AP Physics

Unit 4 - Energy

Intermediate

Conceptual

MCQ

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Step Derivation/Formula Reasoning
1 y = v_0y t – \frac{1}{2} g t^2 for both balls These are the equations of motion in the vertical direction (y) for the two balls, assuming upward motion is positive. The first term in both equations represents the initial vertical velocity component times time (t), and the second term is due to the acceleration due to gravity (g) acting downward.
2 v_0y up = v_0, v_0y angle = v_0 \cos(45^\circ) = \frac{v_0}{\sqrt{2}} The initial vertical velocities. For the straight up throw, the entire velocity is vertical, hence v_0y up = v_0. For the angled throw, the vertical component is v_0 \cos(45^\circ) since the projection is at 45°.
3 Total time in air for each ball can be calculated using the equation: t_\text{total} = \frac{2v_{0y}}{g} The time of flight until each ball returns to the original level of projection can be determined from the formula, substituting in each ball’s initial vertical speed. This accounts for the time to ascend to the peak and to descend back to the ground level.
4 t_\text{straight up} = \frac{2v_0}{g}, t_\text{at angle} = \frac{2(v_0/\sqrt{2})}{g} = \frac{\sqrt{2}v_0}{g} Conclusion: t_\text{straight up} > t_\text{at angle}. The time taken for each is different due to differences in their initial vertical velocities.
5 PE + KE_i = KE_f

mgh + \frac{1}{2}mv^2 = KE_f

Height and total speeds are the same in both cases regardless of direction.

Since mechanical energy is conserved (ignoring air resistance), the final kinetic energy will be equal to kinetic + potential energy of the ball as it was thrown. Since both balls start with the same energy (same height and speed), the final kinetic energies of both balls must be the same. This would imply identical, final speeds.
6 Answer: (b) Both with the same speed, based on  the conservation of mechanical energy, (b) as the correct statement.

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KinematicsForces
\Delta x = v_i t + \frac{1}{2} at^2F = ma
v = v_i + atF_g = \frac{G m_1m_2}{r^2}
a = \frac{\Delta v}{\Delta t}f = \mu N
R = \frac{v_i^2 \sin(2\theta)}{g} 
Circular MotionEnergy
F_c = \frac{mv^2}{r}KE = \frac{1}{2} mv^2
a_c = \frac{v^2}{r}PE = mgh
 KE_i + PE_i = KE_f + PE_f
MomentumTorque and Rotations
p = m v\tau = r \cdot F \cdot \sin(\theta)
J = \Delta pI = \sum mr^2
p_i = p_fL = I \cdot \omega
Simple Harmonic Motion
F = -k x
T = 2\pi \sqrt{\frac{l}{g}}
T = 2\pi \sqrt{\frac{m}{k}}
ConstantDescription
gAcceleration due to gravity, typically 9.8 , \text{m/s}^2 on Earth’s surface
GUniversal Gravitational Constant, 6.674 \times 10^{-11} , \text{N} \cdot \text{m}^2/\text{kg}^2
\mu_k and \mu_sCoefficients of kinetic (\mu_k) and static (\mu_s) friction, dimensionless. Static friction (\mu_s) is usually greater than kinetic friction (\mu_k) as it resists the start of motion.
kSpring constant, in \text{N/m}
M_E = 5.972 \times 10^{24} , \text{kg} Mass of the Earth
M_M = 7.348 \times 10^{22} , \text{kg} Mass of the Moon
M_M = 1.989 \times 10^{30} , \text{kg} Mass of the Sun
VariableSI Unit
s (Displacement)\text{meters (m)}
v (Velocity)\text{meters per second (m/s)}
a (Acceleration)\text{meters per second squared (m/s}^2\text{)}
t (Time)\text{seconds (s)}
m (Mass)\text{kilograms (kg)}
VariableDerived SI Unit
F (Force)\text{newtons (N)}
E, PE, KE (Energy, Potential Energy, Kinetic Energy)\text{joules (J)}
P (Power)\text{watts (W)}
p (Momentum)\text{kilogram meters per second (kgm/s)}
\omega (Angular Velocity)\text{radians per second (rad/s)}
\tau (Torque)\text{newton meters (Nm)}
I (Moment of Inertia)\text{kilogram meter squared (kgm}^2\text{)}
f (Frequency)\text{hertz (Hz)}

General Metric Conversion Chart

Example of using unit analysis: Convert 5 kilometers to millimeters. 

  1. Start with the given measurement: \text{5 km}

  2. Use the conversion factors for kilometers to meters and meters to millimeters: \text{5 km} \times \frac{10^3 \, \text{m}}{1 \, \text{km}} \times \frac{10^3 \, \text{mm}}{1 \, \text{m}}

  3. Perform the multiplication: \text{5 km} \times \frac{10^3 \, \text{m}}{1 \, \text{km}} \times \frac{10^3 \, \text{mm}}{1 \, \text{m}} = 5 \times 10^3 \times 10^3 \, \text{mm}

  4. Simplify to get the final answer: \boxed{5 \times 10^6 \, \text{mm}}

Prefix

Symbol

Power of Ten

Equivalent

Pico-

p

10^{-12}

Nano-

n

10^{-9}

Micro-

µ

10^{-6}

Milli-

m

10^{-3}

Centi-

c

10^{-2}

Deci-

d

10^{-1}

(Base unit)

10^{0}

Deca- or Deka-

da

10^{1}

Hecto-

h

10^{2}

Kilo-

k

10^{3}

Mega-

M

10^{6}

Giga-

G

10^{9}

Tera-

T

10^{12}

  1. Some answers may be slightly off by 1% depending on rounding, etc.
  2. Answers will use different values of gravity. Some answers use 9.81 m/s2, and other 10 m/s2 for calculations.
  3. Variables are sometimes written differently from class to class. For example, sometime initial velocity v_i is written as u ; sometimes \Delta x is written as s .
  4. Bookmark questions that you can’t solve so you can come back to them later. 
  5. Always get help if you can’t figure out a problem. The sooner you can get it cleared up the better chances of you not getting it wrong on a test!

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