SIMBAD references

2016ApJ...817L..17B - Astrophys. J., 817, L17 (2016/February-1)

The in situ formation of giant planets at short orbital periods.

BOLEY A.C., GRANADOS CONTRERAS A.P. and GLADMAN B.

Abstract (from CDS):

We propose that two of the most surprising results so far among exoplanet discoveries are related: the existences of both hot Jupiters and the high frequency of multi-planet systems with periods P ≲ 200 days. In this paradigm, the vast majority of stars rapidly form along with multiple close-in planets in the mass range of Mars to super-Earths/mini-Neptunes. Such systems of tightly packed inner planets are metastable, with the time scale of the dynamical instability having a major influence on final planet types. In most cases, the planets consolidate into a system of fewer, more massive planets, but long after the circumstellar gas disk has dissipated. This can yield planets with masses above the traditional critical core of ∼10 M, yielding short-period giants that lack abundant gas. A rich variety of physical states are also possible given the range of collisional outcomes and formation time of the close-in planets. However, when dynamical consolidation occurs before gas dispersal, a critical core can form that then grows via gas capture into a short-period gas giant. In this picture the majority of Hot and Warm Jupiters formed locally, rather than migrating down from larger distances.

Abstract Copyright:

Journal keyword(s): planets and satellites: dynamical evolution and stability - planets and satellites: formation

Simbad objects: 9

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2016ApJ...817L..17B and select 'bookmark this link' or equivalent in the popup menu