On Saturday, July 6, 2019 at 10:32:54 AM UTC-5, smitra wrote:
>
> https://arxiv.org/abs/1711.01945 
>
>
> A followup article which focuses more on the mathematical issues is 
> under construction, the key points are: 
>
> 1) In interstellar space, simple organic compounds captured in small ice 
> grains were subject to UV radiation and occasional heating due to 
> incident cosmic rays (CR). This induced a bond percolation process that 
> led to large clusters of organic molecules on a time scale of $\gtrsim 
> 10^6$ years. 
>
> 2) On a proto-planet, such clusters can merge into loosely bound 
> superclusters. The deep interior of such superclusters can provide for 
> chemical micro-environments in which conventional models of abiogenesis 
> driven by cold-warm cycles can be considered. 
>
> 3) Rapid fluctuations in the chemical potentials of certain chemical 
> compounds that can penetrate the supercluster, will be damped down. Long 
> term gradual and periodic changes then dominate, allowing any 
> biochemical systems inside the superclusters to more easily evolve 
> toward exploiting the conditions in their micro-environments, compared 
> to a similar system in the outside environment. 
>
> 4) As the supercluster breaks up, the system experiences more of the 
> shorter term fluctuations that has more of a random character. The 
> system can then evolve to adapt to these fluctuations, when doing so 
> right from the start might not have worked. 
>
> 5) On a small fraction of the superclusters these processes led to 
> microbes capable of surviving in the outside environment. 
>
> 6) Microbes were transferred to Earth via a collision of a 
> microbe-containing proto-planet with the Moon. Fragments containing 
> microbes resulting from the giant impact rained down on the Earth. 
>
>
> Saibal 
>
>
>
Interesting.

@philipthrift 

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