부산대학교 도서관

Recent exoplanet observations have revealed a diversity of exoplanetary systems, which suggests the ubiquity of radial planetary migration. One powerful known mechanism of planetary migration is planetesimal-driven migration (PDM), which makes planets undergo significant migration through gravitational scattering with planetesimals. Here, we present the results of our high-resolution self-consistent $N$-body simulations of PDM, in which gravitational interactions among planetesimals, the gas drag, and Type-I migration are all taken into account. Our results show that even small protoplanets can actively migrate through PDM. Moreover, a fair fraction of them migrate outward. This outward migration can give a solution for the ''planet migration problem'' caused by Type-I migration and explain the origin of Jovian planets.
Comment: 25 pages, 13 figures, submitted