Back Roche-lob Afrikaans حيز روش Arabic Lóbulu de Roche AST Повърхност на Рош Bulgarian Lòbul de Roche Catalan Roche lobe Danish Lóbulo de Roche Spanish Rocheren lobulua Basque لب روش Persian Rochen pinta Finnish
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In astronomy, the Roche lobe is the region around a star in a binary system within which orbiting material is gravitationally bound to that star. It is an approximately teardrop-shaped region bounded by a critical gravitational equipotential, with the apex of the teardrop pointing towards the other star (the apex is at the L1 Lagrangian point of the system).
The Roche lobe is different from the Roche sphere, which approximates the gravitational sphere of influence of one astronomical body in the face of perturbations from a more massive body around which it orbits. It is also 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. The Roche lobe, Roche limit, and Roche sphere are named after the French astronomer Édouard Roche.