Gravitational Potential Energy Equation:
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Gravitational potential energy (U) is the energy an object possesses due to its position in a gravitational field. It represents the work done against gravity to bring masses from infinity to their current positions.
The calculator uses the gravitational potential energy equation:
Where:
Explanation: The negative sign indicates that the force is attractive. The potential energy increases (becomes less negative) as the distance between objects increases.
Details: This concept is fundamental in astrophysics, orbital mechanics, and understanding celestial motion. It helps calculate escape velocities, orbital energies, and is essential for space mission planning.
Tips: Enter masses in kilograms and distance in meters. All values must be positive, with distance greater than zero. For astronomical calculations, use scientific notation (e.g., 5.972e24 for Earth's mass).
Q1: Why is gravitational potential energy negative?
A: The negative sign indicates that work must be done against gravity to separate the objects. Zero potential energy is defined at infinite separation.
Q2: How does this relate to gravitational force?
A: The gravitational force is the negative derivative of potential energy with respect to distance (\( F = -\frac{dU}{dr} \)).
Q3: Can this be used for objects near Earth's surface?
A: For small height changes near Earth, we typically use the simplified \( U = mgh \), where g is gravitational acceleration (9.81 m/s²).
Q4: What are typical values for celestial bodies?
A: For Earth-Sun system: ~-5.3 × 10³³ J. For a 1kg object at Earth's surface: ~-6.25 × 10⁷ J.
Q5: How is this different from gravitational potential?
A: Gravitational potential is potential energy per unit mass (\( \Phi = \frac{U}{m} \)), measured in J/kg.