New Horizons: Anticipated Scientific Investigations at the Pluto System
arXiv:0709.4270 · 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 acheive 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).
40 pages, 9 figures, 7 tables; To appear in a special volume of Space Science Reviews on the New Horizons mission
References in corpus (9)
- Ralph: A Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission
- The Discovery of Two New Satellites of Pluto
- The New Horizons Pluto Kuiper belt Mission: An Overview with Historical Context
- The Solar Wind Around Pluto (SWAP) Instrument Aboard New Horizons
- ALICE: The Ultraviolet Imaging Spectrograph aboard the New Horizons Pluto-Kuiper Belt Mission
- Orbits and photometry of Pluto's satellites: Charon, S/2005 P1 and S/2005 P2
- The Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) on the New Horizons Mission
- Charon's radius and density from the combined data sets of the 2005 July 11 occultation
- New Constraints on Additional Satellites of the Pluto System
Cited by in corpus (27)
- Surface Compositions Across Pluto and Charon
- The Geology of Pluto and Charon Through the Eyes of New Horizons
- The Atmosphere of Pluto as Observed by New Horizons
- Ralph: A Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission
- Possible ring material around centaur (2060) Chiron
- Pluto's global surface composition through pixel-by-pixel Hapke modeling of New Horizons Ralph/LEISA data
- Structure and Composition of Pluto's atmosphere from the New Horizons Solar Ultraviolet Occultation
- The Pluto System After New Horizons
- Near-Infrared Spectral Monitoring of Pluto's Ices: Spatial Distribution and Secular Evolution
- Plutos interaction with its space environment: Solar Wind, Energetic Particles & Dust
- Circumbinary Chaos: Using Pluto's Newest Moon to Constrain the Masses of Nix & Hydra
- Overview of the New Horizons Science Payload
- The New Horizons Kuiper Belt Extended Mission
- Volatile transport on inhomogeneous surfaces: I. Analytic expressions, with application to Pluto's day
- Absorption Coefficients of the Methane-Nitrogen Binary Ice System: Implications for Pluto
- Visible-Infrared spectroscopy of ungrouped and rare meteorites brings further constraints on meteorite-asteroid connections
- Solar Wind at 33 AU: Setting Bounds on the Pluto Interaction for New Horizons
- Remote Sensing D/H Ratios in Methane Ice: Temperature-Dependent Absorption Coefficients of CH3D in Methane Ice and in Nitrogen Ice
- Near-Infrared Spectral Monitoring of Pluto's Ices II: Recent Decline of CO and N Ice Absorptions
- Measuring temperature and ammonia hydrate ice on Charon in 2015 from Keck/OSIRIS spectra
- Exploration of trans-Neptunian objects using the Direct Fusion Drive
- Pluto's Ultraviolet Spectrum, Surface Reflectance, and Airglow Emissions
- On the existence of regular and irregular outer moons orbiting the Pluto-Charon system
- Ejecta Transfer in the Pluto System
- Impact Craters on Pluto and Charon and Terrain Age Estimates
- Physical studies of Centaurs and Trans-Neptunian Objects with the Atacama Large Millimeter Array
- Pluto's Atmosphere Does Not Collapse