Beverly Hills stargazing forecast tonight
Hourly clear-sky conditions for observing: cloud by layer, transparency, estimated seeing, moonlight and true astronomical darkness.
Cloud or fog is the strongest score limit at the best sampled time.
The score describes tonight’s conditions. Site darkness helps you choose what to observe.
Tonight in context · local sky & season
October historically: 22.0 qualifying nights/month on average (2005–2024). Regional cloud and darkness history, not tonight’s probability or a comparison with the conditions score.
A qualifying historical night has at least 3 hours of astronomical darkness and mean nighttime cloud ≤30%. This does not measure steady air or target visibility. Seasonal history →
Saturn: about 9.0h above 20° during this observing night’s darkness. Longest sampled dark-time opportunity among our four planet targets; not a weather ranking. Planet times →
Position calculations use roughly 20-minute samples. Clouds, skyglow and local obstructions still matter. Milky Way timing →
45% high cirrus. Visual observers shrug it off; long exposures integrate it. What this means →
Also limiting: Seeing. See the guide →
The night, hour by hour
Colour = score · Luminance = everything elseCloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Score inspectorWhy this hour scored what it did Open peakClose
The sky is staying closed.
None of the five observing modes reaches a reliable setup window. Skip the empty charts and use tonight to make the next clear session easier.
Three useful moves, no dead chart.
The forecast detail above remains available when you need the measurements. These are the useful next decisions.
Your target still carries into clear-night recommendations and future alert rules.
Deep-sky visual is your current default.
Palomar Observatory
163 km away · Brightened sky · 20.4–21.0 mag/arcsec²
The next week of nights
Cloud or fog is the strongest score limit at the best sampled time.
Cloud or fog is the strongest score limit at the best sampled time.
20:00–06:00
23:00–00:00
05:00–06:00
23:00–00:00
23:00–00:00
Open a night for its forecast times. Later forecasts may have wider time steps; missing hours are not interpolated.
Tonight · 10 Oct · forecast times
Cloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Tomorrow · 11 Oct · forecast times
Cloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Monday · 12 Oct · forecast times
Cloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Tuesday · 13 Oct · forecast times
Cloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Wednesday · 14 Oct · forecast times
Cloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Thursday · 15 Oct · forecast times
Cloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Friday · 16 Oct · forecast times
Cloud tracks show clear sky — a longer bar is better. The figure inside each track is the raw measurement.
Planning a trip?
Compare the next eight weekends → · Best months to visit → · Moonless nights →
More nearby locations 8 options · openclose
- Brentwood 7 km
- Hollywood 7 km
- Studio City 8 km
- Universal City 8 km
- Koreatown 9 km
- Sherman Oaks 10 km
- Santa Monica 10 km
- Venice 11 km
About this forecast
Exact-coordinate weather, sky geometry and site context.
Sources and scoring details openclose
Conditions for Beverly Hills, California, United States are computed from the MET Norway forecast model for these exact coordinates, combined with sun and moon positions we calculate directly. The score weighs cloud cover by layer, atmospheric transparency, estimated seeing, moonlight and astronomical twilight. Site darkness is shown separately, then used only where artificial skyglow physically changes moon contrast, haze scattering, visual limits and target suitability.