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Beijing, China40.19° N, 116.70° E

Sunrise & Sunset in Beijing Today

Welcome to the definitive solar ephemeris for Beijing (China), situated at geographic coordinates 40.1942° N latitude and 116.6974° E longitude within the Asia/Shanghai timezone. Because Beijing is positioned at mid-latitude coordinates, daylight duration fluctuates predictably throughout the solar year—reaching its maximum duration during the June solstice and its annual minimum near the December solstice.

All timestamps displayed below are computed using client-side spherical astronomy algorithms derived from the U.S. Naval Observatory Astronomical Almanac 2024 and the NOAA Solar Calculator, accounting for standard 34-arcminute atmospheric refraction and 16-arcminute solar semidiameter at sea level.

Sunrise & Sunset in Beijing, China

US Naval Observatory (USNO) Astronomical Almanac 2024 p.C24 & NOAA Solar Model

cos(H) = (cos(90.833°) - sin(δ)·sin(φ)) / (cos(δ)·cos(φ))
Sunrise
09:15 PM
Official Horizon (90°50′)
Sunset
11:22 AM
Official Horizon (90°50′)
Solar Noon
04:18 PM
Highest solar culmination
Day Length
-10h -52m
Golden Hour Photographic Windows (Sun < 6° Elevation)
Morning Golden Hour
09:15 PM10:15 PM
Warm dawn sidelight for landscapes
Evening Golden Hour
10:22 AM11:22 AM
Soft sunset illumination for portraits
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7-Day Solar Forecast for Beijing

Updated daily
DateSunriseSolar NoonSunsetDaylight
Thu, Aug 6Today
09:15 PM04:18 PM11:22 AM-10h -52m
Fri, Aug 7
09:15 PM04:18 PM11:21 AM-10h -54m
Sat, Aug 8
09:16 PM04:18 PM11:20 AM-10h -57m
Sun, Aug 9
09:17 PM04:18 PM11:19 AM-10h -59m
Mon, Aug 10
09:18 PM04:18 PM11:17 AM-11h -1m
Tue, Aug 11
09:19 PM04:18 PM11:16 AM-11h -3m
Wed, Aug 12
09:20 PM04:18 PM11:15 AM-11h -5m

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Frequently Asked Questions

Q1.What is the exact solar noon in Beijing?

Solar noon in Beijing occurs when the sun crosses the local celestial meridian (116.70° E) and reaches its maximum angular elevation above the horizon. Because Beijing operates on Asia/Shanghai, solar noon typically occurs around mid-day, adjusted for the seasonal Equation of Time.

Q2.How does atmospheric refraction affect sunrise and sunset in Beijing?

At latitude 40.19°, standard atmospheric refraction lifts the apparent image of the solar disc by approximately 34 arcminutes (0.566°). Combined with the sun’s 16 arcminute semidiameter, official sunrise and sunset are calculated when the center of the true solar disc is 90°50′ from the zenith.

Q3.When are the golden hour shooting windows in Beijing?

The morning golden hour begins at sunrise and lasts for approximately 60 minutes as the sun climbs to 6° solar elevation. The evening golden hour begins 60 minutes before sunset and concludes as the sun dips below the horizon, providing warm, diffused lighting ideal for outdoor photography.

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