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2Physics Quote:
"Stars with a mass of more than about 8 times the solar mass usually end in a supernova explosion. Before and during this explosion new elements, stable and radioactive, are formed by nuclear reactions and a large fraction of their mass is ejected with high velocities into the surrounding space. Most of the new elements are in the mass range until Fe, because there the nuclear binding energies are the largest. If such an explosion happens close to the sun it can be expected that part of the debris might enter the solar system and therefore should leave a signature on the planets and their moons." -- Thomas Faestermann, Gunther Korschinek (Read Full Article: "Recent Supernova Debris on the Moon" )

Monday, January 08, 2007

3-D Map of Dark Matter

3-dimensional distribution of dark matter in current universe (image courtsey: HubbleSite.org)

Dark matter is an invisible form of matter that accounts for most of the universe's mass, but that so far has eluded direct detection, or even a definitive explanation for its makeup [See our past posting on the evidence of the existence of dark matter].

Now, an international team of astronomers, using NASA's Hubble Space Telescope, has created a comprehensive 3-dimensional map that offers a first look at the weblike large-scale distribution of dark matter in the universe. The map provides the best evidence yet that normal matter, largely in the form of galaxies, accumulates along the densest concentrations of dark matter. The map reveals a loose network of filaments that grew over time and intersect in massive structures at the locations of clusters of galaxies.

Researchers created the map using Hubble's largest survey of the universe, the Cosmic Evolution Survey ("COSMOS") with an international team of 70 astronomers led by Nick Scoville of California Institute of technology. In making the COSMOS survey, Hubble photographed 575 slightly overlapping views of the universe using the Advanced Camera for Surveys' (ACS) Wide Field Camera onboard Hubble. The survey covers a sufficiently wide area of sky allowing for the large-scale filamentary structure of dark matter to be evident. To add 3-D distance information, the Hubble observations were combined with multicolor data from powerful ground-based telescopes.

Almost all current scientific knowledge of the universe is related to only baryonic matter or the normal form of matter that we are familiar with. Now that scientists have begun to map out where dark matter is and how they are distributed alongside the baryonic matter, the next challenge is to determine what it is, and specifically its relationship to normal matter. This 3-D information is thus vital to studying the evolution of the structures of the distribution of matter over cosmic time.

The research results were presented at the 209th meeting of the American Astronomical Society in Seattle, Washington and also appeared online in the journal Nature yesterday.



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