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🔭 Seeing & Atmosphere
Forecast seeing
Transparency
Lifted index
Visibility
AI seeing estimate
Star quality (AI)
☁️ Cloud Cover
AI cloud cover
Cloud trend
Quadrant affected
Forecast clouds (7t)
Forecast clouds (om)
Prediction 1h
💨 Wind & Surface
Wind speed
Gusts
Upper atm. (850 hPa)
Temperature
Humidity
Dew point
⭐ Sky Quality
SQM (sensor)
Cloud sensor (ΔT)
AI confidence
Sky scene (AI)
Precip. probability
Sky color (AI)
🌫️ Calima & Aerosols
Status
AOD (opacity)
Dust µg/m³
PM10 µg/m³
AOD<0.1 = clear · 0.1–0.3 = haze · >0.3 = dust event
🌧️ Rain Station
Status
Today acc.
Rate last 1h
Dew point acc.
Data quality
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All-sky camera La Palma live
All-sky · La Palma · updates every 60s
°C
Temperature
%
Humidity
km/h
Wind
km/h
Gusts
SQM
Sky Quality
ΔT °C
Cloud sensor
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⭐ Verified Sky Data · La Palma 2025

The Numbers Behind Our Sky

Real measurements from our on-site weather station · 786,000+ data points · All values independently verifiable

311
Useful nights / year
≥1h of clear, safe conditions
85%
Clear night rate
287 nights · cloudsSafe sensor
21.57
SQM mean · new moon
mag/arcsec² · all-year average
22.03
SQM peak · winter
Confirmed manual measurement
☀ Clear nights per month
✩ SQM seasonal curve · new moon
📊 Monthly conditions
MonthClearTemp °CHumWind km/hSQM New MoonMilky Way
ⓘ Why SQM varies seasonally — the Milky Way effect

The SQM measures total sky brightness — including the Milky Way. When the galactic core rises (Jun–Sep), it contributes diffuse glow, slightly lowering readings (∼21.57 in August). In winter, the sky reaches peak darkness (up to 22.03 in February). This seasonal variation is only detectable at the world’s darkest sites. Our sky is so dark that the Milky Way itself is the primary source of sky brightness in summer.