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DBL%20Hendrix%20small.png College chemistry, 1983

Derek Lowe The 2002 Model

Dbl%20new%20portrait%20B%26W.png After 10 years of blogging. . .

Derek Lowe, an Arkansan by birth, got his BA from Hendrix College and his PhD in organic chemistry from Duke before spending time in Germany on a Humboldt Fellowship on his post-doc. He's worked for several major pharmaceutical companies since 1989 on drug discovery projects against schizophrenia, Alzheimer's, diabetes, osteoporosis and other diseases. To contact Derek email him directly: derekb.lowe@gmail.com Twitter: Dereklowe

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February 23, 2005

Exobiochemistry

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Posted by Derek

Back in the early days of my pre-Corante blog, I wrote a piece about some other kinds of chemistry that might be used in living systems. There's now a wonderful one-stop review for all sorts of speculations on this topic, which incorporates everything I've ever thought of and plenty more. Steven Benner at the University of Florida, who my fellow Corantean Carl Zimmer has interviewed, and two co-workers (here's his research group) published "Is There a Common Chemical Model for Life in the Universe?" in Current Opinion in Chemical Biology late last year. (here's the abstract; I can't find the full text available yet on the Web.)

I can't say enough good things about this article. This is the sort of topic I've enjoyed thinking about for years, but there were still plenty of things in this review that had never occurred to me. Benner goes over the likely requirements for life as we know it, life as we'd probably recognize it, and life upon which we can barely speculate. As a chemist, he's particularly strong on discussions of the types of bonds that could best form the complex molecules that chemical-metabolism-based life needs. Energetic considerations - how much chemical bond energy is available, how soluble the materials are, how reactive they are at the various temperatures involved - are never far from his mind.

He devotes sections to ideas about living systems without chemical solvents (gas clouds, solid states) and the more familiar solvent-based chemistry. There's plenty of water out there in the universe - which is why bad movies about aliens coming to drain our oceans are so laughable - and it's natural enough that we should concentrate on water-based life. But there's plenty of ammonia out there, too, along with methane, sulfuric acid, and other potential solvents like the supercritical dihydrogen found in the lower layers of gas giant planets.

So, is all this stuff out there? Is life something that is just going to happen to susceptible chemical systems, given enough time? If so, which ones are susceptible? Benner's thoughts are, I think, best summed up by his take on Titan:

"Thus, as an environment, Titan certainly meets all of the stringent criteria outlined above for life. Titan is not at thermodynamic equilibrium. It has abundant carbon-containing molecules and heteroatoms. Titan's temperature is low enough to permit a wide range of bonding, covalent and non-covalent. Titan undoubtedly offers other resources believed to be useful for catalysts necessary for life, including metals and surfaces.

This makes inescapable the conclusion that if life is an intrinsic property of chemical reactivity, life should exist on Titan. Indeed, for life not to exist on Titan, we would have to argue that life is not an intrinsic property of the reactivity of carbon-containing molecules under conditions where they are stable. Rather, we would need to believe that either life is scarce in these conditions, or that there is something special, and better, about the environment that Earth presents (including its water)."

As for me, I can't wait to find out. I want Titan rovers, Jupiter and Saturn dirigibles, Venusian atmosphere sample return, instrument-laden miniature submarines melting down through the ice on Europa and Enceladus: the lot. How much of this will I ever get a chance to see in my lifetime? Current betting is running to "none of it, damn it", but things can change. Depends on how easily and cheaply we can get payloads up to (and out of) Earth orbit.

Comments (6) + TrackBacks (0) | Category: General Scientific News | Life As We (Don't) Know It


COMMENTS

1. Adam on February 24, 2005 10:10 AM writes...

David Grinspoon, and colleague, have written a piece speculating that the apparent large-scale resurfacing on Titan needs a higher heat-source than volcanism. They suggest that acetylene produced in the upper atmosphere might suffice...

http://au.arxiv.org/abs/physics/0501068

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2. Monte Davis on February 24, 2005 12:09 PM writes...

In planetary science, there were generations of growing confidence that we understood in general why our solar system is the way it is (small & rocky close in, big and volatile-rich farther out). We thought we had a handle on principles that would govern all planetary systems. Then we started spotting extra-solar planets... and it's back to the drawing board. We had mistakenly generalized features that now appear to be contingent on details of Sol's case.

Or think about how many biology texts told us "all life depends ultimately on solar energy" before we found the deep-sea vent ecologies.



A lot of good, persuasive thinking has gone into the special-ness of carbon, of C-H-O-N, of water, of Earth's temperature history (cf. Ward & Brownlee's _Rare Earth_). One has to wonder how much of that will suffer the same fate...

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3. Jake McGuire on February 24, 2005 12:41 PM writes...

I think you might be slightly overstating the amount of rethinking that had to go on with the discovery of extrasolar planets. The current means we use to find them (looking for periodic shifts in the radial velocity via the doppler effect) is way more effective at finding hot superjovians than earthlike planets; for instance I don't think we yet have the ability to discover Sol's planetary system (in the way that scientists try to use probes doing earth flybys on their way somewhere else to discover life on earth).

Kepler may/should change that.

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4. Derek Lowe on February 24, 2005 12:47 PM writes...

My impression (as an amateur astronomer) has been that the number of hot superJovian planets has been a surprise all by itself. As a chemist, I have to wonder what sort of compounds have formed in those guys, given the huge energy flux they're hit with. They must be the biggest balls of maroon polymeric gorp imaginable.

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5. Conservative Mutant on February 25, 2005 12:08 AM writes...

Thanks for pointing out that review, Derek. I’ve been interested in Benner’s work on artificial nucleotides for some time, and this prompted me to write a (long!) post on the nucleotide alphabet and the current theory as to why it only has two base pairs.

Permalink to Comment

6. Monte Davis on February 25, 2005 10:29 AM writes...

Jake: of course you're right about the observation bias. I meant that a number of those superjovians are much closer to their primaries than they should be according to our pre-1990s understanding of planet formation.

As for "maroon polymeric gorp," I love it -- but marketing may insist on another name before you try to get funding for the expedition.

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