how transcribed image text Kepler (mass M) is playing at the local park. Due to some fantastically convenient urban planning. there are two merry-go-rounds (MGR) right next to each other. Kepler starts by sitting on the edge of the small MGR (mass 2M). rotating with it at an angular velocity of wo.. The large MGR (mass 4M) is currently stationary. The MGRs can be modeled as solid disks. 2.)If Kepler jumps off the small MGR at Velocity V. as shown in the drawing. what will the final angular velocity (we) of the small MGR be? Your answer should be in terms of V. R and wo only. what will the final angular velocity (o) of the small MGR be? Your answer should be interms of V, R and mo only.2.)If Kepler jumps off the small MGR at Velocity V, as shown in the drawing, MGR'sKepler (mass M) is playing atthe local park. Due to somefantastically convenienturban planning, there are twomerry-go-rounds (MGR)right next to each other.Kepler starts by sitting on theedge of the small MGR(mass 2M), rotating with it atan angular velocity of m.The large MGR (mass 4M) iscurrently stationary. TheMGRS can be modeled asV SmallLarge >2RR4M2MRVКepler, MTop-Down Viewsolid disks.

what will the final angular velocity (o) of the small MGR be? Your answer should be in terms of V, R and mo only. 2.) If Kepler jumps off the small MGR at Velocity V, as shown in the drawing, MGR's Kepler (mass M) is playing at the local park. Due to some fantastically convenient urban planning, there are two merry-go-rounds (MGR) right next to each other. Kepler starts by sitting on the edge of the small MGR (mass 2M), rotating with it at an angular velocity of m. The large MGR (mass 4M) is currently stationary. The MGRS can be modeled as V Small Large > 2R R 4M 2M R V Кepler, M Top-Down View solid disks.

what will the final angular velocity (o) of the small MGR be? Your answer should be in terms of V, R and mo only. 2.) If Kepler jumps off the small MGR at Velocity V, as shown in the drawing, MGR's Kepler (mass M) is playing at the local park. Due to some fantastically convenient urban planning, there are two merry-go-rounds (MGR) right next to each other. Kepler starts by sitting on the edge of the small MGR (mass 2M), rotating with it at an angular velocity of m. The large MGR (mass 4M) is currently stationary. The MGRS can be modeled as V Small Large > 2R R 4M 2M R V Кepler, M Top-Down View solid disks.