Space Science Reviews

, Volume 140, Issue 1, pp 93–127

New Horizons: Anticipated Scientific Investigations at the Pluto System

  • Leslie A. Young
  • S. Alan Stern
  • Harold A. Weaver
  • Fran Bagenal
  • Richard P. Binzel
  • Bonnie Buratti
  • Andrew F. Cheng
  • Dale Cruikshank
  • G. Randall Gladstone
  • William M. Grundy
  • David P. Hinson
  • Mihaly Horanyi
  • Donald E. Jennings
  • Ivan R. Linscott
  • David J. McComas
  • William B. McKinnon
  • Ralph McNutt
  • Jeffery M. Moore
  • Scott Murchie
  • Catherine B. Olkin
  • Carolyn C. Porco
  • Harold Reitsema
  • Dennis C. Reuter
  • John R. Spencer
  • David C. Slater
  • Darrell Strobel
  • Michael E. Summers
  • G. Leonard Tyler
Article

DOI: 10.1007/s11214-008-9462-9

Cite this article as:
Young, L.A., Stern, S.A., Weaver, H.A. et al. Space Sci Rev (2008) 140: 93. doi:10.1007/s11214-008-9462-9

Abstract

The New Horizons spacecraft will achieve a wide range of measurement objectives at the Pluto system, including color and panchromatic maps, 1.25–2.50 micron spectral images for studying surface compositions, and measurements of Pluto’s atmosphere (temperatures, composition, hazes, and the escape rate). Additional measurement objectives include topography, surface temperatures, and the solar wind interaction. The fulfillment of these measurement objectives will broaden our understanding of the Pluto system, such as the origin of the Pluto system, the processes operating on the surface, the volatile transport cycle, and the energetics and chemistry of the atmosphere. The mission, payload, and strawman observing sequences have been designed to achieve the NASA-specified measurement objectives and maximize the science return. The planned observations at the Pluto system will extend our knowledge of other objects formed by giant impact (such as the Earth–moon), other objects formed in the outer solar system (such as comets and other icy dwarf planets), other bodies with surfaces in vapor-pressure equilibrium (such as Triton and Mars), and other bodies with N2:CH4 atmospheres (such as Titan, Triton, and the early Earth).

Keywords

PlutoCharonNixHydraNew Horizons

Copyright information

© Springer Science+Business Media B.V. 2008

Authors and Affiliations

  • Leslie A. Young
    • 1
  • S. Alan Stern
    • 1
  • Harold A. Weaver
    • 2
  • Fran Bagenal
    • 3
  • Richard P. Binzel
    • 4
  • Bonnie Buratti
    • 5
  • Andrew F. Cheng
    • 2
  • Dale Cruikshank
    • 6
  • G. Randall Gladstone
    • 7
  • William M. Grundy
    • 8
  • David P. Hinson
    • 9
  • Mihaly Horanyi
    • 3
  • Donald E. Jennings
    • 10
  • Ivan R. Linscott
    • 9
  • David J. McComas
    • 7
  • William B. McKinnon
    • 11
  • Ralph McNutt
    • 2
  • Jeffery M. Moore
    • 6
  • Scott Murchie
    • 2
  • Catherine B. Olkin
    • 1
  • Carolyn C. Porco
    • 12
  • Harold Reitsema
    • 13
  • Dennis C. Reuter
    • 10
  • John R. Spencer
    • 1
  • David C. Slater
    • 7
  • Darrell Strobel
    • 14
  • Michael E. Summers
    • 15
  • G. Leonard Tyler
    • 9
  1. 1.Southwest Research InstituteBoulderUSA
  2. 2.Johns Hopkins University Applied Physics Lab.LaurelUSA
  3. 3.University of ColoradoBoulderUSA
  4. 4.Massachusetts Institute of TechnologyCambridgeUSA
  5. 5.Jet Propulsion LaboratoryPasadenaUSA
  6. 6.NASA Ames Research CenterMoffett FieldUSA
  7. 7.Southwest Research InstituteSan AntonioUSA
  8. 8.Lowell ObservatoryFlagstaffUSA
  9. 9.Stanford UniversityStanfordUSA
  10. 10.NASA Goddard Space Flight CenterGreenbeltUSA
  11. 11.Washington UniversitySaint LouisUSA
  12. 12.Space Science InstituteBoulderUSA
  13. 13.Ball Aerospace and Technologies CorporationBoulderUSA
  14. 14.Johns Hopkins UniversityBaltimoreUSA
  15. 15.George Mason UniversityFairfaxUSA