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content/Physics and Chemistry of Planet Formation/Planet-disk Torques.md

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Planet-disk torques are the mediators of interaction between still-forming planets carving their way in the disk and the disk material. The complete physics of these torques is not yet fully understood and non-trivial. Often 2D and two-body approximations under several further constraints are used to
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![[closest-approach.png|A body of mass $m$ passes by a second body with an impact parameter (i.e. a distance of closest approach) $b$ and a relative velocity $\sigma$. In the regime of a weak encounter the deflection angle is small and the impulse can be calculated assuming that the trajectory is unperturbed.]]
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![](closest-approach.png)
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*A body of mass $m$ passes by a second body with an impact parameter (i.e. a distance of closest approach) $b$ and a relative velocity $\sigma$. In the regime of a weak encounter the deflection angle is small and the impulse can be calculated assuming that the trajectory is unperturbed.*
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quartz.config.ts

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