Totally Elastic Collision Equation:
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The Totally Elastic Collision Formula calculates the final velocity of object 1 after a perfectly elastic one-dimensional collision. In elastic collisions, both momentum and kinetic energy are conserved, making this formula essential for physics and engineering applications.
The calculator uses the elastic collision equation:
Where:
Explanation: This formula is derived from the conservation of momentum and conservation of kinetic energy principles in one-dimensional elastic collisions.
Details: Understanding elastic collisions is crucial for analyzing particle interactions, designing safety systems, studying molecular dynamics, and solving physics problems involving conservation laws.
Tips: Enter all masses in kilograms and velocities in meters per second. Masses must be positive values greater than zero. The calculator provides the final velocity of object 1 after collision.
Q1: What defines a perfectly elastic collision?
A: A perfectly elastic collision is one where both momentum and kinetic energy are conserved, with no energy lost to heat, sound, or deformation.
Q2: How do I calculate the final velocity of object 2?
A: The formula for object 2 is: \( v_{2f} = \frac{2 m_1}{m_1 + m_2} v_1 + \frac{m_2 - m_1}{m_1 + m_2} v_2 \)
Q3: What are real-world examples of elastic collisions?
A: Billiard ball collisions, atomic and molecular collisions, and some types of particle collisions in particle accelerators.
Q4: What if the masses are equal?
A: If \( m_1 = m_2 \), then \( v_{1f} = v_2 \) and \( v_{2f} = v_1 \) - the objects simply exchange velocities.
Q5: Are there limitations to this formula?
A: This formula applies only to one-dimensional collisions and assumes perfect elasticity. Real-world collisions often involve some energy loss and may be multi-dimensional.