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Showing 1–11 of 11 results
Advanced filters: Author: Robin M. Canup Clear advanced filters
  • Saturn's rings are more than 90–95% water ice, which implies that initially they were almost pure ice because they are continually polluted by rocky meteoroids. Saturn has only one large satellite, Titan, whereas Jupiter has four large satellites; additional large satellites probably existed originally but were lost as they spiralled into Saturn. Now, numerical simulations of the tidal removal of mass from a differentiated, Titan sized satellite as it migrates inward towards Saturn are reported. Planetary tidal forces preferentially strip material from the satellite's outer icy layers, while its rocky core remains intact and is lost to collision with the planet. The result is a pure ice ring.

    • Robin M. Canup
    Research
    Nature
    Volume: 468, P: 943-946
  • Compact exoplanetary systems masses have a similar mass ratio compared to the host star’s mass. Here, authors propose that these planets are surviving remnants of planet accretion during the end stages of stellar infall.

    • Raluca Rufu
    • Robin M. Canup
    ResearchOpen Access
    Nature Communications
    Volume: 16, P: 1-11
  • Jupiter’s large moons Ganymede and Callisto are similar in size and composition, but different in surface and interior characteristics. Simulations with geophysical models of core formation indicate that the difference in impact energy received by the two satellites during the period of late heavy bombardment can explain the dichotomy.

    • Amy C. Barr
    • Robin M. Canup
    Research
    Nature Geoscience
    Volume: 3, P: 164-167
  • The Moon may have accreted from a disk of debris after a giant impact. Simulations suggest that part of the Moon derives from volatile-poor melt in the hot inner disk, with most of the volatile elements condensing later and accreting to Earth.

    • Robin M. Canup
    • Channon Visscher
    • Bruce Fegley Jr
    Research
    Nature Geoscience
    Volume: 8, P: 918-921
  • Earth and the Moon share many puzzling chemical similarities. New analyses show that the last planet-sized body to hit Earth could have been similar enough to Earth to yield a Moon with an Earth-like composition. See Letter p.212

    • Robin M. Canup
    News & Views
    Nature
    Volume: 520, P: 169-170
  • Modelling of satellite growth as a giant planet accumulates hydrogen gas and rock-ice solids from solar orbit finds that the mass fraction of its satellite system is ∼10−4 and regulated by a balance of two competing processes.

    • Robin M. Canup
    • William R. Ward
    Research
    Nature
    Volume: 441, P: 834-839
  • The history of Earth’s formation can be unravelled from the compositions of meteorites, terrestrial and lunar rocks, and observations from space-based telescopes. This Review discusses advances in theories and evidence concerning the dynamical mechanisms and timescales for Earth’s accretion in the Solar System.

    • Alex N. Halliday
    • Robin M. Canup
    Reviews
    Nature Reviews Earth & Environment
    Volume: 4, P: 19-35