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What Is The Formula To Calculate Orbital Angular Momentum

Orbital Angular Momentum Formula:

\[ L = m v r \sin(\theta) \]

kg
m/s
m
degrees

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1. What Is Orbital Angular Momentum?

Orbital angular momentum is a measure of the rotational motion of an object around a point or axis. It describes the quantity of rotation an object possesses due to its motion along an orbital path.

2. How Does The Formula Work?

The formula for orbital angular momentum is:

\[ L = m v r \sin(\theta) \]

Where:

Explanation: The formula calculates the rotational momentum of an object moving in an orbital path, taking into account the perpendicular component of the velocity relative to the radius vector.

3. Importance Of Orbital Angular Momentum

Details: Orbital angular momentum is crucial in understanding celestial mechanics, atomic physics, and rotational dynamics. It's a conserved quantity in closed systems and plays a key role in orbital mechanics and quantum mechanics.

4. Using The Calculator

Tips: Enter mass in kilograms, velocity in meters per second, radius in meters, and angle in degrees. All values must be positive (mass > 0, velocity > 0, radius > 0, angle between 0-180 degrees).

5. Frequently Asked Questions (FAQ)

Q1: What's the difference between orbital and spin angular momentum?
A: Orbital angular momentum relates to motion around an external point, while spin angular momentum is intrinsic to the object itself.

Q2: When is the angular momentum maximum?
A: Angular momentum is maximum when the angle θ is 90 degrees, as sin(90°) = 1.

Q3: What happens when θ = 0° or 180°?
A: When the velocity is parallel or anti-parallel to the radius vector, sin(θ) = 0, so angular momentum is zero.

Q4: Is orbital angular momentum conserved?
A: Yes, in the absence of external torques, orbital angular momentum is conserved in a closed system.

Q5: How is this used in astronomy?
A: It's used to calculate planetary orbits, satellite motion, and understand the dynamics of celestial bodies.

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