Centripetal Force Formula:
From: | To: |
Definition: Centripetal force is the force that keeps an object moving in a circular path, directed towards the center of rotation.
Purpose: This calculator helps determine the force required to maintain circular motion based on mass, velocity, and radius.
The calculator uses the formula:
Where:
Derivation: Starting from Newton's second law \( F = ma \) and the centripetal acceleration \( a = \frac{v^2}{r} \), we substitute to get \( F_c = m \frac{v^2}{r} \).
Details: Understanding centripetal force is crucial in designing circular motion systems like roller coasters, planetary orbits, and centrifuges.
Tips: Enter the mass in kg, velocity in m/s, and radius in m. All values must be > 0.
Q1: What's the difference between centripetal and centrifugal force?
A: Centripetal force is the real force directed towards the center, while centrifugal force is a fictitious force that appears to act outward in a rotating frame of reference.
Q2: What are some real-world examples?
A: Car turning on a curve (friction provides centripetal force), Earth's orbit around the Sun (gravity provides centripetal force), spinning a ball on a string.
Q3: How does radius affect the force?
A: Force is inversely proportional to radius - smaller circles require more force for the same speed.
Q4: What happens if centripetal force disappears?
A: The object will move in a straight line (Newton's first law) tangent to its previous circular path.
Q5: How is this related to angular velocity?
A: The formula can also be written as \( F_c = m \omega^2 r \) where \( \omega \) is angular velocity in radians/second.