Dark Matter Simulation in Milky Way Halo

Dark Matter Simulation in Milky Way Halo

Download Options

Fast Facts
News release ID: STScI-2012-26
Release Date: Jul 10, 2012
Image Use: Copyright
About this image

These illustrations, taken from computer simulations, show a swarm of dark matter clumps around our Milky Way galaxy. Some of the dark-matter concentrations are massive enough to spark star formation. Dark matter is an invisible substance that accounts for most of the universe's mass.

In the first panel, thousands of clumps of dark matter coexist with our Milky Way galaxy, shown in the center.

The green blobs in the second panel are those dark-matter chunks massive enough to obtain gas from the intergalactic medium and trigger ongoing star formation, eventually creating dwarf galaxies.

In the third panel, the red blobs are ultra-faint dwarf galaxies that stopped forming stars long ago. New Hubble Space Telescope observations of three of the puny galaxies reveal that star-making in these faint galaxies shut down more than 13 billion years ago.

The synchronized shutdown is evidence that a global event, such as reionization, swept through the early universe. Reionization is a transitional phase in the early universe when the first stars burned off a fog of cold hydrogen.

Popular theory predicts that most of the Milky Way's satellites contain few, if any, stars and are instead dominated by dark matter. More than a dozen small-fry galaxies have been found so far, all by the Sloan Digital Sky Survey, which scanned just a quarter of the sky.

Dark Matter, Dwarf Galaxies, Galaxies, Infographics


NASA, ESA, and T. Brown and J. Tumlinson (STScI)