Missing Milky Way dark matter

November 9, 2010 By Jon Voisey, Universe Today
A composite image shows a dark matter disk in red. From images in the Two Micron All Sky Survey. Credit: Credit: J. Read & O. Agertz.

Although dark matter is inherently difficult to observe, an understanding of its properties (even if not its nature) allows astronomers to predict where its effects should be felt. The current understanding is that dark matter helped form the first galaxies by providing gravitational scaffolding in the early universe. These galaxies were small and collapsed to form the larger galaxies we see today. As galaxies grew large enough to shred incoming satellites and their dark matter, much of the dark matter should have been deposited in a flat structure in spiral galaxies which would allow such galaxies to form dark components similar to the disk and halo. However, a new study aimed at detecting the Milky Way‘s dark disk have come up empty.

The study concentrated on detecting the by studying the luminous matter embedded in it in much the same way dark matter was originally discovered. By studying the kinematics of the matter, it would allow astronomers to determine the overall mass present that would dictate the movement. That observed mass could then be compared to the amount of mass predicted of both baryonic matter as well as the dark matter component.

The team, led by C. Moni Bidin used ~300 red giant in the ‘s thick disk to map the mass distribution of the region. To eliminate any contamination from the thin disc component, the team limited their selections to stars over 2 kiloparsecs from the galactic midplane and velocities characteristic of such stars to avoid contamination from stars. Once stars were selected, the team analyzed the overall velocity of the stars as a function of distance from the galactic center which would give an understanding of the mass interior to their orbits.

Using estimations on the mass from the visible stars and the interstellar medium, the team compared this visible mass to the solution for mass from the observations of the kinematics to search for a discrepancy indicative of dark matter. When the comparison was made, the team discovered that, “[t]he agreement between the visible mass and our dynamical solution is striking, and there is no need to invoke any dark component.”

While this finding doesn’t rule out the presence of dark matter, it does place constraints on it distribution and, if confirmed in other , may challenge the understanding of how dark matter serves to form galaxies. If dark matter is still present, this study has demonstrated that it is more diffuse than previously recognized or perhaps the disc component is flatter than previously expected and limited to the thin disc. Further observations and modeling will undoubtedly be necessary.

Yet while the research may show a lack of our understanding of dark matter, the team also notes that it is even more devastating for dark matter’s largest rival. While dark matter may yet hide within the error bars in this study, the findings directly contradict the predictions of Modified Newtonian Dynamics (MOND). This hypothesis predicts the apparent gain of mass due to a scaling effect on gravity itself and would have required that the supposed mass at the scales observed be 60% higher than indicated by this study.

Explore further: Hubble provides new evidence for dark matter around small galaxies

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1 / 5 (4) Nov 09, 2010
.. i already goth away, milky my website ...
4 / 5 (4) Nov 09, 2010
Fascinating. The explanation of the formation of spiral galaxies and their components present orbits is one of the most interesting questions of astronomy.
1 / 5 (3) Nov 09, 2010
much of the dark matter should have been deposited in a flat structure in spiral galaxies

....if it behaves like normal matter. It doesn't and here's why.

5 / 5 (2) Nov 09, 2010
"...much the same way dark matter was originally discovered"

Perhaps my understanding of the word "discovered" is off... but doesn't that imply that dark matter definitely exists? I didn't realize we'd gotten that far yet
not rated yet Nov 09, 2010
Shouldn't a star's velocity around the center of a galaxy increase the further it is from the center? Wouldn't a
star's galactic weight decrease toward the center until its galactic weight would be zero at the very center?
3 / 5 (2) Nov 10, 2010
depends what you mean by galactic weight. I would think that the mass of a galaxy is pretty much the same thing as the weight of a galaxy.

But galactic gravity would decrease towards the center of mass except that a large part of the mass may well be at the center already.

Good to see this study actually test MOND and still come up short on dark matter, indicating that both are probably wrong.
1 / 5 (3) Nov 10, 2010
This result is somewhat strange, because Milky Way is already considered heavier than the two times larger Andromeda Galaxy - just because of its high content of dark matter.


If it's true, then the older galaxies should have relatively larger content of dark matter, formed with neutrinos and positrons, evaporated from it during their evolution.

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