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Calculating Tension In A String In Circular Motion

Tension Formula:

\[ T = \frac{m \cdot v^2}{r} + m \cdot g \cdot \cos(\theta) \]

kilograms
m/s
meters
degrees
m/s²

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1. What Is Tension In Circular Motion?

Tension in circular motion refers to the force exerted by a string, rope, or rod on an object moving in a circular path. It provides the necessary centripetal force to keep the object in circular motion while also counteracting gravitational forces.

2. How Does The Calculator Work?

The calculator uses the tension formula:

\[ T = \frac{m \cdot v^2}{r} + m \cdot g \cdot \cos(\theta) \]

Where:

Explanation: The formula accounts for both the centripetal force required for circular motion and the gravitational component based on the object's position.

3. Importance Of Tension Calculation

Details: Calculating tension is crucial for understanding the forces involved in circular motion systems, designing safe mechanical systems, and solving physics problems involving rotational dynamics.

4. Using The Calculator

Tips: Enter mass in kilograms, velocity in m/s, radius in meters, angle in degrees, and gravity in m/s². All values must be positive (mass, radius, gravity > 0; velocity, angle ≥ 0).

5. Frequently Asked Questions (FAQ)

Q1: What happens when θ = 0°?
A: When the object is at the bottom of the circular path (θ = 0°), cos(0°) = 1, and tension is at its maximum: T = (mv²/r) + mg

Q2: What happens when θ = 90°?
A: When the object is at the horizontal position (θ = 90°), cos(90°) = 0, and tension equals the centripetal force: T = mv²/r

Q3: Can tension be negative?
A: No, tension is always a positive value as it represents the magnitude of force in the string. If calculations show negative tension, check your input values.

Q4: What units should I use?
A: Use kilograms for mass, meters per second for velocity, meters for radius, degrees for angle, and m/s² for gravity for consistent results.

Q5: Does this work for vertical circular motion?
A: Yes, this formula specifically applies to objects in vertical circular motion where both centripetal force and gravitational components affect the tension.

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