Solar Time Formula:
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Solar time is a calculation of the passage of time based on the position of the Sun in the sky. It differs from standard time which is based on time zones and may incorporate daylight saving adjustments.
The calculator uses the solar time equation:
Where:
Explanation: The equation accounts for the fact that the Sun appears to move across the sky at a rate of 15 degrees per hour, or 4 minutes per degree of longitude.
Details: Solar time is important for astronomy, navigation, and solar energy applications. It provides the true position of the Sun relative to an observer's location, which differs from standard clock time.
Tips: Enter your local time in 24-hour format, your current longitude, and the standard longitude for your time zone. All values must be valid numerical inputs.
Q1: Why is there a 4-minute difference per degree of longitude?
A: The Earth rotates 360 degrees in 24 hours, which equals 15 degrees per hour or 4 minutes per degree.
Q2: How do I find my standard longitude?
A: Standard longitudes are typically multiples of 15 degrees (0°, 15°, 30°, etc.) corresponding to time zones. For example, UTC is based on 0° longitude.
Q3: Does this calculation account for daylight saving time?
A: No, you should use standard time (not daylight saving time) as your local time input for accurate solar time calculation.
Q4: What's the difference between solar time and sidereal time?
A: Solar time is based on the position of the Sun, while sidereal time is based on the position of distant stars relative to Earth.
Q5: How accurate is this calculation?
A: This provides a good approximation, but for precise calculations, additional factors like the equation of time should be considered.