Long-Term Evolution of the Saturnian System. [PDF]
Ćuk M +7 more
europepmc +1 more source
Titan's spin state as a constraint on tidal dissipation. [PDF]
Downey BG, Nimmo F.
europepmc +1 more source
Synthesis and Characterization of Polypyrrole-Coated Anthracene Microparticles: A New Synthetic Mimic for Polyaromatic Hydrocarbon-Based Cosmic Dust. [PDF]
Chan DH +5 more
europepmc +1 more source
Accurate geometric albedo, shape, and size of Hi'iaka from a stellar occultation. [PDF]
Fernández-Valenzuela E +73 more
europepmc +1 more source
Titan's strong tidal dissipation precludes a subsurface ocean. [PDF]
Petricca F +15 more
europepmc +1 more source
Propyne: Determination of Physical Properties and Unit Cell Parameters under Titan-Relevant Conditions. [PDF]
Marlin TC +6 more
europepmc +1 more source
Resonant Rotation States of the Jovian and Saturnian Satellites
Many of the moons of the giant planets are trapped in a 1:1 spin-orbit resonance. Up to now this special rotation state is confirmed by observations for 8 satellites of Jupiter, 15 satellites of Saturn, 15 satellites of Uranus, and 7 satellites of Neptune[1].
Stark, Alexander +4 more
openaire +1 more source
Tidal Deformation and Dissipation Processes in Icy Worlds. [PDF]
Tobie G +5 more
europepmc +1 more source
Igneous processes in the small bodies of the Solar System II: Small satellites and dwarf planets. [PDF]
Leone G, Tanaka H.
europepmc +1 more source
Io's tidal response precludes a shallow magma ocean. [PDF]
Park RS +20 more
europepmc +1 more source

