The Composition of M-Type Asteroids II: Synthesis of Spectroscopic and Radar Observations ⇑ J.R
Icarus 238 (2014) 37–50 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus The composition of M-type asteroids II: Synthesis of spectroscopic and radar observations ⇑ J.R. Neeley a,b,1, , B.E. Clark a,1, M.E. Ockert-Bell a,1, M.K. Shepard c,2, J. Conklin d, E.A. Cloutis e, S. Fornasier f, S.J. Bus g a Department of Physics, Ithaca College, Ithaca, NY 14850, United States b Department of Physics, Iowa State University, Ames, IA 50011, United States c Department of Geography and Geosciences, Bloomsburg University, Bloomsburg, PA 17815, United States d Department of Mathematics, Ithaca College, Ithaca, NY 14850, United States e Department of Geography, University of Winnipeg, Winnipeg, MB R3B 2E9, Canada f LESIA, Observatoire de Paris, 5 Place Jules Janssen, F-92195 Meudon Principal Cedex, France g Institute for Astronomy, 2680 Woodlawn Dr., Honolulu, HI 96822, United States article info abstract Article history: This work updates and expands on results of our long-term radar-driven observational campaign of Received 7 February 2012 main-belt asteroids (MBAs) focused on Bus–DeMeo Xc- and Xk-type objects (Tholen X and M class Revised 7 May 2014 asteroids) using the Arecibo radar and NASA Infrared Telescope Facilities (Ockert-Bell, M.E., Clark, B.E., Accepted 9 May 2014 Shepard, M.K., Rivkin, A.S., Binzel, R.P., Thomas, C.A., DeMeo, F.E., Bus, S.J., Shah, S. [2008]. Icarus 195, Available online 16 May 2014 206–219; Ockert-Bell, M.E., Clark, B.E., Shepard, M.K., Issacs, R.A., Cloutis, E.A., Fornasier, S., Bus, S.J.
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