User:Mark Widmer/sandbox: Difference between revisions

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imported>Mark Widmer
(Creating page. Possible edit to add to Hill_sphere article.)
 
imported>Mark Widmer
(Hill sphere -- revised possible edit)
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Possible text to add to [[Hill_sphere]] page: NEED TO DOUBLE-CHECK this, as it seems counter-intuitive and ''may be wrong''.
Possible text to add to [[Hill_sphere]] page: NEED TO DOUBLE-CHECK this, as it seems counter-intuitive and ''may be wrong''.


The Hill radius is ''not'' simply the distance at which the gravitational forces exerted on the satellite by the star and by the planet are equal, but is in fact larger than this distance by an additional factor of <math> \left( \frac{M}{9m} \right) ^{1/6} </math>. (The assumption here is that the planet's mass is significantly smaller than that of the star.) This works out to roughly a factor of 6 in the case of Earth and the Sun.
https://en.citizendium.org/wiki/Hill_sphere
 
The Hill radius is ''not'' simply the distance at which the gravitational forces exerted on the satellite by the star and by the planet are equal, but is in fact generally larger than this distance by an additional factor of <math> \left( \frac{M}{9m} \right) ^{1/6} </math>. This works out to roughly a factor of 6 in the case of Earth and the Sun.
 
So long as the planet's mass is less than 1/9 of that of the star. If ''m''&nbsp>&nbsp''M''/9, then the Hill radius will be smaller than the equal-force distance from the planet, but this is rarely the case. Even in the case of Jupiter, ''m'' is about ''M''/1000, well below ''M''/9.

Revision as of 18:55, 3 August 2021

Possible text to add to Hill_sphere page: NEED TO DOUBLE-CHECK this, as it seems counter-intuitive and may be wrong.

https://en.citizendium.org/wiki/Hill_sphere

The Hill radius is not simply the distance at which the gravitational forces exerted on the satellite by the star and by the planet are equal, but is in fact generally larger than this distance by an additional factor of . This works out to roughly a factor of 6 in the case of Earth and the Sun.

So long as the planet's mass is less than 1/9 of that of the star. If m&nbsp>&nbspM/9, then the Hill radius will be smaller than the equal-force distance from the planet, but this is rarely the case. Even in the case of Jupiter, m is about M/1000, well below M/9.