How deep would be the eclipse caused by Jupiter transiting in front of the Solar disk, as observed from a distant star? To calculate it, compute the ratio of the crosssection of the Solar disk minus the cross-section of the Jupiter disk to the crosssection of the Solar disk (find the diameters online), and remove that number from 1 (it is a small number). SHOW YOUR WORK!

How deep would be the eclipse caused by Jupiter transiting in front of the Solar disk, as observed from a distant star? To calculate it, compute the ratio of the crosssection of the Solar disk minus the cross-section of the Jupiter disk to the crosssection of the Solar disk (find the diameters online), and remove that number from 1 (it is a small number). SHOW YOUR WORK!

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How deep would be the eclipse caused by Jupiter transiting in front of the Solar disk, as observed from a distant star?
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Solution from part A: E=-KE = PE/2 Solution from part B: =3/2kt a. (NOTE: Treat the cloud as two equal masses interacting gravitationally across a distance equal to the radius of the cloud.) Use your result from part a to write down the condition for gravitational collapse in terms of the kinetic and potential energies (NOTE: This condition is an INEQUALITY) b. Use your result from part b in order to replace the kinetic energy with its temperature equivalent in your expression for the collapse condition. c. Solve the expression in ii above for the mass.
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