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Stellar rotation is the angular motion of a star about its axis. The rate of rotation can be measured from the spectrum of the star, or by timing the movements of active features on the surface.
Measurement, Degenerate stars & Physical effects
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star rotation angular velocity stars rate mass magnetic momentum stellar field equator rotational result wind rotating also equatorial however gravitational
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Stellar rotation | is a | angular motion of a star about its axis | 0.90 | text |
| starspots | instance of | The more detailed information gathered by this means allows the effects of microturbulence to be distinguished from rotation.If a star displays magnetic surface activity | 0.80 | text |
| then these features can be tracked to estimate the rotation rate | instance of | The more detailed information gathered by this means allows the effects of microturbulence to be distinguished from rotation.If a star displays magnetic surface activity | 0.80 | text |
| the Sun when the angular velocity varies with latitude | instance of | For a star to be stable the rotational velocity must be below this value.Differential rotationSurface differential rotation is observed on stars | 0.80 | text |
| the Sun when the angular velocity varies with latitude | instance of | Differential rotationSurface differential rotation is observed on stars | 0.80 | text |
| the T6 brown dwarf WISEPC J112254.73 | instance of | the discovery of rapidly rotating brown dwarfs | 0.80 | text |
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