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Initial results from the New Horizons exploration of 2014 MU 69 , a small Kuiper Belt object.
- Source :
-
Science (New York, N.Y.) [Science] 2019 May 17; Vol. 364 (6441). - Publication Year :
- 2019
-
Abstract
- The Kuiper Belt is a distant region of the outer Solar System. On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU <subscript>69</subscript> , a cold classical Kuiper Belt object approximately 30 kilometers in diameter. Such objects have never been substantially heated by the Sun and are therefore well preserved since their formation. We describe initial results from these encounter observations. MU <subscript>69</subscript> is a bilobed contact binary with a flattened shape, discrete geological units, and noticeable albedo heterogeneity. However, there is little surface color or compositional heterogeneity. No evidence for satellites, rings or other dust structures, a gas coma, or solar wind interactions was detected. MU <subscript>69</subscript> 's origin appears consistent with pebble cloud collapse followed by a low-velocity merger of its two lobes.<br /> (Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.)
Details
- Language :
- English
- ISSN :
- 1095-9203
- Volume :
- 364
- Issue :
- 6441
- Database :
- MEDLINE
- Journal :
- Science (New York, N.Y.)
- Publication Type :
- Academic Journal
- Accession number :
- 31097641
- Full Text :
- https://doi.org/10.1126/science.aaw9771