This is an old revision of the document!
Example: Calculating the gravitational force exerted by the Earth on the Moon.
Two students are running to make it to class. They turn a corner and collide; coming to a complete stop. What force did they exert on each other.
Facts
Average mass of a person 68kg.
Students come to complete stop.
Choose student 1 as our system.
Lacking
Collision time Δt
Force of collision on student 1 in x-direction.
Approximations & Assumptions
Approximate speed of person 5m/s^-1 (half speed of olympic sprinter)
On average student 1's body compresses a couple of cm on average - assume compression of 2.5cm.
Representations
Δ→psys=→FextΔt
→psys,f=→psys,i+→FextΔt
→vavg=→vf+→vi2=Δ→rΔt
Solution
pfx=pix+Fx,collΔt
0=MVix+Fx,collΔt
Fx,coll=−MVixΔt
negative means −ˆx direction
Need to find collision time Δt
→vavg=→vf+→vi2=Δ→rΔt
In 1D: →vavg=ΔxΔt=→vf+→vi2
Δt=ΔxVavg=Δx→vf+→vi2
0.0255m/s+0m/s2=0.01s
Fx,coll=−MVixΔt=−(68kg)(5m/s)0.01s
=−34,000N