Literature DB >> 26472913

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

S A Stern1, F Bagenal2, K Ennico3, G R Gladstone4, W M Grundy5, W B McKinnon6, J M Moore3, C B Olkin7, J R Spencer7, H A Weaver8, L A Young7, T Andert9, J Andrews7, M Banks10, B Bauer8, J Bauman11, O S Barnouin8, P Bedini8, K Beisser8, R A Beyer3, S Bhaskaran12, R P Binzel13, E Birath7, M Bird14, D J Bogan15, A Bowman8, V J Bray16, M Brozovic12, C Bryan11, M R Buckley8, M W Buie7, B J Buratti12, S S Bushman8, A Calloway8, B Carcich17, A F Cheng8, S Conard8, C A Conrad7, J C Cook7, D P Cruikshank3, O S Custodio8, C M Dalle Ore3, C Deboy8, Z J B Dischner7, P Dumont11, A M Earle13, H A Elliott4, J Ercol8, C M Ernst8, T Finley7, S H Flanigan8, G Fountain8, M J Freeze8, T Greathouse4, J L Green18, Y Guo8, M Hahn19, D P Hamilton20, S A Hamilton8, J Hanley4, A Harch7, H M Hart8, C B Hersman8, A Hill8, M E Hill8, D P Hinson21, M E Holdridge8, M Horanyi2, A D Howard22, C J A Howett7, C Jackman11, R A Jacobson12, D E Jennings23, J A Kammer7, H K Kang8, D E Kaufmann7, P Kollmann8, S M Krimigis8, D Kusnierkiewicz8, T R Lauer24, J E Lee25, K L Lindstrom8, I R Linscott26, C M Lisse8, A W Lunsford23, V A Mallder8, N Martin7, D J McComas4, R L McNutt8, D Mehoke8, T Mehoke8, E D Melin8, M Mutchler27, D Nelson11, F Nimmo28, J I Nunez8, A Ocampo18, W M Owen12, M Paetzold19, B Page11, A H Parker7, J W Parker7, F Pelletier11, J Peterson7, N Pinkine8, M Piquette2, S B Porter7, S Protopapa20, J Redfern7, H J Reitsema7, D C Reuter23, J H Roberts8, S J Robbins7, G Rogers8, D Rose7, K Runyon8, K D Retherford4, M G Ryschkewitsch8, P Schenk29, E Schindhelm7, B Sepan8, M R Showalter21, K N Singer7, M Soluri30, D Stanbridge11, A J Steffl7, D F Strobel31, T Stryk32, M E Summers33, J R Szalay2, M Tapley4, A Taylor11, H Taylor8, H B Throop10, C C C Tsang7, G L Tyler26, O M Umurhan3, A J Verbiscer34, M H Versteeg4, M Vincent7, R Webbert8, S Weidner4, G E Weigle4, O L White3, K Whittenburg8, B G Williams11, K Williams11, S Williams8, W W Woods26, A M Zangari7, E Zirnstein4.   

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.
Copyright © 2015, American Association for the Advancement of Science.

Entities:  

Year:  2015        PMID: 26472913     DOI: 10.1126/science.aad1815

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  21 in total

1.  The rapid formation of Sputnik Planitia early in Pluto's history.

Authors:  Douglas P Hamilton; S A Stern; J M Moore; L A Young
Journal:  Nature       Date:  2016-11-30       Impact factor: 49.962

2.  Planetary science: Pluto's telltale heart.

Authors:  Amy C Barr
Journal:  Nature       Date:  2016-11-30       Impact factor: 49.962

3.  Reorientation and faulting of Pluto due to volatile loading within Sputnik Planitia.

Authors:  James T Keane; Isamu Matsuyama; Shunichi Kamata; Jordan K Steckloff
Journal:  Nature       Date:  2016-11-16       Impact factor: 49.962

4.  Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.

Authors:  William B McKinnon; Francis Nimmo; Teresa Wong; Paul M Schenk; Oliver L White; J H Roberts; J M Moore; J R Spencer; A D Howard; O M Umurhan; S A Stern; H A Weaver; C B Olkin; L A Young; K E Smith
Journal:  Nature       Date:  2016-06-02       Impact factor: 49.962

5.  Planetary science: Pluto's polygons explained.

Authors:  Andrew J Dombard; Sean O'Hara
Journal:  Nature       Date:  2016-06-02       Impact factor: 49.962

6.  The formation of Charon's red poles from seasonally cold-trapped volatiles.

Authors:  W M Grundy; D P Cruikshank; G R Gladstone; C J A Howett; T R Lauer; J R Spencer; M E Summers; M W Buie; A M Earle; K Ennico; J Wm Parker; S B Porter; K N Singer; S A Stern; A J Verbiscer; R A Beyer; R P Binzel; B J Buratti; J C Cook; C M Dalle Ore; C B Olkin; A H Parker; S Protopapa; E Quirico; K D Retherford; S J Robbins; B Schmitt; J A Stansberry; O M Umurhan; H A Weaver; L A Young; A M Zangari; V J Bray; A F Cheng; W B McKinnon; R L McNutt; J M Moore; F Nimmo; D C Reuter; P M Schenk
Journal:  Nature       Date:  2016-09-14       Impact factor: 49.962

7.  Penitentes as the origin of the bladed terrain of Tartarus Dorsa on Pluto.

Authors:  John E Moores; Christina L Smith; Anthony D Toigo; Scott D Guzewich
Journal:  Nature       Date:  2017-01-04       Impact factor: 49.962

8.  Observed glacier and volatile distribution on Pluto from atmosphere-topography processes.

Authors:  Tanguy Bertrand; François Forget
Journal:  Nature       Date:  2016-09-19       Impact factor: 49.962

9.  Vigorous convection as the explanation for Pluto's polygonal terrain.

Authors:  A J Trowbridge; H J Melosh; J K Steckloff; A M Freed
Journal:  Nature       Date:  2016-06-02       Impact factor: 49.962

10.  The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation.

Authors:  J L Ortiz; P Santos-Sanz; B Sicardy; G Benedetti-Rossi; D Bérard; N Morales; R Duffard; F Braga-Ribas; U Hopp; C Ries; V Nascimbeni; F Marzari; V Granata; A Pál; C Kiss; T Pribulla; R Komžík; K Hornoch; P Pravec; P Bacci; M Maestripieri; L Nerli; L Mazzei; M Bachini; F Martinelli; G Succi; F Ciabattari; H Mikuz; A Carbognani; B Gaehrken; S Mottola; S Hellmich; F L Rommel; E Fernández-Valenzuela; A Campo Bagatin; S Cikota; A Cikota; J Lecacheux; R Vieira-Martins; J I B Camargo; M Assafin; F Colas; R Behrend; J Desmars; E Meza; A Alvarez-Candal; W Beisker; A R Gomes-Junior; B E Morgado; F Roques; F Vachier; J Berthier; T G Mueller; J M Madiedo; O Unsalan; E Sonbas; N Karaman; O Erece; D T Koseoglu; T Ozisik; S Kalkan; Y Guney; M S Niaei; O Satir; C Yesilyaprak; C Puskullu; A Kabas; O Demircan; J Alikakos; V Charmandaris; G Leto; J Ohlert; J M Christille; R Szakáts; A Takácsné Farkas; E Varga-Verebélyi; G Marton; A Marciniak; P Bartczak; T Santana-Ros; M Butkiewicz-Bąk; G Dudziński; V Alí-Lagoa; K Gazeas; L Tzouganatos; N Paschalis; V Tsamis; A Sánchez-Lavega; S Pérez-Hoyos; R Hueso; J C Guirado; V Peris; R Iglesias-Marzoa
Journal:  Nature       Date:  2017-10-11       Impact factor: 49.962

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