On the formation of the Kepler-10 planetary system

In this paper, we investigate the conditions required for the 3 and 17 Earth mass solid planets in the Kepler-10 system to have formed through collisions and mergers within an initial population of embryos. By performing a large number of N-body simulations, we show that the total mass of the initia...

תיאור מלא

מידע ביבליוגרפי
מחבר ראשי: Terquem, C
פורמט: Journal article
יצא לאור: 2014