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The early instability scenario: terrestrial planet formation during the giant planet instability, and the effect of collisional fragmentation
Matthew S. Clement, Nathan A. Kaib, Sean N. Raymond +2
The solar system's dynamical state can be explained by an orbital instability among the giant planets. A recent model has proposed that the giant planet instability happened during…
Rubble Pile Asteroids
Kevin J. Walsh
The moniker rubble pile is typically applied to all solar system bodies with Diameter between 200m and 10km - where in this size range there is an abundance of evidence that nearly…
Secular Resonance Between Iapetus and the Giant Planets
Matija Ćuk, Luke Dones, David Nesvorný +1
Using numerical integrations, we find that the orbital eccentricity of Saturn's moon Iapetus undergoes prominent multi-Myr oscillations. We identify the responsible resonant argume…
Mars' Growth Stunted by an Early Giant Planet Instability
Matthew S. Clement, Nathan A. Kaib, Sean N. Raymond +1
Many dynamical aspects of the solar system can be explained by the outer planets experiencing a period of orbital instability sometimes called the Nice Model. Though often correlat…
Asteroid Ryugu Before the Hayabusa2 Encounter
Koji Wada, Matthias Grott, Patrick Michel +31
Asteroid (162173) Ryugu is the target object of Hayabusa2, an asteroid exploration and sample return mission led by Japan Aerospace Exploration Agency (JAXA). Ground-based observat…