The small satellites of Pluto as observed by New Horizons

@article{Weaver2016TheSS,
  title={The small satellites of Pluto as observed by New Horizons},
  author={H. Weaver and Marc W. Buie and Bonnie J. Buratti and William M. Grundy and Tod R. Lauer and Cathy B. Olkin and Alex H. Parker and Simon B. Porter and Mark R. Showalter and John R. Spencer and S. Alan Stern and Anne J. Verbiscer and William B. McKinnon and J. M. Moore and Stuart J. Robbins and Paul M. Schenk and Kelsi N. Singer and Olivier S. Barnouin and Andrew Cheng and Carolyn M. Ernst and C. M. Lisse and Donald E. Jennings and Allen W. Lunsford and Dennis C. Reuter and Douglas P. Hamilton and David E. Kaufmann and Kimberly Ennico and Leslie A. Young and Ross A. Beyer and Richard P. Binzel and Veronica Bray and Andrew L. Chaikin and Jason C. Cook and Dale P. Cruikshank and Cristina M. Dalle Ore and Alissa M. Earle and G. Randall Gladstone and Carly J. A. Howett and Ivan R. Linscott and Francis Nimmo and Joel Wm. Parker and Sylvie Philippe and Silvia Protopapa and H. J. Reitsema and Bernard Schmitt and Ted Stryk and Michael E. Summers and Constantine C. c. Tsang and H. B. Throop and Oliver L. White and Amanda M. Zangari},
  journal={Science},
  year={2016},
  volume={351}
}
New Horizons unveils the Pluto system In July 2015, the New Horizons spacecraft flew through the Pluto system at high speed, humanity's first close look at this enigmatic system on the outskirts of our solar system. In a series of papers, the New Horizons team present their analysis of the encounter data downloaded so far: Moore et al. present the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes… 
Surface compositions across Pluto and Charon
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, as well as their analysis of the encounter data downloaded so far.
The Pluto system after the New Horizons flyby
In July 2015, NASA’s New Horizons mission performed a flyby of Pluto, revealing details about the geology, surface composition and atmospheres of this world and its moons that are unobtainable from
The Pluto System After New Horizons
The New Horizons (NH) flyby of the Pluto–Charon binary planet and its system of four small surrounding satellites in mid-2015 revolutionized our knowledge of this distant planet and its moons. Beyond
Composition of Pluto’s small satellites: Analysis of New Horizons spectral images
Abstract On July 14, 2015, NASA’s New Horizons spacecraft encountered the Pluto-system. Using the near-infrared spectral imager, New Horizons obtained the first spectra of Nix, Hydra, and Kerberos
A White Paper on Pluto Follow On Missions: Background, Rationale, and New Mission Recommendations
The exploration of the binary Pluto-Charon and its small satellites during the New Horizons flyby in 2015 revealed not only widespread geologic and compositional diversity across Pluto, but
Craters of the Pluto-Charon System
Abstract NASA's New Horizons flyby mission of the Pluto-Charon binary system and its four moons provided humanity with its first spacecraft-based look at a large Kuiper Belt Object beyond Triton.
Ices on Charon: Distribution of H 2 O and NH 3 from New Horizons LEISA observations
Abstract Charon, the largest moon of Pluto, appeared as a fairly homogeneous, gray, icy world to New Horizons during closest approach on July 14th, 2015. Charon's sub-Pluto hemisphere was scanned by
Origin of the Pluto–Charon system: Constraints from the New Horizons flyby
Abstract New Horizon's accurate determination of the sizes and densities of Pluto and Charon now permit precise internal models of both bodies to be constructed. Assuming differentiated rock-ice
Pluto's Far Side
Abstract The New Horizons spacecraft provided near-global observations of Pluto that far exceed the resolution of Earth-based datasets. However, most previous Pluto New Horizons analyses focused on
Formation, Composition, and History of the Pluto System: A Post-New Horizons Synthesis
The Pluto-Charon system provides a broad variety of constraints on planetary formation, composition, chemistry, and evolution. Pluto was the first body to be discovered in what is now known as the
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References

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The geology of Pluto and Charon through the eyes of New Horizons
TLDR
Nasa’s New Horizons spacecraft has revealed a complex geology of Pluto and Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes, and these findings massively increase the understanding of the bodies in the outer solar system.
Surface compositions across Pluto and Charon
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, as well as their analysis of the encounter data downloaded so far.
Ejecta transfer in the Pluto system
Abstract The small satellites of the Pluto system (Styx, Nix, Kerberos, and Hydra) have very low surface escape velocities, and impacts should therefore eject a large amount of material from their
Impact and cratering rates onto Pluto
Abstract The New Horizons spacecraft fly-through of the Pluto system in July 2015 will provide humanity’s first data for the crater populations on Pluto and its binary companion, Charon. In
The orbits and masses of satellites of Pluto
Abstract We present the numerically integrated orbits of Pluto’s satellites. The orbits have been fit to a data set that includes Earth-based and Hubble Space Telescope (HST) astrometry of Charon,
A giant impact origin for Pluto's small moons and satellite multiplicity in the Kuiper belt
TLDR
It is argued that dust–ice rings of variable optical depths form sporadically in the Pluto system, and that rich satellite systems may be found—perhaps frequently—around other large Kuiper belt objects.
Discovery of two new satellites of Pluto
TLDR
The discovery of two additional moons around Pluto are reported, provisionally designated S/2005 P 1 ( hereafter P1) and S/ 2005 P 2 (hereafter P2), which makes Pluto the first Kuiper belt object known to have multiple satellites.
Ejecta exchange and satellite color evolution in the Pluto system, with implications for KBOs and asteroids with satellites
In this Note, I present first-order scaling calculations to examine the efficacy of impacts by Kuiper Belt debris in causing regolith exchange between objects in the Pluto system. It is found that
THE FORMATION OF PLUTO'S LOW-MASS SATELLITES
Motivated by the New Horizons mission, we consider how Pluto's small satellites—currently Styx, Nix, Kerberos, and Hydra—grow in debris from the giant impact that forms the Pluto-Charon binary. After
“TNOs are Cool”: A survey of the trans-Neptunian region - VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects
Trans-Neptunian objects (TNO) represent the leftovers of the formation of the Solar System. Their physical properties provide constraints to the models of formation and evolution of the various
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