Lunar Eclipses in Saros Series 175

This page lists all the lunar eclipses in saros series 175 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 182.

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).
11 Feb, 2791 AD
max: 02:09 UT
Penumbral Lunar Eclipse
(penum. mag. 0.00; Saros 175)
In this virtually non-existant eclipse, the Moon barely clips the edge of the Earth's penumbral shadow; although the eclipse will last 7 minutes and 24 seconds, it will be impossible to see in practice.
   
21 Feb, 2809 AD
max: 10:31 UT
Penumbral Lunar Eclipse
(penum. mag. 0.01; Saros 175)
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 1% of the Moon's disc for 32 minutes and 17 seconds, which will be essentially impossible to see.
   
4 Mar, 2827 AD
max: 18:47 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 175)
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 3% of the Moon's disc for 51 minutes and 24 seconds, which will be essentially impossible to see.
   
15 Mar, 2845 AD
max: 02:56 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 175)
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 6% of the Moon's disc for 1 hour and 11 minutes, which will be essentially impossible to see.
   
26 Mar, 2863 AD
max: 10:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.10; Saros 175)
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 10% of the Moon's disc for 1 hour and 31 minutes, which will be essentially impossible to see.
   
5 Apr, 2881 AD
max: 18:48 UT
Penumbral Lunar Eclipse
(penum. mag. 0.15; Saros 175)
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 15% of the Moon's disc for 1 hour and 52 minutes, which will be essentially impossible to see.
   
17 Apr, 2899 AD
max: 02:30 UT
Penumbral Lunar Eclipse
(penum. mag. 0.21; Saros 175)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 13 minutes, just 21% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
28 Apr, 2917 AD
max: 10:02 UT
Penumbral Lunar Eclipse
(penum. mag. 0.29; Saros 175)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 35 minutes, just 29% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
9 May, 2935 AD
max: 17:25 UT
Penumbral Lunar Eclipse
(penum. mag. 0.38; Saros 175)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 56 minutes, just 38% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
20 May, 2953 AD
max: 00:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 175)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 18 minutes, just 48% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
31 May, 2971 AD
max: 07:42 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 175)
This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 38 minutes, just 59% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
   
10 Jun, 2989 AD
max: 14:37 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 175)
This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 72% 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 58 minutes.