Scientists Find Water on Extra-solar Planet 220
amigoro writes "Scientists have, for the first time, conclusively discovered the presence of water vapour in the atmosphere of a planet beyond our Solar System, according to an article appearing in Nature. They made the discovery by analysing the transit of the gas giant HD 189733b across its star, in the Infrared using data from NASA's Spitzer Space Telescope. HD 189733b is a 'hot jupiter', a gas giant that is roughly the size and mass of Jupiter but orbits very close to the star, so no chance of life there."
While a great discovery, Is this surprising? (Score:4, Interesting)
The most common heteroatomic molecule is likely to be water...
Re:While a great discovery, Is this surprising? (Score:3, Interesting)
Re:"no chance of life there" (Score:5, Interesting)
"conclusively"? (Score:3, Interesting)
Re:"no chance of life there" (Score:2, Interesting)
Re:No Chance Of Life?!?! WTF? (Score:2, Interesting)
Hell, there are microbes that live and thrive in the heart of nuclear reactors, surviving both the heat and the radiation with ease. They'd be just the type to find a hot planet ultra-close to the sun a paradise..
Re:"no chance of life there" (Score:1, Interesting)
Compare that to the advantages of intelligence to an organism that must actively search for its food, distinguish useful items from the background, and compete with other mobile animals for limited resources.
And the sizes of biological life are not arbitrary. The surface tension of water sets the surface area to volume ratio of structures that can rely on passive transport of nutrients,as well as those of active transport structures, and the surface to volume ratio of course does not scale linearly. It is logical to assume that any cellular based life that needs water would evolve a familiar relationship between function and size.
Given a similar planet and concept of life, I do not think extraterrestrial life would really be that dissimilar.
Re:Hrrmph! (Score:2, Interesting)
It's the magnetic field (Score:5, Interesting)
On Venus too, it was the magnetic field -- or rather, lack thereof -- that did it. It's not just that some water gets split into hydrogen and oxygen, in which case it would just recombine sooner or later. It's that on Venus the lack of magnetic field allowed the solar winds to gradually wipe away the hydrogen. Venus is heavy enough to hold on th the slightly heavier elements, like Oxygen and Carbon anyway, even without a magnetic field. Hydrogen is a different story.
Outgassing CO2, well:
1. Earth spewed enough of that too, which is how it thawed back when cyanobacteria turned the atmosphere to O2 and the whole planet got deep frozen. (The Sun started a lot "cooler" and gradually warmed up. _Now_ it's warm enough to support life without a greenhouse effect, but in the beginning it wasn't.) I don't think there is any evidence that Venus spewed much more CO2 than Earth. On Earth just a lot of it got, well, buried right back. Say, in the Carboniferous era coal deposits.
The somewhat interesting corolary is that if we had too _little_ outgassing, then we'd have been really screwed. It took, IIRC, some 30% CO2 in the air to thaw that snowball Earth. Too little of it, and the deep freeze might just have continued long enough to be a total extinction event. Or at the very least a 1 billion year (or maybe more) pause in life evolution until the sun output went up some more.
2. Earth's original atmosphere was _methane_, which is a greenhouse gas about 200 times more potent than CO2. So if Venus would have been screwed by its outgassed CO2 atmosphere, the Earth should have been screwed 200 times harder (or close enough. Well over 100 times anyway.) In practice, that atmosphere on Earth just helped keep it warm enough at a time when the Sun was a lot weaker. If Venus had had a CO2 atmosphere at the time, well, it would have been a frozen snowball, quite the opposite of boiling off its water. In practice, it's a lot more likely that Venus started with a mostly Methane atmosphere too, only the hydrogen was swept away whenever some of it got broken up.
Pretty much if you start with water, methane and CO2, and continuously lose hydrogen, you end up with just the oxygen and carbon left, which means a lot of CO2. That's likely the short story of what happened on Venus.
3. There's an interesting extra factor there, which could have doomed Earth anyway, and that is: timing. If life or photosynthesis had started any later, for example, that methane and CO2 atmosphere would have sealed its fate. As I was saying methane is an _extremely_ potent greenhouse gas, so given enough extra time of gradually increasing solar output, it would have just boiled off the oceans. No liquid water, no life, game over.
At the risk of starting a flamewar... (Score:4, Interesting)