Part I: From habitable planets...
Telegraphic ationale.
Habitable-zone models, results and limitations,
relation to η-Earth, future development •
Meaning of "habitable zone" in the case of M dwarfs:
radiative equilibrium, tidal locking and 3-D models around cool stars •
Kepler's Habitable Zone Working Group
Schedule (Monday, 13 July).
Hour | Title | Contributor | |
---|---|---|---|
14:00-14:10 | Welcome and introduction to joint satellite meeting Kepler's HZWG and Part I | Nader Haghighipour | |
14:10-15:40 |
Kepler's Habitable
Zone Working Group meeting (chair: Nader Haghighipour) |
||
15:40-15:55 | Tidal locking around M dwarfs | Eric T. Wolf (U. Colorado, USA) |
|
15:55-16:10 | 3D general circulation models to determine habitable zones around M dwarfs | Jérémy Leconte (CITA/CPS, Canada) |
|
16:10-16:30 | Kepler Habitable Zone Working Group and η-Earth (open discussion) | Convenors, contributors, all. Moderators: Nader Haghighipour, Stephen R. Kane and Ravi K. Kopparapu |
Contact for Part I.
- Ravi K. Kopparapu (PSU, PA, USA): ruk15©psu.edu
- José A. Caballero (CAB, Madrid, Spain): caballero©cab.inta-csic.es