assign 27 

course phy201

swHd|ﷀ]|assignment #027

w囶jֱ޳􊺄t

Physics I

05-03-2009

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22:39:41

Query intro probs set 7, 1-7

Knowing the 9.8 m/s^2 gravitational field strength of the Earth's field at the surface of the Earth, and knowing the radius of the Earth, how do we find the gravitational field strength at a given distance 'above' the surface of the Earth?

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RESPONSE -->

F = 9.8m/s/s * (rE/r)^2 at distance r from the earth

rE = 6400km

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22:39:56

** You have an inverse square force. Square the ratio of Earth radius to orbital radius and multiply by 9.8 m/s^2:

Field strength=(Re/r)^2*9.8m/s^2 **

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RESPONSE -->

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22:42:19

If we double our distance from the center of the Earth, what happens to the gravitational field strength we experience?

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RESPONSE -->

as you move further from the earths gravity the force of attraction decrease hence the gravitational field strength will decrease by 1 / change in dist^2

the change in distance will be the ratio of change in this problem 1/2^2

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22:42:31

** We have an inverse square force so if r2 = 2 * r1 the ratio of the gravitational field will be

g2 / g1 = (1 / r2^2) / (1 / r1^2) = r1^2 / r2^2 = (r1 / r2)^2 = (r1 / (2 * r1))^2 = r1^2 / 4 r1^2 = 1/4.

In a nutshell double the radius gives us 1 / 2^2 = 1/4 the gravitational field. **

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22:47:20

How do we approximate the energy required to move a given mass from the surface of the Earth to a given height 'above' the Earth, where the field strength at the given height differ significantly from that at the surface?

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RESPONSE -->

similar to previous assignments dealing with PE and KE.

The change in height will be then incorp. into the equation for the diffferent heights PE =mgy

KE =m* 9.8m/s/s * rE /r^2

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22:48:36

STUDENT SOLUTION AND INSTRUCTOR RESPONSE:

mass*[(Re + distance)/Re]^2=force

Force*distance=KE

INSTRUCTOR RESPONSE:

The first approximation would be to average the force at the surface and the force at the maximum altitude, then multiply by the distance. The result would give you the work necessary to 'raise' the object against a conservative force, which would be equal to the change in PE.

ADDENDUM FOR UNIVERSITY PHYSICS STUDENTS ONLY:The exact work is obtained by integrating the force with respect to position. You can integrate either G M m / r^2 or g * (RE / r)^2 from r = RE to rMax. **

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RESPONSE -->

im not sure i understand this answer I know I need to find KE and then the different PE from the min and max altitudes but I dont know if my equation represents the same one shown here

No KE difference is assumed. We are looking only at the work required to 'lift' the object without speeding it up.

Energy is required because, in order to 'lift' a mass, a force is required to counter the gravitational pull of the Earth. If we can find the average force required, we need only multiply by the distance. This only gives an approximation (see more about this below). The work done against gravity is done against a conservative force, and is therefore equal to the change in gravitational PE.

You can't use the book's m g y formula because in this case the acceleration of gravity changes significantly from the initial point to the final point.

The work required is equal to the area beneath the graph of F vs. r. The graph is decreasing at a decreasing rate (i.e., decreasing and concave up), and is asymptotic to the positive r axis.

See the Introductory Problem Sets for worked problems of this nature. The approach used there is to approximate the force at the two distances from the center of the Earth, average the two and use this as an approximation to the average force. This approximation is accurate only to the extent that the slope of the F vs. r graph is constant.

For a given mass m we have

F = m * (r_earth / r)^2 * 9.8 m/s^2; simce m * 9.8 m/s^2 is the weight at the surface of the earth we could write this as

F = weight_surface * (r_earth / r)^2, where weight_surface is the weight of the mass at the surface of the Earth..

Either way, this expression gives the force at distance r from the center of the Earth.

So you would plug in the initial distance from the center of the Earth, and the final distance, obtaining two values for the force. Averaging these two values you would have an approximate value for the average force, which would then be multiplied by the distance to get the approximate work.

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22:48:44

Query class notes #24

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22:51:11

Describe the paths of various particles 'shot' parallel to the surface of the Earth from the top of a very high tower, starting with a very small velocity and gradually increasing to a velocity sufficient to completely escape the gravitational field of the Earth.

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RESPONSE -->

there will be two vectors one parallel and one perpindicular. as the velocity increases as well as the distance from the earths surface the force on/by this object will decrease linearly until there is no more force the object escapes orbit

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23:00:53

GOOD STUDENT ANSWER:

Each particle sets out to follow an orbit around the center of mass of the earth. But for particles shot at slower speeds, this path is interupted by the surface of the eath and simply stops there. The faster it is shot, the further x distance becomes before the particle lands. However, if it given a great enough velocity, it will fall around the curviture of the earth. If is shot even faster than that, it will follow an eliptical oribit with varying speeds and distances from center of earth.

GOOD STUDENT ANSWER:

With a very low velocity the projectile will not travlel as far. It will fall to earth in a nearly parabolic fashion since it gains vertical velocity as it travels horizontally at a steady pace.

If the projectile is fired at a very strong velocity it will leave the earths vacinity but will still be pulled by the forces acting on it from the earths center. This will cause it to go only so far at which point it has slowed down considerabley, since it has lost most of its kinetic energy. It turns and begins to gain energy as it approaches the earths area, using the potential energy it gained on the trip out. (Causing it to speed up). The path that this projectile will take will be eliptical, and it will continue to loop around the earth.

If the projectile is fired at the correct velocity to form a circular orbit, it will also fall at a parabolic fashion, although the earth's surface will also be descending at the same rate so that the object will appear to be 'not falling'. It is falling but at the same rate the earth is 'falling' under it. It will circle the earth until something causes it to stop.

INSTRUCTOR RESPONSE:

The path of the projectile will always be an ellipse with the center of the Earth at one focus. For low velocities and low altitude this path is very nearly parabolic before being interrupted by the surface of the Earth.

One of these ellipses is a perfect circle and gives us the circular orbit we use frequently in this section. **

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RESPONSE -->

I thought this object left the earths force...if not i understand it will fall back to earth as a normal projectile because of a small velocity and have a parabolic path because gravity will take over, but if it does escape and is at the right velocity then it will begin to orbit because the parallel and perpindicular components are balanced. If the projectile has a very large velocity not big enough to escape all of earths pull then it will travel until the KE runs out then as the perpindicular and parallel components tend to take over the object is pulled back into earths grav field and orbit.

The gravitational field of the Earth extends forever, but as distance from the Earth increases the strength of the field decreases as 1 / r^2. For example at the distance of the Moon the earth's field is only about 1/3600 times as great as at the surface of the Earth. This is still plenty to hold the Moon in its orbit about the Earth. The Earth's gravitational field also affects the orbits of other planets, even though only one planet ever gets close enough to experience a field which is even one-millionth as great as the field we feel at the surface of the Earth (the other planets are affected chiefly by the gravitational field of the Sun).

The further a projectile or a satellite gets from the Earth, the less gravitational force it experiences, and if it's moving fast enough it will keep going and never come back; but all the while it will experience some force from the Earth, just not enough to ever stop it.

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U젡ʍ[ò

assignment #027

w囶jֱ޳􊺄t

Physics I

05-03-2009

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23:05:25

How many of the velocities in the preceding question would result in a perfectly circular orbit about the Earth?

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RESPONSE -->

two; one would go straight into orbit the other would loop out and as the KE ran out and motion slowed begin to curve back towards earth increasing its KE until it reached the right velocity and fall into orbit

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23:07:57

Is it necessary in order to achieve a circular orbit to start the object out in a direction parallel to the surface of the Earth?

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RESPONSE -->

yes to obtain the correct parallel and perpindicular components to hold it in orbit

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23:08:06

** If you have just one 'shot' then you must start out parallel to the surface of the Earth. The reason is that any circle about the center must be perpendicular at every point to a radial line--a line drawn from the center to the circle. Any radial line will intercept the surface of the Earth and must be perpendicular to it, and the circular orbit must also be perpendicular to this line. Therefore the orbit and the surface are perpendicular to the same line and are therefore parallel. **

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23:08:44

Principles of Physics and General College Physics Problem 5.2: A jet traveling at 525 m/s moves in an arc of radius 6.00 km. What is the acceleration of the jet?

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RESPONSE -->

a = v^2/r

a = 14.6m/s/s

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23:10:52

The jet will have centripetal acceleration a_cent = v^2 / r, where v is its speed and r the radius of the circle on which it is traveling. In this case we have v = 525 m/s and r = 6.00 km = 6000 meters.

The centripetal acceleration is therefore

a_cent = v^2 / r = (525 m/s)^2 / (6000 m) = 45 m/s^2, approx.. One 'g' is 9.8 m/s^2, so this is about (45 m/s^2) / (9.8 m/s^2) = 4.6 'g's'.

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RESPONSE -->

lets try this problem again

a = v^2/r

a = 535m/s^2 / 6000m

a = 45m/s/s

g = 45/9.8

4.6

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23:12:13

Univ. Why is it that the center of mass doesn't move?

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RESPONSE -->

because of the perpindicular component; it will always begin from the same position and in order to stay in orbit must be that distance r for a particular mass

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23:12:22

** There is no net force on the system as a whole so its center of mass can't accelerate. From the frame of reference of the system, then, the center of mass remains stationary. **

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&#This looks good. See my notes. Let me know if you have any questions. &#

assign 27 

course phy201

RyɜϑWxLxassignment #027

027. Newton's Law of Universal Gravitation

Physics II

05-03-2009

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20:44:29

`q001. Note that this assignment contains 8 questions.

Masses attract each other. The forces of attraction are equal and opposite: The force exerted by one small concentrated mass on another is equal in magnitude but in the opposite direction from the force exerted on it by the other. Greater masses exert greater attractions on one another.

If two such objects remain separated by the same distance while one object increases to 10 times its original mass while the other remains the same, there will be 10 times the original force.

If both objects increase to 10 times their original masses, there will be 100 times the original force.

The force of attraction is inversely proportional to the square of the distance between the objects. That means that if the objects move twice as far apart, the force becomes 1 / 2^2 = 1/4 as great; if they move 10 times as far apart, the force becomes 1 / 10^2 = 1/100 as great.

The same statements hold for spherical objects which have mass distributions which are symmetric about their centers, provided we regard the distance between the objects as the distance between their centers.

Suppose a planet exerts a force of 10,000 Newtons on a certain object (perhaps a satellite) when that object is 8000 kilometers from the center of the planet. How much force does the satellite exert on the planet?

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RESPONSE -->

F=10000N

r = 8000km

force must be equal and opposite so the sat. stays in motion.

force = inverse of distance^2

F = 1 / 800000^2

F = 1.6 * 10^-8

confidence assessment: 1

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20:48:28

The gravitational forces exerted by the planet and the object are equal and opposite, and are both forces of attraction, so that the object must be exerting a force of 10,000 Newtons on the planet. The object is pulled toward the planet, and the planet is pulled toward the object.

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RESPONSE -->

doesnt look like i paid much attention to the previous statements. Force of attraction was already given so I did not need to use the equation. It is a difficult concept to accept that a sat. will have the same force on the earth considering the difference in mass

self critique assessment: 1

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20:50:32

`q002. If the object and the planet are both being pulled by the same force, why is it that the object accelerates toward the planet rather than the planet accelerating toward the object?

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RESPONSE -->

F=ma

a = F/m

the sat. has a smaller mass therefore resulting in a larger acceleration. As it gets closer to earth its force on the planet is overtaken because the closer it comes to the center the stronger the gravitational force.

confidence assessment: 2

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20:50:46

Presumably the planet is much more massive than the object. Since the acceleration of any object is equal to the net force acting on it divided by its mass, the planet with its much greater mass will experience much less acceleration. The minuscule acceleration of the planet toward a small satellite will not be noticed by the inhabitants of the planet.

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RESPONSE -->

self critique assessment: 2

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20:54:20

`q003. If the mass of the object in the preceding exercise is suddenly cut in half, as say by a satellite burning fuel, while the distance remains at 8000 km, then what will be the gravitational force exerted on it by the planet?

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RESPONSE -->

The force would be less since the mass decreased?

confidence assessment: 2

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20:56:07

Halving the mass of the object, while implicitly keeping the mass of the planet and the distance of the object the same, will halve the force of mutual attraction from 10,000 Newtons to 5,000 Newtons.

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RESPONSE -->

it was reduced by half the same ration as the mass was cut. This would be the same situaiton if the planets mass was cut in half.?

self critique assessment: 2

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20:58:47

`q004. How much force would be experienced by a satellite with 6 times the mass of this object at 8000 km from the center of a planet with half the mass of the original planet?

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RESPONSE -->

F = 10000

D = 8000km

1/2 planet mass = 5000N

6 * mass = F

6 * 5000 = 30000N

confidence assessment: 1

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21:01:18

The distance is the same as in the previous examples, so increasing the mass by a factor of 6 would to result in 6 times the force, provided everything else remained the same; but halving the mass of the planet would result in halving this force so the resulting force would be only 1/2 * 6 = 3 times is great as the original, or 3 * 10,000 N = 30,000 N.

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RESPONSE -->

again i need to remember the force is equal and opposite so the planet and sat. force on each other will be the same. This answered my quesiton in the previous problem; no matter which object has the mass change

self critique assessment: 2

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21:04:31

`q005. How much force would be experienced by the original object at a distance of 40,000 km from the center of the original planet?

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RESPONSE -->

F = 10000

D = 8000km

D2 = 40000km

40000/8000 = 5

F = 10000/5

F = 2000

The greater the distance between objects the less attraction there will be; its easy to think of the relationship similar to two magnets

confidence assessment: 3

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21:07:45

The object is 40,000 km / (8000 km) = 5 times as far from the planet as originally. Since the force is proportional to the inverse of the square of the distance, the object will at this new distance experience a force of 1 / 5^2 = 1/25 times the original, or 1/25 * 10,000 N = 400 N.

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RESPONSE -->

i only considered the 1:5 ration and it made sense how i reached answer however as I see I should have used the inverse equation to find the F because there is a large difference in my answer.

1/5^2 = .04

.04 * 10000 = 400N

self critique assessment: 2

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21:13:59

`q006. The relationship between the force of attraction and the masses and separation can be expressed by a proportionality. If the masses of two small, uniformly spherical objects are m1 and m2, and if the distance between these masses is r, then the force of attraction between the two objects is given by F = G * m1 * m2 / r^2. G is a constant of proportionality equal to 6.67 * 10^-11 N m^2 / kg^2. Find the force of attraction between a 100 kg uniform lead sphere and a 200 kg uniform lead sphere separated by a center-to-center distance of .5 meter.

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RESPONSE -->

F = G *m1 *m2 / r^2

G = 6.7 * -11Nm^2/kg^2

m =100kg

m2=200kg

d=.5m

F = 6.7* 10^-11Nm^2/kg^2 * 100kg *200kg /.5^2

F = 5.36 *10^-6

confidence assessment: 2

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21:15:03

We are given the two masses m1 = 100 kg and m2 = 200 kg and the separation r = .5 meter between their centers. We can use the relationship

F = G * m1 * m2 / r^2

directly by simply substituting the masses and the separation. We find that the force is

F = 6.67 * 10^-11 N m^2 / kg^2 * 100 kg * 200 kg / (.5 m)^2 = 5.3 * 10^-6 Newton.

Note that the m^2 unit in G will be divided by the square of the m unit in the denominator, and that the kg^2 in the denominator of G will be multiplied by the kg^2 we get from multiplying the two masses, so that the m^2 and the kg^2 units disappear from our calculation.

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RESPONSE -->

F is in N because kg and m will be cancelled

self critique assessment: 2

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21:20:41

`q007. If these two objects were somehow suspended so that the net force on them was just their mutual gravitational attraction, at what rate would the first object accelerate toward the second, and if both objects were originally are rest approximately how long would it take it to move the first centimeter?

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RESPONSE -->

m=100

m2=200

d = .5m

F = 5.3*10^-6

F = ma

a = F/m

a = 5.3*10^-6 N / 100kg

a = 5.3*10^-8

ds = v0dt + .5a dt^2

t = sqrt ds/.5a

t = 614 sec

confidence assessment: 2

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21:22:06

A mass of 100 kg subject a net force of 5.3 * 10^-6 N will have acceleration of a = 5.3 * 10^-6 N / (100 kg) = 5.3 * 10^-8 m/s^2.

At this rate to move from rest (v0 = 0) thru the displacement of one centimeter (`ds = .01 m) would require time `dt such that `ds = v0 `dt + .5 a `dt^2; since v0 = 0 this relationship is just `ds = .5 a `dt^2, so

`dt = `sqrt( 2 `ds / a)

= `sqrt( 2 * .01 m / (5.3 * 10^-8 m/s^2) )

= `sqrt( 3.8 * 10^5 m / (m/s^2) ) = 6.2 * 10^2 sec, or about 10 minutes.

Of course the time would be a bit shorter than this because the object, while moving somewhat closer (and while the other object in turn moved closer to the center of gravity of the system), would experience a slightly increasing force and therefore a slightly increasing acceleration.

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RESPONSE -->

again equations of uniform accel are key to this problem.

self critique assessment: 2

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21:24:04

`q008. At what rate would the second object accelerate toward the first?

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RESPONSE -->

m2=200kg

F = 5.3*10^-6

F = ma

a = 5.3E-6N /200kg

a = 2.7 E ^ -8

confidence assessment: 3

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21:25:16

The second object, with its 200 kg mass, would also a subject to a net force of 5.3 * 10^-6 N and would therefore experience and acceleration of

a = 5.3 * 10^-6 N / (200 kg) = 2.7 * 10^-8 m/s^2.

This is half the rate at which the first object changes its velocity; this is due to the equal and opposite nature of the forces and to the fact that the second object has twice the mass of the first.

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RESPONSE -->

the acceleration will be slower than the first obj due to the larger mass which was obvious from looking at the equation F = ma.

self critique assessment: 2

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&#Good responses. See my notes and let me know if you have questions. &#