With
all the changes happening in the sciences lately, it is no small wonder that
astronomers are beginning to re-think the “big picture” in their theories. For
centuries, humans have wondered about the possibility of life elsewhere in the
universe, and since the advancement of space technology, the hunt has become
ever more insistent. Yet, with each little hint of the possibility of life, one
or more factors always seem to be missing. Some astronomers are now beginning
to reformulate their search plans and not look just for other solar systems
elsewhere, but try to determine if there are specific areas throughout our
galaxy that are more life-friendly.
In
every solar system, depending on the class of the central star(s), there is a
certain distance away from the center that is the most temperate area for
supporting life as we know it. This zone is usually referred to by astronomers
as the life zone, “habitable zone,” or even the “Goldilocks zone,” because it
is not too hot or too cold. For instance, in our solar system, Mercury and
Venus are much closer to our own sun, and as such experience much higher
average temperatures year-round. Jupiter, Saturn, Uranus, and Neptune are all
much, much further away from the sun than Earth, and are all much colder.
Astronomers are still very hopeful about the possibility of life on Mars.
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Image credit: NASA/JPL-Caltech/ESA/CXC/STScI. |
So, if there is a specific life
zone in every solar system, does the same rule apply for galaxies? Some
astronomers are beginning to believe so, arguing that the centers of galaxies
tend to be much more metal-heavy, which is much more conducive to planetary
formation, so the odds are in favor of a planet forming with life on it. The
flipside of the argument, however, is that the centers of galaxies also tend to
be home to more supernovae. While all the constant light would be annoying, any
life on planets in the galactic center would have to worry about much more
serious problems like ozone depletion and literally having the planet fried by
all manner of ray emissions from the multitude of stars. For now, the
researchers will continue to scan the center of our own galaxy (pictured here)
for more evidence and see how their theories unfold.
Credit:
SPACE.com.
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