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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”:

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