Official Sunrise & Sunset
Calculated at a solar zenith angle of 90.8333° (accounting for 34 arcminutes of atmospheric refraction and 16 arcminutes of solar semi-diameter).
Calculate today's sunrise, sunset, solar noon, civil dawn/dusk, and daylight duration for any city worldwide using precise NOAA astronomical algorithms.
The timing of sunrise, sunset, and natural daylight is governed by Earth's axial tilt (23.44°) and elliptical orbit around the Sun. This solar calculator implements pure NOAA astronomical equations to compute the exact solar zenith angles, true solar time, and day length for any calendar date across the globe. To visualize the live terminator line and night shadows on a world map, explore the World Day & Night Map. For nighttime celestial tracking, consult our Moon Phase Calendar, or track live solar arcs on the Real-Time World Clock.
Calculated at a solar zenith angle of 90.8333° (accounting for 34 arcminutes of atmospheric refraction and 16 arcminutes of solar semi-diameter).
Calculates precise transition phases when the sun drops 6°, 12°, and 18° below the horizon for skywatchers and navigators.
Determines the exact minute the sun crosses the local celestial meridian and reaches its peak daily elevation angle.
Find the optimal natural lighting windows for photography when the sun is between 6° above the horizon and official sunset.
Mathematical support for Midnight Sun (24h continuous daylight) and Polar Night (continuous darkness) in Arctic and Antarctic latitudes.
High precision solar ephemeris computed in your browser without lag, rate limits, or external server dependencies.
Sunrise and sunset times are dictated by spherical trigonometry, the Earth's 23.44° axial tilt, and atmospheric optics. The NOAA astronomical engine calculates exact solar zenith thresholds to model each phase of daylight and dusk:
Because Earth is tilted at 23.44° relative to its orbital plane, day length varies dramatically with latitude throughout the year. At the Equator (0°), day length remains nearly constant at 12 hours year-round. Moving toward polar latitudes, summer solstices produce the Midnight Sun (24 hours of continuous sunlight), while winter solstices result in Polar Night.
To view the real-time curved terminator boundary separating day and night across the continents, explore our World Day & Night Map, or track celestial cycles on our Moon Phase Calendar.
Learn about NOAA solar calculation formulas, civil/nautical/astronomical twilight definitions, and polar day/night handling.
Sunrise is the moment when the upper edge of the sun first appears above the eastern horizon. You can find today local sunrise time by selecting your city in our solar calculator, which computes times based on precise latitude and longitude coordinates.
Sunset is the moment when the trailing edge of the sun disk disappears completely below the western horizon. Our calculator evaluates exact sunset, solar noon, and day length for any global location using NOAA astronomical algorithms.
Sunrise and sunset times change throughout the year because Earth is tilted on its rotational axis by approximately 23.5 degrees relative to its orbital plane around the Sun. As Earth orbits the Sun, this axial tilt causes daylight duration to expand during summer months and contract during winter months.
Solar times depend directly on geographical latitude and longitude. Locations farther east experience sunrise earlier than locations to the west within the same time zone, while latitude dictates how dramatically day length varies between summer and winter solstices.
Dawn is the period of twilight that occurs before sunrise, beginning when the morning sky first starts lightening while the sun is still below the horizon. Sunrise occurs only when the physical disk of the sun breaks above the horizon.
Sunset is the exact moment the sun dips completely below the horizon, while dusk is the twilight phase that follows sunset, concluding when complete night begins at the end of astronomical twilight.
Yes. Advancing civil clocks by one hour during daylight saving time makes sunrise and sunset appear to happen one hour later by the clock. While the physical solar cycle remains unchanged, the shift provides an extra hour of natural evening daylight for civil activities.