Did Comet Crashes Help Spark Earth Life?

Manipulating an orbiting asteroid would require more effort than was employed to develop the first nuclear bomb during the Manhattan Project.

Billions ofyears ago, comets may have ferried life-sustaining water to our planet'ssurface, but that may not be all that we should thank these dirty snowballs for.Researchers are simulating comet impacts to see if they might help proliferatethe left-handedness in molecules that life on Earth depends upon.

There isevidence from meteorite studies that amino acids may have been deliveredto Earth from space.

"Thereis interest in how these building blocks came to be on primordial Earth,"says Jennifer Blank of the SETI Institute.

She and hercolleagues study comets as a second avenue for depositing these biological compoundson Earth. Their current work, which is supported by NASA's Exobiology andEvolutionary Biology Program, is looking at how the fireand brimstone of a comet impact may benefit the formation of complexmolecules of a particular handedness.

Since thatpioneering work, researchers have come to believe that Earth's early atmospherewas in fact more oxidative, containing mostly nitrogen and carbon dioxide.

"Withoutthe reducing atmosphere, the Miller mechanism becomes much less efficient at producingamino acids," Blank says.

One way toget around this is to make the amino acids in space and have them come crashingdown on-board meteorites and comets. There is ample evidence that meteorites carryamino acids. And just recently, an amino acid wasdiscovered in comet material brought back by NASA's Stardust spacecraft.

Blank andher colleagues were curious as to what happens to these biomolecules when the"space capsule" they are riding in smacks into the Earth.

The teamhas focused their work on comets, rather than meteors. Although comets are lessprevalent in the inner solar system, they have a few possible advantages overtheir dry rocky counterparts when it comes to delivering biologically relevantmaterial to a planet's surface.?

"Cometsgive you all the ingredients, like a compact evolution kit," Blank says.

Of course,the primordial Earth was stocked with its own water, but "if a comet ormeteor were to land in the ocean, any interesting chemistry would quickly bediluted away," says co-investigator George Cooper of NASA Ames. A cometimpact on dry land would give the organic molecules on board the chance to amplifytheir numbers in the localized puddle.

"It'snot super high-tech, but it is rather involved as far as the structuralcomplexity is concerned," Blank explains.?

She and hercolleagues take special care to ensure that the metal container doesn't leakfrom the impact. Afterwards, they carefully drill down to the chamber and drawout their "shocked" liquid sample.

"It'sthe coolest thing," Blank recounts. "People told us, 'Nothing isgoing to survive, so why should we fund you?'"

Normally,the 1,000-degree-temperatures inside the smashed "comet" woulddestroy any amino acids. But Blank believes the temperature rises and falls toofast for the molecules to react. There is also enormous pressure of 10,000atmospheres that may be preventing the breakdown of compounds.

It isperhaps conceivable that a comet impact fused together the first rudimentary proteinpieces (called "peptides") and thereby got the whole ball rolling.

Blank's groupis now running simulations to see if they can model how the energy barrier toamino acid bonding changes under the high temperature and pressure of a cometimpact.

"Itwill be a great discovery if they can get definite evidence as to formation ofsugars, peptides, or enantiomeric excess," says Yoshihiro Furukawa of Tohoku University in Japan, who was not involved with this work.

 

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Michael Schirber
Contributing Writer

Michael Schirber is a freelance writer based in Lyons, France who began writing for Space.com and Live Science in 2004 . He's covered a wide range of topics for Space.com and Live Science, from the origin of life to the physics of NASCAR driving. He also authored a long series of articles about environmental technology. Michael earned a Ph.D. in astrophysics from Ohio State University while studying quasars and the ultraviolet background. Over the years, Michael has also written for Science, Physics World, and New Scientist, most recently as a corresponding editor for Physics.