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Potential Energy To Kinetic Energy Calculator

Energy Conversion Formula:

\[ \frac{1}{2} m v^2 = m g h \]

kg
m/s
m/s²
m

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1. What is Energy Conversion?

The principle of energy conservation states that energy cannot be created or destroyed, only converted from one form to another. This calculator demonstrates the conversion between potential energy (stored energy due to position) and kinetic energy (energy of motion).

2. How Does the Calculator Work?

The calculator uses the energy conversion formula:

\[ \frac{1}{2} m v^2 = m g h \]

Where:

Explanation: The left side represents kinetic energy, while the right side represents gravitational potential energy. This equation shows how potential energy converts to kinetic energy as an object falls.

3. Importance of Energy Conservation

Details: Understanding energy conversion is fundamental in physics and engineering. It explains phenomena from simple falling objects to complex mechanical systems and is a cornerstone principle in the study of mechanics.

4. Using the Calculator

Tips: Enter mass in kilograms, velocity in meters per second, gravity in m/s² (default is Earth's gravity 9.8 m/s²), and height in meters. All values must be positive numbers.

5. Frequently Asked Questions (FAQ)

Q1: What is the standard value for gravity on Earth?
A: The standard value is approximately 9.8 m/s², though it varies slightly depending on location and altitude.

Q2: Can this calculator be used for other planets?
A: Yes, simply adjust the gravity value to match the gravitational acceleration of the celestial body you're calculating for.

Q3: What units should I use for accurate results?
A: For consistent results, use kilograms for mass, meters per second for velocity, m/s² for gravity, and meters for height.

Q4: Does this equation account for air resistance?
A: No, this is an ideal equation that assumes no energy loss due to air resistance or other non-conservative forces.

Q5: What if I want to calculate the velocity from height?
A: You can rearrange the equation to solve for velocity: \( v = \sqrt{2gh} \)

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