In an interesting new research, astronomers have determined that dwarf spheroidal galaxies, which contain few stars relative to their total mass, are formed by indulging in a cosmic dance. Dwarf spheroidal galaxies appear to be made mostly of dark matter – a mysterious substance detectable only by its gravitational influence, which outweighs normal matter by a factor of five to one in the universe as a whole. Astronomers have found it difficult to explain the origin of dwarf spheroidal galaxies. Previous theories require that dwarf spheroidals orbit near large galaxies like the Milky Way, but this does not explain how dwarfs that have been observed in the outskirts of the “Local Group” of galaxies could have formed. “These systems are ‘elves’ of the early universe, and understanding how they formed is a principal goal of modern cosmology,” said lead author Elena D’Onghia of the Harvard-Smithsonian Center for Astrophysics (CfA). D’Onghia and her colleagues used computer simulations to examine two scenarios for the formation of dwarf spheroidals. While the first scenario features an encounter between two dwarf galaxies far from giants like the Milky Way, with the dwarf spheroidal later accreted into the Milky Way, the second scenario simulates an encounter between a dwarf galaxy and the forming Milky Way in the early universe. The team found that the galactic encounters excite a gravitational process which they term “resonant stripping,” leading to the removal of stars from the smaller dwarf over the course of the interaction and transforming it into a dwarf spheroidal. “Like in a cosmic dance, the encounter triggers a gravitational resonance that strips stars and gas from the dwarf galaxy, producing long visible tails and bridges of stars,” explained D’Onghia. “This mechanism explains the most important characteristic of dwarf spheroidals, which is that they are dark-matter dominated,” added co-author Gurtina Besla. The long streams of stars pulled off by gravitational interactions should be detectable. For example, the recently discovered bridge of stars between Leo IV and Leo V, two nearby dwarf spheroidal galaxies, may have resulted from resonant stripping.
Posts Tagged ‘Dark Matter’
How Real Science Works — A Commentary
January 27th, 2009
admin At Cern, the Large Hadron Collider could recreate conditions that last prevailed when the universe was less than a trillionth of a second old. Above is one of the collider’s massive particle detectors, called the Compact Muon Solenoid. Valerio Mezzanotti for The New York TimesFrom The American Thinker:The Large Hadron Collider is the largest collaborative scientific effort in history.
Dark Matter Filaments Stoked Star Birth In Early Galaxies
January 22nd, 2009
admin From The New Scientist:Tendrils of dark matter channelled gas deep into the hearts of some of the universe’s earliest galaxies, a new computer simulation suggests. The result could explain how some massive galaxies created vast numbers of stars without gobbling up their neighbours.Dramatic bursts of star formation are thought to occur when galaxies merge and their gas collides and heats up. Evidence of these smash-ups is fairly easy to spot, since they leave behind mangled pairs of galaxies that eventually merge, their gas settling into a bright, compact centre.Read more ….
The Strangest Things in Space
January 8th, 2009
admin Mini-Black HolesIf a radical new “braneworld” theory of gravity is correct, then scattered throughout our solar system are thousands of tiny black holes, each about the size of an atomic nucleus. Unlike their larger brethren, these mini-black holes are primordial leftovers from the Big Bang and affect space-time differently because of their close association with a fifth dimensionCosmic Microwave BackgroundAlso known as the CMB, this radiation is a primordial leftover from the Big Bang that birthed the universe.
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