Lunar Eclipses in Saros Series -11

This page lists all the lunar eclipses in saros series -11 which are in our database. Note that the beginning of this series is not included in our database, so the list below only covers the latter part of the series.

This series is partnered with solar Saros series -4.

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).
16 May, 1999 BC
max: 16:54 UT
Partial Lunar Eclipse
(umbral mag. 0.21; Saros -11)
The Earth's shadow on the moon was clearly visible in this eclipse, with 21% of the Moon in shadow; the partial eclipse lasted for 1 hour and 43 minutes.
   
26 May, 1981 BC
max: 23:55 UT
Partial Lunar Eclipse
(umbral mag. 0.07; Saros -11)
A tiny bite out of the Moon may have been visible at maximum, though just 7% of the Moon was shadowed in a partial eclipse which lasted for 1 hour and 1 minute. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
7 Jun, 1963 BC
max: 07:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.93; Saros -11)
At maximum eclipse, 93% 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 13 minutes overall.
   
17 Jun, 1945 BC
max: 14:10 UT
Penumbral Lunar Eclipse
(penum. mag. 0.81; Saros -11)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 81% 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 57 minutes.
   
28 Jun, 1927 BC
max: 21:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros -11)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 69% 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 40 minutes.
   
9 Jul, 1909 BC
max: 04:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros -11)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 23 minutes, just 58% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
20 Jul, 1891 BC
max: 12:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros -11)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 6 minutes, just 48% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
30 Jul, 1873 BC
max: 20:06 UT
Penumbral Lunar Eclipse
(penum. mag. 0.39; Saros -11)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 49 minutes, just 39% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
11 Aug, 1855 BC
max: 03:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.32; Saros -11)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 34 minutes, just 32% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
21 Aug, 1837 BC
max: 11:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.26; Saros -11)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 19 minutes, just 26% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
1 Sep, 1819 BC
max: 20:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros -11)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 6 minutes, just 21% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
12 Sep, 1801 BC
max: 04:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.18; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 18% of the Moon's disc for 1 hour and 55 minutes, which was essentially impossible to see.
   
23 Sep, 1783 BC
max: 13:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 16% of the Moon's disc for 1 hour and 48 minutes, which was essentially impossible to see.
   
3 Oct, 1765 BC
max: 21:40 UT
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 14% of the Moon's disc for 1 hour and 43 minutes, which was essentially impossible to see.
   
15 Oct, 1747 BC
max: 06:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 14% of the Moon's disc for 1 hour and 42 minutes, which was essentially impossible to see.
   
25 Oct, 1729 BC
max: 15:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 14% of the Moon's disc for 1 hour and 42 minutes, which was essentially impossible to see.
   
6 Nov, 1711 BC
max: 00:10 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros -11)
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 44 minutes, which was essentially impossible to see.
   
16 Nov, 1693 BC
max: 09:05 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 16% of the Moon's disc for 1 hour and 47 minutes, which was essentially impossible to see.
   
27 Nov, 1675 BC
max: 18:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 16% of the Moon's disc for 1 hour and 48 minutes, which was essentially impossible to see.
   
8 Dec, 1657 BC
max: 02:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros -11)
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 49 minutes, which was essentially impossible to see.
   
19 Dec, 1639 BC
max: 11:48 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 16% of the Moon's disc for 1 hour and 48 minutes, which was essentially impossible to see.
   
29 Dec, 1621 BC
max: 20:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros -11)
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 44 minutes, which was essentially impossible to see.
   
10 Jan, 1602 BC
max: 05:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.13; Saros -11)
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 36 minutes, which was essentially impossible to see.
   
20 Jan, 1584 BC
max: 13:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.10; Saros -11)
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 23 minutes, which was essentially impossible to see.
   
31 Jan, 1566 BC
max: 22:16 UT
Penumbral Lunar Eclipse
(penum. mag. 0.05; Saros -11)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 5% of the Moon's disc for 1 hour and 3 minutes, which was essentially impossible to see.