-
Seminar Detail
High Resolution Imaging of Young Planets
Presenter: Ben Zuckerman ()
June 27, 2005 11:00 AM Pacific
Current, state of the art, imaging with the Hubble Space Telescope and
with adaptive optics on large ground-based telescopes is insufficiently
sensitive to detect starlight reflected from old cold extrasolar planets.
However, massive planets with ages less than 100 million years are
sufficiently self-luminous to be within our grasp now. This talk will
focus on the first successful infrared imaging detections of extrasolar
planets and on what can be learned now and in the near future from direct
imaging of such planets.Participation Instructions
CONNECTION INFORMATION:
Sites who would like to connect via Polycom MUST notify Diane Hawks at dhawks@mail.arc.nasa.gov at least three hours before the seminar. If you need Polycom help during the live event, call the videoconferencing helpdesk at (650) 604-6412
The slides from the seminar can be viewed real-time using WebEx at: <https://nasa.webex.com/nasa/j.php?ED=85414242&UID=29189962>
Meeting number: 921 035 642
Password: 1K*Falcon
If you've never joined a WebEx meeting before, please allow an extra 5-10 minutes to install the plug-in. Explorer is the recommended browser. Sites without a Polycom system can hear the seminar over the telephone while viewing the slides in WebEx. The NASA conference phone number for this is (877) 891-6023, passcode 381880.
Alternatively, participants without a Polycom system can view the webcast at: http://vanseg-1.arc.nasa.gov/2005/AB050627-01.ram There is a 30 second delay for the webcast, so viewers will need to advance the slides manually in WebEx. Questions can be posted in the WebEx chat area to be answered at the end of the talk.
December 21, 2007
