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Probably not. As for our being an artefact, why?
It is dangerous to extrapolate from a sample size of one.
Your suggestion that we could exist as nothing but a Matrix-like simulation is untestable (unless you could find a bug in the system).
Quote from: Ophiolite on 23/10/2013 09:01:26It is dangerous to extrapolate from a sample size of one. Which is why it is worth applying Bayesian statisics and asking what if anything is remarkable about your tiny sample.
This leads quite nicely to the Drake equation which suggests (a) there is a nonzero probability that something we might call life either exists, may have existed, or will exist somewhere else in the universe
(b) we are most unlikely to find it.
Such cautious statistical analysis is a long way from the Goldilocks or anthropocentric extrapolation, even if conclusion (b) is indistinguishable from the Goldilocks result!
Hold on! The sample size is at least a dozen planetary objects (i.e. including large moons) , and thousands of smaller chunks of rock, in the solar system, of which only one is known to support life and only two others (Mars and Europa) might have or have had the capability of doing so - assuming that life involves selfreplicating systems that transpire water.
Now given the very small range of orbital radii around any given star, within which water will remain liquid, and the minimum size of planet needed to retain water in its atmosphere, it's unlikely that any star will have more than one Earthlike planet in the right orbit.
So we are beginning to put some real numbers into Drake. We need a star of similar age and composition to the sun to provide a reasonably stable energy input without too much ionising radiation, and since that pretty much defines the mass range of the candidate star, we can begin counting candidates.