Lunar Eclipses in Saros Series 180

This page lists all the lunar eclipses in saros series 180 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 187.

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).
28 Aug, 2827 AD
max: 00:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.05; Saros 180)
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 5% of the Moon's disc for 1 hour and 3 minutes, which will be essentially impossible to see. 		   
7 Sep, 2845 AD
max: 07:40 UT
Penumbral Lunar Eclipse
(penum. mag. 0.18; Saros 180)
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 18% of the Moon's disc for 1 hour and 54 minutes, which will be essentially impossible to see. 		   
18 Sep, 2863 AD
max: 15:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.29; Saros 180)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 25 minutes, just 29% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
28 Sep, 2881 AD
max: 23:00 UT
Penumbral Lunar Eclipse
(penum. mag. 0.40; Saros 180)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 47 minutes, just 40% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
10 Oct, 2899 AD
max: 06:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.49; Saros 180)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 3 minutes, just 49% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
21 Oct, 2917 AD
max: 14:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.58; Saros 180)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 16 minutes, just 58% of the Moon's disc will be in partial shadow (with no part of it in complete shadow). 		   
1 Nov, 2935 AD
max: 22:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 180)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 65% 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. 		   
12 Nov, 2953 AD
max: 07:14 UT
Penumbral Lunar Eclipse
(penum. mag. 0.71; Saros 180)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 71% 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 34 minutes. 		   
23 Nov, 2971 AD
max: 15:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 180)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 76% 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 40 minutes. 		   
4 Dec, 2989 AD
max: 00:08 UT
Penumbral Lunar Eclipse
(penum. mag. 0.80; Saros 180)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 80% 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 44 minutes.