Sunrise Sunset Calculator
Determine daily sunrise and sunset times for any location. Calculate daylight hours, twilight periods, and track seasonal light changes.
Interested in Advertising?
Tell us more, and we'll get back to you.
Contact Us
Determine daily sunrise and sunset times for any location. Calculate daylight hours, twilight periods, and track seasonal light changes.
Tell us more, and we'll get back to you.
Contact UsDetermine daily sunrise and sunset times for any location. Calculate daylight hours, twilight periods, and track seasonal light changes.
Share the current inputs or ask ChatGPT to explain the calculation in context.
Ever wondered why sunrise times change throughout the year, or why the golden hour produces such magical light? The movement of the Sun across our sky follows precise mathematical patterns that humans have studied for millennia. Today, we can predict these solar events down to the second, thanks to our deep understanding of Earth's motion and modern computational methods.
Imagine a photographer planning a coastal sunrise session. The calculator shows sunrise at 6:12 AM, civil twilight beginning at 5:44 AM, and solar noon at 12:38 PM for the selected coordinates. The method is to use the event time for the Sun's ideal-horizon position, then add practical buffers. Arriving at 6:10 AM would be too late because composition, parking, tide, and tripod setup all happen before the first visible edge of the Sun. A better plan is to arrive during civil twilight, scout the foreground, and be ready before color develops.
Now adjust the assumptions. If the same location has a ridge east of the viewpoint, visible sunrise may occur several minutes after the astronomical value. If fog or marine cloud is likely, golden-hour color may not appear even though the calculation is correct. If the site is near a time-zone boundary or daylight saving transition, the local clock time deserves an extra check. For hiking, boating, field work, or construction, build in a safety margin and carry lighting rather than relying on the final minute before sunset.
The same method helps solar and garden planning. Compare dates near the solstices and equinoxes instead of trusting one result, because daylight range and sunrise direction can change substantially through the year. Pair the calculator with a map for azimuth, a forecast for clouds and smoke, and an on-site check for buildings or trees. When a result shows no sunrise or no sunset at high latitude, treat it as a possible polar-day or polar-night condition rather than an automatic error.
Common mistakes include entering the wrong longitude sign, forgetting daylight saving time, using city-center coordinates for a remote site, or assuming twilight means the same thing for every activity. Civil, nautical, and astronomical twilight answer different questions. Choose the event definition that matches the rule, photograph, journey, or observation you are planning.
For operational schedules, write down the location, coordinate source, time zone, date, event definition, and backup plan. A sunrise result used for a photo walk can tolerate a few minutes of uncertainty. A sunrise result used for marine navigation, remote field work, or safety-critical access should be checked against authoritative local guidance and real conditions. The calculation is a strong planning aid, but it cannot see clouds, closed roads, tides, smoke, terrain, or equipment delays.
When comparing multiple locations, keep the same date and time-zone assumptions. Changing both the place and the date at once makes it harder to know whether the difference came from latitude, longitude, season, or clock rules. Change one factor at a time when planning trips or solar studies.
Save the calculated time with the coordinate pair, not only the place name, so another person can reproduce the same sunrise or sunset estimate later.
This is especially important for parks, coastlines, and mountain viewpoints with broad or ambiguous names.
Sunrise and sunset times depend strongly on latitude and longitude. A location name may cover a large city, park, county, or coastline, so coordinates are often more reliable than a label. A few miles east or west can shift solar time, and moving north or south changes day length, especially away from the equator. For photography, hiking, marine work, or solar planning, use the coordinates of the actual site rather than the nearest downtown. Elevation and local terrain add another layer. A mountain ridge, tall building, forest edge, or ocean horizon can make the visible sunrise later or sunset earlier than the astronomical value. The calculator gives the Sun's position relative to an ideal horizon. Field conditions decide when light reaches your eyes or camera.
Solar events are calculated from Earth geometry, then displayed in civil time. Time zone selection matters. A location near the western edge of a time zone can have later clock sunrise and sunset than a location near the eastern edge, even on the same date. Daylight saving time shifts the clock by one hour but does not change the Sun. If a result looks off by about an hour, check whether daylight saving applies on that date. Also watch for travel across time zones and calendar dates near midnight UTC. For scheduling, write the local date, local time zone, and location together. This is especially important for flights, remote shoots, field crews, astronomy sessions, and calls between regions. A correct solar calculation can still be used incorrectly if the clock context is missing.
Astronomical sunrise and sunset usually refer to the moment the upper edge of the Sun appears or disappears at the horizon, with a standard correction for atmospheric refraction and the Sun's apparent radius. That means sunrise can occur before the geometric center of the Sun reaches the horizon. Weather changes the experience. Haze, clouds, smoke, fog, and terrain can delay the first visible light or hide the Sun completely. For photography, the usable light often begins before sunrise and continues after sunset. For legal or operational rules, use the definition specified by the relevant authority. Hunting, aviation, sailing, construction, and religious observance may use different standards. The calculator is a planning reference, and the meaning of sunrise should match the task.
Twilight periods describe how far the Sun is below the horizon. Civil twilight is bright enough for many outdoor activities without artificial light. Nautical twilight keeps the horizon visible at sea while many stars appear. Astronomical twilight ends when the sky becomes dark enough for faint observations. These periods can matter more than sunrise or sunset alone. A runner may care about civil dawn, a navigator about nautical twilight, and an astrophotographer about astronomical darkness. At high latitudes, twilight can last a long time or never fully end during part of the year. When planning outdoor work, safety, or photography, check both the event time and the twilight window. The best time for the task may be before sunrise or after sunset rather than at the exact solar edge.
Day length changes through the year because Earth's axis is tilted. Near the equator, sunrise and sunset stay relatively steady. Farther from the equator, summer days lengthen and winter days shorten. Near the polar circles, the Sun may stay above or below the horizon for extended periods. These extremes affect travel, sleep, agriculture, solar production, wildlife, and outdoor safety. If the calculator returns no sunrise or no sunset for a high latitude date, that may be correct. It can indicate midnight sun, polar night, or a day where the Sun only grazes the horizon. For projects that span weeks or months, compare several dates rather than relying on one day. Seasonal change can be larger than expected.
A precise solar time does not guarantee the expected light. Clouds can erase golden hour color, haze can soften contrast, and clear dry air can make shadows sharper. For photography or field work, combine calculated solar times with weather, cloud cover, smoke, tide, access, and terrain checks. Visit the site in advance if the event matters. Note where the Sun will rise or set on the horizon, because the azimuth changes across the year. A winter sunset may line up with a street or valley that the summer sunset misses completely. The calculator tells when the solar event occurs. A map, forecast, and on site view tell whether that event will be visible and useful.
Solar noon is the time when the Sun reaches its highest point for the day. It is not always 12:00 on the clock because longitude within the time zone and the equation of time shift it. Solar noon helps photographers, gardeners, solar panel owners, and hikers understand the symmetry of daylight around the day. If sunrise and sunset look uneven around clock noon, solar noon explains why.
The time of sunrise or sunset tells when the event happens, while azimuth tells where on the horizon it happens. Direction changes through the year. A window, street, ridge, or beach may line up with sunrise in one season and miss it in another. For photography, architecture, and site planning, pair the calculator time with a map or compass direction so you know where the light will come from.
Outdoor plans should not rely on the last minute of daylight. Trails, boats, construction sites, and remote roads need a margin for delays, terrain, weather, and slower travel in dim light. If sunset is at 6:20, plan to finish critical tasks before then and carry lighting anyway. Twilight can help, but clouds and tree cover can make it feel dark earlier than the calculated time.
For trips, shoots, and solar studies, check the day before and the day after the target date. Solar times change gradually, but the rate of change varies by season and latitude. Around equinoxes the change can be noticeable from day to day. Around solstices it can be slower. Comparing nearby dates helps choose backups and shows whether a delay will matter.
Standard sunrise and sunset calculations include an average atmospheric refraction correction, but real refraction varies with temperature, pressure, and weather near the horizon. Unusual conditions can shift the visible edge of the Sun by a small amount. For everyday planning this is minor. For precise observation, navigation, or scientific timing, record local conditions and use methods designed for that level of accuracy.
An ideal horizon is rare. Buildings, hills, trees, dunes, and mountains can hide the Sun well after calculated sunrise or before calculated sunset. If visibility matters, estimate the obstruction angle or check the site with a mapping tool. A high ridge to the east can make morning light arrive much later than the calculator time, while an ocean horizon may match the calculation closely.
Solar panels, daylighting studies, and garden planning depend on patterns, not one date. Check representative dates near solstices and equinoxes, then compare the range of daylight and Sun direction. This shows whether a site gets reliable winter light or only strong summer light. A single sunny day can be misleading if the project needs year round performance.
Sunrise and sunset times are calculated using the sun's declination angle, the observer's latitude, and the equation of time. The sun rises when its center reaches 0.833 degrees below the horizon, accounting for atmospheric refraction and the sun's apparent diameter.
Earth's 23.5-degree axial tilt causes the sun's path across the sky to shift seasonally. During summer in the Northern Hemisphere, the sun follows a higher, longer arc producing later sunsets and earlier sunrises. The opposite occurs in winter.
Civil twilight is the period when the sun is between 0 and 6 degrees below the horizon. There is enough natural light for most outdoor activities without artificial lighting. Nautical twilight extends to 12 degrees and astronomical twilight to 18 degrees below the horizon.
Locations closer to the equator experience relatively consistent 12-hour days year-round. As latitude increases, seasonal variation grows dramatically. Above the Arctic or Antarctic circles, there are periods of 24-hour daylight in summer and 24-hour darkness in winter.
The equation of time accounts for the difference between solar time and clock time, caused by Earth's elliptical orbit and axial tilt. This difference can be up to 16 minutes and affects the exact moment of solar noon, shifting sunrise and sunset times throughout the year.