Escape Velocity Formula:
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Escape velocity is the minimum speed needed for an object to break free from the gravitational attraction of a massive body without further propulsion. It depends on the mass of the body and the distance from its center.
The calculator uses the escape velocity formula:
Where:
Explanation: The equation shows that escape velocity increases with the mass of the body and decreases with distance from its center.
Details: Escape velocity is crucial in space missions, satellite launches, and understanding celestial mechanics. It determines whether rockets can leave Earth's gravity or if atmospheres can retain gases.
Tips: Enter the gravitational constant (default is 6.67430 × 10-11 m³/kg·s²), mass of the celestial body in kg, and distance from center in meters. All values must be positive.
Q1: What's Earth's escape velocity?
A: Approximately 11.186 km/s at Earth's surface (M = 5.972 × 1024 kg, r = 6.371 × 106 m).
Q2: Does escape velocity depend on the object's mass?
A: No, escape velocity is independent of the escaping object's mass.
Q3: How does altitude affect escape velocity?
A: Escape velocity decreases with increasing altitude since r increases in the denominator.
Q4: What's the escape velocity at a black hole's event horizon?
A: At the event horizon, escape velocity equals the speed of light, which is why light cannot escape.
Q5: Can escape velocity be achieved without rockets?
A: In theory yes (e.g., electromagnetic launch systems), but currently rockets are the only practical method.