Though the Milky Way is taking a good beating from nearby
mini-galaxies that sometimes slam into it, our galaxy is not likely to de
destroyed by this process as some scientists had predicted, a new study finds.
Circling around the
Milky Way are between 20 and 25 known satellite dwarf
galaxies, which are smaller clumps of stars bound in orbit around the Milky
Way by gravitational attraction.
Some pessimists
predicted the Milky Way was doomed to a grizzly death by dismemberment if enough
of these galaxies collide with it. In fact, scientists think many satellite
galaxies have already rammed into the Milky Way, though so far it has endured.
A new computer simulation indicates that rather than tearing
apart a galaxy, collisions with dwarf galaxies serve to puff up the host's
pancake-shaped galactic disk. Indeed, evidence of this puffiness has been found
in the form of rings and flares of stars around the edges of other galaxies'
disks.
"Our simulations showed that the satellite galaxy
impacts don't destroy spiral galaxies — they actually drive their evolution, by
producing this flared shape and creating stellar rings — spectacular rings of
stars that we've seen in many spiral galaxies in the universe," said study
leader Stelios Kazantzidis, an astronomer at Ohio State University.
Though our galaxy may not be in danger from dwarf galaxies,
astronomers do expect it to eventually collide with the nearest full-size
galaxy, Andromeda. In a few billion years, the two spirals should smash into
each other head on.
"The collision with Andromeda is a collision between
two essentially equal-mass galaxies, whereas satellite bombardment involves
encounters with much smaller systems compared to the Milky Way,"
Kazantzidis told SPACE.com.
Luckily, even that fender bender doesn't necessarily spell
the end for the galaxies' inhabitants. Stars are generally spaced wide enough
apart within the galaxies that after the merger, most individual stars should
intermingle without actually crashing into each other.
In fact, the merging will likely set off a firestorm of new
star formation, adding to the richness of the two melded galaxies.
The new simulation helps scientists understand how smaller
collisions affect a galaxy's development.
"We can't know for sure what's going to happen to the
Milky Way, but we can say that our findings apply to a broad class of galaxies
similar to our own," Kazantzidis said.
The model is the most detailed to date of collisions between
spiral galaxies and satellites. It revealed the kind of detailed features that
should result from these impacts, which align well with observed characteristics
of other galaxies seen in the universe.
"Every spiral galaxy has a complex formation and
evolutionary history," Kazantzidis said. "We would hope to understand
exactly how the Milky Way formed and how it will evolve. We may never succeed
in knowing its exact history, but we can try to learn as much as we can about
it, and other galaxies like it."
The research is detailed in two papers published in the
Astrophysical Journal in August 2009 and November 2008.
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