Small Stars with Small Planets and Big Consequences
The field of extrasolar planets is rapidly evolving. The quest to discover ever more and ever smaller exoplanets has pushed the field in two primary directions: 1) toward a comprehensive assessment of the frequency and statistics of various types of exoplanet — used to constrain planet formation and evolution theories — and 2) toward characterizing the composition, atmosphere and evolution of individual exoplanets as though they were planets in our own Solar System. I will discuss the importance of low-mass stars in this context, emphasizing the phenomenal results from the NASA's Kepler Mission, and our efforts to characterize individual terrestrial exoplanets orbiting low-mass stars with existing and novel ground-based instrumentation.
|Date: ||Tuesday, 1 October 2013|
|Where: ||McGill University|
| ||Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)|
|Contact: ||Robert Rutledge|