Oral Program EX3

EX3

Formation and Dynamical Evolution of Planetary Systems
Co-Convener: Diego Turrini 
Oral Program
 / Tue, 29 Sep, 09:00–12:30  / Room Neptune
Poster Program
 / Attendance Tue, 29 Sep, 17:45–19:15  / Poster Area

Tuesday, 29 September 2015
Room Neptune
09:00–09:15
EPSC2015-115
On the detectability of quasi-circular co-orbital planets. Application to the radial velocity technique.
A. Leleu, P. Robutel, and A.C.M. Correia
09:15–09:30
EPSC2015-121
Coorbital motion in the co-planar RTBP: family of Quasi-satellite periodic orbits
A. Pousse, P. Robutel, and A. Vienne
09:30–09:45
EPSC2015-143
On the rotation of co-orbital bodies
p. Robutel, A. Leleu, and A. Correia
09:45–10:00
EPSC2015-730
Evolution of angular-momentum-losing exoplanetary systems
C. Damiani and A.-F. Lanza
10:00–10:15
EPSC2015-449
Secular architecture of giant-planet dominated binary star systems
A. Bazso, E. Pilat-Lohinger, B. Funk, and S. Eggl
10:15–10:30
EPSC2015-322
Formation of giant planetary systems: effect of the eccentricity and inclination damping
S. Sotiriadis, A.-S. Libert, B. Bitsch, and A. Crida
Coffee break
11:00–11:15
EPSC2015-243
Asteroid flux and water transport towards circumprimary habitable zones in binary star systems
D. Bancelin, E. Pilat-Lohinger, S. Eggl, H. Lammer, C. Johnston, T.I. Maindl, and R. Dvorak
11:15–11:30
EPSC2015-434
Possible new members of Datura asteroid family
A. Rosaev and E. Plavalova
11:30–11:45 EPSC2015-646
Chemical composition of planets for different scenarios of formation of volatile species in the disc (withdrawn)
U. Marboeuf, A. Thiabaud, C. Walsh, M. N. Drozdovskaya, C. Eistrup, E. F. van Dishoeck, Y. Alibert, and W. Benz
11:45–12:00
EPSC2015-794
Extreme, variable debris disks produced by giant impacts during terrestrial planet formation
A.P. Jackson
12:00–12:15
EPSC2015-772 | presentation
The fossil Oort cloud and the dynamics beyond Neptune
M. Saillenfest, M. Fouchard, G. Tommei, and G. Valsecchi
12:15–12:30
EPSC2015-766
PRIME: Studying Low-Velocity Impacts in Microgravity
J. Colwell, J. Brisset, A. Dove, A. Whizin, H. Nagler, and N. Brown