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In astrophysics, the Yarkovsky effect is a force acting on a rotating body in space caused by the anisotropic emission of thermal photons, which carry momentum. It is usually considered in relation to meteoroids or small asteroids (about 10 cm to 10 km in diameter), as its influence is most significant for these bodies.
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effect yarkovsky asteroid orbit asteroids radiation force body small bodies thermal axis sun direction seasonal may rotating meteoroids time object
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Yarkovsky effect | is a | force acting on a rotating body in space caused by the anisotropic emission of thermal photons | 0.90 | text |
| Yarkovsky effect | is a | consequence of the fact that change in the temperature of an object warmed by radiation | 0.90 | text |
| Yarkovsky effect | measured by | The | 0.60 | section |
| Yarkovsky effect | measured by | Golevka | 0.60 | section |
| Yarkovsky effect | measured by | Arecibo | 0.60 | section |
| Yarkovsky effect | measured by | Without | 0.60 | section |
| Yarkovsky effect | measured by | Yarkovsky | 0.60 | section |
| Yarkovsky effect | measured by | This | 0.60 | section |
| Yarkovsky effect | measured by | These | 0.60 | section |
| Yarkovsky effect | measured by | Calculations | 0.60 | section |
| Yarkovsky effect | measured by | The Yarkovsky | 0.60 | section |
| Yarkovsky effect | related to External links | Nugent | 0.60 | section |
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