The geology and geophysics of Kuiper Belt object (486958) Arrokoth
SCIENCE, 367(6481), 998-+.
By: J. Spencer, S. Stern, J. Moore, H. Weaver, K. Singer, C. Olkin, A. Verbiscer, W. McKinnon ..., J. Parker, R. Beyer, J. Keane, T. Lauer, S. Porter, O. White, B. Buratti, M. El-Maarry, C. Lisse, A. Parker, H. Throop, S. Robbins, O. Umurhan, R. Binzel, D. Britt, M. Buie, A. Cheng, D. Cruikshank, H. Elliott, G. Gladstone, W. Grundy, M. Hill, M. Horanyi, D. Jennings, J. Kavelaars, I. Linscott, D. McComas, R. McNutt, S. Protopapa, D. Reuter, P. Schenk, M. Showalter, L. Young, A. Zangari, A. Abedin, C. Beddingfield, S. Benecchi, E. Bernardoni, C. Bierson, D. Borncamp, V. Bray, A. Chaikin, R. Dhingra, C. Fuentes, T. Fuse, P. Gay, S. Gwyn, D. Hamilton, J. Hofgartner, M. Holman, A. Howard, C. Howett, H. Karoji, D. Kaufmann, M. Kinczyk*, B. May, M. Mountain, M. Patzold, J. Petit, M. Piquette, I. Reid, H. Reitsema, K. Runyon, S. Sheppard, J. Stansberry, T. Stryk, P. Tanga, D. Tholen, D. Trilling, L. Wasserman
TL;DR:
The age, composition, and formation process of the most pristine object yet visited by a spacecraft is determined, and improved stereo imaging constrains the object’s shape and topography and allows us to generate a stereographic terrain model.
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TL;DR:
The New Horizons spacecraft completed its MU69 flyby on 1 January 2019, with a closest approach distance of 3538 km—less than one-third of its closest distance to Pluto.
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TL;DR:
Changes in topography across radar-bright deposits hosted in flat-floored, complex craters using individual edited Mercury Laser Altimeter tracks are investigated and it is shown that the two populations cannot be distinguished.
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