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Extraterrestrial Life: Homework #5 Due, in class, Thursday April 10th
 

Summary: Extraterrestrial Life: Homework #5
Due, in class, Thursday April 10th
1) Briefly explain the radial velocity (or Doppler) method for detecting
extrasolar planets. Why does this technique work best for finding massive
planets, and those in short period orbits around their host stars?
2) What is meant by the term "hot Jupiters"? Why is the existence of these
planets surprising in the context of the theory of planet formation that was
developed to explain the properties of the Solar System?
3) The planet Saturn has a mass of 5.7 x 1026
kg and orbits the Sun at a
distance of 1.4 x 1012
m. If Saturn were the only planet in the Solar System,
calculate the velocity with which the Sun would move around the center
of mass of the Sun + Saturn system.
4) An extrasolar planet orbits a Solar mass star in a circular orbit at a
distance of 0.05 AU. Calculate the orbital velocity of the planet and the
orbital period of the planet.
5) The same extrasolar planet (orbiting at 0.05 AU) has a radius of 9 x 107
m.
If the atmosphere of the planet reflects 50% of the star's light, calculate the

  

Source: Armitage, Phil - Department of Astrophysical and Planetary Sciences, University of Colorado at Boulder

 

Collections: Physics