324 AD
max: 11:22 UT
Penumbral Lunar Eclipse
(penum. mag. 0.32; Saros 162)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 27 minutes, just 32% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
15 Sep, 2342 AD
max: 19:10 UT
Penumbral Lunar Eclipse
(penum. mag. 0.43; Saros 162)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 48 minutes, just 43% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
26 Sep, 2360 AD
max: 03:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.52; Saros 162)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 4 minutes, just 52% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
7 Oct, 2378 AD
max: 11:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.61; Saros 162)
This subtle penumbral 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 17 minutes.
   
17 Oct, 2396 AD
max: 19:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 162)
This subtle penumbral 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 27 minutes.
   
29 Oct, 2414 AD
max: 03:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 162)
This subtle penumbral 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 3 hours and 35 minutes.
   
8 Nov, 2432 AD
max: 11:55 UT
Penumbral Lunar Eclipse
(penum. mag. 0.79; Saros 162)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 79% 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 41 minutes.
   
19 Nov, 2450 AD
max: 20:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 162)
At maximum eclipse, 83% 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 3 hours and 46 minutes overall.
   
30 Nov, 2468 AD
max: 05:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.86; Saros 162)
At maximum eclipse, 86% 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 3 hours and 49 minutes overall.
   
11 Dec, 2486 AD
max: 13:43 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 162)
At maximum eclipse, 88% 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 3 hours and 52 minutes overall.
   
22 Dec, 2504 AD
max: 22:30 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 162)
At maximum eclipse, 89% 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 3 hours and 54 minutes overall.
   
3 Jan, 2523 AD
max: 07:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.90; Saros 162)
At maximum eclipse, 90% 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 3 hours and 55 minutes overall.
   
13 Jan, 2541 AD
max: 16:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.91; Saros 162)
At maximum eclipse, 91% 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 3 hours and 56 minutes overall.
   
25 Jan, 2559 AD
max: 00:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 162)
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 3 hours and 57 minutes overall.
   
4 Feb, 2577 AD
max: 09:44 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 162)
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 3 hours and 58 minutes overall.
   
15 Feb, 2595 AD
max: 18:27 UT
Penumbral Lunar Eclipse
(penum. mag. 0.94; Saros 162)
The Moon will approach within 4% of the Earth's umbral shadow at maximum eclipse; 94% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 3 hours exactly. While less dramatic than a partial eclipse (as no part of the Moon will be in complete shadow), a shading across the Moon should be readily visible to observers.
   
27 Feb, 2613 AD
max: 03:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 162)
The Moon will approach within 2% of the Earth's umbral shadow at maximum eclipse; 96% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 4 hours and 2 minutes. While less dramatic than a partial eclipse (as no part of the Moon will be in complete shadow), a shading across the Moon should be readily visible to observers.
   
10 Mar, 2631 AD
max: 11:38 UT
Partial Lunar Eclipse
(umbral mag. 0.01; Saros 162)
While technically a partial eclipse, the Moon barely clips the Earth's umbral shadow, which may be very difficult to observe in practice; though a shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse. The partial eclipse will last for 17 minutes and 42 seconds.
   
20 Mar, 2649 AD
max: 20:05 UT
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 162)
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 44 minutes and 42 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
   
1 Apr, 2667 AD
max: 04:21 UT
Partial Lunar Eclipse
(umbral mag. 0.09; Saros 162)
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 6 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
   
11 Apr, 2685 AD
max: 12:32 UT
Partial Lunar Eclipse
(umbral mag. 0.15; Saros 162)
At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 24 minutes, with just 15% of the Moon in shadow at maximum.
   
23 Apr, 2703 AD
max: 20:31 UT
Partial Lunar Eclipse
(umbral mag. 0.22; Saros 162)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 22% of the Moon in shadow; the partial eclipse will last for 1 hour and 41 minutes.
   
4 May, 2721 AD
max: 04:24 UT
Partial Lunar Eclipse
(umbral mag. 0.30; Saros 162)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 30% of the Moon in shadow; the partial eclipse will last for 1 hour and 57 minutes.
   
15 May, 2739 AD
max: 12:07 UT
Partial Lunar Eclipse
(umbral mag. 0.40; Saros 162)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 40% of the Moon in shadow; the partial eclipse will last for 2 hours and 13 minutes.
   
25 May, 2757 AD
max: 19:44 UT
Partial Lunar Eclipse
(umbral mag. 0.50; Saros 162)
The Earth's shadow on the moon will be clearly visible in this eclipse, with 50% of the Moon in shadow; the partial eclipse will last for 2 hours and 27 minutes.
   
6 Jun, 2775 AD
max: 03:13 UT
Partial Lunar Eclipse
(umbral mag. 0.61; Saros 162)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 41 minutes, with 61% of the Moon in darkness at maximum.
   
16 Jun, 2793 AD
max: 10:37 UT
Partial Lunar Eclipse
(umbral mag. 0.73; Saros 162)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 53 minutes, with 73% of the Moon in darkness at maximum.
   
27 Jun, 2811 AD
max: 17:54 UT
Partial Lunar Eclipse
(umbral mag. 0.86; Saros 162)
The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 4 minutes, with 86% of the Moon in darkness at maximum.
   
8 Jul, 2829 AD
max: 01:09 UT
Partial Lunar Eclipse
(umbral mag. 1.00; Saros 162)
The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 14 minutes. With 100% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.
   
19 Jul, 2847 AD
max: 08:20 UT
Total Lunar Eclipse
(umbral mag. 1.13; Saros 162)
A shallow total eclipse will see the Moon in relative darkness for 53 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 22 minutes in total.
   
29 Jul, 2865 AD
max: 15:29 UT
Total Lunar Eclipse
(umbral mag. 1.27; Saros 162)
The Moon will be plunged into darkness for 1 hour and 14 minutes, in a deep total eclipse which will see the Moon 27% 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 29 minutes in total.
   
9 Aug, 2883 AD
max: 22:39 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 162)
The Moon will be plunged into darkness for 1 hour and 27 minutes, in a deep total eclipse which will see 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 be stained a deep red colour. The partial eclipse will last for 3 hours and 34 minutes in total.
   
21 Aug, 2901 AD
max: 05:49 UT
Total Lunar Eclipse
(umbral mag. 1.54; Saros 162)
The Moon will be plunged into darkness for 1 hour and 35 minutes, in a deep total eclipse which will see the Moon 54% 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 38 minutes in total.
   
1 Sep, 2919 AD
max: 13:01 UT
Total Lunar Eclipse
(umbral mag. 1.67; Saros 162)
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 41 minutes in total.
   
11 Sep, 2937 AD
max: 20:17 UT
Total Lunar Eclipse
(umbral mag. 1.79; Saros 162)
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 42 minutes in total.
   
23 Sep, 2955 AD
max: 03:36 UT
Total Lunar Eclipse
(umbral mag. 1.81; Saros 162)
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 43 minutes in total.
   
3 Oct, 2973 AD
max: 11:02 UT
Total Lunar Eclipse
(umbral mag. 1.70; Saros 162)
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 43 minutes in total.
   
14 Oct, 2991 AD
max: 18:32 UT
Total Lunar Eclipse
(umbral mag. 1.60; Saros 162)
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 42 minutes in total.