Ir reflectante spectra of Antartic carbonaceous chondrites to better characterize the surfaces of asteroids targetted by sample return missions

CHARACTERIZE THE SURFACES OF ASTEROIDS TARGETTED BY SAMPLE RETURN MISSIONS. J.M.Trigo-Rodriguez, J.Llorca, J.M. Madiedo , J. Alonso-Azcarate, A. S. Rivkin, S. Fornasier, I. Belskaya, R. Binzel, C.E. Moyano-Cambero, J. Dergham, and J. Cortes. 1 Institute of Space Sciences (CSIC-IEEC). Campus UAB, Faculty Sciences, C5-p2. Bellaterra, Spain. 2 Institut de Tecniques Energetiques i Centre de Recerca en Nanoenginyeria. Universitat Politecnica de Catalunya, Diagonal 647, ETSEIB. Barcelona, Spain. 3 Facultad de Ciencias Experimentales, Universidad de Huelva, Spain 4 Universidad de Castilla-La Mancha, Campus Fabrica de Armas, 45071 Toledo, Spain. John Hopkins University Applied Physics Laboratory, Laurel, MD, USA. 6 LESIA, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon, France. Department of Earth, Atmospheric, and Planetary Sciences, Massachuseeetts Institute of Technology, Cambridge, MA, USA.