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Planet Nine is a hypothetical large planet in the far outer Solar System, first proposed in 2014, which would explain the unusual orbital configuration of a group of trans-Neptunian objects (TNOs) whose orbits lie mostly beyond the Kuiper belt. The planet would have an estimated mass of around 10 Earths and an estimated radius of 13,000 to 26,000 km (8,100 to 16,000 mi) (approximately two to four Earths). On 20 January 2016, researchers Konstantin Batygin and Michael E. Brown at Caltech announced additional indirect evidence of Planet Nine based on a new scientific model of the orbits of several...