The Formation of Galaxies
Theoretical investigations indicate that galaxies formed from a diluted
but lumpy mixture of hydrogen and helium gas - the primordial elements
forged in the Big Bang. They also indicate that two vastly different
scales of mass prevailed less than 100 million years after the Big
Bang, which ultimately affected the formation of galaxies. (See the
later discussion of dark matter and the
formation of structure.)
Two Scales of Matter
Matter either was clumped into vast collections more than a million
times the mass of the Milky Way, or into small clumps one million times
smaller than the mass of our Milky Way. Superclusters of galaxies may
have evolved from the former.
Globular clusters such as
M15 in the adjacent image
may have evolved from the
latter.
Results from Recent Observations
As we look deeper into the Universe
and therefore
back in time, galaxies appear to emit
more of their light in the
blue part of the visible spectrum.
This blue light is a sign that very young,
massive and luminous stars are forming
(see the discussion of the
spiral arms in spiral galaxies,for example).
Since we see these galaxies as
they were between 5 and 10 billion years ago, we appear to be
witnessing events that occurred within a few billion years after these
galaxies were formed.
Astronomers also have noticed that as they examine the images of these
distant blue galaxies, the images are frequently distorted or contain
what appear to be multiple nuclei. The Milky Way seen at a similar
great distance would look like a uniformed flattened disk, with a
single bright nucleus -- the galactic center. Nearby
"multiple-nuclei" galaxies that have been studied show the cores of
individual galaxies colliding and merging into one single system of
stars and gas. These collisions are violent, and take millions of
years to play out. But in at least some instances, such as NGC 1275,
recently observed with the Hubble Space Telescope, galaxy collisions
can actually
trigger the formation of massive stars.
Cosmic Cannibalism
In the depths of space, we may be witnessing collisions between smaller
galaxies triggering
the formation of massive luminous stars.
The
images, rich in blue light, gives tantalizing evidence that
"environment" may have been more important than cosmic "genetics."
Galactic cannibalism was far more common in the ancient past. Galaxies
may have grown to their current size by consuming their neighbors. The
ultimate building blocks may indeed have been the paltry
million-solar-mass clumps that theoreticians believe were abundant
before the Universe was a few million years old.
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