%R 2017PDSS..275M
%A Magri, C.;Howell, E.S.;Nolan, M.C.;Taylor, P.A.;Fernandez, Y.R;Mueller, M.;Vervack, R.J.;Benner, L.A.M.;Giorgini, J.D.;Ostro, S.J.;Scheeres, D.J.;Hicks, M.D.;Rhoades, H.;Somers, J.M.;Gaftonyuk, N.M.;Kouprianov, V.V.;Krugly, Yu.N.;Molotov, I.E.;Busch, M.W.;Margot, J.L.;Benishek, V.;Protitch-Benishek, V.;Galad, A.;Higgins, D.;Kusnirak, P.;Pray, D.P.
%T Shape and Rotation of (8567) 1996 HW1 V1.0
%D 10/2017
%J NASA Planetary Data System, EAR-A-I0037-5-SHAPE8567-V1.0
%U http://pdsquery.jpl.nasa.gov/query?Identifier=EAR-A-I0037-5-SHAPE8567-V1.0&resclass=data.dataset
%B We present the three-dimensional shape and rotation state of near-Earth asteroid (8567) 1996 HW1 based on radar images and optical lightcurves (Magri et al., 2011). 1996 HW1 was observed in 2008 using the 12.6-cm radar at Arecibo Observatory. Optical lightcurves were obtained at several observatories and used to further constrain the shape modeling.