Impact craters on 2014 MU69: Implications for Kuiper belt object size-frequency distributions and planetesimal formation

Kelsi N Singer1, John R Spencer2, William B McKinnon3, Alan Stern4, Sarah Greenstreet5, Brett Gladman6, Stuart J Robbins2, Kirby Runyon7, Paul Schenk8, J.J. Kavelaars9, Tod Lauer10, Alex H Parker11, Harold A Weaver Jr12, Catherine Olkin1, Jeffery Moore13, Joel Wm Parker2, Anne Verbiscer14 and William M Grundy15, (1)Southwest Research Institute Boulder, Boulder, CO, United States, (2)Southwest Research Institute, Boulder, CO, United States, (3)Washington Univ, Saint Louis, MO, United States, (4)Southwest Research Institute San Antonio, San Antonio, TX, United States, (5)B612 Foundation, Planetary Society, Mill Valley, United States, (6)University of British Columbia, Vancouver, Canada, (7)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (8)Lunar and Planetary Institute, Houston, TX, United States, (9)National Research Council of Canada, NRC-Herzberg Astronomy and Astrophysics, Victoria, BC, Canada, (10)National Optical Astronomy Observatory, Tucson, AZ, United States, (11)Southwest Research Institute Boulder, Boulder, United States, (12)The Johns Hopkins University, Laurel, MD, United States, (13)NASA Ames Research Center, Moffett Field, United States, (14)University of Virginia, Charlottesville, VA, United States, (15)Lowell Observatory, Flagstaff, AZ, United States