The Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) on the New Horizons Mission Ralph L. McNutt, Jr.1,6, Stefano A. Livi2, Reid S. Gurnee1, Matthew E. Hill1, Kim A. Cooper1, G. Bruce Andrews1, Edwin P. Keath3, Stamatios M. Krimigis1,4, Donald G. Mitchell1, Barry Tossman3, Fran Bagenal5, John D. Boldt1, Walter Bradley3, William S. Devereux1, George C. Ho1, Stephen E. Jaskulek1, Thomas W. LeFevere1, Horace Malcom1, Geoffrey A. Marcus1, John R. Hayes1, G. Ty Moore1, Bruce D. Williams, Paul Wilson IV3, L. E. Brown1, M. Kusterer1, J. Vandegriff1 1The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA 2Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA 3The Johns Hopkins University Applied Physics Laboratory, retired 4 Academy of Athens, 28 Panapistimiou, 10679 Athens, Greece 5The University of Colorado, Boulder, CO 80309, USA 6443-778-5435, 443-778-0386,
[email protected] The Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) comprises the hardware and accompanying science investigation on the New Horizons spacecraft to measure pick-up ions from Pluto’s outgassing atmosphere. To the extent that Pluto retains its characteristics similar to those of a “heavy comet” as detected in stellar occultations since the early 1980s, these measurements will characterize the neutral atmosphere of Pluto while providing a consistency check on the atmospheric escape rate at the encounter epoch with that deduced from the atmospheric structure at lower altitudes by the ALICE, REX, and SWAP experiments on New Horizons. In addition, PEPSSI will characterize any extended ionosphere and solar wind interaction while also characterizing the energetic particle environment of Pluto, Charon, and their associated system.