Sidereal Time Formula:
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Sidereal time is a timekeeping system that astronomers use to locate celestial objects. It is based on Earth's rotation relative to distant stars rather than the Sun.
The calculator uses the sidereal time formula:
Where:
Explanation: The formula converts longitude to time (15° = 1 hour) and adds it to GST to get local sidereal time.
Details: Sidereal time is essential for telescope pointing, astronomical observations, and satellite tracking. It helps determine which celestial objects are visible at a given time and location.
Tips: Enter GST in hours and longitude in degrees (positive for east, negative for west). The result will be in hours (0-24).
Q1: What's the difference between sidereal and solar time?
A: A sidereal day is about 4 minutes shorter than a solar day because Earth moves in its orbit around the Sun.
Q2: How do I get Greenwich Sidereal Time?
A: GST can be calculated from the date and time using astronomical algorithms or obtained from astronomical almanacs.
Q3: Why divide longitude by 15?
A: Earth rotates 15 degrees per hour, so dividing longitude by 15 converts degrees to hours.
Q4: What if my LST result is negative or >24?
A: The calculator automatically normalizes the result to the 0-24 hour range.
Q5: How precise is this calculation?
A: For most amateur astronomy purposes, this calculation is sufficiently precise.