I think what will really help us to get at a better estimate
is to answer the question whether there exists life in our
solar system that evolved independently of that on Earth.
That's definitely the big question. But you left out the elephant in the room: is there life right here on Earth that's evolved independently? Abiogenesis doesn't simply halt after it's achieved its "goal". Perhaps we take the common-origin hypothesis for granted (that the "tree of life" has one root, and is in fact a tree), but it's actually nontrivial, strong evidence about the rate of abiogenesis, right under our noses. If it's true.There's no hard reason why another, orthogonal family of life couldn't coexist with DNA/RNA life. We have 10^7 extant species of DNA/RNA life; that's an existence proof that hostile, competing "types" of life can coexist. Suppose we found terrestrial "XNA life" with a biochemistry totally unrelated to anything else, with no possible common origin or lateral gene transfer. Then we would know life on Earth developed independently N >= 2 times, instead of N >= 1. That would change a lot; we could update P(life | Earth-like planet) from the subjective probability range [10^-Graham's number, 1) to something more like [10^-4, 1).
What's really surprising is that this is completely untested! We genuinely don't know if there's "alien" life on Earth, because we don't know how to look for it. There's no black-box tool to approach unknown biochemistry:
Some have postulated the existence of a 'shadow biosphere'
on Earth, teeming with life that has gone undiscovered
because scientists simply don't know where to look. It could
contain life that relies on a fundamentally different
biochemistry, using different forms of amino acids or even
entirely novel ways of storing, replicating and executing
inherited information that do not rely on DNA or
proteins. [...] The trick is deciding what to look for and
how to detect it. The usual way that researchers search for
new organisms — by sequencing DNA or RNA — will not pick up
life that does not depend on them.
http://www.nature.com/news/life-changing-experiments-the-bio... ...We could even be oblivious to unfamiliar forms of life
right under our noses...
http://www.sciencemag.org/news/2015/02/shadow-biosphere-migh...v2.0 life would have to evolve in the changed environment - which would be considerably less hospitable, because the most useful chemical processes and energy sources will be colonised by v1.0 life.
v1.0 life will (more or less literally) get the low hanging fruit. v2.0 would have to evolve around the edges, which means the probability gradient is higher and therefore less likely.
So although it's a very valid point I'm not sure if it's a sufficient argument against the hypothesis of having two independently evolved and fundamentally different types of life on a given planet.
This would be good stuff for a science fiction story as well.
The only way to die if a UV ray split you, or you fall into a volcano (there are no fire, because the atmosphere has very few oxygen), or a nasty oxygen molecule reacts with you, or ...
Well, there are many ways to die, but they are not targeting you, so perhaps you can hide from the sun under a rock. Or to be more clear, since you doesn't have any kind of senses or mobility, perhaps you are lucky and get beached under a rock. Perhaps the rock also makes a nice place to concentrate other molecules during the low tide.
Perhaps it's not a good idea to be near the surface and it's better to be lucky and get near a underwater sea vent with tasty hydrogen. I think the details of the first steps are not clear for anyone (in particular for me).
Once a stupid life for appears, the first thing it would do is eat all the free food. In particular, before the first life form the half of the amino acid were L and half D. We have used all the L amino acids (and created many more than the original supply), and we have also eaten all the original D amino acids. So there are very few of them floating around freely, it would be very hard to start an alternative D-tree.
A new life form will be targeted by the existing life form, like the free D amino acids. The competition will be extremely hard. So I think it's a winner take all task.
Moreover, then some moron decides to release a lot of oxygen to the atmosphere. Oxygen is extremely toxic for most life forms, and more toxic for isolated molecules that are barely alive ...
About the shadow biosphere: Perhaps we (humans) can't detect or identify them, but the bacteria and archaea can probably live there and eat them barely-alive. Our cousins can keep all the out-of-tree competition at bay.
If you are the first almost live form, you have plenty of
time, and can evolved in an environment that has plenty of
food. Something like the brown goo of Titan, with lots of
hydrocarbons and other small molecules that you can pick up
for free.
But there's no food on Titan anywhere! There's no oxidizers for hydrocarbons to react with; hence no accessible chemical energy.That's likely generic for pre-biotic environments. Planets don't naturally form redox gradients; if there's a large redox potential, that's reactive chemistry, which will react away to equilibrium over geologic time. It takes work to maintain such a gradient; for example, Earth's oxidizing atmosphere is actively maintained by life. Oxygen is geologically removed from atmospheres, reacting with exposed rock surfaces (oxygen weathering). It takes active expenditure of work (solar energy) to keep it existing.
There is some chemical energy in abiotic planets, but only small amounts, at very low power levels compared to Earth's aerobic biosphere (which eats something like 10^14 watts!). There's photochemistry caused by solar UV light, and there's atmospheric lightning (which is a major player in the Earth's N2 cycle). Most important is geochemical energy; i.e. primordial chemical gradients that aren't yet at equilibrium, because the two reactants are physically separated by rock layers. On Europa for example, a very slow process brings rocks into contact with the ocean, where slow serpentinization reactions can occur: oxidation of Fe++ to Fe+++ by water, with the production of H2. This would be the food source of Europa life, if it's there.
I'm not sure if this is for or against your comment, but I hope you find this interesting:
"A cave in Romania that was sealed for 5.5M years" http://www.bbc.com/earth/story/20150904-the-bizarre-beasts-l... HN discussion: https://news.ycombinator.com/item?id=11682816 (889 points, 38 days ago, 163 comments)