The rate at which a nebular cloud rotates increases as the cloud collapses to form systems of stars and planets. Consider a smallsegment of a nebular cloud with a mass m of 1.9 x 102" kg, tangential velocity vinitial equal to 6.8 km s-1 located at an orbitaldistance rinitial = 2.5 x 10* km. After the cloud collapses, the same small segment is located at an orbital distancerinal = 3.2 x 10° km. Calculate the change of the rotational velocity, Ao, for the cloud segment, assuming perfectly circularorbits. Perform your work and report your solution using two significant figures.Δω-16605rad s-!

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The rate at which a nebular cloud rotates increases as the cloud collapses to form systems of stars and planets. Consider a small segment of a nebular cloud with a mass m of 1.9 × 10²" kg, tangential velocity vinitial equal to 6.8 km s located at an orbital distance rinitial = 2.5 × 10“ km. After the cloud collapses, the same small segment is located at an orbital distance rinal = 3.2 x 10° km. Calculate the change of the rotational velocity, Ao, for the cloud segment, assuming perfectly circular orbits. Perform your work and report your solution using two significant figures. Δω- 16605 rad s-

The rate at which a nebular cloud rotates increases as the cloud collapses to form systems of stars and planets. Consider a small segment of a nebular cloud with a mass m of 1.9 × 10²" kg, tangential velocity vinitial equal to 6.8 km s located at an orbital distance rinitial = 2.5 × 10“ km. After the cloud collapses, the same small segment is located at an orbital distance rinal = 3.2 x 10° km. Calculate the change of the rotational velocity, Ao, for the cloud segment, assuming perfectly circular orbits. Perform your work and report your solution using two significant figures. Δω- 16605 rad s-

Stars and Galaxies (MindTap Course List)

10th Edition

ISBN:9781337399944

Author:Michael A. Seeds

Publisher:Michael A. Seeds

Chapter15: The Milky Way Galaxy

Section: Chapter Questions

Problem 10P

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