User:Mark Widmer/sandbox: Difference between revisions
imported>Mark Widmer (→Hill sphere of the Sun: Working on potential new section "Hill sphere of the Sun" (in progress)) |
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It is reasonable to consider two phenomena that could determine the Sun's Hill radius. One is the effect of the galaxy as a whole, as the Sun orbits the galactic center every xxx years. However, the distribution of the matter in the galaxy is such that the net gravitational force on the Sun is not inversely proportional to the distance from the galaxy's center. An inverse-square dependence is assumed in deriving the above formulas for the Hill radius. | It is reasonable to consider two phenomena that could determine the Sun's Hill radius. One is the effect of the galaxy as a whole, as the Sun orbits the galactic center every xxx years. However, the distribution of the matter in the galaxy is such that the net gravitational force on the Sun is not inversely proportional to the distance from the galaxy's center. An inverse-square dependence is assumed in deriving the above formulas for the Hill radius. | ||
Rather than considering the effect of the galaxy as a whole on objects orbiting the Sun, one can consider the effect of individual stars. In particular, that of the nearby Alpha Centauri star system. However, as the Sun and Alpha Centauri are not in bound orbits about each other, the earlier Hill radius formulas do not apply. | |||
In the absence of a simple calculation, one can use the farthest distance to objects known to orbit the Sun to at least get a minimum value for the Hill radius. | |||
==Hill sphere of objects that orbit Earth== | ==Hill sphere of objects that orbit Earth== | ||
Revision as of 20:13, 18 August 2021
Sandbox. Mark Widmer (talk) 01:17, 5 August 2021 (UTC)
Draft for additions to Hill_sphere New sections:
Hill sphere of the Sun
The formulas listed earlier are not applicable to calculating a Hill radius for the Sun, even though the Sun must have a Hill sphere owing to the presence of other stars in the galaxy that will significantly perturb the orbit of any object that is far enough away.
It is reasonable to consider two phenomena that could determine the Sun's Hill radius. One is the effect of the galaxy as a whole, as the Sun orbits the galactic center every xxx years. However, the distribution of the matter in the galaxy is such that the net gravitational force on the Sun is not inversely proportional to the distance from the galaxy's center. An inverse-square dependence is assumed in deriving the above formulas for the Hill radius.
Rather than considering the effect of the galaxy as a whole on objects orbiting the Sun, one can consider the effect of individual stars. In particular, that of the nearby Alpha Centauri star system. However, as the Sun and Alpha Centauri are not in bound orbits about each other, the earlier Hill radius formulas do not apply.
In the absence of a simple calculation, one can use the farthest distance to objects known to orbit the Sun to at least get a minimum value for the Hill radius.
Hill sphere of objects that orbit Earth
The Moon -- added to article
Artificial satellites in low-Earth orbit -- added to article