Re: Life in the atmospheres of L-class stars.
From: Jonathan Silverlight (jsilverlight_at_spam.merseia.fsnet.co.uk.invalid)
Date: 03/28/05
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Date: Mon, 28 Mar 2005 22:20:56 +0100
In message <d28nr5$51f$1@sparta.btinternet.com>, Mike Dworetsky
<platinum198@pants.btinternet.com> writes
>"Orbitan" <orbitan7@yahoo.com> wrote in message
>news:1111969881.083736.276010@g14g2000cwa.googlegroups.com...
>>
>> L class have a surface temperature range
>> of from 2200K to 1400K, and they are named
>> based upon their spectra. They are about
>> half way between being stars and brown dwarfs.
>>
>> Their upper atmosphere is characterised by the
>> fact that its temperature will allow the condensation
>> of some types of dust with melting points and boiling
>> points at extremely high temperatures.
>>
>> Several questions:
>>
>> Can anything even remotely with the complexity of
>> life be automatically excluded in all circumstances
>> in these temperature ranges?
>>
>
>Probably it can be excluded, for the simple reason that complex molecules we
>think are needed for life as we know it cannot exist at such temperatures
>(akin to a welding torch). It's difficult to discuss life as we do not know
>it.
But that's when things get interesting :-) Arthur Clarke has written two
memorable short stories in which the inhabitants of the Sun are highly
complex arrangements of plasma, and David Brin has written a novel on
the same theme. But so far it's purely science fiction, and no-one knows
if it's possible.
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