Orbital Angular Momentum Formula:
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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.
The formula for orbital angular momentum is:
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.
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.
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).
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.