Openquery28

course PHY 121

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028. `query 28 PRELIMINARY STUDENT QUESTION: Again I am still having trouble with what equations to use...for PE change we would use the equation PE = Gmm/r1 - Gmm/r2 same as the Force equation or do we just find dPE by grav. Force * ds both are listed in my notes. As far as

KE I assume m*9.8m/s/s *rE/r^2

INSTRUCTOR RESPONSE: PE = -G M m / r^2 so going from radius r1 to radius r2 we would have `dPE = GMm/r1 - GMm/r2.

If r1 and r2 don't differ by much, then G M m / r1 and G M m / r2 won't differ by much, and it would be important to use an appropriate number of significant figures in calculating the difference.

Alternatively the difference can be expressed in terms of the common denominator r1 * r2 as G M m * ( r2 - r1) / (r2 * r1), where the common factor G M m has been factored out.

As another alternative if r1 and r2 are proportionally close, you can figure out the average force and multiply by `dr = r2 - r1, as described below:

`dPE, i.e., the change in gravitational PE, is also equal to average gravitational force * change in distance from planet center:

• `dPE = F_ave * `dr

This is valid if `dr is small compared to r1 and r2, for the following reasons and with the associated cautions:

Gravitational force is not linearly related to r (i.e., the graph of F vs. r is not a straight line), so the average force on an interval is not equal to the average of the initial and final force.

However if the proportional change in r is small enough the curvature of the graph won't be noticeable, and the average force could be approximated by the average of initial and final force. In fact it is possible that the proportional change in r is small enough that over the relevant interval there is no significant change in the force itself.

• In these cases the change in PE is more easily found using F_ave * `dr.

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Question: `qQuery class notes #26

Explain how we use proportionality along with the radius rE of the Earth to determine the gravitational acceleration at distance r from the center of the Earth to obtain an expression for the gravitational acceleration at this distance. Explain how we use this expression and the fact that centripetal forces is equal to v^2 / r to obtain the velocity of a satellite in circular orbit.

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Your solution: a = k/(rE)2.

9.8m/s^2 = k/(rE)^2

k = 9.8m/s^2*(rE^2).. Substituting it back in,

a = [9.8m/s^2 * rE^2]/r^2.

a also = v^2/r, so

[9.8m/s^2 * rE^2]/r^2 = v^2/r.

confidence rating:

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Given Solution: `a** The proportionality is accel = k / r^2. When r = rE, accel = 9.8 m/s^2 so

9.8 m/s^2 = k / rE^2.

Thus k = 9.8 m/s^2 * rE^2, and the proportionality can now be written

accel = [ 9.8 m/s^2 * (rE)^2 ] / r^2. Rearranging this gives us

accel = 9.8 m/s^2 ( rE / r ) ^2.

If we set the acceleration equal to v^2 / r, we obtain

v^2 / r = g ( rE / r)^2 so that

v^2 = g ( rE / r) and

v = sqrt( 2 g rE / r).

Thus if we know the radius of the Earth and the acceleration of gravity at the surface we can calculate orbital velocities without knowing the universal gravitational constant G or the mass of the Earth.

If we do know G and the mass of the Earty, we can proceed as follows:

The gravitational force on mass m at distance r from the center of the Earth is

F = G m M / r^2

Where M is the mass of the Earth and m the mass of the satellite. Setting this equal to the centripetal force m v^2 / r on the satellite we have

m v^2 / r = G m M / r^2, which we solve for v to get

• v = sqrt( G M / r).

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Self-critique (if necessary): I got really lost in the middle of this problem.. I had trouble understanding what the question was asking and how to translate that into an equation. I understand the equations in the given answer but am still confused over the phrasing of the question.

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Self-critique Rating:

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Question: `qPrinciples of Physics and Gen Phy problem 5.30 accel of gravity on Moon where radius is 1.74 * 10^6 m and mass 7.35 * 10^22 kg.

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Your solution: aof gravity = G(mass)/r^2 = [6.67*10^-11 (7.35 * 10^22 kg)] / (1.74 * 10^6 m)^2. = 1.6m/s^2.

confidence rating:

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Given Solution: `a** The acceleration due to gravity on the Moon is found using the equation

g' = G (Mass of Moon)/ radius of moon ^2

g' = (6.67 x 10^-11 N*m^2/kg^2)(7.35 X 10^22 kg) / (1.74 X 10^6 m) = 1.619 m/s^2 **

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Self-critique (if necessary): OK

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Question: `qQuery class notes #28. Explain how we can calculate the average angular velocity and the angular acceleration of an object which rotates from rest through a given angle in a given time interval, assuming constant angular acceleration.

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Your solution: avg. angular velocity = `d(position)/(`dt).

angular acceleration = `d(angular velocity)/`dt.

If you know the `dt , you know that the vi = 0 and if you know the given angle, you can calculate the avg. angular velocity, which you can then use to calculate the ave. acceleration.

confidence rating:

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Given Solution: **This situation is strictly analogous to the one you encountered early in the course. As before acceleration is change in velocity / change in clock time. However now it's angular acceleration.

We have

angular acceleration = change in angular velocity / change in clock time.

The average angular velocity is change in angular position / change in clock time.

This question assumes you know the angle through which the object rotates, which is its change in angular position, as well as the change in clock time.

So you can calculate the average angular velocity.

If angular accel is uniform and initial angular velocity is zero then the final angular velocity is double the average angular velocity. In this case the change in angular velocity is equal to the final angular velocity, which is double the average angular velocity.

From this information you can calculate angular acceleration. **

Principles of Physics and General College Physics Problem 7.46: Center of mass of system 1.00 kg at .50 m to left of 1.50 kg, which is in turn .25 m to left of 1.10 kg.

Using the position of the 1.00 kg mass as the x = 0 position, the other two objects are respectively at x = .50 m and x = .75 m.

The total moment of the three masses about the x = 0 position is 1.00 kg * (0 m) + 1.50 kg * (.50 m) + 1.10 kg * (.75 m) = 1.58 kg m.

The total mass is 1.00 kg + 1.50 kg + 1.10 kg = 3.60 kg, so the center of mass is at position

x_cm = 1.58 kg m / (3.60 kg) = .44 meters,

placing it a bit to the left of the 1.50 kg mass.

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Self-critique (if necessary): OK

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Question: `qQuery problem 7.50 3 cubes sides L0, 2L0 and 3L0; center of mass.

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Your solution: Cube 2 will be 2^3 = 8 times bigger than the first.

Cube 3 = 3^3 = 27 times bigger.

confidence rating:

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Given Solution: ** The mass of the second will be 2^3 = 8 times as great as the first. It takes 8 1-unit cubes to make a 2-unit cube.

The mass of the third will be 3^3 = 27 times as great as the first. It takes 27 1-unit cubes to make a 3-unit cube.

In the x direction the distance from left edge to center of first cube is 1/2 L0 (the center of the first cube).

In the y direction the distance is from lower edge to center of the first cube is 1/2 L0 (the center of the first cube).

In the x direction the distance from left edge to center of the second cube is L0 + L0 (the L0 across the first cube, another L0 to the center of the second), or 2 L0.

In the y direction the distance from lower edge to center of the second cube is L0 (the center of the second cube).

In the x direction the distance from left edge to center of the third cube is L0 + 2 L0 + 3/2 L0 (the L0 across the first cube, another 2 L0 across the second and half of 3L0 to the center of the third), or 9/2 L0.

In the x direction the distance from lower edge to center of the first cube is 3/2 L0 (the center of the third cube).

Moments about left edge and lower edge of first cube:

If m1 is the mass of the first cube then in the x direction you have total moment

m1 * L0/2 + 8 m1 * (2 L0) + 27 M1 * (9/2 L0) = 276 m1 L0 / 2 = 138 m1 L0.

The total mass is m1 + 8 m1 + 27 m1 = 36 m1 so the center of mass is at

center of mass in x direction: 138 m1 L0 / (36 m1) = 3.83 L0.

In the y direction the moment is

m1 * L0/2 + 8 m1 * (L0) + 27 m1 * ( 3/2 L0) = 45 m1 L0

so the center of mass is at

center of mass in y direction: 45 m1 L0 / (36 m1) = 1.25 L0. **

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Self-critique (if necessary):

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Question: `qWhat is the mass of the second cube as a multiple of the mass of the first?

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Your solution: 2^3 = 8 times.

confidence rating:

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Given Solution: ** 3 dimensions: the mass will be 2^3 = 8 times as great. It takes 8 1-unit cubes to make a 2-unit cube. *

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Self-critique (if necessary):

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Question: `qWhat is the mass of the third cube as a multiple of the mass of the first

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Your solution: 3^3 = 27 times bigger.

confidence rating:

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Given Solution: ** The mass of the third cube is 3^3 = 27 times the mass of the first. **

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Self-critique (if necessary):

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Question: `qHow far from the outside edge of the first cube is its center of mass?

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Your solution: 1/2 the length.

confidence rating:

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Given Solution: `a** In the x direction the distance is 1/2 L0 (the center of the first cube).

In the y direction the distance is also 1/2 L0 (the center of the first cube). **

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Self-critique (if necessary):

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Question: `qHow far from the outside edge of the first cube is the center of mass of the second cube?

Your solution: twice the length of the first, so 2L0.

confidence rating:

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Given Solution: `a** In the x direction the distance is L0 + L0 (the L0 across the first cube, another L0 to the center of the second), or 2 L0.

In the x direction the distance is L0 (the center of the second cube). **

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Self-critique (if necessary): OK

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Question: `qHow far from the outside edge of the first cube is the center of mass of the third cube?

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Your solution: 1.5L0 in the y direction. 4.5 in the L0 direciton.

confidence rating:

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Given Solution: ** In the x direction the distance is L0 + 2 L0 + 3/2 L0 (the L0 across the first cube, another 2 L0 across the second and half of 3L0 to the center of the third), or 9/2 L0.

In the x direction the distance is 3/2 L0 (the center of the third cube). **

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Self-critique (if necessary): It’s easy for me to think about it in terms of simple math but harder when I try to do the L0 + 2L0 + 3/2L0.

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Question: `qHow do you use these positions and the masses of the cubes to determine the position of the center of mass of the system?

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Your solution: The first cube, the second cube is 8 times the first, and the third is 27 times the first. So mass [(m) * L0/2] + [8m *2L0] + [27m*4.5L0] = 138mL0.

138mL0 / 36m = 1.25L0.

m*L0/2 + 8m*1.5L0 + 27*1.5L0 = 45mL0/36m = 1.25L0.

confidence rating:

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Given Solution: ** In the x direction you have moment m1 * L0/2 + 8 m1 * (2 L0) + 27 M1 * (9/2 L0) = 276 m1 L0 / 2 = 138 m1 L0. The total mass is m1 + 8 m1 + 27 m1 = 36 m1 so the center of mass is at 138 m1 L0 / (36 m1) = 3.83 L0.

In the y direction the moment is m1 * L0/2 + 8 m1 * (L0) + 27 m1 * ( 3/2 L0) = 45 m1 L0 so the center of mass is at 45 m1 L0 / (36 m1) = 1.25 L0. **

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Self-critique (if necessary): OK

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&#Good responses. Let me know if you have questions. &#