NOAA Solar Calculator

Find Sunrise, Sunset, Solar Noon and Solar Position for Any Place on Earth

Show:
Drag the large red pin to the desired location and enter the date and time at which to calculate the sun position.

Location:
Latitude - An angular measurement of north-south location on Earth's surface. Latitude ranges from -90 at the south pole, to zero at the equator, to +90 at the north pole." data-toggle="popover" role="button" tabindex="0">
Longitude - An angular measurement of east-west location on Earth's surface. Longitude ranges from -180 in the western hemisphere to +180 in the eastern, with zero at the prime meridian, which passes through Greenwich, England." data-toggle="popover" role="button" tabindex="0">
time zone and UTC offset are automatically determined when possible based on the given location and date. Once the location has been set, the user may manually override the time zone or UTC offset by selecting them here." data-toggle="popover" role="button" tabindex="0">
UTC offset is automatically determined when possible, based on the given time zone and date. The user can manually override this value by entering it here after location, time zone and date have been set." data-toggle="popover" role="button" tabindex="0">
Date:
 :   : 

Result
Equation of time - an astronomical term accounting for changes in the time of solar noon for a given location over the course of a year. Earth's elliptical orbit and Kepler's law of equal areas in equal times are the culprits behind this phenomenon." data-toggle="popover" role="button" tabindex="0">
(minutes):
Solar Declination - The declination of the sun. The solar declination varies from -23.44° at the (northern hemisphere) winter solstice, through 0° at the vernal equinox, to +23.44° at the summer solstice. The variation in solar declination is the astronomical description of the sun going south (in the northern hemisphere) for the winter. " data-toggle="popover" role="button" tabindex="0">
(in°):
Solar Noon - Defined for a given day for a specific longitude, it is the time when the sun crosses the meridian of the observer's location. At solar noon, a shadow cast by a vertical pole will point either directly north or directly south, depending on the observer's latitude and the time of year." data-toggle="popover" role="button" tabindex="0">
(hh:mm:ss):
Apparent Sunrise - Due to atmospheric refraction, sunrise occurs shortly before the sun crosses above the horizon. Light from the sun is bent, or refracted, as it enters earth's atmosphere. This effect causes the apparent sunrise to be earlier than the actual sunrise." data-toggle="popover" role="button" tabindex="0">
(hh:mm):
Apparent Sunset - Due to atmospheric refraction, sunset occurs shortly after the sun crosses below the horizon. Light from the sun is bent, or refracted, as it enters earth's atmosphere. This effect causes the apparent sunset to be later than the actual sunset." data-toggle="popover" role="button" tabindex="0">
(hh:mm):
Azimuth/Elevation - An angular coordinate system for locating positions in the sky. Azimuth is measured clockwise from true north to the point on the horizon directly below the object. Elevation is measured vertically from that point on the horizon up to the object." data-toggle="popover" role="button" tabindex="0">
(in °) at Local Time:

Sunrise/Sunset Tables

Tables with times of sunrise, sunset and solar noon for each day of the year for the location and year specified in the form above can be created by clicking on the button below.


Tables will open up in a new tab/window

Interested in Doing Your Own Calculations?

Details about the calculations and spreadsheets that can be used to calculate solar data are available on the solar calculation details page.

Having Trouble?

Questions?

Feel free to write to us with any questions or comments at Webmaster.

Solar Calculation Resources: