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Axial parallelism (also called gyroscopic stiffness, gyroscopic inertia, gyroscopic rigidity, or "rigidity in space") is the characteristic of a rotating body in which the direction of the axis of rotation remains fixed as the object moves through space. In astronomy, this characteristic is found in astronomical bodies in orbit. It is the same effect…
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axial earth's axis parallelism orbit moon's years body direction fixed rotation also tilt around orbital 18 lunar motion called characteristic
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Axial parallelism | related to Earth's axial parallelism | The Earth's | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | Polaris | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | North Star | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | Together | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | Earth's | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | It | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | Sun | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | Minor | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | As | 0.60 | section |
| Axial parallelism | related to Earth's axial parallelism | Vega | 0.60 | section |
| Axial parallelism | related to Other astronomical examples | Axial | 0.60 | section |
| Axial parallelism | related to Other astronomical examples | For | 0.60 | section |
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