|
The past twenty years have seen a revolution in our knowledge of planets outside
our solar system, driven entirely by improvements in the sensitivity of
observations. In this field, the theorists have been forced to play a game of catchup.
Tonight, I will fill you in on some of our theoretical progress by focusing on
planetary systems with exotic dynamics, namely planets that reside in star systems
containing more than one sun. To understand these systems, I'll begin with a
problem in classical celestial mechanics, the so-called "Three-Body Problem".
Though seemingly simple, it is notoriously difficult to solve exactly. Indeed, it has
been proved that there exists no general analytic solution for the motion of three
gravitationally interacting objects. Nonetheless, I will show how we can use
celestial mechanics and computer simulations to understand "Tatooine-like"
systems and their parent stars. Understanding the origins of such systems has
implications for mysteries ranging from the progenitors of supernovae to the reionization
of the universe after the formation of the first galaxies. |
|
Kaitlin Kratter received
her PhD from the University of Toronto and joined the Astronomy Dept. at
Arizona, after positions at the Harvard-Smithsonian Center for
Astrophysics and CU Boulder. Her work focuses on the extremes of star
and planet formation, including planetary systems orbiting multiple
stars. When not exploring the Universe from her office, she enjoys
running in Arizona.s spectacular desert mountain ranges. |
Introduction by Lars
Bildsten |