Article View: sci.space
Article #141Re: HRMS for ETI
From: Stanley Friesen
Date: Fri, 30 Oct 1992 18:18
Date: Fri, 30 Oct 1992 18:18
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In article <1992Oct30.023542.4610@cs.rochester.edu> dietz@cs.rochester.edu (Paul Dietz) writes: |In article <1346@tdat.teradata.COM> swf@tdat.teradata.com (Stanley Friesen) writes: | |> This last is an extremely unlikely requirement. The basic upshot of the |> Urey experiment and its follow-ups is that organics form spontaneously |> under most non-oxidizing 'medium-energy' conditions. The presence of |> organics in interstellar dust clouds just confirms this basic ubiquity. | |The Miller-Urey experiment is widely acknowledged to be irrelevant, |as it assumed an atmosphere that likely bears little resemblance |to the early earth. Specifically, methane and ammonia are unlikely |to have been abundant in the early atmosphere, as they are destroyed |within centuries by UV light. That is why I specified 'and follow-ups'. Almost every variant atmosphere that was either reducing or 'neutral' has yielded organics. The results do *not* depend particularly on the exact original chemistry - though the exact set of organics produced does vary with the initial conditions. |When performed with more reasonable gas mixtures, the experiments have |much lower yields. And, in any case, all that these experiments |indicate is that some of the basic molecules of life are rather stable |(and, importantly, that others are not), not that a particular source |is where they first came from. They show them to be formed under a wide variety of conditions, so they are liekly to be present on most otherwise suitable planets - perhaps from *multiple* sources. In short, it is more *lack* of organics is more extraordinary, and thus more unlikely, than thier presence. |The unstated assumption here is that life would *not* have had a hard |time originating back then. We simply don't know enough about how |life started to say this. Not really, the all I was talking about here was the fact that our oxidizing atmosphere destroys all unprotected organics. | |Au contraire! Our ignorance about origin of life is profound, and |very little progress has been made in dispelling it. There is no |really plausible model for the origin of life. We're missing at least |one, and possibly several, fundamental ideas. | Have you read Cairns-Smith's "Seven Clues to the Origin of Life"? I consider that to be an extremely plausible model (though the best reasons are not in that, now out-of-date, book). Also, one could argue, based on the usual defnitions of life, that the recently produced self-replicatinf RNA molecule *is* alive, and thus we *have* made life in the laboratory. (Of course the exact definition of life in the boundry cases is decidedly difficult, so one could also make a case that it is not alive). -- sarima@teradata.com (formerly tdatirv!sarima) or Stanley.Friesen@ElSegundoCA.ncr.com
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Path: arc1-ca.pugleaf.net!sparky!uunet!tdat!swf From: swf@teradata.com (Stanley Friesen) Newsgroups: sci.space,sci.bio Subject: Re: HRMS for ETI Message-ID: <1357@tdat.teradata.COM> Date: 30 Oct 92 18:18:25 GMT References: <1cl20hINNec3@gap.caltech.edu> <1992Oct28.130939.9964@cs.rochester.edu> <1346@tdat.teradata.COM> <1992Oct30.023542.4610@cs.rochester.edu> Sender: news@tdat.teradata.COM Reply-To: swf@tdat.teradata.com (Stanley Friesen) Organization: NCR Teradata Database Business Unit Lines: 55