An object moves in a circular orbit starting from rest. the orbit has a radius of 10 m. it takes 10 revolutions to reach its final speed of 10 m/s. a) how far did it travel from rest to its final speed (in meters)?
b) if it accelerated at a constant rate, what was its tangential accelerate during that time?
c) once it reaches its final speed, what is its centripetal acceleration?

This punnett square shows the cross between two pants. one parent has round seeds (rr). and the other parent has wrinkled seeds (rr) which best describes their offspring as shown in this cross?

While the change in blank will remain the same during a collision, the force needed to bring an object to a stop can be blank if the time if collision is blank

Visualize the problem and identify special cases first examine the problem by drawing a picture and visualizing the motion. apply newton's 2nd law, ∑f⃗ =ma⃗ , to each body in your mind. don't worry about which quantities are given. think about the forces on each body: how are these consistent with the direction of the acceleration for that body? can you think of any special cases that you can solve quickly now and use to test your understanding later? one special case in this problem is if m2=0, in which case block 1 would simply fall freely under the acceleration of gravity: a⃗ 1=−gj^.