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First Oort Cloud Object May Have Been Discovered
SpuriousLogic alerts us to the discovery of what may be the first object ever discovered from the inner edge of the Oort cloud. 2006 SQ372 was found on images from the Sloan Digital Sky Survey. Its discoverers theorize that this comet-like object and the planetoid Sedna, first spotted in 2003, might be Oort denizens. Sedna is in a stable orbit but 2006 SQ372 has been perturbed by the gravity of Uranus and/or Neptune, simulations suggest, so its orbital history is unknowable. 2006 SQ372 will travel out to 1,600 AU on this orbit, making it the most distant solar-system object yet found. The Oort cloud is believed to extend ten times that far, or about a quarter of a light-year. "Theoretical models of the formation of the Oort Cloud predict that it should also host a massive inner part, but comets from this region never make it near Earth. To see the long-period comets from the inner region of the Oort Cloud requires observing comets whose orbits always stay well outside Saturn's orbit — like 2006 SQ372."
Yes, this is the "Nemesis" theory, which was popular in the '70s and '80s for explaining "regular" extinction events. However, the events are less "regular" than suggested by proponents of the theory, and if such a star really existed, Infrared All Sky Surveys would have detected it by now. They haven't, so it doesn't exist.
A dwarf planet and a plutoid are not mutually exclusive. A plutoid is a subset of dwarf planets that are further from the Sun than Neptune. Sedna has not yet been designated a dwarf planet or a plutoid because there is currently a debate in the IAU about the characteristics of a body for its self gravity to round it. Sedna is currently classified as a planetoid (or minor planet). However, Sedna is considered a strong candidate to become both a dwarf planet and a plutoid since a) its estimated diameter of ~1500 km is larger than the 800 km that is expected to round a rocky dwarf planet, and b) it is likely made of a significant fraction of ice which would significantly lower the diameter needed to round it. I don't expect the debate in the IAU to be resolved anytime soon, but I think Sedna will be reclassified because its characteristics overwhelmingly support the likelihood that it has enough gravity to round itself.