Name | Will attend | Topic | Abstract | Additional material | Presentation |
---|---|---|---|---|---|
Benner, Lance | Yes | Arecibo and Goldstone Radar Imaging of Contact Binary Asteroids | yes | [ppt, 3.9 MB] | |
Boue, Gwenael | Yes | (student of Jacques Laskar, Observatory of Paris) | no | ||
Carry, Benoit | Yes | (Marcello student, ESO) | no | ||
Delbo, Marco | Yes | Thermal Infrared Observations of Binary NEAs | yes | ||
Durech, Josef | 90% | Detection of binary NEAs from sparse photometry | yes | [pdf, 1.3 MB] | |
Fahnestock, Eugene | Yes | Primary Surface Particle Motion and YORP-Driven Expansion of Asteroid Binaries | yes | article | [ppt, 5.1 MB] |
Fulchignoni, Marcello | Yes | no | |||
Harris, Alan | Yes | On the shapes and spins of "rubble pile" asteroids | yes | article
article | [ppt, 1.2 MB] |
Hestroffer, Daniel | Yes | [mov, 10.7 MB] | |||
Holsapple, Keith | Yes | Do 100 km Asteroids Spin-Fission Into Binaries? | yes | [ppt, 5.1 MB] | |
Howell, Ellen | Yes | The Composition of NEA binaries | yes | ||
Marchis, Franck | Yes | Survey of Binary Asteroid with Spitzer/IRS | yes | article | |
Margot, Jean-Luc | Yes | The Eccentric Mutual Orbit and Shape of 2004 DC | yes | ||
Michel, Patrick | Yes | Binary formation as a result of collisional disruption and gravitational reaccumulation | yes | ||
Nolan, Mike | Yes | What we see / can see with the radar about binaries | [ppt, 6.5 MB] | ||
Pravec, Petr | Yes | Binaries among small main belt asteroids | yes | article | [ppt, 1.5 MB] |
Richardson, Derek | Yes | Implications of cohesion for binary asteroid formation | yes | article | [pdf, 12.2 MB] |
Rossi, Alessandro | Yes | Evolution of NEAs rotation rate | yes | [pdf, 568 KB] | |
Scheeres, Dan | Yes | Reconfigurations and fission of rubble pile asteroids | yes | article | |
Taylor, Patrick | Yes | The Tidal Interaction of Binary Asteroid Components | yes | ||
Vokrouhlicky, David | Yes | Pairs of asteroids probably of common origin | yes | article | [ppt, 3.2 MB] |
Walsh, Kevin | Yes | Binary Asteroid Formation via Spin-up | yes |