Constraints on planet X/Nemesis from Solar System's inner dynamics

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

References in corpus (12)

• Extremely high precision VLBI astrometry of PSR J0437-4715 and implications for theories of gravity
• An Outer Planet Beyond Pluto and Origin of the Trans-Neptunian Belt Architecture
• Coupling dynamical and collisional evolution of small bodies II : Forming the Kuiper Belt, the Scattered Disk and the Oort Cloud
• Constraints on the acceleration of the solar system from high-precision timing
• Upper limits on density of dark matter in Solar system
• Searching for primordial black hole dark matter with pulsar timing arrays
• Astrometric Microlensing Constraints on a Massive Body in the Outer Solar System with Gaia
• A Search for Distant Solar System Bodies in the Region of Sedna
• Biases in Cometary Catalogues and Planet X
• Density of dark matter in Solar system and perihelion precession of planets
• What Can the Cosmic Microwave Background Tell Us About the Outer Solar System?
• Mesolensing Explorations of Nearby Masses: From Planets to Black Holes

Cited by in corpus (6)

• Constraints on the location of a putative distant massive body in the Solar System from recent planetary data
• Planet X revamped after the discovery of the Sedna-like object 2012 VP${}_{113}$?
• Formation of Super-Earth Mass Planets at 125-250 AU from a Solar-type Star
• Nemesis Reconsidered
• A Southern Sky and Galactic Plane Survey for Bright Kuiper Belt Objects
• Observational Constraints on Planet Nine: Astrometry of Pluto and Other Trans-Neptunian Objects