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guapka [62]
3 years ago
12

A sled and rider, gliding over horizontal, frictionless ice at 4.3 m/s , have a combined mass of 74 kg . the sled then slides ov

er a rough spot in the ice, slowing down to 2.9 m/s . part a what impulse was delivered to the sled by the friction force from the rough spot?
Physics
1 answer:
mezya [45]3 years ago
4 0
The impulse of a force is defined as
I=F \Delta t
where F is the intensity of the force and \Delta t the time of application of this force.

We can rewrite the previous relationship by using Newton's second law:
F= ma
substituting, the equation for the impulse becomes
I = m a \Delta t

But the acceleration is the variation of the velocity in the time interval:
a= \frac{\Delta v}{\Delta t}
so we can rewrite I as
I = m  \frac{\Delta v}{\Delta t} \Delta t = m \Delta v

the combined mass of sled and rider is m=74 kg, while the variation of velocity is 
\Delta v = 2.9 m/s - 4.3 m/s = -1.4 m/s
and so we can calculate the impulse of the friction force:
I= (74 kg)(-1.4 m/s)=-103.6 kg m/s
where the negative sign means the friction force acts against the motion, to decelerate the system.
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Answer: u_{1}=-0.075m/s and  u_{2}=0.500m/s

Explanation:

An elastic collision is one in which both the total kinetic energy of the system and the linear momentum are conserved. That is, during the collision there is no sound, heat or permanent deformations in the bodies as a result of the impact.

Now, in the case of the satellites described here, we have:

m_{1}v_{1}+m_{2}v_{2}=m_{1}u_{1}+m_{2}u_{2}   (1)  Conservation of momentum

\frac{1}{2}m_{1}v_{1}^{2} +\frac{1}{2}m_{2}v_{2}^{2} =\frac{1}{2}m_{1}u_{1}^{2} +\frac{1}{2}m_{2}u_{2}^{2}   (2)  Conservation of kinetic energy

Where:

m_{1}=2.5(10)^{3}kg is the mass of the first satellite

m_{2}=7.5(10)^{3}kg is the mass of the second satellite

v_{1}=0.150m/s is the initial velocity of the first satellite

v_{2}=0m/s is the initial velocity of the second satellite (we are told it is at rest)

u_{1} is the final relative velocity of the first satellite

u_{2} is the final relative velocity of the second satellite

Now, as we know the second satellite is at rest before the collision, equations (1) and (2) change to:

m_{1}v_{1}=m_{1}u_{1}+m_{2}u_{2}   (3)

\frac{1}{2}m_{1}v_{1}^{2}=\frac{1}{2}m_{1}u_{1}^{2} +\frac{1}{2}m_{2}u_{2}^{2}   (4)

Solving this system of equations we have the equations for u_{1}  and u_{2}:

u_{1}=\frac{v_{1}(m_{1}-m_{2})}{m_{1}+m_{2}}   (5)

u_{2}=\frac{2m_{1}v_{1}}{m_{1}+m_{2}}   (6)

Substituting the known values on both equations:

u_{1}=\frac{0.150m/s(2.5(10)^{3}kg-7.5(10)^{3}kg)}{2.5(10)^{3}kg+7.5(10)^{3}kg}   (7)

u_{1}=-0.075m/s   (8)   This is the final relative velocity of the first satellite

u_{2}=\frac{2(2.5(10)^{3}kg)(0.150m/s)}{2.5(10)^{3}kg+7.5(10)^{3}kg}   (9)

u_{2}=0.500m/s   (10)  his is the final relative velocity of the second satellite

7 0
4 years ago
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