Planetary Formation Sim Suggests Many Water Worlds
StefanJ writes "Researchers at the University of Washington -- supported by the NASA's Astrobiology Institute, its Planetary Atmospheres program, and Intel -- have come up with a new simulation of planetary formation that suggests that not only are terrestrial planets (small, rocky worlds, as opposed to gas giants) are common, but that water worlds (the subset of terrestrials that have sufficient water to support Life As We Know It) may be plentiful as well.
A key factor as to how 'wet' a planetary system's terrestrial worlds get: The eccentricity of the orbits of the system's jovian worlds.
It will be a while before we have telescopes good enough to actually see terrestrial planets and spec out their atmospheric composition, allowing us to reality-check these simulations. But it's still cool to play with sims like this. I can't wait for the home version!
(Emergency backup link to Science Daily article based on the press release.)"
Albert Einstein -
Only two things are infinite, the universe and human stupidity, and I'm not sure about the former.
Uh...you do realise that the Earth is a water-rich planet of the type they're talking about, right?
So, this is not based in reality _quite yet_. There is only one data point!
Slashdot: Failed Car Analogies. Amateur Lawyering. Anecdote Battles.
The formation of water worlds would seem to hinge on the relative abundances of H, O, and C as well as the ability of other heavier elements to bind these crucial light elements. The inner system of a forming star seems like a hostile place for hydrogen. Between the hot accreting planets, their low gravitiation pull, and stellar winds, I'd bet that its too easy for a small rocky inner world to lose all its hydrogen and other volatiles.
Assuming that hydrogen is retained (locked up in the rocks), it then becomes a matter of the C-O balance. If carbon is too prevalent, it will scavenge all the oxygen from the atmosphere and lead to a CO2/hydrocarbon atmosphere (other things, like FE also scavenge oxygen). Only if there is enough oxygen will you get water.
I wonder how accurately the sim modelled the balance of elements and chemical reaction cycles.
Two wrongs don't make a right, but three lefts do.
An interesting thought, but, damn, there are a lot of variables. Apart from the ones you named, you could also play with varying the amounts of other important for life elements and chemical (oxygen, carbon, nitrogen, etc.), change the kind of star our sun is, varying the amounts of life-affecting compounds (like methane). It's really mind boggling. I suppose we could just limit the things one could vary in the simulation. It would still be an interesting exercise in trying to determine the upper and lower bounds of what might constitute a "class M" world.
my pet machine
"We have 2/3's of a watery planet right here, that we are yet to explore in great detail."
I hate comments like this. As if astronomers can just take up deep sea diving and marine biology.
Let's settle this once and for all: Diversification is a GOOD thing. We do not gain anything by 'focusing' on what YOU think is important. I'm a 3d artist. Do you think that somehow qualifies me to do cancer research?
So knock it off. We do a little bit of everything on this planet. Over-focus on one thing, and you neglect other areas of research that benefit man-kind. You're not being insightful here.
"Derp de derp."