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Looking High and Very Low -
Quest for the Origins of Life
Rivers of molten rock and oceans of sulfurous boiling water. Intense solar
radiation and a constant hail of comets and asteroids. This was the picture when
life on Earth-the only life in the universe that we know of-sparked into existence
approximately 3.8 billion years ago.
It seems surprising that life could flourish, let alone take hold, in such
an environment. Generally, we imagine that water, air, and sunlight, along with
a "livable" climate, are the prerequisites for life. While that may
be true for most animals bigger than a bread box, scientists are finding that
life, at least among smaller organisms, can sustain itself in conditions never
before thought possible.
Part of NASAs mission is to investigate the presence of life in the universe.
How did life begin on Earth? Can it happen on other planets or in different ways?
Studying the extremes of life on Earth and the building blocks of life present
elsewhere in the solar system brings us closer to understanding how and why life
can come into being. 
Taking It to the Extreme
In the late 1970s, oceanographers discovered the first communities living
around geothermal vents on the ocean floor. Beyond the reach of the sun and under
incredible water pressure, these tiny ecosystems thrive without photosynthesis,
previously thought to be the energy source for all life on Earth. The entire food
chain of these communities, from microorganisms to animals, is based on microbes
that produce energy through chemical reactions with minerals spewed from beneath
the ocean floor by the vents.
Since that first discovery, scientists have tracked down other microbes and
larger organisms in a variety of extreme environments, often where minerals and
water provide the sole energy sources. These tough little life forms live, for
example, on the bottom of perpetually frozen Antarctic lakes, in acid lakes, and
in pools on cave floors that have seen no sunlight for millions of years.
Many microorganisms have found a home more than a mile below the Earths
surface, where temperatures can exceed 150°C. In fact, some now estimate that
microbial life hidden sub-surface may compose at least half of the Earths
biomass, giving newfound importance to the lives of these poorly understood organisms.

Our comprehension of the extremes life can tolerate is continually expanding.
Microbes found in the undersea Japan Trench, nearly 20,000 feet deep, live under
water pressures of up to several million tons per square inch. Certain lichens
and bacteria can survive at -45°C, a temperature where any surface water,
along with most water-based organisms, would turn to ice. Many organisms adapted
to extreme environments have no need for oxygen, and may even find it poisonous.
The tenacity of microscopic life has led some scientists to suggest an alternative
origin for life on Earth. If the surface world of 3.8 billion years ago was too
hostile to support the sunlight-fueled primordial soup of traditional theory,
perhaps it formed beneath the crust, where water, geothermal energy and organic
compounds were in abundance. 
Could It Happen Anywhere?
The discovery of life on Earth in what were previously unthinkable environments
has opened up new concepts for life on other planets. If Earth possesses a sub-surface
biosphere, other planets may as well. Liquid water, still considered a prerequisite
for life as we know it, may exist or have existed on several planets and moons
in our solar system. While this liquid water would be or have been present in
distinctly un-Earth-like environments, they can no longer be dismissed out of
hand as unsuitable for life.
If liquid exists below Europa's frozen surface, this satellite of Jupiter
may have the potential to harbor life.
The Jovian moon Europa is thought to have surface ice, organic molecules, and
a constant internal energy supply. If water exists below the surface, as is suggested
by that moons cracked and frosty outer layer, the circumstances could be
sufficient to sustain life. The living evidence found in sub-freezing Earth environments
brings the idea within the realm of possibility. 
Titan, a satellite of Saturn, has the potential to answer many questions about
the formation of the building blocks of life. Apart from Earth, it is the only
other planetary body in the solar system with a significant atmosphere composed
primarily of nitrogen. Too cold to harbor liquid water, it is nevertheless a factory
for organic compounds. More than a dozen have been identified. The base compounds
that form DNA have been detected in meteorites. Observing organic evolution in
process on Titan may give us a clue as to how these compounds were first formed
and ejected into space.
Titans example begs the question of whether life can spring from a biochemistry
different from our own. Is water the only medium that can support life? Must DNA
be the genetic code? To be considered alive, a thing must meet two criteria: it
must carry the information necessary for reproduction and it must posses the ability
to evolve. This definition puts no limits on the materials from which life is
made. Still, we have only the one example of life here on Earth.
What are the origins of life? In piecing together this most fundamental of
puzzles, scientists will continue to send probes under the Earths crust,
into the oceans depths, and out across the solar system. Along the way,
we are discovering as much about our own world as we are about our celestial neighbors.
And, after all, as we scan the universe for evidence of life, we have to be sure
that we know it when we see it. 

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Studying our solar system helps us understand the origins of
life, just as studying life on Earth helps us understand the potential for life
to exist elsewhere.

If liquid exists below Europa's frozen surface, this satellite
of Jupiter may have the potential to harbor life.
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