Volume 466, Number 2, May I 2007
|Page(s)||717 - 728|
|Section||Planets and planetary systems|
|Published online||29 January 2007|
Giant collisions involving young Jupiter
Physikalisches Institut, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland e-mail: firstname.lastname@example.org
Accepted: 29 November 2006
We present high-resolution, three-dimensional simulations using a smooth particle hydrodynamics (SPH) code of giant impacts involving young Jupiter-like planets. Our aim is to explore the effect of such impacts on the structure and evolution of the planet and discuss the likelihood of detecting these post-impact planets. For this, we considered head-on and off-axis impacts by an Earth-like planet onto a young Jupiter at five different ages: 1 Myr, 10 Myr, 30 Myr, 100 Myr, and 1 Gyr. We briefly discuss the short-term post-impact evolution and concentrate on computing the long-term cooling of the planet. We find that the bright IR afterglow lasts for about 106 yr if the impact involves a 1 Myr old planet and up to 108 yr if the impact occurs on an older planet (~30 Myr). We estimate that, about 10 to 100 young planetary systems must be observed to detect one candidate for such post-impact object. Given that their luminosity is only increased by a roughly 50%, this frequency does not make them ideal observing targets. We note nevertheless that the detection of this kind of post giant-impact planet would represent an important milestone in observationally establishing the current planet formation theories that are based on collisions.
Key words: stars: planetary systems / stars: planetary systems: formation / solar system: formation
© ESO, 2007
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