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Keyword: photoevaporation Clear all
2 claims from 1 paper
Physics and Astronomy › Astro and Planetary Science
Photoevaporation of the Jovian circumplanetary disk
Oberg, Kamp, Cazaux and Rab · Astronomy and Astrophysics · 2020
The authors modelled how far-ultraviolet radiation from the Sun's birth cluster could evaporate Jupiter's circumplanetary disk, and what this implies for how the Galilean moons formed and are arranged.
Unchecked2 claimsShow 2 claims
- UncheckedFor low Jovian disk accretion rates (below 10^-12 solar masses a year), photoevaporation trimming the disk explains why no more moons lie beyond Callisto.“For CPD accretion rates $\dot M < 10^{-12} M_{\odot}$ yr$^{-1}$, photoevaporative truncation explains the lack of additional satellites outside the orbit of Callisto.”
- UncheckedFor light Jovian circumplanetary disks (below 10^-6.2 solar masses), photoevaporation could clear the disk before Callisto migrates into the Laplace resonance.“For CPDs of mass $M_{\rm CPD} < 10^{-6.2 M_{\odot}}$ , photoevaporation can disperse the disk before Callisto is able to migrate into the Laplace resonance.”
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