Mean radius and shape of Pluto and Charon from New Horizons images
arXiv:1603.00821 · doi:10.1016/j.icarus.2016.06.027
Abstract
Approach images taken by the LORRI imaging system during the New Horizons spacecraft encounter have been used to determine the mean radii and shapes of Pluto and Charon. The primary observations are limb locations derived using three independent approaches. The resulting mean radii of Pluto and Charon are 1188.3 +/- 1.6 km and 606.0 +/- 1.0 km, respectively (2-sigma). The corresponding densities are 1854 +/- 11 kg m-3 and 1701 +/- 33 kg m-3 (2-sigma). The Charon radius value is consistent with previous Earth-based occultation estimates. The Pluto radius estimate is consistent with solar occultation measurements performed by the ALICE and Fine Sun Sensor instruments on New Horizons. Neither Pluto nor Charon show any evidence for tidal/rotational distortions; upper bounds on the oblateness are <0.6% and <0.5%, respectively.
revised version submitted to Icarus (Pluto special issue)
References in corpus (10)
- The Pluto system: Initial results from its exploration by New Horizons
- The Geology of Pluto and Charon Through the Eyes of New Horizons
- The Atmosphere of Pluto as Observed by New Horizons
- Long-Range Reconnaissance Imager on New Horizons
- Pluto's lower atmosphere structure and methane abundance from high-resolution spectroscopy and stellar occultations
- ALICE: The Ultraviolet Imaging Spectrograph aboard the New Horizons Pluto-Kuiper Belt Mission
- The density of mid-sized Kuiper belt object 2002 UX25 and the formation of the dwarf planets
- Complete Tidal Evolution of Pluto-Charon
- Charon's radius and density from the combined data sets of the 2005 July 11 occultation
- Tectonic Activity on Pluto After the Charon-Forming Impact
Cited by in corpus (42)
- Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt Object
- Reorientation of Sputnik Planitia implies a Subsurface Ocean on Pluto
- Structure and Composition of Pluto's atmosphere from the New Horizons Solar Ultraviolet Occultation
- The Pluto System After New Horizons
- Pluto's Haze as a Surface Material
- Study of the plutino object (208996) 2003 AZ84 from stellar occultations: size, shape and topographic features
- Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016
- The mass and density of the dwarf planet (225088) 2007 OR10
- Trans-Neptunian objects and Centaurs at thermal wavelengths
- Doubly Synchronous Binary Asteroid Mass Parameter Observability
- Large-scale cryovolcanic resurfacing on Pluto
- Primordial N2 provides a cosmochemical explanation for the existence of Sputnik Planitia, Pluto
- A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS measured from stellar occultations
- Tidal Dissipation in Dual-Body, Highly Eccentric, and Non-synchronously Rotating Systems: Applications to Pluto-Charon and the Exoplanet TRAPPIST-1e
- Stellar occultations by Trans-Neptunian Objects
- The Wide-Binary Origin of The Pluto-Charon System
- Tidally locked rotation of the dwarf planet (136199) Eris discovered from long-term ground based and space photometry
- The New Horizons and Hubble Space Telescope Search For Rings, Dust, and Debris in the Pluto-Charon System
- The visible and thermal light curve of the large Kuiper belt object (50000) Quaoar
- Turbulence in particle laden midplane layers of planet forming disks
- New Constraints on Pluto's Sputnik Planitia Ice Sheet from a Coupled Reorientation-Climate Model
- A Pluto-Charon Sonata: The Dynamical Architecture of the Circumbinary Satellite System
- Limits on the number of primordial Scattered Disk objects at Pluto mass and higher from the absence of their dynamical signatures on the present day trans-Neptunian Populations
- A Pluto--Charon Sonata: Dynamical Limits on the Masses of the Small Satellites
- A Pluto-Charon Concerto: An Impact on Charon as the Origin of the Small Satellites
- On the structure and long-term evolution of ice-rich bodies
- Light curves of transneptunian objects from the K2 mission of the Kepler Space Telescope
- On the Estimation of Circumbinary Orbital Properties
- A bimodal distribution of haze in Pluto's atmosphere
- Distribution and Energy Balance of Pluto's Nitrogen Ice, as seen by New Horizons in 2015
- Charon: A brief history of tides
- A Pluto--Charon Concerto II. Formation of a Circumbinary Disk of Debris After the Giant Impact
- A Pluto-Charon Sonata III. Growth of Charon from a Circum-Pluto Ring of Debris
- Tidal evolution of the Pluto-Charon binary
- On the Origin of the Pluto System
- The trans-Neptunian object (119951) 2002 KX14 revealed via multiple stellar occultations
- The influence of Equation of State on impact dynamics between Pluto-like bodies
- Vital Signs: Seismology of ocean worlds
- Surface Volatile Composition as Evidence for Hydrothermal Processes Lasting Longer in Triton's Interior than Pluto's
- The Cohesive Object Sequence: The Mass-Density Distribution of Astronomical Objects from Asteroids to Stars
- Synchronisation of a tidal binary by inward orbital migration. The case of Pluto and Charon
- The Tidal-Thermal Evolution of the Pluto-Charon System