The New Horizons Kuiper Belt Extended Mission

@article{Stern2018TheNH,
  title={The New Horizons Kuiper Belt Extended Mission},
  author={S. Alan Stern and H. Weaver and John R. Spencer and H. A. Elliott and The New Horizons Team},
  journal={Space Science Reviews},
  year={2018},
  volume={214},
  pages={1-23}
}
The central objective of the New Horizons prime mission was to make the first exploration of Pluto and its system of moons. Following that, New Horizons has been approved for its first extended mission, which has the objectives of extensively studying the Kuiper Belt environment, observing numerous Kuiper Belt Objects (KBOs) and Centaurs in unique ways, and making the first close flyby of the KBO 486958 2014 MU69. This review summarizes the objectives and plans for this approved mission… 

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References

SHOWING 1-10 OF 65 REFERENCES

New Horizons: Anticipated Scientific Investigations at the Pluto System

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

The solar system beyond Neptune

A new frontier in our solar system opened with the discovery of the Kuiper Belt and the extensive population of icy bodies orbiting beyond Neptune. Today the study of all of these bodies,

The atmosphere of Pluto as observed by New Horizons

TLDR
The New Horizons team presents the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes, and their analysis of the encounter data downloaded so far.

THE FIRST HIGH-PHASE OBSERVATIONS OF A KBO: NEW HORIZONS IMAGING OF (15810) 1994 JR1 FROM THE KUIPER BELT

NASA’s New Horizons spacecraft observed (15810) 1994 JR1, a 3:2 resonant Kuiper belt object (KBO), using the LOng Range Reconnaissance Imager (LORRI) on 2015 November 2 from a distance of 1.85 au and

Pluto’s interaction with its space environment: Solar wind, energetic particles, and dust

TLDR
Preliminary results from the two New Horizons instruments that measure charged particles are the Solar Wind Around Pluto (SWAP) instrument and the Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) instrument are described, which suggest that very few atmospheric molecules are escaping upstream and becoming ionized.

Ralph: A Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission

The New Horizons instrument named Ralph is a visible/near infrared multi-spectral imager and a short wavelength infrared spectral imager. It is one of the core instruments on New Horizons, NASA’s

The Solar Wind Around Pluto (SWAP) Instrument Aboard New Horizons

Abstract The Solar Wind Around Pluto (SWAP) instrument on New Horizons will measure the interaction between the solar wind and ions created by atmospheric loss from Pluto. These measurements provide

Surface reflectance properties of distant Solar system bodies

The recent discoveries of over 40 new objects with orbits beyond 30 au represent the first sampling of a reservoir of objects lying beyond Neptune, known as the Kuiper Belt (or Edgeworth-Kuiper

WILL NEW HORIZONS SEE DUST CLUMPS IN THE EDGEWORTH–KUIPER BELT?

Debris disks are thought to be sculptured by neighboring planets. The same is true for the Edgeworth–Kuiper debris disk, yet no direct observational evidence for signatures of giant planets in the

THE NEW HORIZONS SOLAR WIND AROUND PLUTO (SWAP) OBSERVATIONS OF THE SOLAR WIND FROM 11–33 au

The Solar Wind Around Pluto (SWAP) instrument on National Aeronautics and Space Administration's New Horizons Pluto mission has collected solar wind observations en route from Earth to Pluto, and
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