Mr. Rogers AP Physics C Study Guide: AP Physics C Mechanics 1st Semester Exam

1st Quarter Topics >

Kinematics(1)

Vector Addition(2)

Projectile Motion(2)

Newton's Laws(3)

2nd Quarter Topics >

Newton's Laws(4)

Friction(5) Mech Energy(7) Momentum
Online Quiz - 1st Semester Exam: This quiz will is similar to your semester exam.

Additional practice: work problems in both the Barron's and Princeton review study books (see syllabus).

The information below is slanted specifically for the First Semester exam and has generally not been covered in other venues, but is also not all inclusive. Consult the study guides from previous units for the complete picture.

 

Mathematical models

     
Universal Gravity Equation   Pendulum Oscillation
F = [G(m2m1)] / r2 G = universal gravity constant

r = distance between center of mass of  m2 & m1

The attraction forces acting on the 2 masses form an action reaction pair..

  f = 1/(2p) (g / L)^0.5

T = 1 / f         

(f = frequency, T = period)

Gravity Field Strength (Acceleration due to Gravity)   Spring and Mass System Oscillation
g = [G(m2)] / r2 Plugging  in the radius and mass of Earth yields g = 9.8 m/s2
  f = 1/(2p) (k / m)^0.5

T = 1 / f

 

Gravitational Potential Energy   Angular or Rotational Motion
U = - m1[G(m2) /r]
  • For 2 masses at indeterminate distance. usually  m1 represents an object and m2 a planet.
  • Note U = 0 at infinity.
  • The right side is negative since U must decrease as the object falls toward the planet

 

 
d = rq q is the angular displacement in radians. Remember, there are 2p radians in a circle or in one revolution.
v = rw w is the angular velocity.
a = ra a is the angular acceleration
w = at + wo

q = 1/2 at2 + wot

Note that kinematics equations for angular or rotational motion are identical to those of linear motion except that the angular parameters are substituted for the linear ones.

Key Principles

Solving rotational kinematics problems is identical to solving linear kinematics problems except that the linear parameters of a, v, and d are replace with their rotational counterparts.

 

  Center of mass can be considered a balance point. For a seesaw, the center of mass is directly above the fulcrum when the seesaw is balanced.

Example Problems

Finding g for an unknown planet

If an unknown planet has 1/2 the radius and twice the mass, what is the value of g on the planet.

g unknown (2 / (1/2)2 )(g Earth)          

               =   8 (g Earth)

Explanation: The above comes directly from the universal gravity equation. Gravity force is directly proportional to mass and inversely proportional to the square of the distance between the centers of mass of the objects

  Angular or rotational motion kinematics

A fan is switched on. It has an angular acceleration of 10 rad/s2. After 10 seconds, what is the fan's angular velocity and displacement?

w = at + wo

    = (10 rad/s2)(10 s) + 0

   = 100 rad/s

q = 1/2 at2 + wot

   = 1/2 (10 rad/s2)(10 s)2 + 0

   = 500 radians

  

Elliptical Orbits

For an elliptical orbit of a mass =m around a planet, the velocity at the closest point = vc and the closest distance = Rc with the furthest distance = Rf. What is the kinetic energy at the furthest distance?

First find the velocity vf

vf = (Rc/ Rf) vc

 

K = 1/2 m v 2

    = 1/2 m [(Rc/ Rf) vc] 2

  Pendulums

A pendulum with a mass of m and length of L swings with a frequency of 3 Hz. What will the frequency be for a pendulum with a mass of 3m and a length of 1/4 L?

f = 1/(2p) (g / L)^0.5

  = 1/(2p) [g / (1/4 L)]^0.5

  = 1/(2p) [4 g / L]^0.5

  = (2) 1/(2p) [g / L]^0.5

but 1/(2p) [g / L]^0.5 = original f, therefore

f  = 2 (3 Hz)

   = 6 Hz

 

Vocabulary

Period   Angular Displacement
Frequency   Angular Velocity
Center of Mass   Angular Acceleration
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