Masses of Nix and Hydra
arXiv:0712.1261 · doi:10.1088/0004-6256/135/3/777
Abstract
A four-body orbit solution for the Pluto system yields GM values of 870.3 +/- 3.7, 101.4 +/- 2.8, 0.039 +/- 0.034, and 0.021 +/- 0.042 km3 sec-2 for Pluto, Charon, Nix, and Hydra, respectively. Assuming a Charon-like density of 1.63 gm cm-3, the implied diameters for Nix and Hydra are 88 and 72 km, leading to visual geometric albedos of 0.08 and 0.18, respectively, though with considerable uncertainty. The eccentricity of Charon's orbit has a significant nonzero value; however, the 0.030 +/- 0.009 deg yr-1 rate at which the line of apsides precesses is insufficient to explain the difference in the longitude of periapsis seen in the orbits fitted to the 1992-1993 and 2002-2003 data sets. The mean orbital periods for Hydra, Nix, and Charon are in the ratios of 6.064 +/- 0.006 : 3.991 +/- 0.007 : 1, but we have not identified any resonant arguments that would indicate the existence of a mean motion resonance between any pairs of satellites.
14 pages, 6 figures, 6 tables
References in corpus (6)
- The Discovery of Two New Satellites of Pluto
- Orbits and photometry of Pluto's satellites: Charon, S/2005 P1 and S/2005 P2
- The orbit, mass, size, albedo, and density of (65489) Ceto/Phorcys: A tidally-evolved binary Centaur
- Charon's radius and density from the combined data sets of the 2005 July 11 occultation
- The Orbit, Mass, and Albedo of Transneptunian Binary 1999 RZ253
- The Orbit and Albedo of Transneptunian Binary 1997 CQ29
Cited by in corpus (29)
- Orbits and Masses of the Satellites of the Dwarf Planet Haumea = 2003 EL61
- The Pluto System After New Horizons
- Pluto's atmosphere from the 29 June 2015 ground-based stellar occultation at the time of the New Horizons flyby
- Circumbinary Chaos: Using Pluto's Newest Moon to Constrain the Masses of Nix & Hydra
- Complete Tidal Evolution of Pluto-Charon
- Pluto's atmosphere from stellar occultations in 2012 and 2013
- Orbits of Near-Earth Asteroid Triples 2001 SN263 and 1994 CC: Properties, Origin, and Evolution
- Interpreting the Densities of the Kuiper Belt's Dwarf Planets
- (47171) 1999 TC36, A Transneptunian Triple
- The Formation of Pluto's Low Mass Satellites
- Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016
- The Mutual Orbit, Mass, and Density of the Large Transneptunian Binary System Varda and Ilmarë
- Ejecta Exchange, Color Evolution in the Pluto System, and Implications for KBOs and Asteroids with Satellites
- Tectonic Activity on Pluto After the Charon-Forming Impact
- Levy Flights of Binary Orbits due to Impulsive Encounters
- Orbits, masses, and evolution of main belt triple (87) Sylvia
- On the Origin of Pluto's Small Satellites by Resonant Transport
- Measuring temperature and ammonia hydrate ice on Charon in 2015 from Keck/OSIRIS spectra
- Dynamical capture in the Pluto-Charon system
- JWST observations of stellar occultations by solar system bodies and rings
- Detailed survey of the phase space around Nix and Hydra
- A Pluto-Charon Sonata: The Dynamical Architecture of the Circumbinary Satellite System
- A Pluto-Charon Concerto: An Impact on Charon as the Origin of the Small Satellites
- A Pluto--Charon Sonata: Dynamical Limits on the Masses of the Small Satellites
- Evolution of a ring around the Pluto-Charon binary
- Ejecta Transfer in the Pluto System
- Past and present dynamics of the circumbinary moons in the Pluto-Charon system
- Constraining multiple systems with GAIA
- A Pluto--Charon Sonata IV. Improved Constraints on the Dynamical Behavior and Masses of the Small Satellites