...provide fresh insights into how planets might evolve within a binary star system. Presenting their results at the recent AAAS meeting ... cloud may be the result of gravitational forces unique to binary stars and may also be the key to the formation of ...
... system is as follows: There are two binary stars (a star binary is a system of two stars orbiting around a common centre of mass). One of the binaries also features a so-called contact binary, i.e. a kind of “lone companion.” According to Dr. Lohr...
... non-zero eccentricity of the planet orbits, are qualitatively consistent with formation by a strong encounter with singular or binary stars, thus ruling out other theories such as an excess due to high metallicity or high stellar masses. This could...
... and launch it in 2009. And even when we launched, there were skeptics predicting that we would find eclipsing binary stars but very few planets. What has surprised all of us is the huge incidence of compact multiple planet systems...
... to aid in its own accretion processes. Accordingly, this limits the amount of material left to build planets. Solitary stars or binary stars whose companions are much further away (> 100 AU) thus have a higher fraction of discs surrounding them. Not...
... found to date; a finding which challenges assumptions about which stars can host planets. Located approximately 325 light-years away in the constellation Centaurus, b Centauri is a young binary star system that has at least six times the mass...