Why does constant-speed circular motion involve acceleration?
Yes. Its velocity changes direction continuously, so its acceleration points inward even though its speed remains constant.
Study 5 - Circular Motion and Gravitation with 12 free online flashcards. Review key terms, definitions, and concepts with this interactive flashcard deck.
Why does constant-speed circular motion involve acceleration?
Yes. Its velocity changes direction continuously, so its acceleration points inward even though its speed remains constant.
What is the direction of tangential velocity?
The instantaneous velocity is tangent to the circular path and perpendicular to the radius from the center to the object.
Is centripetal force a separate physical interaction?
No. Centripetal force is the net inward radial force, which may be supplied by tension, friction, gravity, the normal force, or combinations of these.
What is the period of circular motion?
The period, T, is the time required for one complete revolution.
What equations relate angular speed, frequency, and period?
Angular speed is related to frequency by ω=2πf, or to period by ω=T2π.
How are circular-path speed, radius, period, and frequency related?
For uniform circular motion, the speed is v=T2πr=2πrf.
What accelerations occur in nonuniform circular motion?
It has both radial and tangential acceleration: a=ac+at. The tangential component changes speed, while the radial component changes direction.
What is the maximum speed on a level curve?
The maximum speed is vmax=μsgr. It does not depend on the car’s mass.
What determines the ideal banking angle?
For an ideal banked curve without friction, tanθ=rgv2, so θ=tan−1(rgv2).
Which part of tension turns a conical pendulum?
In a conical pendulum, Tcosθ=mg vertically and Tsinθ supplies the inward radial force.
How do radial equations differ at the top and bottom of a loop?
At the top, both forces can point inward, so N+mg=mrv2. At the bottom, gravity points outward, so N−mg=mrv2.
What is Newton’s law of universal gravitation?
Newton’s law of universal gravitation is Fg=Gr2m1m2. The force is attractive and acts along the line between the centers of mass.