Sunrise Calculator - Astronomical Solar Transit Estimation

Use this Sunrise Calculator to determine the precise local time of sunrise, sunset, and solar noon for any date and coordinate location on Earth.

Updated: June 30, 2026 • Free Tool

Sunrise Calculator

Enter latitude in degrees. Use positive values for North (e.g., 40.7128) and negative values for South (e.g., -33.8688).

Enter longitude in degrees. Use positive values for East (e.g., 151.2093) and negative values for West (e.g., -74.0060).

Select the calendar year (between 1901 and 2099) for which you want to run the calculation.

Select the month of the year (1 for January through 12 for December).

Select the day of the month (1 to 31).

Your local timezone offset relative to Coordinated Universal Time (UTC). For example, Eastern Daylight Time (EDT) is -4, GMT/UTC is 0.

Results

Sunrise Time
0
Sunset Time 0
Solar Noon 0
Day Length 0
Solar Declination 0degrees
Equation of Time 0minutes
Calculation Status 0

What Is Sunrise Calculator?

A sunrise calculator is an astronomical tool that computes the exact local clock time when the upper edge of the Sun becomes visible above the geographic horizon. It processes geographic coordinates (latitude and longitude), calendar dates, and timezone parameters to model the relative position of the Earth and the Sun. These solar calculations are essential for a wide range of academic, scientific, and recreational activities, ranging from photography scheduling to civil engineering and renewable solar energy planning.

  • Outdoor Photography and Film Planning: Determine the exact arrival of the golden hour, which begins immediately at sunrise, to capture landscapes and outdoor scenes under optimal natural lighting conditions.
  • Agriculture and Crop Management: Calculate solar light exposure patterns to optimize planting schedules, harvest planning, and greenhouse lighting setups based on daily changes in day length.
  • Aviation and Marine Operations: Calculate daylight transitions to comply with transport regulations regarding night flights, vessel operation logs, and navigation visual rules.
  • Renewable Solar Energy Placement: Estimate daily solar exposure duration to evaluate optimal angles and tracking schedules for solar panels and photovoltaic arrays.

In astronomical terms, sunrise is defined as the precise instant when the upper limb of the solar disk appears on the horizon. This is distinct from civil twilight, which describes the period when light is present but the solar disk itself is still below the horizon. The timing varies continuously throughout the calendar year due to the Earth's axial tilt of approximately twenty-three and a half degrees.

Because the Earth rotates at a uniform rate, the time of sunrise depends strictly on the observer's latitude and longitude. An observer situated further east will experience sunrise earlier than an observer further west within the same timezone. By entering your specific coordinates into the calculator, you bypass standard timezone approximations to receive coordinates-specific results.

To see the complete profile of daylight duration, sunset times, and twilight phases alongside sunrise, our daylight calculator provides a comprehensive daily light breakdown for any coordinate.

How Sunrise Calculator Works

The mathematical foundation of this sunrise calculator is based on Jean Meeus' astronomical algorithms and the standard NOAA solar equations. The calculation models the eccentricity of the Earth's orbit and the orientation of the Earth's axis to determine solar transit times.

cos(H) = (cos(90.833) / (cos(latitude) * cos(declination))) - tan(latitude) * tan(declination)
  • H (Hour Angle): The angular distance of the Sun from the observer's meridian, representing the time interval before or after solar noon.
  • Latitude: The observer's angular distance north or south of the equator, measured in decimal degrees.
  • Declination: The angle of the Sun relative to the Earth's equator, varying between +23.45 degrees and -23.45 degrees depending on the season.
  • 90.833 Degrees: The solar zenith angle used at sunrise, representing 90 degrees plus 0.833 degrees of correction for atmospheric refraction and the Sun's radius.

New York Summer Solstice Approximation

1. Day of Year (n) = 181 (June 30). 2. Fractional Year (gamma) = 2 * pi * (181 - 1) / 365 = 3.10 radians. 3. Equation of time = -3.259 minutes; Declination = 23.236 degrees. 4. cos(H) for latitude 40.7128 N yields H = 113.5 degrees. 5. Sunrise UTC time = 720 - 4 * (-74.006 + 113.5) - (-3.259) = 565 UTC minutes. 6. Adjusted for EDT (UTC-4) offset = 565 - 240 = 325 local minutes, which represents 5:27 AM.

On June 30 in New York, the sun rises at 5:27 AM EDT, reflecting the long summer day length where the sun rises far north of east.

London Winter Solstice Approximation

1. Day of Year (n) = 355 (December 21). 2. Fractional Year (gamma) = 2 * pi * (355 - 1) / 365 = 6.09 radians. 3. Equation of time = 2.171 minutes; Declination = -23.420 degrees. 4. cos(H) for latitude 51.5074 N yields H = 58.7 degrees. 5. Sunrise UTC time = 720 - 4 * (-0.1278 + 58.7) - 2.171 = 483 UTC minutes. 6. Adjusted for UTC+0 offset = 483 local minutes, representing 8:03 AM.

On December 21 in London, the sun rises at 8:03 AM GMT, reflecting the short winter day length with the sun rising far south of east.

According to Wikipedia Solar Calculations, the exact times of sunrise and sunset are calculated using mathematical models that estimate solar declination and the Equation of Time from the fractional year angle.

Because solar declination and equation of time stem directly from Earth's elliptical path, using the earth orbit calculator helps you visualize how solar zenith angles change with orbital velocity and eccentricity.

Key Concepts Explained

Understanding solar calculations requires familiarity with three fundamental astronomical parameters.

Equation of Time

The Equation of Time describes the discrepancy between apparent solar time (sundial time) and mean solar time (standard clock time). This variance arises because the Earth's orbit is elliptical rather than circular, and the Earth's equator is tilted relative to its orbital plane. This causes the length of a solar day to fluctuate slightly throughout the year, accumulating a variance of up to 16 minutes.

Solar Declination

Solar declination is the latitude at which the Sun is directly overhead at solar noon. It changes continuously as the Earth orbits the Sun, reaching its peak of +23.44 degrees at the northern summer solstice and its minimum of -23.44 degrees at the northern winter solstice.

Atmospheric Refraction Correction

When we observe the Sun rising, Earth's atmosphere acts like a lens, bending the rays of light upward. As a result, the Sun appears above the horizon before its geometric center has actually reached it. To account for this refraction (averaging 34 arcminutes) and the Sun's semi-diameter (16 arcminutes), astronomers define sunrise when the center of the Sun is geometrically 90.833 degrees from the zenith.

Local Coordinate Variances

Geographical positioning determines the local solar horizon. Latitude alters the path length of the sun across the sky, changing daylight duration. Longitude shifts the exact time solar noon is reached relative to standard local time meridian zones, dictating the offsets applied to standard clock coordinates.

To study how the atmosphere bends the sun's rays to advance the sunrise, the angle of refraction calculator shows how light path deviations change depending on medium density and incidence angle.

How to Use This Calculator

To calculate the precise sunrise time for your location, follow these simple steps using the sunrise calculator.

  1. 1 Identify Your Latitude and Longitude: Obtain your coordinates in decimal degrees. Use a GPS device, digital map service, or local survey charts. North latitude and East longitude are positive; South latitude and West longitude are negative.
  2. 2 Select the Target Date: Enter the specific calendar year, month, and day for your calculation. The calculator accounts for leap years automatically.
  3. 3 Enter the Timezone Offset: Provide the timezone offset relative to Coordinated Universal Time (UTC) for the target date, adjusting for Daylight Saving Time if it is active on that date.
  4. 4 Interpret Calculated Output Metrics: View the generated clock times for sunrise, sunset, and solar noon, alongside calculated declinations and daylight durations to finalize planning.

If you are hiking near the Grand Canyon on October 15, you can enter Latitude 36.0544, Longitude -112.1401, and timezone offset -7. The calculator processes the solar declination for October 15 to output the exact time you need to be at the canyon rim to observe the sunrise.

If you are observing sunrise across a large body of water and want to calculate how much of the distant horizon is hidden by the Earth's curve, our earth curvature calculator provides the geometric dip parameters.

Benefits of Using This Calculator

Using a dedicated sunrise calculator offers critical advantages over manual lookup tables.

  • Exact Coordinates-Specific Results: Standard weather reports provide sunrise times for nearest major cities. This tool calculates the time for your exact coordinate location, which is crucial for remote field studies.
  • Grids and Map Alignment Integration: By combining coordinate data with geodetic checks, you can plan surveys and fieldwork with high spatial precision.
  • Timezone and Daylight Shifts Correction: The calculator isolates astronomical UTC values and applies your custom timezone offset, avoiding errors from automatic system offsets.
  • Automated Non-Standard Coordinate Math: Calculations for extreme latitudes and polar regions resolve automatically without numerical breakdown, flagging midnight sun and polar night periods.

The automated nature of the tool eliminates the risk of coordinate mismatch errors, making astronomical computations accessible to researchers without manual orbital tracking overhead.

When you want to find the exact compass heading of the rising sun using a local sighting compass, the magnetic declination calculator converts the calculated true astronomical azimuth into magnetic degrees.

Factors That Affect Your Results

Several environmental and geodetic variables can influence the results generated by the sunrise calculator compared to what you actually see.

Local Topography and Obstructions

Theoretical calculations assume a flat, unobstructed horizon at sea level. If you are surrounded by mountains, hills, or dense urban structures, the Sun will appear later as it must clear these physical obstructions.

Observer Elevation Above Sea Level

An observer standing at a high elevation (such as a mountain peak) will see the Sun rise slightly earlier than an observer at sea level. This occurs because the visible horizon dips downward from a higher vantage point.

Atmospheric Conditions

The standard correction of 34 arcminutes of refraction is based on average temperature and pressure. Extreme cold temperatures or high atmospheric pressure can increase refraction, causing the Sun to appear even earlier.

  • The calculator does not handle elevation changes directly. The theoretical model assumes a standard flat sea-level horizon.
  • Local microclimates, weather patterns, and mountain shadows will shift the apparent sunrise time relative to the calculated astronomical time.

The standard correction of 34 arcminutes of refraction is based on average temperature and pressure. Extreme cold temperatures or high atmospheric pressure can increase refraction, causing the Sun to appear even earlier.

According to U.S. Naval Observatory, astronomical calculations for sunrise and sunset times assume a standard atmospheric refraction value of 34 arcminutes and a solar semi-diameter of 16 arcminutes at sea level.

Once the sun has risen above the horizon, using the angle of incidence calculator helps you determine the angle at which solar rays strike a flat surface, which is critical for agricultural and solar power panel efficiency.

Sunrise Calculator featured image showing the sun rising over a mathematical horizon with latitude, longitude, declination, and equation of time equations
Sunrise Calculator featured image showing the sun rising over a mathematical horizon with latitude, longitude, declination, and equation of time equations

Frequently Asked Questions

Q: Why does the calculator use a solar zenith angle of 90.833 degrees?

A: A zenith angle of 90 degrees corresponds to a geometric horizon. The calculator adds 0.833 degrees (50 arcminutes) because of two physical effects: atmospheric refraction, which bends light around the Earth's curvature by about 34 arcminutes, and the Sun's angular radius, which is approximately 16 arcminutes. This ensures the calculation reflects when the top edge of the Sun is visible, rather than its center.

Q: How does atmospheric refraction affect the calculated sunrise time?

A: Atmospheric refraction bends light rays passing through Earth's air layers. This upward bending makes the Sun visible about 2 to 3 minutes before it geometrically clears the horizon. The exact deviation varies with temperature and pressure, but the calculator uses the standard astronomical correction of 34 arcminutes.

Q: What is the difference between solar noon and civil noon?

A: Solar noon is the moment when the Sun crosses the local meridian and reaches its highest point in the sky. Civil noon is exactly 12:00 PM on standard clock time. They rarely coincide because timezone boundaries are wide and the Earth's orbital speed varies throughout the year, causing solar noon to drift by up to 30 minutes from 12:00 PM.

Q: Why does the sunrise calculator fail at high latitudes near the poles?

A: At high latitudes during summer and winter, the Sun may remain entirely above or below the horizon for extended periods. When this occurs, the mathematical formula cos(H) yields a value greater than 1 or less than -1, which has no arccosine. The calculator detects this and outputs 'Polar night' or 'Midnight sun' instead of clock times.

Q: How does elevation affect the actual time of sunrise?

A: Higher elevation dips the observer's horizon, allowing them to see over the Earth's curve. As a rough approximation, every 100 meters of elevation advance the apparent sunrise by about one minute. This calculator assumes a sea-level horizon, so mountaintop observations will occur slightly ahead of the computed time.