Sunrise & Sunset Times Today — Free Solar Calculators

Check today's sunrise and sunset times, golden hour, blue hour, day length, and sun angles for any location. Simple, fast, and free.

Quick Answer

Sunrise and sunset times depend on your latitude, longitude, and the date. At 40°N latitude (New York, Madrid, Beijing), April sunrise is ~6:20 AM and sunset is ~7:40 PM. Day length ranges from ~9 hours at winter solstice to ~15 hours at summer solstice.

Golden hour (best photography light) starts ~1 hour after sunrise and ~1 hour before sunset. Blue hour occurs during civil twilight (sun 0-6° below horizon).

Calculate Exact Sunrise & Sunset for Your Location →

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Sunrise & Sunset Times for Major Cities (Today's Approximate Values)

City Latitude Summer Sunrise Summer Sunset Winter Sunrise Winter Sunset
New York40.7°N5:25 AM8:31 PM7:16 AM4:32 PM
London51.5°N4:43 AM9:21 PM8:04 AM3:53 PM
Tokyo35.7°N4:25 AM7:01 PM6:47 AM4:28 PM
Sydney33.9°S5:37 AM8:09 PM7:01 AM4:53 PM
Dubai25.2°N5:28 AM7:12 PM6:56 AM5:33 PM
Reykjavik64.1°N2:55 AM12:04 AM11:22 AM3:30 PM
Los Angeles34.1°N5:42 AM8:08 PM6:55 AM4:44 PM
Paris48.9°N5:46 AM9:57 PM8:43 AM4:54 PM
Singapore1.3°N6:59 AM7:12 PM6:59 AM7:03 PM
São Paulo23.5°S5:33 AM6:50 PM6:47 AM5:22 PM

Summer = June solstice, Winter = December solstice. Times are approximate local time. Get exact times for your location →

About SunCalc

SunCalc provides free, accurate solar calculators for sunrise, sunset, golden hour, blue hour, and day length. Whether you are a photographer planning a shoot, a gardener tracking sunlight, or simply curious about the sun, all results are instant with no sign-up required.

How Sunrise and Sunset Times Are Calculated

Sunrise and sunset times depend on latitude, longitude, and the date. The calculation uses the solar declination angle (how far north or south of the celestial equator the sun is, which changes throughout the year as Earth orbits the sun) and the hour angle (the sun's angular distance from the observer's meridian). Solar noon — when the sun is at its highest point in the sky — occurs when the sun crosses the observer's meridian, which is local apparent solar time 12:00. This differs from clock noon by the equation of time (up to ±16 minutes due to Earth's elliptical orbit and axial tilt) and the observer's longitude within their time zone.

The Golden Hour and Blue Hour for Photography

The golden hour is the period shortly after sunrise and before sunset when sunlight is warm in colour (2,000–3,500 K colour temperature) and travels at a low angle, casting long soft shadows and minimising harsh contrast. It lasts approximately 20–60 minutes depending on latitude and season — longer at high latitudes where the sun moves more obliquely across the sky. The blue hour occurs before sunrise and after sunset during civil twilight, when the sun is between 0° and 6° below the horizon. The sky appears a deep, even blue because scattered indirect sunlight provides ambient illumination without direct sun. Photographers prize both periods for portraiture, architecture, and landscape work.

Day Length, Solstices, and Seasonal Variation

The length of the day — time between sunrise and sunset — varies dramatically with latitude and season. At the equator, day length is nearly constant at 12 hours year-round. At 50° north latitude (London, Vancouver), day length ranges from about 7.5 hours at the winter solstice to 16.5 hours at the summer solstice. At the Arctic Circle (66.5° north), the sun does not set for several days around the summer solstice (midnight sun) and does not rise for several days around the winter solstice (polar night). The summer solstice (around June 21 in the Northern Hemisphere) is the longest day; the winter solstice (around December 21) is the shortest.

Day Length by Latitude — Seasonal Comparison

Latitude Example City Summer Solstice Equinox Winter Solstice Variation
0° (Equator)Singapore12h 7m12h 7m12h 6m~1 min
25°NDubai13h 44m12h 8m10h 33m3h 11m
35°NTokyo14h 35m12h 9m9h 45m4h 50m
40°NNew York15h 5m12h 9m9h 15m5h 50m
51°NLondon16h 38m12h 10m7h 50m8h 48m
64°NReykjavik21h 8m12h 16m4h 7m17h 1m

Day length = time between sunrise and sunset. Higher latitudes have more extreme seasonal variation. Calculate daylight hours for your latitude →

What is a Sunrise & Sunset Calculator?

A sunrise and sunset calculator determines the exact times the sun appears above and disappears below the horizon for any location on Earth and any date. It uses astronomical algorithms based on Earth's orbital mechanics, axial tilt, and the observer's geographic coordinates to compute solar position throughout the day.

These calculations are essential for photographers planning golden hour and blue hour shoots, farmers and gardeners optimizing planting schedules around daylight hours, solar energy professionals sizing panel installations, and outdoor event planners who need to know exactly when natural light will be available.

SunCalc goes beyond basic sunrise and sunset times by also calculating solar noon, solar elevation angles, twilight phases (civil, nautical, and astronomical), golden hour windows, blue hour windows, and seasonal daylight comparisons -- all computed instantly in your browser with no downloads or sign-ups required.

Frequently Asked Questions

How are sunrise and sunset times calculated?

Sunrise and sunset times are calculated using the solar declination angle (which changes throughout the year due to Earth's axial tilt), the observer's latitude and longitude, and the hour angle. The sun is considered to rise and set when its center is 0.833 degrees below the horizon, accounting for atmospheric refraction and the sun's apparent diameter.

What is the golden hour in photography?

The golden hour is the period shortly after sunrise and before sunset when sunlight has a warm color temperature (2,000-3,500K) and arrives at a low angle. This creates soft, diffused light with long shadows and minimal harsh contrast. It typically lasts 20-60 minutes depending on your latitude and the season.

What is the blue hour?

The blue hour occurs during civil twilight, when the sun is between 0 and 6 degrees below the horizon. The sky takes on a deep, even blue color because indirect scattered sunlight provides ambient illumination without direct sun. It happens just before sunrise and just after sunset, lasting roughly 20-40 minutes.

Why does day length vary throughout the year?

Day length varies because Earth's rotational axis is tilted 23.44 degrees relative to its orbital plane. During summer in the Northern Hemisphere, the North Pole tilts toward the sun, giving longer days. During winter, it tilts away, giving shorter days. At the equator, day length stays near 12 hours year-round.

How accurate are SunCalc's calculations?

SunCalc uses standard astronomical algorithms based on the solar position equations. Results are typically accurate to within 1-2 minutes for sunrise and sunset times. Minor variations can occur due to local terrain, altitude, and atmospheric conditions that affect refraction.

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