Can large icy moons accrete undifferentiated

@article{Monteux2012CanLI,
  title={Can large icy moons accrete undifferentiated},
  author={Julien Monteux and Gabriel Tobie and Ga{\"e}l Choblet and Mathieu Le Feuvre},
  journal={Icarus},
  year={2012},
  volume={237},
  pages={377-387}
}

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References

SHOWING 1-10 OF 72 REFERENCES

Accretional heating of the satellites of Saturn and Uranus

We consider the heating of the larger satellites of Saturn and Uranus (with the exception of Titan) by deposition of impactor kinetic energy during satellite accretion. Satellite growth takes place

Thermal evolution of a growing Mars

[1] We developed a new numerical model which can simulate the thermal history and metal-silicate separation of a growing Mars. In this model the thermal disturbance caused by planetesimal impacts is

Thermal evolution of Earth and Moon growing by planetesimal impacts

Improved estimates of impact energy partitioning are combined with models of planetesimal size distribution and planetary growth to infer the early thermal evolutions of the earth and the moon. The

Titan's Accretion and Long Term Thermal History

We investigate Titan’s long-term thermal evolution starting with its accretion history in the context of the SEMM regular satellite formation model [1-3]. Our formation model allows for a size

A rigid and weathered ice shell on Titan

A strong inverse correlation between gravity and topography at long wavelengths that are not dominated by tides and rotation is reported, arguing that negative gravity anomalies produced by crustal thickening at the base of the ice shell overwhelm positive gravity anomalies created by the small surface topography, giving rise to this inverse correlation.
...