- Press Release
- Mar 21, 2023
Exploring The Recycling Model Of Phobos Formation: Rubble-pile Satellites
Phobos is the target of the return sample mission Martian Moons eXploration by JAXA that will analyze in great details the physical and compositional properties of the satellite from orbit, from the surface and in terrestrial laboratories, giving clues about its formation.
Some models propose that Phobos and Deimos were formed after a giant impact giving rise to an extended debris disk. Assuming that Phobos formed from a cascade of disruptions and re-accretions of several parent bodies in this disk, and that they are all characterized by a low material cohesion, Hesselbrock & Milton (2017) have showed that a recycling process may happen during the assembling of Phobos, by which Phobos’ parents are destroyed into a Roche-interior ring and reaccreted several times.
In the current paper we explore in details the recycling model, and pay particular attention to the characteristics of the disk using 1D models of disk/satellite interactions. In agreement with previous studies we confirm that, if Phobos’ parents bodies are gravitational aggregates (rubble piles), then the recycling process does occur. However, Phobos should be accompanied today by a Roche-interior ring. Furthermore, the characteristics of the ring are not reconcilable with today`s observations of Mars’ environment, which put stringent constraints on the existence of a ring around Mars.
The recycling mechanism may or may not have occurred at the Roche limit for an old moon population, depending on their internal cohesion. However, the
Phobos we see today cannot be the outcome of such a recycling process.
Gustavo Madeira, Sebastien Charnoz, Yun Zhang, Ryuki Hyodo, Patrick Michel, Hidenori Genda, Silvia Giuliatti Winter
Comments: Accept in The Astronomical Journal
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2302.12556 [astro-ph.EP] (or arXiv:2302.12556v1 [astro-ph.EP] for this version)
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From: Gustavo Madeira Dr
[v1] Fri, 24 Feb 2023 10:16:27 UTC (7,340 KB)