Homework for Exam #1

Assignment #1 Section 11-2 Due: Wed. Jan.9
Assignment #2 Section 11-3 Due: Fri. Jan. 11
Assignment #3 Notes on Kepler’s 1 st Law Due: Mon. Jan.14
Assignment #4 Notes on Kepler’s 2nd Law Due: Tue. Jan. 15
Assignment #5 Section 14-1 Due: Wed. Jan. 16
Assignment #6 Section 14-2 Due: Fri. Jan. 18
Assignment #7 Section 14-3 Due: Tue. Jan. 22
EXAM #1 - FRIDAY JANUARY 25 - CHAPTERS 11 & 14
Topic Summery

START for CHAPTER 11

Assignment #1 Section 11-2 Due: Wed. Jan. 9
1-1. You drop a 3.50 kg rock from a height of 1.25 m on Mars whose mass is 6.419x10 23kg and mean equatorial radius is 3393 km {on the Moon whose mass is 7.349x10 22kg and mean radius is 1738 km}.
(A) At what rate will the rock accelerate downward ?
(B) How long will the rock take to reach the ground ?

1-2. At what distance above the Earth’s surface will the acceleration of gravity drop by 10.0% {20.0%} of value at the Earth’s surface of 9.80 m/s 2. The equatorial radius of the Earth is 6378 km and its mass is 5.974x10 24kg.

1-3. The mass of the Moon is 7.349x10 22kg {Sun is 1.99x10 30kg} and its mean distance from the Earth is 3.84x10 8m {1.49x10 11m}.

{Ans: #1} {1-1.}
(A) 1.62 m/s 2
(B) 1.24 s

{1-2}.
753 km

{1-3.}
(A) 3.56x1022N
(B) 2.58x108m


Assignment #2 Section 11-3 Due: Fri. Jan. 11

2-1. An 5.90 kg object is launched straight up at 9.50 km/s {8.10 km/s} from the surface of the Earth at the Earth’s North Pole (polar radius 6356 km).

2-2. Determine the velocity that an air molecule would need to escape from the surface of the Moon {Mercury m = 7.28x10 23kg, R = 2400 km} ? Both the Moon and Mercury rotates slowly so you can neglect any rotational effects.

2-3. If an object of 3.00 kg {11.0 mg} object falls (from rest) from a great distance (infinity) into a black hole, calculate the kinetic energy of the object when it reaches the event horizon, R = 2GM/c2.
{Ans: #2} {2-1.}
(A) -176 MJ
(B) 6970 km

{2-2.}
6.36 km/s

{2-3.}
4.95x1011J


Assignment #3 Notes on Kepler’s 1 st Law Due: Mon. Jan. 14
3-1. A moon of Neptunian is in a nearly circular orbit at 73,000 miles {150,000 miles} from the planet's center. If Neptune has a mass of 1.03x10 26kg,

3-2. Mars’ closest moon Phobos ( m = 9.60x10 15kg) {fictitious moon ( m = 2.70x10 15kg)} orbits Mars once every 7.66 hours {30.3 hr}. When Phobos {the fictitious moon} is at its closest, it is 9,210 km {18,000 km} from Mars’ center. Recall that the mass of Mars is 6.419x10 23kg.

{ANS: #3} 3-1.
(A) v = 5.34 km/s
(B) T = 3.29 days

3-2.
(A) 23,500 km
(B) 1.07 km/s
(C) -2.47x1021J


Assignment #4 Notes Kepler’s 2nd Law Date Due: Tue. Jan. 15
4.
A rock is launched from the surface of the Earth (assume R = 6378 km} at a speed of 2.60 km/s {7.80 km/s} at an angle of 32.0 0 relative to local horizontal. Neglecting air resistance and any rotational motion of the Earth:

{ANS:#4} (A)
a = 6210 km
(B)
e = .530
(C)
h = 3130 km
(D)
s = 12,400 km


START for CHAPTER 14

Assignment #5 Section 14-1 Due: Wed. Jan. 16
5. Each blade of an electric shaver moves back and forth in simple harmonic motion over a distance of 3.30 mm {2.50 mm}; making 1500 {1800} complete oscillations every 15.0 seconds.
{ANS:} #5 (A)
754 rad/s
(C)
x(t) = (1.25 mm) sin[(754 rad/s) t]
(D
-47.1 cm/s to left
(E)
±1.18 mm


Assignment #6 Section 14-2 Due: Fri. Jan.18
6. A 1.80 kg {36.0 kg} block (on a frictionless, horizontal surface) is attached to a massless, horizontal spring with a spring constant of 29.0 N/cm. The block is pushed to the left so that the spring is compressed 12.0 cm and then the block is given an initial speed of 4.70 m/s {53.0 cm/s} to the right.
{ANS:} #6 (A)
25.9 J
(B)
13.4 cm
(C)
700 ms
(D)
v(t) = (1.20 m/s) cos[(8.98 rad/s) t - 1.11 rad] or
v(t) = (1.20 m/s) sin[(8.98 rad/s) t +.460 rad]
(E)
16.8 J

Assignment #7 Section 14-3 Due: Tue. Jan. 22
7. A physical pendulum is constructed from a 396 cm {2.60 m} long, thin, vertical rod that is pivoted 83.0 cm from its top. The mass of the rod is 3.90 kg. The rod is pulled to the side through an angle of 3.80 o and released at time t = 0.
{ANS:} #7 (A)
I = 3.06 kg-m 2
(B)
2.59 s
(C)
-.161 rad/s
(D)
.352 s
(E)
x = 75.1 cm from center of rod

EXAM #1 FRIDAY JANUARY 25 CHAPTERS 11 & 14

Newton’s Law of Gravity

Gravitational Potential Energy

Kepler’s Laws of Planetary Motion

Elliptical Orbits

Semimajor Axis & Eccentricity

Perihelion & Aphelion

Orbital Velocity & Position


Simple Harmonic Motion

Equations of Motion x(t), v(t), a(t)

Amplitude & Phase Angle

Period & Angular Frequency

Potential & Kinetic Energy

Hook's Law & Spring Constant

Simple & Physical Pendulum