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The Pluto system: Initial results from its exploration by New Horizons.

Authors :
Stern SA
Bagenal F
Ennico K
Gladstone GR
Grundy WM
McKinnon WB
Moore JM
Olkin CB
Spencer JR
Weaver HA
Young LA
Andert T
Andrews J
Banks M
Bauer B
Bauman J
Barnouin OS
Bedini P
Beisser K
Beyer RA
Bhaskaran S
Binzel RP
Birath E
Bird M
Bogan DJ
Bowman A
Bray VJ
Brozovic M
Bryan C
Buckley MR
Buie MW
Buratti BJ
Bushman SS
Calloway A
Carcich B
Cheng AF
Conard S
Conrad CA
Cook JC
Cruikshank DP
Custodio OS
Dalle Ore CM
Deboy C
Dischner ZJ
Dumont P
Earle AM
Elliott HA
Ercol J
Ernst CM
Finley T
Flanigan SH
Fountain G
Freeze MJ
Greathouse T
Green JL
Guo Y
Hahn M
Hamilton DP
Hamilton SA
Hanley J
Harch A
Hart HM
Hersman CB
Hill A
Hill ME
Hinson DP
Holdridge ME
Horanyi M
Howard AD
Howett CJ
Jackman C
Jacobson RA
Jennings DE
Kammer JA
Kang HK
Kaufmann DE
Kollmann P
Krimigis SM
Kusnierkiewicz D
Lauer TR
Lee JE
Lindstrom KL
Linscott IR
Lisse CM
Lunsford AW
Mallder VA
Martin N
McComas DJ
McNutt RL Jr
Mehoke D
Mehoke T
Melin ED
Mutchler M
Nelson D
Nimmo F
Nunez JI
Ocampo A
Owen WM
Paetzold M
Page B
Parker AH
Parker JW
Pelletier F
Peterson J
Pinkine N
Piquette M
Porter SB
Protopapa S
Redfern J
Reitsema HJ
Reuter DC
Roberts JH
Robbins SJ
Rogers G
Rose D
Runyon K
Retherford KD
Ryschkewitsch MG
Schenk P
Schindhelm E
Sepan B
Showalter MR
Singer KN
Soluri M
Stanbridge D
Steffl AJ
Strobel DF
Stryk T
Summers ME
Szalay JR
Tapley M
Taylor A
Taylor H
Throop HB
Tsang CC
Tyler GL
Umurhan OM
Verbiscer AJ
Versteeg MH
Vincent M
Webbert R
Weidner S
Weigle GE 2nd
White OL
Whittenburg K
Williams BG
Williams K
Williams S
Woods WW
Zangari AM
Zirnstein E
Source :
Science (New York, N.Y.) [Science] 2015 Oct 16; Vol. 350 (6258), pp. aad1815.
Publication Year :
2015

Abstract

The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition; its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected.<br /> (Copyright © 2015, American Association for the Advancement of Science.)

Details

Language :
English
ISSN :
1095-9203
Volume :
350
Issue :
6258
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
26472913
Full Text :
https://doi.org/10.1126/science.aad1815