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A contact binary is a small Solar System body, such as a minor planet or comet, that is composed of two bodies that have gravitated toward each other until they touch, resulting in a bilobated, peanut-like overall shape. Contact binaries are distinct from true binary systems such as binary asteroids where both components are separated. The term is also…
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| binary asteroids where both components are separated | instance of | Contact binaries are distinct from true binary systems | 0.80 | text |
| 69230 Hermes are plausible sources for contact binaries in the NEA population | instance of | effect.High-mass ratio and doubly-synchronous binary systems | 0.80 | text |
| since they are subject to the binary YORP effect | instance of | effect.High-mass ratio and doubly-synchronous binary systems | 0.80 | text |
| which acts over timescales of 1 | instance of | effect.High-mass ratio and doubly-synchronous binary systems | 0.80 | text |
| 000 | instance of | effect.High-mass ratio and doubly-synchronous binary systems | 0.80 | text |
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