Photometric Properties of Dwarf Planets and Other Kuiper Belt Objects Determined from New Horizons
Photometric Properties of Dwarf Planets and Other Kuiper Belt Objects Determined from New Horizons
Anne Verbiscer1, Simon Porter2, Susan Benecchi3, J.J. Kavelaars4, Harold A Weaver Jr5, John R Spencer6, Marc W Buie6, Bonnie J Buratti7, Paul Helfenstein8, Alex H Parker2, Catherine Olkin9, Joel Wm Parker6, S Alan Stern10, Leslie Ann Young9, Kimberly Ennico Smith11, Kelsi N Singer6 and The New Horizons Science Team, (1)University of Virginia, Charlottesville, VA, United States, (2)Southwest Research Institute Boulder, Boulder, United States, (3)Planetary Science Institute Tucson, Tucson, AZ, United States, (4)National Research Council of Canada, NRC-Herzberg Astronomy and Astrophysics, Victoria, BC, Canada, (5)The Johns Hopkins University, Laurel, MD, United States, (6)Southwest Research Institute, Boulder, CO, United States, (7)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (8)Cornell University, Ithaca, NY, United States, (9)Southwest Research Institute Boulder, Boulder, CO, United States, (10)Southwest Research Institute Boulder, Dept Space Studies, Boulder, CO, United States, (11)NASA Ames Research Center, Moffett Field, CA, United States
