 the roche lobe is the region of space around a star in a binary system within which orbiting material is gravitationally bound to that star. if the star expands past its roche lobe, then the material can escape the gravitational pull of the star. if the star is in a binary system then the material will fall in through the inner lagrangian point. it is an approximately tear-drop shaped region bounded by a critical gravitational equipotential, with the apex of the tear-drop pointing towards the other star (and the apex is at the  lagrangian point of the system). it is different from the roche limit which is the distance at which an object held together only by gravity begins to break up due to tidal forces. it is different from the roche sphere which approximates the gravitational sphere of influence of one astronomical body in the face of perturbations from another heavier body around which it orbits. the roche lobe, roche limit and roche sphere are named after the french astronomer Ãdouard roche. ==definition of the roche lobes==  in a binary system with a circular orbit, it is often useful to describe the system in a coordinate system that rotates along with the objects. in this non-inertial frame, one must consider centrifugal force in addition to gravity. the two together can be described by a potential, so that, for example, the stellar surfaces lie along equipotential surfaces. close to each star, surfaces of equal gravitational potential are approximately spherical and concentric with the nearer star. far from the stellar system, the equipotentials are approximately ellipsoidal and elongated parallel to the axis joining the stellar centers. a critical equipotential intersects itself at the  lagrangian point of the system, forming a two-lobed figure-of-eight with one of the two stars at the center of each lobe. this critical equipotential defines the roche lobes. where matter moves relative to the co-rotating frame it will seem to be acted upon by a coriolis force. this is not derivable from the roche lobe model as the coriolis force is a non-[[conservative
Binary_stars Gravitation