Astrowiki/Nemesis
From BluWiki
|
This Page is Part of Astrowiki
Contributions wanted. - BluWiki is unique in that original page authors normally decide who can edit their page. By putting this banner up, the author(s) of this page are soliciting your assistance. Please help them by contributing useful information to it. You might find more information about what is wanted in the discussion of this page.
|
Nemesis is a hypothetical brown or red dwarf star that orbits the sun at 50,000 to 100,000 AU. The predicted orbit of such a star could explain the periodicity in the rate of mass extinctions beacuse it would disrupt the orbit of objects in the oort cloud and send them twards the planets every 26 million years.The Nemesis hypothese could also explain the observations that predict Planet X .







