Chapter 5: Circular Motion; Gravitation

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Chapter 5: Circular Motion; Gravitation

Sect. 5-1: Uniform Circular Motion Motion of a mass in a circle at constant speed. Constant speed  The Magnitude (size) of the velocity vector v is constant. BUT the DIRECTION of v changes continually! v = |v| = constant r r v  r

The motion of a mass in a circle at Constant Speed. Is there an acceleration? To answer this, think about Newton’s 1st Law & Newton’s 2nd Law! v = |v| = constant r r

 An object moving in a circle undergoes acceleration!! A mass moving in circle at Constant Speed. Acceleration  Rate of change of velocity a = (Δv/Δt) Constant speed  Magnitude (size) of velocity vector v is constant. v = |v| = constant BUT the DIRECTION of v changes continually!  An object moving in a circle undergoes acceleration!!

Centripetal (Radial) Acceleration Look at the velocity change Δv in the limit that the time interval Δt becomes infinitesimally small & get: Similar triangles  (Δv/v) ≈ (Δℓ/r) As Δt  0, Δθ  0, A B As Δt  0, Δv   v & Δv is in the radial direction  a  aR is radial!

(Δv/v) = (Δℓ/r)  Δv = (v/r)Δℓ Direction: Radially inward! Note that the acceleration (radial) is aR = (Δv/Δt) = (v/r)(Δℓ/Δt) As Δt  0, (Δℓ/Δt)  v Magnitude: Direction: Radially inward! Centripetal  “Toward the center” Centripetal acceleration: Acceleration toward the center.

 aR  v always!! Radially inward always! Typical figure for particle moving in uniform circular motion, radius r (speed v = constant): v : Tangent to the circle always! a = aR: Centripetal acceleration. Radially inward always!  aR  v always!!

Period & Frequency  T = (1/f) A particle moving in uniform circular motion of radius r (speed v = constant) Description in terms of period T & frequency f: Period T  time for one revolution (time to go around once), usually in seconds. Frequency f  the number of revolutions per second.  T = (1/f)

Particle moving in uniform circular motion, radius r (speed v = constant) Circumference = distance around= 2πr  Speed: v = (2πr/T) = 2πrf  Centripetal acceleration: aR = (v2/r) = (4π2r/T2)

Example 5-1: Acceleration of a revolving ball A 150-g ball at the end of a string is revolving uniformly in a horizontal circle of radius 0.600 m. The ball makes 2.00 revolutions per second. Calculate its centripetal acceleration. Figure 5-10. Caption: A small object moving in a circle, showing how the velocity changes. At each point, the instantaneous velocity is in a direction tangent to the circular path. Answer: a = v2/r; we can find v from the radius and frequency. v = 7.54 m/s, so a = 94.7 m/s2. r r

Example 5-2: Moon’s Centripetal Acceleration The Moon’s nearly circular orbit about the Earth has a radius of about 384,000 km and a period T of 27.3 days. Calculate the acceleration of the Moon toward the Earth. Answer: Again, find v from r and the period; first convert r and T into meters and seconds, respectively. Then a = 2.72 x 10-3 m/s2 = 2.78 x 10-4 g.