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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).
Regions, Mass transfer & Definition
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roche lobe system mass star potential binary transfer sphere gravitational l1 gravity region orbit two point equipotential debris donor one
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Roche lobe | is a | region around a star in a binary system within which orbiting material is gravitationally bound to that star | 0.90 | text |
| a W Ursae Majoris variable | instance of | the system manifests as a contact binary | 0.80 | text |
| Roche lobe | related to Definition | In | 0.60 | section |
| Roche lobe | related to Definition | The | 0.60 | section |
| Roche lobe | related to Definition | Close | 0.60 | section |
| Roche lobe | related to Definition | Far | 0.60 | section |
| Roche lobe | related to Definition | L1 Lagrangian | 0.60 | section |
| Roche lobe | related to Definition | This | 0.60 | section |
| Roche lobe | related to Definition | Roche | 0.60 | section |
| Roche lobe | related to External links | From Hot Jupiters | 0.60 | section |
| Roche lobe | related to External links | Super-Earths | 0.60 | section |
| Roche lobe | related to External links | Roche Lobe Overflow | 0.60 | section |
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