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In celestial mechanics, an orbit is the curved trajectory of an object under the influence of an attracting force. Alternatively, it is known as an orbital revolution, because it is a rotation around an axis external to the moving body. Examples for orbits include the trajectory of a planet around a star, a natural satellite around a planet, or an…
History, Planetary orbits & Newton's laws
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orbits orbital body object bodies gravity gravitational motion energy time point planet sun mass force planets system period around law
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Orbit | is a | curved trajectory of an object under the influence of an attracting force | 0.90 | text |
| Orbit | is a | special case | 0.90 | text |
| a planet | instance of | or an artificial satellite around an object or position in space | 0.80 | text |
| moon | instance of | or an artificial satellite around an object or position in space | 0.80 | text |
| asteroid | instance of | or an artificial satellite around an object or position in space | 0.80 | text |
| or Lagrange point | instance of | or an artificial satellite around an object or position in space | 0.80 | text |
| or Lagrange point.For most situations | instance of | or an artificial satellite around an object or position in space | 0.80 | text |
| orbital motion is adequately approximated by Newtonian mechanics | instance of | or an artificial satellite around an object or position in space | 0.80 | text |
| which explains gravity as a force obeying an inverse-square law | instance of | or an artificial satellite around an object or position in space | 0.80 | text |
| deferent | instance of | theoretical mechanisms | 0.80 | text |
| epicycles were added by Ptolemy | instance of | theoretical mechanisms | 0.80 | text |
| a star | instance of | The adjustments needed to accommodate the theory of relativity become appreciable in cases where the object is in the proximity of a significant gravitational source | 0.80 | text |
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