Constraints on planet X/Nemesis from Solar System's inner dynamics
arXiv:0904.1562 · doi:10.1111/j.1365-2966.2009.15458.x
Abstract
We put full 3D constraints on a putative planet X by using the dynamics of the inner planets of the solar system. In particular, we compute the mimium distance of X as a function of its heliocentric latitude and longitude for different values of its mass.
LaTex, MNRAS macros. 12 pages, 4 figures, 3 tables. To appear in Monthly Notices of the Royal Astronomical Society (MNRAS). Some typos fixed