Chapter 11 talks about the tidal heating of Jupiter's moons, but tidal forces will also be important when we move Jupiter very close to the sun. At its current orbit, Jupiter's rotational period is only about 10 hours. Since Hot Jupiters are tidally locked, we must slow down the rotational period of Jupiter to match the orbital period. Explain in a few sentences, using the concepts of tidal forces and energy conservation (where does the energy go?), how this is possible. (You may also want to reference tidal friction from Chapter 4.)