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Dark Matter: Now More Mysterious Than Ever
By Adam Mann October 17, 2011 | 2:47 pm | Categories: Space
Astronomers have one more reason to scratch their heads over the unseen material known as dark matter. Observations of two dwarf galaxies, Fornax and Sculptor, show the dark matter within them is spread out smoothly rather than heaped into a central bulge, contradicting cosmological models.
Researchers know dark matter comprises a far greater percentage of the universe than the ordinary matter making up things like people and stars. Because of this, the distribution of dark matter determines the structure of the cosmos. Galaxies form when they are attracted to and anchored by large clumps of dark matter.
The dwarf galaxies Fornax and Sculptor are themselves made of 99 percent dark matter and only 1 percent normal matter. It is impossible to directly see the dark matter but, by observing the rotation of stars around each galactic center, researchers can detect its influence and map out its distribution.
While dark matter neither emits or scatters light, its existence can derived only from the gravitational effects on visible matter.
"After completing this study, we know less about dark matter than we did before," the study's lead author Matt Walker, a Hubble Fellow at the Harvard-Smithsonian Center for Astrophysics, said.
"Stars in a dwarf galaxy swarm like bees in a beehive instead of moving in nice, circular orbits like a spiral galaxy," said Peñarrubia.
"That makes it much more challenging to determine the distribution of dark matter." The new measurements suggest two options: normal matter impacts dark matter more severely than previously thought, or dark matter is not "cold," or slow-moving, as widely accepted today.
Originally posted by greenCo
Oh.. Boncho is really a scientist.
Good post!