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New Horizons 2015 flyby of the Pluto system has resulted in high-resolution topographic maps of Pluto and Charon, the most distantobjects so mapped. DEM’s over ~30% of each object were produced at 100-300 m vertical and 300-800 m spatial resolutions, inhemispheric maps and high-resolution linear mosaics. Both objects reveal more relief than was observed at Triton. The dominant800-km wide informally named Sputnik Planum bright ice deposit on Pluto lies in a broad depression 3 km deep, flanked bydispersed mountains 3-5 km high. Impact craters reveal a wide variety of preservation states from pristine to eroded, and longfractures are several km deep with throw of 0-2 km. Topography of this magnitude suggests the icy shell of Pluto is relatively coldand rigid. Charon has global relief of at least 10 km, including ridges of 2-3 km and troughs of 3-5 km of relief. Impact craters areup to 6 km deep. Vulcan Planum consists of rolling plains and forms a topographic moat along its edge, suggesting viscous flow

the international archives of the photogrammetry, remote sensing and spatial information sciences/international archives of the photogrammetry, remote sensing and spatial information sciences

TOPOGRAPHIC MAPPING OF PLUTO AND CHARON USING NEW HORIZONS DATA