Flat rotation curves were the first clear evidence that the dynamics of galaxies do not follow the same rules as planetary systems. But they do follow rules. These include asymptotic flatness, Tully-Fisher, the luminosity-size-rotation curve shape relation (aka the `universal‘ rotation curve), Renzo’s rule, and the central density relation.

These various relations sound like a hodge-podge of random astronomical effects. This is misleading. There is a great deal of organization in the data. The surface density of stars and gas, and the acceleration (gbar) determined by their gravitational potential, plays a defining role. Indeed, the known relations are all manifestations of a single, more fundamental relation, the radial acceleration relation.

The radial acceleration relation connects what you see in galaxies with what you get for the gravitational force. This would be a trivial statement if galaxies behave as planetary systems do. They would follow the 1:1 dotted line in the figure. Instead, they bend away from that line.
Indeed, the data are consistent with a single effective force law, which can be written
Other functional forms could also work. But they would all necessarily have a critical acceleration scale g† ≈ 10-10 m s-2. This is an important scale that is ubiquitous in extragalactic astronomy. It seems to be a new fundamental scale in physics.
The critical acceleration marks the onset of the missing mass problem. Above this scale, there is no need for dark matter. Below it, the difference between the 1:1 line and the data is what we attribute to dark matter. The more the observed acceleration exceeds that which can be explained by the stars and gas, the larger the mass discrepancy.
Irrespective of interpretation, the data establish the radial acceleration relation in a purely empirical way. There is nothing but data here. The axes are independent: one is measured from rotation curves, the other from photometry. These need not be well connected – the dark matter could cause any sort of acceleration independently of the stars and gas. But they are intimately coupled.
There are no deviations from the radial acceleration relation beyond those attributable to experimental error. The residuals do not correlate with mass, size, surface brightness, color, environment, how many intelligent civilizations a galaxy hosts, or anything else. The scale that matters is not luminosity or halo mass or size. It is the acceleration determined from the surface density of stars and gas.
The radial acceleration relation is a fundamental relation. In effect, it is a law of nature. Third in our counting, but first in importance, as both flat rotation curves and the Tully-Fisher relation follow from it. It must be explained by any theory that claims to provide a satisfactory description of galaxy dynamics.
Thank you for such a clear and concise summary of your recent paper. This is an important issue in the debate regarding the so-called “missing matter” and this summary, as well as your paper, will provide an excellent starting point for a serious and learned discussion on how to address this matter and to determine, what, if anything, really is “missing”.
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Congratulations Stacy and co-authors on your article. I thought it was cleverly neutral, yet fair to MOND (“Indeed, our results were anticipated over three decades ago by MOND”). I’m surprised at Milgrom’s reaction, claiming that the paper “involves no conceptually new insight, or a newly discovered relation”. The conceptual neutrality was deliberate, as far as i can tell. And as for novelty, well even if one had anticipated the relation (although, was it predicted in its actual form ?), it’s another matter to have it confirmed in the data. So, unless others had observed the relation before, that is a discovery.
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Thanks. Yes, indeed, we were trying to be neutral. Just the facts. The novel thing here is the near-IR data. These give such a direct mapping to stellar mass, the relation just falls out.
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Hi, there. Where could I download the data to play with different functional forms for the fit?
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The data are on-line at the SPARC webspage: http://astroweb.case.edu/SPARC/
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