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Sunset Time Calculator

Sunset Equation:

\[ Sunset = 12 + \frac{1}{15} \times \arccos(-\tan(lat) \times \tan(decl)) \]

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1. What is the Sunset Time Equation?

The sunset time equation calculates the approximate time of sunset based on geographic latitude and solar declination. It provides an astronomical method to determine when the sun disappears below the horizon at a specific location and date.

2. How Does the Calculator Work?

The calculator uses the sunset equation:

\[ Sunset = 12 + \frac{1}{15} \times \arccos(-\tan(lat) \times \tan(decl)) \]

Where:

Explanation: The equation calculates the hour angle when the sun reaches the horizon, then converts this angle to time relative to solar noon.

3. Importance of Sunset Time Calculation

Details: Accurate sunset time calculation is essential for astronomy, navigation, agriculture, photography, and various outdoor activities. It helps in planning daily schedules and understanding seasonal daylight variations.

4. Using the Calculator

Tips: Enter latitude between -90° and 90° (negative for southern hemisphere), and declination between -23.5° and 23.5° (varies by date). The result shows sunset time in hours from midnight.

5. Frequently Asked Questions (FAQ)

Q1: What is solar declination?
A: Solar declination is the angle between the rays of the sun and the plane of the Earth's equator. It varies throughout the year due to Earth's axial tilt.

Q2: Why does the equation use 12 as a reference?
A: 12 represents solar noon, when the sun is at its highest point in the sky. Sunset time is calculated relative to this reference point.

Q3: How accurate is this calculation?
A: This provides a theoretical sunset time. Actual sunset may vary due to atmospheric refraction, elevation, and local topography.

Q4: What happens at extreme latitudes?
A: Near the poles, there may be periods of midnight sun (no sunset) or polar night (no sunrise), which this equation accounts for mathematically.

Q5: How do I find the declination for a specific date?
A: Solar declination can be calculated using specialized astronomical formulas or obtained from astronomical almanacs for specific dates.

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