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Our sun's undiscovered stellar nemesis is still out there, says physicist
explained
Nemesis is a hypothetical red dwarf or brown dwarf, originally postulated in 1984 to be orbiting the Sun at a distance of about 95,000 AU (1.5 light-years), somewhat beyond the Oort cloud, to explain a perceived cycle of mass extinctions in the geological record, which seem to occur more often at intervals of 26 million years. In a 2017 paper, Sarah Sadavoy and Steven Stahler argued that the Sun was probably part of a binary system at the time of its formation, leading them to suggest "there probably was a Nemesis, a long time ago". Such a star would have separated from this binary system over four billion years ago, meaning it could not be responsible for the more recent cycles of mass extinctions.
From Wikipedia: Nemesis (hypothetical star) (CC BY-SA 4.0) ↗A distant companion would orbit far beyond the planets and, on each pass, gravitationally jostle the Oort cloud. That would knock some comets onto paths falling toward the inner solar system in bursts.
It shows how scientists try to explain where dangerous comets come from, and how an elegant idea can persist even when searches come up empty. If Nemesis existed it would be a dim red or brown dwarf, which is why astronomers keep looking.
Searching for a hidden object by its gravitational effects has worked before, as with Neptune in 1846, and failed before, as with the hunted planet Vulcan near Mercury. Nemesis so far belongs with the second group.
The name Nemesis comes from the Greek goddess of retribution.
Illustrative photo · Anynobody, CC BY-SA 3.0, via Wikimedia Commons
