A70.0-kg ice hockey goalie, originally at rest, has a 0.280-kg hockey puck slapped at him at a velocity of 45.5 m/s. suppose the goalie and the puck have an elastic collision, and the puck is reflected back in the direction from which it came. what would the final velocities of the goalie and the puck be in this case? assume that the collision is completely elastic.

mₐ vᵢₐ + mᵦ vᵢᵦ = mₐ vfₐ + mᵦ vfᵦ ==> [i and f means initial and final velocities] 

0.5 mₐ vᵢₐ² + 0.5 mᵦ vᵢᵦ² = 0.5 mₐ vfₐ² + 0.5 mᵦ vfᵦ² 

The collision is completely specified given the two initial velocities and the masses of the two objects. Combining the two equations above gives us a solution to the final velocities for an elastic collision of two objects: 

vfₐ = [(mₐ - mᵦ) vᵢₐ + 2 mᵦ vᵢᵦ]/[mₐ + mᵦ] 

vfᵦ = [2 mₐ vᵢₐ − (mₐ - mᵦ) vᵢᵦ]/[mₐ + mᵦ] 

substituting the values 

mₐ = 70 kg 
mᵦ = 0.280 kg 
vᵢₐ = 0 m/s 
vᵢᵦ = 45.5 m/s 

=> vfₐ = [(70 - 0.280) 0 + 2(0.280) 45.5]/[70 + 0.28] 

= 1.35 m/s >(in the original direction of the puck) 

and 

=> vfᵦ = [0 − (70 - 0.280) 45.5]/[ 70 + 0.28] = -45.14 m/s (opposite direction) 

Final speeds are therefore:

goalie = 1.35 m/s

puck = 45.14 m/s (opposite direction)

answer: d. a cme increases the amount of energy in the solar wind

explanation:

coronal mass ejections, also called cmes, are large clouds of plasma and magnetic field that erupt from the sun. only when the cloud is aimed at earth will the cme hit earth and therefore cause impacts. high-speed solar wind streams come from areas on the sun known as coronal holes.

come closer and become far apart and become steam/gas