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      Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt Object

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          Abstract

          The Kuiper Belt is a distant region of the Solar System. On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU69, a Cold Classical Kuiper Belt Object, a class of objects that have never been heated by the Sun and are therefore well preserved since their formation. Here we describe initial results from these encounter observations. MU69 is a bi-lobed contact binary with a flattened shape, discrete geological units, and noticeable albedo heterogeneity. However, there is little surface color and compositional heterogeneity. No evidence for satellites, ring or dust structures, gas coma, or solar wind interactions was detected. By origin MU69 appears consistent with pebble cloud collapse followed by a low velocity merger of its two lobes.

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          Author and article information

          Journal
          02 April 2020
          Article
          10.1126/science.aaw9771
          2004.01017
          d172c56a-600a-4401-b3cc-dc528704969e

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          Science 364, eaaw9771 (2019)
          43 pages, 8 figure
          astro-ph.EP

          Planetary astrophysics
          Planetary astrophysics

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