Asteroid shapes from near and far
|Convener: Anna Marciniak | Co-conveners: Thomas Müller , Josef Durech|
The session is focused on reconstructing asteroid shapes using various observing techniques and modelling methods: from in-situ imaging, through radar ranging, adaptive optics, lightcurve inversion, to occultation fitting and thermophysical modelling. Types of targets range from the nearest NEAs, through Main Belt to the most distant TNOs and Centaurs.
Abstracts relevant to any aspect of the above described studies are welcome.