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grive | 2 years ago
Some external circumstances could change reducing them to a pile of oxides, but the systems themselves were perfectly self-perpetuating -- i.e. time-independent, or put another way 'given enough time' is not sufficient.
Of course, before the heat-death of the universe entropy-reducing systems will break down, but that's not an interesting observation.
> Some physical processes decrease entropy locally, sometimes by incredible amounts.
I think that's the more interesting observation. How to qualify life beyond only 'local entropy reduction systems'.
My uninformed opinion is that it is both 'entropy-reducing' and 'context-dependent' systems that should be considered 'alive' (not sure though that this is sufficient). Dependence on their context means that those systems will have a feedback-loop with their environment, allowing for example non-linear causality and thus complexity to emerge.
A star radiating away their stored negative entropy is an all give and no take, no dependency, full autonomy system. Of course they can still be impacted by external effects, but sustaining their own internal processes does not require such inputs, they are incidental to them emitting away their stored energy. Once started, their schedule (when they will deplete themselves, collapse, etc) is known and predictable, thus not alive.
fluoridation|2 years ago
Excuse the snark, but it's exactly as interesting as saying that some living systems are immortal until they're no longer immortal. If a protocell or a virus stops being alive (if we grant that it's alive) when it falls into a fire then it's not immortal just because it has no metabolism.
>Once started, their schedule (when they will deplete themselves, collapse, etc) is known and predictable, thus not alive.
Actually, no. For example, a star could hypothetically fall into another much larger than it and prolong its life, if we were to say that it lives. The only reason it's predictable is because a star can't move on its own to hunt weaker stars, and because (at least at this time in the history of the universe) stars are far enough apart that they rarely fall into each other. If that was a common occurrence it would be much more difficult to predict how long until a star burns out.
grive|2 years ago
>> "Some external circumstances could change reducing them to a pile of oxides"
(or some other transformations I guess in case of fire.)
That was precisely not what I was talking about (or put another way if you still require abundant explicitness): not the kind of immortality I was describing. Maybe I was not clear enough.
> For example, a star could hypothetically fall into another much larger than it and prolong its life
Well, once again:
>> Of course they can still be impacted by external effects, but sustaining their own internal processes does not require such inputs