I guess this discussion is mostly over, but since I am intensely interested in astrobiology I will make some quick notes.
- NASA's intent.
NASA, together with astronomers, are pushing for a new generation of large telescopes, here space telescopes. The observational constraint is that if life is likely, they can observe it soon. If not, they can start to constrain its likelihood from above.
- Search for life.
Besides the search for inhabited planets in the radiative habitable zone, we will eventually need to investigate many or most of our system's tidal habitable zones (ice moons). Because a) they constitute the perhaps largest type of biosphere volume, and because b) we can't observe a frequency of biosignatures elsewhere.
- Likelihood for life.
Almeisan said:
But, what if life is not common? Some things only happen once, even in near-infinitely large universes.
Ophiolite said:
Until we have expanded our knowledge of life beyond a sample size of one, such speculations are interesting, but barely constitute science.
Nothing happens 'only once' in a sufficiently large universe, because the permutations among a finite number of particles in a finite observable universe is finite, see e.g. Tegmark.
But that isn't interesting, because we are restricting severely as in everyday life, "if that hadn't happen I wouldn't have ...".
What is relevant here is that emergence of life is a result of a process. And processes that result on the order of one ( zero, one, a few) events would be very finetuned.
The statistics of emergence do constitute science (and shows that emergence is a process; but see also below). See e.g. Lineweaver on how to do statistics here. Loosely, the rapid emergence we observe allows us to claim that the process is likely on at least the order of ~ 10 %/billion years.- Fermi's Question and the Hart-Tipler Conjecture
When we read "Fermi's Paradox" we see the result of a political process. Fermi asked the question "where are they" and answered that space travel and habitability cartography is difficult. (Which they are.)
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http://www.universetoday.com/119735/beyond-fermis-paradox-ii-questioning-the-hart-tipler-conjecture/ ]
- Emergence of life.
Almeisan said:
I don't think there is good evidence. We can't even get steps of abiogenesis to happen even in controlled lab experiments.
Ophiolite said:
They offer plausible partial pathways, but there is nothing like a cohesive, demonstrable route from non-life to life.
Almeisan said:
We have no idea how abiogenesis happened. ... We struggle to deliberately make synthetic life de novo when we can do so much in both biochemistry and molecular biology.
Cosmologists have not demonstrated how to make a universe within a lifetime in a lab. Yet we study the emergence of the universe.
Evolutionists have not demonstrated how to make whales within the lifetime in a lab. Yet we study the emergence of whales from land living ancestors.
So what do we know, and what do we need to test?
- We know that there are a number of trait homologies between geophysical systems of Hadean and modern cells. So we know the generic phylogenetic tree as much as we know other generic trees of similar complexity. (We also know emergence is a result of a process, first growth of the geophysical systems that it happened in, then evolution after self-replicators emerged.)
- There were also obvious constraints that were in tension with those observations. But whether you adhere to the "pure" RNA world (RNA protocells) of Szostak et al or the "dirty" RNA world (RNA vents) of Russell et al, the last 5 roadblocks I know of fell in the last year. (I have a referenced write up, but it is too long for a PF comment.)
- What remains is to test the two main pathways sufficiently.* This has been ongoing for, oh, a decade now, and it seems astrobiologists expect it will take a few more decades. I'm frankly surprised that people persist in claiming that there are observational problems.
*Meanwhile, if you want to do research strategy, the bottom-up pathway of Szostak is as simple as possible while the top-down pathway of Russell is as complex as the phylogeny constraints makes it. Ironically, or rather consequentially, that translates to the largest prior for Szostak but the largest posterior for Russell. So if I was into betting...