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In astrodynamics or celestial mechanics a parabolic trajectory is a Kepler orbit with the eccentricity (e) equal to 1 and is an unbound orbit that is exactly on the border between elliptical and hyperbolic. When moving away from the source it is called an escape orbit, otherwise a capture orbit. It is also sometimes referred to as a C 3 = 0…
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trajectory parabolic orbit velocity displaystyle body escape standard central radial hyperbolic energy orbiting mu gravitational parameter equation also orbital distance
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Parabolic trajectory | is a | Kepler orbit with the eccentricity | 0.90 | text |
| Parabolic trajectory | is a | non-periodic trajectory on a straight line where the relative velocity of the two objects is always the escape velocity | 0.90 | text |
| Parabolic trajectory | related to Barker's equation | Barker's | 0.60 | section |
| Parabolic trajectory | related to Energy | Under | 0.60 | section |
| Parabolic trajectory | related to history | In | 0.60 | section |
| Parabolic trajectory | related to history | Galileo | 0.60 | section |
| Parabolic trajectory | related to history | MS | 0.60 | section |
| Parabolic trajectory | related to history | Gal | 0.60 | section |
| Parabolic trajectory | related to history | Discorsi | 0.60 | section |
| Parabolic trajectory | related to Radial parabolic trajectory | There | 0.60 | section |
| Parabolic trajectory | related to Velocity | The | 0.60 | section |
These clusters group vocabulary that occurs around closely connected concepts in the source material.
Bridges can reveal useful research angles that are easy to miss in a flat list of related terms.