SkyAlmanac

Moon · May 2026

Moon calendar for Clermont-Ferrand, Auvergne-Rhône-Alpes, France: May 2026

Daily moon phases, illumination, moonrise and moonset in Clermont-Ferrand, Auvergne-Rhône-Alpes, France for May 2026. Full moon: May 1, 2026, May 31, 2026. All times are shown in the local time of Clermont-Ferrand, Auvergne-Rhône-Alpes, France.

← April 2026 June 2026 →
Full moonFriday, May 1, 2026, 7:27 PM
Full moonSunday, May 31, 2026, 10:55 AM
New moonSaturday, May 16, 2026, 9:30 PM
Day Phase Illumination Moonrise Moonset
1 Full Moon 100% 8:45 PM 6:23 AM
2 Full Moon 99% 9:58 PM 6:42 AM
3 Waning Gibbous 97% 11:04 PM 7:31 AM
4 Waning Gibbous 93% 11:59 PM 7:58 AM
5 Waning Gibbous 87% 8:36 AM
6 Waning Gibbous 81% 12:41 AM 9:40 AM
7 Waning Gibbous 72% 1:36 AM 10:32 AM
8 Waning Gibbous 63% 2:11 AM 11:58 AM
9 Last Quarter 54% 2:27 AM 12:54 PM
10 Last Quarter 43% 2:56 AM 2:11 PM
11 Waning Crescent 33% 3:30 AM 3:30 PM
12 Waning Crescent 23% 3:38 AM 4:25 PM
13 Waning Crescent 15% 3:53 AM 5:44 PM
14 Waning Crescent 8% 4:18 AM 7:15 PM
15 Waning Crescent 3% 4:27 AM 8:25 PM
16 New Moon 0% 5:05 AM 9:52 PM
17 New Moon 1% 5:37 AM 11:28 PM
18 Waxing Crescent 4% 6:18 AM
19 Waxing Crescent 9% 7:29 AM 12:26 AM
20 Waxing Crescent 17% 8:28 AM 1:34 AM
21 Waxing Crescent 27% 10:03 AM 2:10 AM
22 Waxing Crescent 38% 11:32 AM 2:29 AM
23 First Quarter 49% 12:33 PM 3:04 AM
24 First Quarter 60% 2:04 PM 3:31 AM
25 Waxing Gibbous 70% 3:25 PM 3:37 AM
26 Waxing Gibbous 79% 4:23 PM 3:50 AM
27 Waxing Gibbous 87% 5:36 PM 4:16 AM
28 Waxing Gibbous 92% 6:30 PM 4:25 AM
29 Waxing Gibbous 97% 7:44 PM 4:47 AM
30 Full Moon 99% 8:43 PM 5:31 AM
31 Full Moon 100% 9:49 PM 5:54 AM

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Frequently asked questions

When is the full moon in May 2026 in Clermont-Ferrand, Auvergne-Rhône-Alpes, France?

The full moon peaks on Friday, May 1, 2026, 7:27 PM; Sunday, May 31, 2026, 10:55 AM (local time).

When is the new moon in May 2026?

The new moon falls on Saturday, May 16, 2026, 9:30 PM (local time) — the darkest nights of the month, best for stargazing.

Data: Meeus astronomical algorithms. How we calculate this

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