sunrise sunset calculator

Sunrise Sunset Calculator – Accurate Solar Times & Daylight Duration

Sunrise Sunset Calculator

Calculate precise sunrise, sunset, and twilight times for any location on Earth. Our Sunrise Sunset Calculator uses high-precision solar algorithms to provide accurate daylight data.

Positive for North, Negative for South (e.g., 40.7128 for NYC)
Please enter a valid latitude between -90 and 90.
Positive for East, Negative for West (e.g., -74.0060 for NYC)
Please enter a valid longitude between -180 and 180.
Select the date for calculation
Hours from UTC (e.g., -5 for EST)
Total Daylight Duration
12h 00m
Sunrise 06:00 AM
Solar Noon 12:00 PM
Sunset 06:00 PM

Visual Day/Night Cycle

Midnight Noon Midnight

The light blue area represents the duration of daylight calculated by the Sunrise Sunset Calculator.

Twilight Phases and Solar Data
Phase Start Time End Time Description
Civil Twilight Sun is 6° below horizon. Ideal for outdoor activities.
Nautical Twilight Sun is 12° below horizon. Horizon is visible at sea.
Astronomical Twilight Sun is 18° below horizon. Sky is completely dark.

What is a Sunrise Sunset Calculator?

A Sunrise Sunset Calculator is a specialized tool used to determine the exact moments when the upper limb of the sun appears on and disappears from the horizon. This calculation is vital for photographers, astronomers, farmers, and outdoor enthusiasts who rely on natural light cycles. Unlike simple estimates, a professional Sunrise Sunset Calculator accounts for geographic coordinates, atmospheric refraction, and the Earth's axial tilt.

Who should use it? Pilots use it for flight planning, religious practitioners for prayer times, and solar energy technicians to estimate peak generation periods. A common misconception is that sunrise and sunset occur at the same time for everyone on a specific longitude; however, latitude and elevation significantly alter these times.

Sunrise Sunset Calculator Formula and Mathematical Explanation

The math behind a Sunrise Sunset Calculator involves spherical trigonometry and the Julian calendar. The primary goal is to find the "Hour Angle" (H).

The fundamental formula used is:

cos(H) = (sin(h) - sin(φ) * sin(δ)) / (cos(φ) * cos(δ))
Variable Meaning Unit Typical Range
H Hour Angle Degrees 0 to 180°
h Solar Altitude Degrees -0.833° (for sunrise)
φ (phi) Observer Latitude Degrees -90° to 90°
δ (delta) Solar Declination Degrees -23.44° to 23.44°

Step-by-Step Derivation

  1. Calculate the Julian Day from the current date.
  2. Determine the Mean Solar Time and Solar Mean Anomaly.
  3. Calculate the Equation of the Center and Ecliptic Longitude.
  4. Find the Solar Declination based on the Earth's tilt.
  5. Solve for the Hour Angle to find the time difference from Solar Noon.

Practical Examples (Real-World Use Cases)

Example 1: Winter Solstice in London

Inputs: Latitude 51.5074° N, Longitude 0.1278° W, Date: Dec 21.
Output: The Sunrise Sunset Calculator shows sunrise at approximately 08:04 AM and sunset at 03:53 PM. This demonstrates the short Daylight Duration in northern latitudes during winter.

Example 2: Equinox in Quito, Ecuador

Inputs: Latitude 0.1807° S, Longitude 78.4678° W, Date: March 20.
Output: Sunrise and sunset occur almost exactly 12 hours apart (06:12 AM and 06:12 PM), illustrating the "equal night" phenomenon at the equator.

How to Use This Sunrise Sunset Calculator

  1. Enter Coordinates: Input your Latitude and Longitude. Use decimal format.
  2. Select Date: Choose the specific day you wish to analyze.
  3. Set Timezone: Ensure the UTC offset matches your local time to get accurate clock times.
  4. Interpret Results: The primary result shows total Daylight Duration. The intermediate values provide specific times for Solar Noon and twilight phases.
  5. Visual Aid: Use the dynamic chart to visualize the sun's path relative to your location.

Key Factors That Affect Sunrise Sunset Calculator Results

  • Atmospheric Refraction: The atmosphere bends light, making the sun visible before it actually crosses the horizon. Most calculators add 34 arcminutes to account for this.
  • Elevation: Being higher up (e.g., on a mountain) allows you to see the sun earlier and longer.
  • Earth's Elliptical Orbit: The Earth moves faster or slower depending on its distance from the sun, affecting Solar Noon.
  • Axial Tilt: The 23.5° tilt is the primary reason for seasonal changes in Daylight Duration.
  • Horizon Obstructions: Mountains or buildings can block the "theoretical" sunrise, though the Sunrise Sunset Calculator assumes a flat sea-level horizon.
  • Timezone Definitions: Political timezone boundaries often deviate from solar time, requiring the UTC offset adjustment.

Frequently Asked Questions (FAQ)

Why does the sunrise time change every day?

It changes due to the Earth's orbit around the sun and its axial tilt, which changes the angle at which sunlight hits your specific latitude.

What is the difference between Civil and Nautical Twilight?

Civil Twilight is when there is enough light to see objects clearly, while Nautical Twilight is darker, used by sailors to navigate via stars.

Is solar noon always at 12:00 PM?

No. Solar Noon varies based on your longitude within a timezone and the Equation of Time. It can vary by up to 30 minutes from clock noon.

Does elevation affect the Sunrise Sunset Calculator?

Yes, higher elevations see the sun earlier. This calculator assumes sea level; for every 1000m of height, sunrise is roughly 1-2 minutes earlier.

What is Astronomical Twilight?

Astronomical Twilight is the period when the sun is between 12 and 18 degrees below the horizon. After this, the sky is considered perfectly dark for telescopes.

Why is the day length exactly 12 hours on the Equinox?

On the equinox, the Earth's axis is not tilted toward or away from the sun, resulting in nearly equal daylight and darkness worldwide.

Can this calculator work for the North Pole?

Yes, though in summer or winter, you may see "24 hours of light" or "24 hours of darkness" results.

What is Solar Declination?

Solar Declination is the angle between the rays of the sun and the plane of the Earth's equator.

Related Tools and Internal Resources

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