Gravitational Potential Energy Formula:
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Gravitational potential energy is the energy an object possesses due to its position in a gravitational field. The formula PE = -G M m / r calculates the potential energy between two masses separated by a distance r, where G is the gravitational constant.
The calculator uses the gravitational potential energy formula:
Where:
Explanation: The negative sign indicates that the potential energy is zero at infinite separation and decreases (becomes more negative) as objects get closer.
Details: Calculating gravitational potential energy is essential in astrophysics, orbital mechanics, and understanding gravitational interactions between celestial bodies. It helps predict orbital paths, escape velocities, and energy conservation in gravitational systems.
Tips: Enter the gravitational constant (typically 6.67430e-11), masses of both objects in kilograms, and the distance between them in meters. All values must be positive numbers.
Q1: Why is the potential energy negative?
A: The negative sign indicates that work must be done against gravity to separate the objects. The zero point is set at infinite separation.
Q2: Can this formula be used for objects on Earth's surface?
A: For objects near Earth's surface, the simplified formula PE = mgh is typically used. This formula is more appropriate for astronomical distances.
Q3: What is the significance of the gravitational constant?
A: The gravitational constant (G) is a fundamental physical constant that determines the strength of the gravitational force between objects.
Q4: How accurate is this calculation?
A: This calculation assumes point masses or spherical symmetry. For irregularly shaped objects, the calculation becomes more complex.
Q5: What are typical values for astronomical calculations?
A: For planetary systems, masses are typically in units of 10²⁴ kg for planets and 10³⁰ kg for stars, with distances measured in millions of kilometers.