Where the Solar system meets the solar neighbourhood: patterns in the distribution of radiants of observed hyperbolic minor bodies
Around the same time our ancestors left Africa, a dim red dwarf star came to within 0.8 light-years of our Sun, marking the closest known flyby of a star to our Solar System. New research suggests Scholz’s Star, as it’s known, left traces of this interstellar encounter by perturbing some comets in the outer Oort Cloud.
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Scholz’s Star, this research suggested, just grazed the outer reaches of the Oort Cloud, that remote bubble of debris that marks the outermost limits of the Sun’s dominant gravitational influence. The red dwarf has been drifting ever since, and it’s now about 20 light-years away. The University of Rochester researchers who conducted the 2015 study said it was unlikely that Scholz’s Star, with a mass around 9 percent of the Sun, and it’s brown dwarf, at about 6 percent the Sun’s mass, were able to disturb or jostle any of the objects in the Oort Cloud to a significant degree.
But new research published this week in Monthly Notices of the Royal Astronomical Society suggests this interpretation was wrong, and that Scholz’s Star did in fact influence the trajectories of some Oort Cloud objects. In the study, astronomer brothers Carlos de la Fuente Marcos and Raúl de la Fuente Marcos from Complutense University of Madrid, along with Sverre J. Aarseth from the University of Cambridge, identified the movements of dozens of known Oort Cloud objects as having been influenced by this ancient encounter.











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