Physical characterisation of near-Earth asteroid (1620) Geographos
B. RozitisDepartment of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996-1410, USASimon GreenPlanetary and Space Sciences, Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK
2014en
ABI
Аннотация
Context. The Yarkovsky (orbital drift) and YORP (spin state change) effects play important roles in the dynamical and physical evolution of asteroids. Thermophysical modelling of these observed effects, and of thermal-infrared observations, allows a detailed physical characterisation of an individual asteroid to be performed.
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