Encyclopedia of Evolution.pdf - Online Reading Center
Encyclopedia of Evolution.pdf - Online Reading Center
Encyclopedia of Evolution.pdf - Online Reading Center
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• Chemical composition <strong>of</strong> the Earth. Most known planets from other<br />
solar systems are gaseous. But if the solid planets were like many<br />
asteroids, which have a great deal <strong>of</strong> carbon and water, then the<br />
Earth would have either a massive greenhouse effect from carbon<br />
dioxide, or would have been completely covered with deep<br />
oceans, not having the shallow waters that appear necessary for<br />
the evolution <strong>of</strong> life.<br />
• Size <strong>of</strong> the Earth. If the Earth had been a little smaller, it would<br />
by now have completely cooled and lost its magnetic field. This<br />
would have allowed cosmic radiation to rip away the atmosphere<br />
and water and life. This appears to be what happened<br />
on Mars. On a larger planet, gravitation would be so strong that<br />
complex life might not be possible. On a larger planet, all geological<br />
forms might collapse underneath an ocean; not only would<br />
there be no terrestrial life but also no erosion <strong>of</strong> nutrients into<br />
the ocean. As a result, the entire ocean would be nutrient-poor,<br />
just as the middle <strong>of</strong> the oceans on Earth is today.<br />
• Habitable zone <strong>of</strong> the solar system. Within the solar system, Earth<br />
is in just the right place, the only planet in the habitable zone. If<br />
the Earth were one percent further away from the sun, it would<br />
experience a runaway ice age; if it were five percent closer, it<br />
would experience a runaway greenhouse effect, sometime during<br />
its history. If the Earth were closer to a smaller star, the star’s<br />
gravity would hold the Earth in an orbit in which one side would<br />
always face the sun—just as the moon always faces the Earth.<br />
Under such conditions, one side <strong>of</strong> the Earth would burn up, the<br />
other would freeze, and extremely strong winds would result.<br />
As some observers have said, humans should “thank their lucky<br />
star,” but also their extremely lucky solar system and Moon. Without<br />
the concatenation <strong>of</strong> all <strong>of</strong> these unlikely events, the Earth<br />
would have had an extremely unstable history, losing its oceans,<br />
or fluctuating in temperature so greatly that only bacterial life<br />
gist Simon Conway Morris to comment that the universe<br />
“smells faintly <strong>of</strong> mothballs.” There are at least 27 kinds<br />
<strong>of</strong> organic molecules, some quite complex, in the tails <strong>of</strong><br />
Halley’s and Hale-Bopp comets.<br />
• Organic molecules are common in the carbonaceous chondrite<br />
asteroids left over from the initial formation <strong>of</strong> our<br />
solar system. Even in the 1830s it was known that carbonaceous<br />
meteorites contained organic molecules. The<br />
Murchison meteorite, a carbonaceous meteorite that fell in<br />
Australia in 1969, contained at least 74 kinds <strong>of</strong> molecules,<br />
<strong>of</strong> which eight are amino acids found today in living cells,<br />
as well as fatty acids, glycerol, and purine and pyrimidine<br />
bases (found in nucleic acids such as DNA). This was also<br />
true <strong>of</strong> the Tagish Lake meteorite, which fell in Canada in<br />
2000. Careful analysis discounted the possibility that these<br />
molecules were terrestrial contaminants.<br />
The nebular and comet-tail chemicals are very sparse—<br />
only a few molecules per cubic meter. How could they be<br />
concentrated and delivered to the Earth? An immense<br />
amount <strong>of</strong> comet dust rains on Earth: about 40,000 tons<br />
per year. However, it is unlikely that a significant amount<br />
<strong>of</strong> organic material would have survived on meteorites. The<br />
origin <strong>of</strong> life<br />
could have survived. On a cosmic scale, even the nearly complete<br />
freezing <strong>of</strong> the Earth that occurred most recently about 700 million<br />
years ago is a mild occurrence (see snowball earth).<br />
According to Peter Ward and Donald Brownlee, when<br />
you consider all <strong>of</strong> these factors, it is possible that the Earth is<br />
the only planet that has been stable enough for complex life to<br />
evolve—even in the entire universe. At the very least, they claim,<br />
the universe is not like Star Trek, full <strong>of</strong> humanoids with whom<br />
humans can make contact. Some people have used these very<br />
same data to claim that the Earth has been prepared for our<br />
arrival by a higher intelligence (see anthropic principle). However,<br />
such a principle is unnecessary. While it is unlikely for all<br />
<strong>of</strong> these lucky things to have happened right here in this part<br />
<strong>of</strong> this galaxy, it could very well be that humans exist and think<br />
about such things in this place and not somewhere else simply<br />
because this place is where the luck happened to occur. At the<br />
same time, it might also mean that the rest <strong>of</strong> the universe, even<br />
if chock-full <strong>of</strong> bacteria, is a very lonely place for creatures with<br />
higher intelligence.<br />
Further <strong>Reading</strong><br />
Basalla, George. Civilized Life in the Universe: Scientists on Intelligent<br />
Extraterrestrials. Oxford, U.K.: Oxford University Press, 2005.<br />
Conway Morris, Simon. Life’s Solution: Inevitable Humans in a<br />
Lonely Universe. Cambridge University Press, 2003.<br />
Jackson, Randal. “PlanetQuest: The search for another Earth.” Jet<br />
Propulsion Laboratory, California Institute <strong>of</strong> Technology. Available<br />
online. URL: http://planetquest.jpl.nasa.gov/index.cfm.<br />
Accessed April 24, 2006.<br />
Sagan, Carl. Cosmos. New York: Random House, 1980.<br />
Ward, Peter D., and Donald Brownlee. Rare Earth: Why Complex<br />
Life is Uncommon in the Universe. New York: Copernicus, 2000.<br />
presence <strong>of</strong> organic molecules in outer space does not explain<br />
where terrestrial organic molecules came from. It demonstrates<br />
that the universe has produced immense amounts<br />
<strong>of</strong> the very kinds <strong>of</strong> organic molecules from which life is<br />
made—and this could have happened on the early Earth as<br />
easily as anyplace else in the universe. Because organic molecules<br />
are so common in the universe, the presence <strong>of</strong> PAH<br />
(polycyclic aromatic hydrocarbons) in the famous Mars<br />
meteorite is not itself evidence <strong>of</strong> life.<br />
The study <strong>of</strong> life outside <strong>of</strong> the Earth is called astrobiology<br />
(“star-life”), formerly called exobiology (“outside life”).<br />
Astronomer Jonathan Lunine notes that since the discovery <strong>of</strong><br />
ALH84001, astronomers and the National Aeronautics and<br />
Space Administration (NASA) have had a renewed interest in<br />
astrobiology and even in the possibility <strong>of</strong> panspermia.<br />
How<br />
Assuming that life evolved from organic molecules that<br />
formed on the Earth, how could this have occurred? The<br />
question is not new. Charles Darwin wrote a letter to Joseph<br />
Hooker, dated February 1, 1871, in which he made his<br />
famous reference to life originating in a “warm little pond”: