Quote:
Originally Posted by Robert Tulip
As you can see I have some glaring holes in my understanding of astrophysics! At least I am eager to learn, so thank you very much for this explanation. It still leaves me wondering though, gravitysimulator.com says
"Although it is convienent to think of the Sun as the stationary anchor of our solar system, it actually moves as the planets tug on it, causing it to orbit the solar system's barycenter."
Is this right?
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Quote:
Originally Posted by tusenfem
No, technically it is not, because if the pull of the planets would influence where the sun is, why is it not displaced in the direction of maximum pull and have the barycentre at the opposite side?
S------J-------Sun--BC The planets pulling on the Sun
S------J-------BC--Sun The planets orbiting the CoM
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Since I made the statement in question, let me clarify.
The second of your two diagrams is correct. But the first one does not illustrate what I was trying to say. Even in the second of your diagrams, the planets can still pull the sun in the direction of the barycenter.
Consider the following 4 illustrations. They contain a purple planet and a yellow star orbiting a common barycenter. The star : planet mass ratio is 10:1. The barycenter is marked by the green dot.
In frame #1, the barycenter is inbetween the star and the planet as it must be, and is 10x closer to the more massive star. The star's velocity vector is to the right of the screen, and the planet's is to the left. At this instantaneous moment, the
y-component of their velocities are 0. If the star and planet didn't pull on each other, despite having mass, they would continue on these straight-line paths. There would still be a barycenter as the objects still have mass. But these objects would not orbit the barycenter. Rather, they would distance themselves from the barycenter for eternity. The barycenter would never disappear. It would always be be located between the two masses, 10x closer to the star.
But since they do pull on each other, as the planet and star distance themselves on the
x-axis, their pulls slow their
x-component velocities, and also introduce
y-component velocity: up for the star, and down for the planet. Their mutual pulls are bending their otherwise-straight line trajectories into circular orbits around the barycenter.
In frames #2-4, the velocity vectors change, as do the directions of the pulls, but the result is the same. By pulling on each other, the masses cause each other to orbit the barycenter, rather than distance themselves from it in the directions of the instantaneous velocities.
