Sunrise Sunset Calculator
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Contact UsEver 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.
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.
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