Lunar Eclipses in Saros Series 2

This page lists all the lunar eclipses in saros series 2 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 9.

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).
21 Jan, 1983 BC
max: 21:16 UT
Total Lunar Eclipse
(umbral mag. 1.42; Saros 2)
The Moon was plunged into darkness for 1 hour and 26 minutes, in a deep total eclipse which saw the Moon 42% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 31 minutes in total.
   
2 Feb, 1965 BC
max: 05:30 UT
Total Lunar Eclipse
(umbral mag. 1.47; Saros 2)
The Moon was plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which saw the Moon 47% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 32 minutes in total.
   
12 Feb, 1947 BC
max: 13:35 UT
Total Lunar Eclipse
(umbral mag. 1.55; Saros 2)
The Moon was plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which saw the Moon 55% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
23 Feb, 1929 BC
max: 21:35 UT
Total Lunar Eclipse
(umbral mag. 1.63; Saros 2)
A dramatic total eclipse lasting 1 hour and 36 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 34 minutes in total.
   
6 Mar, 1911 BC
max: 05:25 UT
Total Lunar Eclipse
(umbral mag. 1.72; Saros 2)
A dramatic total eclipse lasting 1 hour and 39 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 35 minutes in total.
   
16 Mar, 1893 BC
max: 13:10 UT
Total Lunar Eclipse
(umbral mag. 1.83; Saros 2)
A dramatic total eclipse lasting 1 hour and 40 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 35 minutes in total.
   
27 Mar, 1875 BC
max: 20:48 UT
Total Lunar Eclipse
(umbral mag. 1.81; Saros 2)
A dramatic total eclipse lasting 1 hour and 40 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 35 minutes in total.
   
7 Apr, 1857 BC
max: 04:22 UT
Total Lunar Eclipse
(umbral mag. 1.69; Saros 2)
A dramatic total eclipse lasting 1 hour and 38 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 33 minutes in total.
   
18 Apr, 1839 BC
max: 11:52 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 2)
The Moon was plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which saw the Moon 57% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 31 minutes in total.
   
28 Apr, 1821 BC
max: 19:20 UT
Total Lunar Eclipse
(umbral mag. 1.43; Saros 2)
The Moon was plunged into darkness for 1 hour and 26 minutes, in a deep total eclipse which saw the Moon 43% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 27 minutes in total.
   
10 May, 1803 BC
max: 02:47 UT
Total Lunar Eclipse
(umbral mag. 1.30; Saros 2)
The Moon was plunged into darkness for 1 hour and 15 minutes, in a deep total eclipse which saw the Moon 30% 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 23 minutes in total.
   
20 May, 1785 BC
max: 10:13 UT
Total Lunar Eclipse
(umbral mag. 1.16; Saros 2)
A shallow total eclipse saw the Moon in relative darkness for 58 minutes exactly. 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 17 minutes in total.
   
31 May, 1767 BC
max: 17:42 UT
Total Lunar Eclipse
(umbral mag. 1.03; Saros 2)
The Moon barely edged into total eclipse for 25 minutes and 24 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 9 minutes in total.
   
11 Jun, 1749 BC
max: 01:13 UT
Partial Lunar Eclipse
(umbral mag. 0.90; Saros 2)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 1 minute, with 90% of the Moon in darkness at maximum.
   
22 Jun, 1731 BC
max: 08:48 UT
Partial Lunar Eclipse
(umbral mag. 0.77; Saros 2)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 51 minutes, with 77% of the Moon in darkness at maximum.
   
2 Jul, 1713 BC
max: 16:27 UT
Partial Lunar Eclipse
(umbral mag. 0.65; Saros 2)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 40 minutes, with 65% of the Moon in darkness at maximum.
   
14 Jul, 1695 BC
max: 00:13 UT
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 2)
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 28 minutes.
   
24 Jul, 1677 BC
max: 08:05 UT
Partial Lunar Eclipse
(umbral mag. 0.44; Saros 2)
The Earth's shadow on the moon was clearly visible in this eclipse, with 44% of the Moon in shadow; the partial eclipse lasted for 2 hours and 15 minutes.
   
4 Aug, 1659 BC
max: 16:05 UT
Partial Lunar Eclipse
(umbral mag. 0.35; Saros 2)
The Earth's shadow on the moon was clearly visible in this eclipse, with 35% of the Moon in shadow; the partial eclipse lasted for 2 hours and 2 minutes.
   
15 Aug, 1641 BC
max: 00:12 UT
Partial Lunar Eclipse
(umbral mag. 0.27; Saros 2)
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 48 minutes.
   
26 Aug, 1623 BC
max: 08:28 UT
Partial Lunar Eclipse
(umbral mag. 0.20; Saros 2)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 34 minutes, with just 20% of the Moon in shadow at maximum.
   
5 Sep, 1605 BC
max: 16:53 UT
Partial Lunar Eclipse
(umbral mag. 0.14; Saros 2)
At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 21 minutes, with just 14% of the Moon in shadow at maximum.
   
17 Sep, 1587 BC
max: 01:24 UT
Partial Lunar Eclipse
(umbral mag. 0.10; Saros 2)
A tiny bite out of the Moon may have been visible at maximum, though just 10% of the Moon was shadowed in a partial eclipse which lasted for 1 hour and 8 minutes. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
27 Sep, 1569 BC
max: 10:04 UT
Partial Lunar Eclipse
(umbral mag. 0.07; Saros 2)
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 55 minutes and 54 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
8 Oct, 1551 BC
max: 18:50 UT
Partial Lunar Eclipse
(umbral mag. 0.04; Saros 2)
A tiny bite out of the Moon may have been visible at maximum, though just 4% of the Moon was shadowed in a partial eclipse which lasted for 45 minutes and 24 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
19 Oct, 1533 BC
max: 03:43 UT
Partial Lunar Eclipse
(umbral mag. 0.03; Saros 2)
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 38 minutes exactly. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
30 Oct, 1515 BC
max: 12:38 UT
Partial Lunar Eclipse
(umbral mag. 0.02; Saros 2)
A tiny bite out of the Moon may have been visible at maximum, though just 2% of the Moon was shadowed in a partial eclipse which lasted for 32 minutes exactly. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
9 Nov, 1497 BC
max: 21:38 UT
Partial Lunar Eclipse
(umbral mag. 0.02; Saros 2)
A tiny bite out of the Moon may have been visible at maximum, though just 2% of the Moon was shadowed in a partial eclipse which lasted for 29 minutes and 36 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
21 Nov, 1479 BC
max: 06:37 UT
Partial Lunar Eclipse
(umbral mag. 0.02; Saros 2)
A tiny bite out of the Moon may have been visible at maximum, though just 2% of the Moon was shadowed in a partial eclipse which lasted for 27 minutes and 24 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
1 Dec, 1461 BC
max: 15:36 UT
Partial Lunar Eclipse
(umbral mag. 0.01; Saros 2)
A tiny bite out of the Moon may have been visible at maximum, though just 1% of the Moon was shadowed in a partial eclipse which lasted for 25 minutes and 6 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
   
13 Dec, 1443 BC
max: 00:32 UT
Partial Lunar Eclipse
(umbral mag. 0.01; Saros 2)
While technically a partial eclipse, the Moon barely clipped the Earth's umbral shadow, which may have been very difficult to observe in practice; though a shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse. The partial eclipse lasted for 17 minutes and 42 seconds.
   
23 Dec, 1425 BC
max: 09:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.97; Saros 2)
The Moon approached within 0% of the Earth's umbral shadow at maximum eclipse; 97% of the Moon's disc was partially shaded by the Earth, with the overall eclipse lasting 4 hours and 3 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.
   
3 Jan, 1406 BC
max: 18:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.95; Saros 2)
The Moon approached within 2% of the Earth's umbral shadow at maximum eclipse; 95% of the Moon's disc was partially shaded by the Earth, with the overall eclipse lasting 4 hours and 1 minute. 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.
   
14 Jan, 1388 BC
max: 02:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.92; Saros 2)
At maximum eclipse, 92% 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 59 minutes overall.
   
25 Jan, 1370 BC
max: 11:22 UT
Penumbral Lunar Eclipse
(penum. mag. 0.88; Saros 2)
At maximum eclipse, 88% 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 55 minutes overall.
   
4 Feb, 1352 BC
max: 19:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.83; Saros 2)
At maximum eclipse, 83% 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.
   
16 Feb, 1334 BC
max: 03:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 2)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 76% 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 42 minutes.
   
26 Feb, 1316 BC
max: 12:04 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 2)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 68% 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 32 minutes.
   
9 Mar, 1298 BC
max: 19:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 2)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 19 minutes, just 59% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
20 Mar, 1280 BC
max: 03:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 2)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 4 minutes, just 49% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
31 Mar, 1262 BC
max: 11:24 UT
Penumbral Lunar Eclipse
(penum. mag. 0.37; Saros 2)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 43 minutes, just 37% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
10 Apr, 1244 BC
max: 18:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.25; Saros 2)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 15 minutes, just 25% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
22 Apr, 1226 BC
max: 02:20 UT
Penumbral Lunar Eclipse
(penum. mag. 0.12; Saros 2)
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.