Tidal forces will eventually slow the Earth's rotation and move the Moon farther from the Earth, thus keeping the Moon orbiting above one point on the Earth all the time. What is another example of a planetary-body system like this: A moon appears stationary in the sky as seen from one half of the main body, while the moon in question cannot be seen from the other half of the main body

work: w = fd (given)

work done by chet   =50*1 = 50 j

work done by mika =40*2 = 80 j

work done by sara =30*1.5 = 45 j

work done by bill =60*0.5 = 30 j

students in order from the greatest amount of work done to the least is mika> chet> sara> bill

hence option (b) is correct.

  distance on the y-axis and time on the x-axis.

explanation:

the instantaneous velocity = change in position/time taken

the slope of the graph should give instantaneous velocity.

  slope of a graph = change in value of y -axis / change in values of x -axis

  comparing both the equations

    change in value of y -axis = change in position

  change in values of x -axis = time taken

so position values should be on the y axis and time values should be on the x axis.

distance on the y-axis and time on the x-axis.

you can cut your hand off if your not