Chapter 8: Problem 32
To what radius would Earth have to shrink, with no change in mass, for escape speed at its surface to be \(30 \mathrm{km} / \mathrm{s} ?\)
Chapter 8: Problem 32
To what radius would Earth have to shrink, with no change in mass, for escape speed at its surface to be \(30 \mathrm{km} / \mathrm{s} ?\)
All the tools & learning materials you need for study success - in one app.
Get started for freeGiven Earth's mass, the Moon's distance and orbital period, and the value of \(G,\) could you calculate the Moon's mass? If yes, how? If no, why not?
A projectile is launched vertically upward from a planet of mass \(M\) and radius \(R ;\) its initial speed is twice the escape speed. Derive an expression for its speed as a function of the distance \(r\) from the planet's center.
You're preparing an exhibit for the Golf Hall of Fame, and you realize that the longest golf shot in history was Astronaut Alan Shepard's lunar drive. Shepard, swinging single-handed with a golf club attached to a lunar sample scoop, claimed his ball went "miles and miles." The record for a single-handed golf shot on Earth is \(257 \mathrm{m}\). Could Shepard's ball really have gone "miles and miles"? Assume the ball's initial speed is independent of gravitational acceleration.
Show that the form \(\Delta U=m g \Delta r\) follows from Equation 8.5 when \(r_{1} \simeq r_{2} .\) [Hint: Write \(r_{2}=r_{1}+\Delta r\) and apply the binomial approximation (Appendix A).]
To what fraction of its current radius would Earth have to shrink (with no change in mass) for the gravitational acceleration at its surface to triple?
What do you think about this solution?
We value your feedback to improve our textbook solutions.