DATA Speed calibration Slow 0 25 3 Moderate 0.428 0.325 7 59 Fast d. 741 0. 770 . 97 3 Collisions 264. $ 253. Collision # 2 4 YIE 295 D O O 0 342 0749 586 637ANALYSTS I. Show a sample calcul ridof the mined Can I motrestate in Collision #2 (ar En. 1 in the manual) 1 . 26 5 4 * 79 5 ) + ( 264 0 * Viz ) =0. = (2 654 7 0 392 ) +( 2648x. 24 9) 2. Show a sample calculation of the final total inameaturn in Collision #2 feee Eq- S in the manual) 3. Calculate the ratio py/pe for Collision #2. Explain your result in the Discussion & Couchwing. A. Show a sample calculation of the initial kinetic energy in Collision #4 (ee Eq. 1 in the manuel) 1265 ( 94)) +6) = 0 + - ( 632 ) 5. Show a sample calculation of the final kinetic energy in Collision #4 (are By. 4 in the manual) 6. Calculare the ratio KE,/KE, for Collision #4. Explain your result in the Deesuasion & ConclusionFill in the table below and use it to classify each collision as clastic or inelastic. Collision # KE KE. Collision type (rinde one) 995 0 .5 Elastic / Taeleetic 32 Elastic Marlesric 9 % Tinsthis / Inelastic 4 1.13 Finstig / Tarlastic Explain your masoning for why each collision is elastic/inclassic. "Texnuss momentum/energy i conserved" is only part of the anwer Explain why momentum/ caergy is or is not conserved and how you made that determination using the data you collected Refer to the Introduction of the lab manual for belp. (Hint: what is a system and when is it isolated?) its inlsatic because of the frictuon and sound for the first two.The energy that an object has due to its motion is called kinetic energy and is denfed as K = =mv- (1) where m is the object's mass and v is its speed. An object will also have gravitational potential energy that depends on its location relative to an arbitrary reference point. Near the surface of Earth, where the gravitational field is more or less uniform, gravitational potential energy can be written as U. = mgy (2) where g is the acceleration due to gravity (9.81m/s') and y is the height relative to an arbitrary reference point. Elastic potential energy is contained in a deformed elastic object just as a stretched or compressed spring. This kind of energy is expressed as Us = sky (3) where k is the spring constant and y is the displacement of the spring from it's equilibrium position. The total mechanical energy of an object is the sum of all kinetic and potential energies associated with the object: E =K+U, +Us (4) When a system is isolated from its surroundings such that no energy is gained or lost, the total