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Sunrise & Sunset Time Calculator

Enter your latitude, longitude, UTC offset, and date to calculate local sunrise, sunset, solar noon, daylight hours, and solar declination.
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Luis GonzalezCreated by Luis GonzalezLast updated:

How to Use This Calculator

  1. 1

    Select the Date

    Choose the specific date for which you want to calculate sunrise and sunset times.

  2. 2

    Enter Latitude

    Input your location's latitude in decimal degrees (positive for North, negative for South).

  3. 3

    Enter Longitude

    Input your location's longitude in decimal degrees (positive for East, negative for West).

  4. 4

    Specify UTC Offset

    Enter your local UTC offset in hours (e.g., -4 for Eastern Daylight Time). This converts results to your local time.

  5. 5

    Review Your Results

    The calculator will display local sunrise, sunset, solar noon, daylight duration, and solar declination.

Example Calculation

A planner in New York City (40.7128°N, -74.0060°W, UTC-4) wants to know the precise sunrise and sunset times for April 25, 2026.

Date

2026-04-25

Latitude (°)

40.7128

Longitude (°)

-74.0060

UTC Offset (hrs)

-4

Results

06

05 EDT

Tips

Verify UTC Offset

Ensure your UTC offset is accurate, especially if daylight saving time is in effect. An incorrect offset will lead to inaccurate local sunrise/sunset times.

Understand Twilight Phases

Beyond just sunrise and sunset, consider civil, nautical, and astronomical twilight. These phases define different levels of ambient light, crucial for activities like stargazing or navigation.

Latitude's Influence on Extremes

The closer you are to the poles, the more extreme the variations in daylight duration. High latitudes experience 'midnight sun' in summer and 'polar night' in winter, where the sun may not rise or set for extended periods.

Precisely Predicting Sunrise and Sunset Times Worldwide

The Sunrise & Sunset Time Calculator offers precise calculations for sunrise, sunset, solar noon, and daylight duration for any global location and date. This essential tool utilizes advanced solar geometry to provide accurate local times, which are invaluable for outdoor enthusiasts, photographers, architects, and anyone whose activities are governed by natural light cycles. Understanding that daylight can vary from 8 hours in winter to over 16 hours in summer for mid-latitude cities, this calculator empowers users to plan effectively and connect with the rhythms of the sun in 2025.

Precision in Astronomical Timekeeping and Observation

Accurate sunrise and sunset times are paramount for astronomers, forming the bedrock of observation planning and instrument calibration. These precise calculations enable astronomers to schedule deep-sky imaging sessions during periods of true darkness, avoiding the interference of twilight. They are also vital for studies involving solar system objects, ensuring that observations are timed correctly relative to the sun's position. The concept of civil, nautical, and astronomical twilight—each defining a progressively darker phase after sunset or before sunrise—is critical for observatories, determining when conditions are optimal for different types of celestial viewing. Moreover, accurate solar timekeeping is fundamental for tracking transient celestial events, such as meteor showers or satellite passes, where timing is everything.

The Solar Geometry Behind Sunrise and Sunset

The Sunrise & Sunset Time Calculator employs complex solar geometry algorithms to determine the sun's precise position relative to any point on Earth. It accounts for the Earth's tilt, orbit, and rotation, calculating the solar declination and hour angle for a given date and location.

The underlying process involves:

  1. Date Conversion: Converting the input date into a Julian day to precisely track Earth's position in its orbit.
  2. Solar Mean Anomaly & Equation of Center: Calculating the sun's apparent angular position and correcting for Earth's elliptical orbit.
  3. Solar Declination: Determining the sun's angular distance north or south of the celestial equator.
  4. Hour Angle: Calculating the hour angle when the sun's center is at the horizon (accounting for atmospheric refraction and the sun's angular radius).
  5. Sunrise/Sunset Calculation: Using the latitude, solar declination, and hour angle to find the local solar times of sunrise and sunset.
  6. UTC & Time Zone Conversion: Adjusting these solar times to the specified UTC offset for local clock time.
💡 Understanding the sun's position relative to Earth is fundamental to astronomy, much like understanding the distances of other planets from the sun. Our Planet Distance from Sun Calculator can help you explore solar system geometry further.

Calculating New York City's Solar Schedule

Let's determine the sunrise, sunset, and solar noon for New York City (Latitude: 40.7128°N, Longitude: -74.0060°W) on April 25, 2026, with a UTC offset of -4 hours (Eastern Daylight Time).

  1. Input Date: 2026-04-25
  2. Input Latitude: 40.7128°
  3. Input Longitude: -74.0060°
  4. Input UTC Offset: -4 hours

The calculator first determines the solar declination for April 25th, which is approximately 13.0° North. Using this, along with New York's latitude, it computes the hour angles for sunrise and sunset. These are then converted to UTC times and finally adjusted by the -4 hour offset for local EDT.

For this specific date and location, the calculator would yield:

  • Sunrise: Approximately 06:05 EDT
  • Sunset: Approximately 19:40 EDT
  • Solar Noon: Approximately 12:52 EDT
  • Daylight Duration: Approximately 13 hours and 35 minutes
  • Night Duration: Approximately 10 hours and 25 minutes
  • Solar Declination: 13.0°

This information shows a spring day with significantly more daylight than darkness, typical for New York City as it approaches summer.

💡 Just as we calculate the sun's precise position, astronomers use similar principles to determine the orientation of distant objects. The Saturn Ring Tilt Calculator offers insight into another fascinating celestial angle.

Solar Timing Standards for Diverse Fields

Precise solar timing is crucial across a variety of fields, extending far beyond general interest. In aviation regulations, pilots operating under Visual Flight Rules (VFR) often rely on civil twilight definitions for legal flight during marginal light conditions, typically 30 minutes before sunrise or after sunset. Marine navigation historically used sunrise and sunset for celestial navigation fixes, helping mariners determine their position by observing the sun's altitude at these precise moments. For wildlife research, accurate sunrise and sunset data is essential for tracking diurnal and nocturnal animal activity patterns, informing conservation efforts and behavioral studies. Furthermore, legal definitions of 'daylight hours' often dictate permissible construction noise, public event timings, or even hunting seasons, directly referencing solar events. These benchmarks underscore how deeply solar timing is embedded in operational standards and regulatory frameworks.

Frequently Asked Questions

What is solar declination and why does it change?

Solar declination is the angular position of the sun, either north or south of the Earth's celestial equator. It changes throughout the year due to the Earth's axial tilt (approximately 23.45°) relative to its orbit around the sun. This tilt causes the sun to appear to move between the Tropic of Cancer and the Tropic of Capricorn. Solar declination is zero at the equinoxes and reaches its maximum values at the solstices, directly influencing seasonal variations in daylight hours and sun elevation.

How does solar noon differ from local clock noon?

Solar noon is the exact moment when the sun reaches its highest point in the sky for a given location, directly bisecting the period between sunrise and sunset. It rarely aligns with 12:00 PM local clock time. Differences arise due to a location's longitude within its time zone, the Equation of Time (which accounts for Earth's orbital eccentricity and axial tilt), and daylight saving adjustments. Solar noon is a more accurate indicator of the sun's true zenith.

What is the significance of daylight duration?

Daylight duration, the period between sunrise and sunset, is a crucial metric for various applications. It impacts energy consumption (lighting, solar power generation), agricultural planning (crop growth cycles), human well-being (circadian rhythms, mood), and outdoor activity scheduling. The variation in daylight duration throughout the year is a primary driver of seasonal changes and is most pronounced at higher latitudes, where it can range from a few hours to nearly 24 hours.

Can this calculator predict polar night or midnight sun?

Yes, this calculator is designed to predict polar night (when the sun remains below the horizon for 24 hours or more) and midnight sun (when the sun remains above the horizon for 24 hours or more). These phenomena occur at latitudes greater than approximately 66.5° North or South, within the Arctic and Antarctic circles, during their respective winter and summer seasons. The calculator will indicate 'Polar night' for sunrise and 'Midnight sun' for sunset in these extreme conditions.