This catalog has a page for every eclipse from 2000 BC to 3000 AD, 23,962 in all, shown in groups of 20 years at a time. You can go to any eclipse by selecting the milennium, century and 20-year period from the navigation tabs above; then click on an eclipse's date in the list below to to go its page.

You can see the solar or lunar eclipses separately by clicking "Solar Eclipses" or "Lunar Eclipses" in the top-right tabs.

All Eclipses, 1800–1781 BC

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).
9 Mar, 1800 BC
max: 07:11 UT
Partial Lunar Eclipse
(umbral mag. 0.46; Saros -6)
The Earth's shadow on the moon was clearly visible in this eclipse, with 46% of the Moon in shadow; the partial eclipse lasted for 2 hours and 35 minutes.
   
23 Mar, 1800 BC
max: 11:34 UT
Total Solar Eclipse
(umbral mag. 1.05; Saros 20)
A dramatic total eclipse plunged the Sun into darkness for 3 minutes and 55 seconds at maximum, creating an amazing spectacle for observers in a broad path up to 197 km wide.
1 Sep, 1800 BC
max: 19:42 UT
Partial Lunar Eclipse
(umbral mag. 0.52; Saros -1)
The Earth's shadow on the moon was clearly visible in this eclipse, with 52% of the Moon in shadow; the partial eclipse lasted for 2 hours and 25 minutes.
   
16 Sep, 1800 BC
max: 19:23 UT
Annular Solar Eclipse
(umbral mag. 0.92; Saros 25)
A small annular eclipse covered only 92% of the Sun in a very broad path, 388 km wide at maximum, and lasted 7 minutes and 32 seconds.
11 Feb, 1799 BC
max: 19:52 UT
Partial Solar Eclipse
(umbral mag. 0.47; Saros -8)
A small partial eclipse barely darkened the Sun. With just 47% of the Sun covered for viewers closest to the center, this was of limited interest.
   
26 Feb, 1799 BC
max: 07:28 UT
Total Lunar Eclipse
(umbral mag. 1.80; Saros 4)
A dramatic total eclipse lasting 1 hour and 46 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 56 minutes in total.
13 Mar, 1799 BC
max: 04:00 UT
Partial Solar Eclipse
(umbral mag. 0.48; Saros 30)
A small partial eclipse barely darkened the Sun. With just 48% of the Sun covered for viewers closest to the center, this was of limited interest.
7 Aug, 1799 BC
max: 02:55 UT
Partial Solar Eclipse
(umbral mag. 0.03; Saros -3)
With only 3% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
   
22 Aug, 1799 BC
max: 11:46 UT
Total Lunar Eclipse
(umbral mag. 1.78; Saros 9)
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 34 minutes in total.
5 Sep, 1799 BC
max: 18:50 UT
Partial Solar Eclipse
(umbral mag. 0.33; Saros 35)
A small partial eclipse barely darkened the Sun. With just 33% of the Sun covered for viewers closest to the center, this was of limited interest.
1 Feb, 1798 BC
max: 09:51 UT
Hybrid Solar Eclipse
(umbral mag. 1.00; Saros 2)
A fleeting hybrid eclipse covered a narrow path at most 19 km wide and lasted for just 28 seconds at the point of maximum eclipse.
   
15 Feb, 1798 BC
max: 09:46 UT
Partial Lunar Eclipse
(umbral mag. 0.52; Saros 14)
The Earth's shadow on the moon was clearly visible in this eclipse, with 52% of the Moon in shadow; the partial eclipse lasted for 2 hours and 40 minutes.
27 Jul, 1798 BC
max: 11:01 UT
Total Solar Eclipse
(umbral mag. 1.01; Saros 7)
The Sun was darkened for 1 minute and 30 seconds by a dramatic total eclipse covering a narrow path at most 75 km wide. This was a sight worth seeing.
   
12 Aug, 1798 BC
max: 00:05 UT
Partial Lunar Eclipse
(umbral mag. 0.57; Saros 19)
The Earth's shadow on the moon was clearly visible in this eclipse, with 57% of the Moon in shadow; the partial eclipse lasted for 2 hours and 41 minutes.
6 Jan, 1797 BC
max: 08:18 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros -14)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours exactly, just 48% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
21 Jan, 1797 BC
max: 17:10 UT
Annular Solar Eclipse
(umbral mag. 0.95; Saros 12)
The Sun was 95% covered in a moderate annular eclipse, lasting 5 minutes and 49 seconds and covering a broad path up to 181 km wide.
4 Feb, 1797 BC
max: 18:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.31; Saros 24)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 32 minutes, just 31% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
1 Jul, 1797 BC
max: 14:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.35; Saros -9)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 59 minutes, just 35% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
16 Jul, 1797 BC
max: 01:37 UT
Total Solar Eclipse
(umbral mag. 1.07; Saros 17)
A dramatic total eclipse plunged the Sun into darkness for 6 minutes and 1 second at maximum, creating an amazing spectacle for observers in a broad path up to 220 km wide.
31 Jul, 1797 BC
max: 05:27 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 29)
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 2 hours and 4 minutes, which was essentially impossible to see.
26 Dec, 1797 BC
max: 00:00 UT
Partial Lunar Eclipse
(umbral mag. 0.75; Saros -4)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 49 minutes, with 75% of the Moon in darkness at maximum.
   
9 Jan, 1796 BC
max: 17:47 UT
Annular Solar Eclipse
(umbral mag. 0.92; Saros 22)
A small annular eclipse covered only 92% of the Sun in a very broad path, 556 km wide at maximum, and lasted 6 minutes and 29 seconds.
20 Jun, 1796 BC
max: 14:46 UT
Partial Lunar Eclipse
(umbral mag. 0.67; Saros 1)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 1 minute, with 67% of the Moon in darkness at maximum.
   
5 Jul, 1796 BC
max: 18:37 UT
Total Solar Eclipse
(umbral mag. 1.06; Saros 27)
A dramatic total eclipse plunged the Sun into darkness for 3 minutes and 53 seconds at maximum, creating an amazing spectacle for observers in a very broad path, 313 km wide at maximum.
30 Nov, 1796 BC
max: 01:31 UT
Partial Solar Eclipse
(umbral mag. 0.17; Saros -6)
With only 17% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
   
15 Dec, 1796 BC
max: 14:36 UT
Total Lunar Eclipse
(umbral mag. 1.75; Saros 6)
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 36 minutes in total.
29 Dec, 1796 BC
max: 17:54 UT
Partial Solar Eclipse
(umbral mag. 0.14; Saros 32)
With only 14% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
26 May, 1795 BC
max: 23:19 UT
Partial Solar Eclipse
(umbral mag. 0.79; Saros -1)
A moderate partial eclipse, with 79% of the Sun covered for viewers closest to the center, created an interesting spectacle.
   
9 Jun, 1795 BC
max: 20:50 UT
Total Lunar Eclipse
(umbral mag. 1.56; Saros 11)
The Moon was plunged into darkness for 1 hour and 37 minutes, in a deep total eclipse which saw the Moon 56% 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 41 minutes in total.
25 Jun, 1795 BC
max: 09:21 UT
Partial Solar Eclipse
(umbral mag. 0.01; Saros 37)
With only 1% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
19 Nov, 1795 BC
max: 11:23 UT
Hybrid Solar Eclipse
(umbral mag. 1.01; Saros 4)
The Sun was darkened for 1 minute and 5 seconds by a dramatic hybrid eclipse covering a narrow path at most 58 km wide. This was a sight worth seeing.
   
4 Dec, 1795 BC
max: 23:41 UT
Partial Lunar Eclipse
(umbral mag. 0.38; Saros 16)
The Earth's shadow on the moon was clearly visible in this eclipse, with 38% of the Moon in shadow; the partial eclipse lasted for 2 hours and 19 minutes.
16 May, 1794 BC
max: 04:16 UT
Annular Solar Eclipse
(umbral mag. 0.96; Saros 9)
The Sun was 96% covered in a moderate annular eclipse, lasting 5 minutes and 3 seconds and covering a broad path up to 166 km wide.
   
30 May, 1794 BC
max: 10:00 UT
Partial Lunar Eclipse
(umbral mag. 0.22; Saros 21)
The Earth's shadow on the moon was clearly visible in this eclipse, with 22% of the Moon in shadow; the partial eclipse lasted for 1 hour and 41 minutes.
25 Oct, 1794 BC
max: 05:54 UT
Penumbral Lunar Eclipse
(penum. mag. 0.05; Saros -12)
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 11 minutes, which was essentially impossible to see.
   
9 Nov, 1794 BC
max: 02:13 UT
Total Solar Eclipse
(umbral mag. 1.05; Saros 14)
A dramatic total eclipse plunged the Sun into darkness for 3 minutes and 54 seconds at maximum, creating an amazing spectacle for observers in a path up to 153 km wide.
24 Nov, 1794 BC
max: 01:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 26)
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 2 hours exactly, which was essentially impossible to see.
19 Apr, 1793 BC
max: 20:22 UT
Partial Lunar Eclipse
(umbral mag. 0.28; Saros -7)
The Earth's shadow on the moon was clearly visible in this eclipse, with 28% of the Moon in shadow; the partial eclipse lasted for 1 hour and 51 minutes.
   
4 May, 1793 BC
max: 04:56 UT
Annular Solar Eclipse
(umbral mag. 0.95; Saros 19)
The Sun was 95% covered in a moderate annular eclipse, lasting 4 minutes and 53 seconds and covering a broad path up to 190 km wide.
13 Oct, 1793 BC
max: 06:47 UT
Partial Lunar Eclipse
(umbral mag. 0.26; Saros -2)
The Earth's shadow on the moon was clearly visible in this eclipse, with 26% of the Moon in shadow; the partial eclipse lasted for 1 hour and 59 minutes.
   
28 Oct, 1793 BC
max: 17:29 UT
Total Solar Eclipse
(umbral mag. 1.02; Saros 24)
The Sun was darkened for 1 minute and 36 seconds by a dramatic total eclipse covering a path up to 95 km wide. This was a sight worth seeing.
24 Mar, 1792 BC
max: 21:42 UT
Partial Solar Eclipse
(umbral mag. 0.02; Saros -9)
With only 2% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
   
9 Apr, 1792 BC
max: 10:30 UT
Total Lunar Eclipse
(umbral mag. 1.61; Saros 3)
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 40 minutes in total.
23 Apr, 1792 BC
max: 08:37 UT
Partial Solar Eclipse
(umbral mag. 0.71; Saros 29)
A moderate partial eclipse, with 71% of the Sun covered for viewers closest to the center, created an interesting spectacle.
18 Sep, 1792 BC
max: 13:10 UT
Partial Solar Eclipse
(umbral mag. 0.09; Saros -4)
With only 9% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
   
2 Oct, 1792 BC
max: 14:41 UT
Total Lunar Eclipse
(umbral mag. 1.64; Saros 8)
A dramatic total eclipse lasting 1 hour and 37 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 37 minutes in total.
18 Oct, 1792 BC
max: 04:33 UT
Partial Solar Eclipse
(umbral mag. 0.29; Saros 34)
A small partial eclipse barely darkened the Sun. With just 29% of the Sun covered for viewers closest to the center, this was of limited interest.
14 Mar, 1791 BC
max: 11:21 UT
Total Solar Eclipse
(umbral mag. 1.05; Saros 1)
A dramatic total eclipse plunged the Sun into darkness for 3 minutes and 42 seconds at maximum, creating an amazing spectacle for observers in a very broad path, 266 km wide at maximum.
   
29 Mar, 1791 BC
max: 17:51 UT
Partial Lunar Eclipse
(umbral mag. 0.63; Saros 13)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 55 minutes, with 63% of the Moon in darkness at maximum.
7 Sep, 1791 BC
max: 14:10 UT
Annular Solar Eclipse
(umbral mag. 0.92; Saros 6)
A small annular eclipse covered only 92% of the Sun in a very broad path, 558 km wide at maximum, and lasted 6 minutes and 33 seconds.
   
22 Sep, 1791 BC
max: 04:46 UT
Partial Lunar Eclipse
(umbral mag. 0.82; Saros 18)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 55 minutes, with 82% of the Moon in darkness at maximum.
17 Feb, 1790 BC
max: 02:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros -15)
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 2 hours and 4 minutes, which was essentially impossible to see.
   
4 Mar, 1790 BC
max: 04:08 UT
Total Solar Eclipse
(umbral mag. 1.07; Saros 11)
A dramatic total eclipse plunged the Sun into darkness for 5 minutes and 36 seconds at maximum, creating an amazing spectacle for observers in a broad path up to 221 km wide.
18 Mar, 1790 BC
max: 19:01 UT
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros 23)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 47 minutes, just 30% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
13 Aug, 1790 BC
max: 10:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.30; Saros -10)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 27 minutes, just 30% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
27 Aug, 1790 BC
max: 14:17 UT
Annular Solar Eclipse
(umbral mag. 0.95; Saros 16)
The Sun was 95% covered in a moderate annular eclipse, lasting 5 minutes and 52 seconds and covering a broad path up to 196 km wide.
11 Sep, 1790 BC
max: 20:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.55; Saros 28)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 11 minutes, just 55% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
6 Feb, 1789 BC
max: 06:47 UT
Partial Lunar Eclipse
(umbral mag. 0.52; Saros -5)
The Earth's shadow on the moon was clearly visible in this eclipse, with 52% of the Moon in shadow; the partial eclipse lasted for 2 hours and 37 minutes.
   
21 Feb, 1789 BC
max: 19:19 UT
Total Solar Eclipse
(umbral mag. 1.02; Saros 21)
The Sun was darkened for 1 minute and 55 seconds by a dramatic total eclipse covering a path up to 104 km wide. This was a sight worth seeing.
1 Aug, 1789 BC
max: 21:38 UT
Partial Lunar Eclipse
(umbral mag. 0.54; Saros 0)
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.
   
15 Aug, 1789 BC
max: 20:26 UT
Annular Solar Eclipse
(umbral mag. 1.00; Saros 26)
A large annular eclipse covered over 99% of the Sun, creating a dramatic spectacle for observers in only a tiny path, just 9 km wide; it lasted a brief 12 seconds at the point of maximum eclipse.
11 Jan, 1788 BC
max: 12:48 UT
Partial Solar Eclipse
(umbral mag. 0.31; Saros -7)
A small partial eclipse barely darkened the Sun. With just 31% of the Sun covered for viewers closest to the center, this was of limited interest.
   
25 Jan, 1788 BC
max: 17:47 UT
Total Lunar Eclipse
(umbral mag. 1.81; Saros 5)
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.
10 Feb, 1788 BC
max: 04:36 UT
Partial Solar Eclipse
(umbral mag. 0.06; Saros 31)
With only 6% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
7 Jul, 1788 BC
max: 01:48 UT
Partial Solar Eclipse
(umbral mag. 0.50; Saros -2)
A moderate partial eclipse, with 50% of the Sun covered for viewers closest to the center, created an interesting spectacle.
   
22 Jul, 1788 BC
max: 01:11 UT
Total Lunar Eclipse
(umbral mag. 1.77; Saros 10)
A dramatic total eclipse lasting 1 hour and 46 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 55 minutes in total.
5 Aug, 1788 BC
max: 09:40 UT
Partial Solar Eclipse
(umbral mag. 0.47; Saros 36)
A small partial eclipse barely darkened the Sun. With just 47% of the Sun covered for viewers closest to the center, this was of limited interest.
31 Dec, 1788 BC
max: 12:21 UT
Annular Solar Eclipse
(umbral mag. 0.92; Saros 3)
A small annular eclipse covered only 92% of the Sun in a very broad path, 446 km wide at maximum, and lasted 7 minutes and 3 seconds.
   
15 Jan, 1787 BC
max: 09:18 UT
Partial Lunar Eclipse
(umbral mag. 0.57; Saros 15)
The Earth's shadow on the moon was clearly visible in this eclipse, with 57% of the Moon in shadow; the partial eclipse lasted for 2 hours and 31 minutes.
26 Jun, 1787 BC
max: 18:44 UT
Total Solar Eclipse
(umbral mag. 1.06; Saros 8)
A dramatic total eclipse plunged the Sun into darkness for 4 minutes and 13 seconds at maximum, creating an amazing spectacle for observers in a broad path up to 235 km wide.
   
11 Jul, 1787 BC
max: 01:27 UT
Partial Lunar Eclipse
(umbral mag. 0.41; Saros 20)
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 29 minutes.
6 Dec, 1787 BC
max: 12:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.42; Saros -13)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 57 minutes, just 42% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
   
20 Dec, 1787 BC
max: 13:40 UT
Annular Solar Eclipse
(umbral mag. 0.95; Saros 13)
The Sun was 95% covered in a moderate annular eclipse, lasting 5 minutes and 41 seconds and covering a broad path up to 172 km wide.
5 Jan, 1786 BC
max: 00:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.27; Saros 25)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 18 minutes, just 27% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
31 May, 1786 BC
max: 19:32 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros -8)
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 39 minutes.
   
16 Jun, 1786 BC
max: 08:04 UT
Hybrid Solar Eclipse
(umbral mag. 1.01; Saros 18)
The Sun was darkened for 1 minute and 23 seconds by a dramatic hybrid eclipse covering a narrow path at most 44 km wide. This was a sight worth seeing.
30 Jun, 1786 BC
max: 05:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.16; Saros 30)
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 56 minutes, which was essentially impossible to see.
25 Nov, 1786 BC
max: 19:32 UT
Partial Lunar Eclipse
(umbral mag. 0.54; Saros -3)
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 43 minutes.
   
9 Dec, 1786 BC
max: 21:59 UT
Hybrid Solar Eclipse
(umbral mag. 1.00; Saros 23)
A fleeting hybrid eclipse covered only a tiny path, just 9 km wide and lasted for a brief 12 seconds at the point of maximum eclipse.
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.
   
4 Jun, 1785 BC
max: 14:28 UT
Annular Solar Eclipse
(umbral mag. 0.95; Saros 28)
The Sun was 95% covered in a moderate annular eclipse, lasting just moments and covering only an extremely narrow strip.
30 Oct, 1785 BC
max: 01:23 UT
Partial Solar Eclipse
(umbral mag. 0.32; Saros -5)
A small partial eclipse barely darkened the Sun. With just 32% of the Sun covered for viewers closest to the center, this was of limited interest.
   
13 Nov, 1785 BC
max: 19:46 UT
Total Lunar Eclipse
(umbral mag. 1.76; Saros 7)
A dramatic total eclipse lasting 1 hour and 45 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 55 minutes in total.
28 Nov, 1785 BC
max: 12:06 UT
Partial Solar Eclipse
(umbral mag. 0.41; Saros 33)
A small partial eclipse barely darkened the Sun. With just 41% of the Sun covered for viewers closest to the center, this was of limited interest.
25 Apr, 1784 BC
max: 01:02 UT
Partial Solar Eclipse
(umbral mag. 0.87; Saros 0)
This was a deep partial eclipse, with 87% of the Sun covered for viewers closest to the center. This provided a significant spectacle for those who saw it.
   
10 May, 1784 BC
max: 03:32 UT
Total Lunar Eclipse
(umbral mag. 1.25; Saros 12)
The Moon was plunged into darkness for 1 hour and 9 minutes, in a deep total eclipse which saw 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 have been stained a deep red colour. The partial eclipse lasted for 3 hours and 20 minutes in total.
19 Oct, 1784 BC
max: 15:57 UT
Hybrid Solar Eclipse
(umbral mag. 1.01; Saros 5)
A fleeting hybrid eclipse covered a narrow path at most 38 km wide and lasted for 35 seconds at the point of maximum eclipse.
   
2 Nov, 1784 BC
max: 19:31 UT
Partial Lunar Eclipse
(umbral mag. 0.63; Saros 17)
The Moon was strikingly shadowed in this deep partial eclipse which lasted 2 hours and 55 minutes, with 63% of the Moon in darkness at maximum.
31 Mar, 1783 BC
max: 08:53 UT
Penumbral Lunar Eclipse
(penum. mag. 0.09; Saros -16)
In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 9% of the Moon's disc for 1 hour and 27 minutes, which was essentially impossible to see.
   
14 Apr, 1783 BC
max: 06:33 UT
Hybrid Solar Eclipse
(umbral mag. 1.00; Saros 10)
A fleeting hybrid eclipse covered a narrow path at most 17 km wide and lasted for 30 seconds at the point of maximum eclipse.
29 Apr, 1783 BC
max: 18:46 UT
Penumbral Lunar Eclipse
(penum. mag. 0.77; Saros 22)
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 77% 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 49 minutes.
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.
   
9 Oct, 1783 BC
max: 01:09 UT
Annular Solar Eclipse
(umbral mag. 0.96; Saros 15)
The Sun was 96% covered in a moderate annular eclipse, lasting 4 minutes and 46 seconds and covering a path up to 148 km wide.
23 Oct, 1783 BC
max: 01:32 UT
Penumbral Lunar Eclipse
(penum. mag. 0.51; Saros 27)
This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 15 minutes, just 51% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
20 Mar, 1782 BC
max: 14:07 UT
Partial Lunar Eclipse
(umbral mag. 0.34; Saros -6)
The Earth's shadow on the moon was clearly visible in this eclipse, with 34% of the Moon in shadow; the partial eclipse lasted for 2 hours and 16 minutes.
   
3 Apr, 1782 BC
max: 19:09 UT
Total Solar Eclipse
(umbral mag. 1.05; Saros 20)
A dramatic total eclipse plunged the Sun into darkness for 4 minutes and 36 seconds at maximum, creating an amazing spectacle for observers in a broad path up to 209 km wide.
13 Sep, 1782 BC
max: 04:13 UT
Partial Lunar Eclipse
(umbral mag. 0.47; Saros -1)
The Earth's shadow on the moon was clearly visible in this eclipse, with 47% of the Moon in shadow; the partial eclipse lasted for 2 hours and 20 minutes.
   
28 Sep, 1782 BC
max: 03:11 UT
Annular Solar Eclipse
(umbral mag. 0.92; Saros 25)
A small annular eclipse covered only 92% of the Sun in a very broad path, 395 km wide at maximum, and lasted 8 minutes and 19 seconds.
23 Feb, 1781 BC
max: 04:02 UT
Partial Solar Eclipse
(umbral mag. 0.39; Saros -8)
A small partial eclipse barely darkened the Sun. With just 39% of the Sun covered for viewers closest to the center, this was of limited interest.
   
8 Mar, 1781 BC
max: 14:27 UT
Total Lunar Eclipse
(umbral mag. 1.69; Saros 4)
A dramatic total eclipse lasting 1 hour and 45 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 55 minutes in total.
23 Mar, 1781 BC
max: 11:50 UT
Partial Solar Eclipse
(umbral mag. 0.59; Saros 30)
A moderate partial eclipse, with 59% of the Sun covered for viewers closest to the center, created an interesting spectacle.
1 Sep, 1781 BC
max: 20:02 UT
Total Lunar Eclipse
(umbral mag. 1.72; Saros 9)
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 34 minutes in total.
   
16 Sep, 1781 BC
max: 02:33 UT
Partial Solar Eclipse
(umbral mag. 0.38; Saros 35)
A small partial eclipse barely darkened the Sun. With just 38% of the Sun covered for viewers closest to the center, this was of limited interest.