A spherical satellite of approximately uniform density with radius 5.4 m and mass 300 kg is originally moving with velocity <2600, 0, 0>m/s, and is originally rotating with an angular speed 2 rad/s, in the direction shown in the diagram. A small piece of space junk of mass 5.1 kg is initially moving toward the satellite with velocity <−2200, 0, 0>m/s. The space junk hits the edge of the satellite as shown in the figure below, and moves off with a new velocity <−1300, 480, 0>m/s. Both before and after the collision, the rotation of the space junk is negligible. What is the rise in the internal energy of the satellite and space junk combined?

Principles of Physics: A Calculus-Based Text
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ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
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Chapter10: Rotational Motion
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Problem 53P
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A spherical satellite of approximately uniform density with radius 5.4 m and mass 300 kg is originally moving with velocity <2600, 0, 0>m/s, and is originally rotating with an angular speed 2 rad/s, in the direction shown in the diagram. A small piece of space junk of mass 5.1 kg is initially moving toward the satellite with velocity <−2200, 0, 0>m/s. The space junk hits the edge of the satellite as shown in the figure below, and moves off with a new velocity <−1300, 480, 0>m/s. Both before and after the collision, the rotation of the space junk is negligible.

What is the rise in the internal energy of the satellite and space junk combined?

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