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Verifying
On 11/11/2017 9:50 PM, jacobnavia wrote:
Le 10/11/2017 à 08:10, Jos Bergervoet a écrit : We know what the rotation curves are, so the acceleration of stars on average is known, and it is known that this does not fit with the gravity of known matter in the galaxies. So you do not need the observations as you describe here to get this information. What we do *not* know is: 1) Is there more matter than the known matter, so stronger gravity and therefore restoring agreement with the movement? That would be a nice solution. And if space between the stars wasn't empty but filled with some kind of very thin gas? Yes, but then this gas would have to be undiscovered until now for some reason. Which means it has to consist of things we can't easily see, e.g. particles like axions or sterile neutrinos. It can also be a collection of massive, as of yet undiscovered, black holes. Actually they are now starting to be discovered by LIGO. But you'd still need quite a lot of them to have enough extra mass.. 2) Is there another force that adds to the effect of gravity so together they give agreement with the motion? The first possibility leads to the hunt for dark matter, the second to the search for a "fifth force" Dark matter was supposed to be in some kind of "halo" outside the galaxy. No, dark matter is supposed to form a cloud with the galaxy immersed in it. Probably densest in the galaxy itself but also extending to some region (halo) outside the galaxy. The stars then, are pulled by the outside. No they are not! Whatever the distribution in the radial direction, gravity *always pulls inwards*, except if the distribution is completely confined to a shell, in which case in the empty inner region it gives gravity zero, but is *still* not pulling outwards! (Do your 1/r^2 exercises again, for a distributed mass with spherically symmetric distribution, only a function of r.) A fifth force would have a vector centered in the center of the milky way. Yes, if it is to explain the rotation curves. But a cloud of dark matter would also pull inwards. Is it possible then, to figure out this from the orbit of a known star, say, the sun? No, a fifth force or a cloud of unseen mass will both give more inward attraction (to the galactic center) for this star, you can't see the difference. The observations with telescopes as discussed above will not help with these questions at all, they will just reproduce the already observed disagreement between motion and the gravity of known matter. Which then leaves us again with the same two questions. A fifth force would perturb the orbit of the sun in a different way than matter in a halo. No, as proposed solutions for the motion of the stars, both these things of course are supposed to influence the orbits of the stars in the same way (giving them more inward acceleration). Besides, even if it is weak it has been there since eons. After all this time (age of the sun around 5GY) some perturbation should be observable. Of course. The whole structure of the universe (zooming in from the largest levels) would have to agree with any new force, or new kind of matter we introduce! It looks like this: http://www.atlasoftheuniverse.com/universe.html Shouldn't an analysis of the orbit of the sun give an answer to that? [[Mod. note -- Interstellar space is indeed filled with a "very thin gas": https://en.wikipedia.org/wiki/Interstellar_medium https://en.wikipedia.org/wiki/Intracluster_medium This is already included in counts of "known matter". -- jt]] And it should not only be in agreement with the orbit of the sun, but with all galaxies, clusters, filaments, voids, and anything else we observe in the universe. -- Jos |
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