Direct Detection of Extra-solar Planets Using High Contrast Imaging
James R. Graham
University of Toronto
Large astronomical telescopes coupled with new adaptive optics technologies
enable high contrast imaging. Current systems approach a dynamic range
of nearly a million to one on scales near the diffraction limit. In the
next decade a new generation of instruments will improve contrast by
another one to two orders of magnitude and provide images of extra-solar
planetary systems.
Date: | Mardi, le 8 mars 2011 |
Heure: | 16:00 |
Lieu: | Université McGill |
| Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103) |
Contact: | Robert Rutledge |
|