james_davis_nicoll: (Default)
james_davis_nicoll ([personal profile] james_davis_nicoll) wrote2014-12-04 01:46 am

Old Joke

which this reminded me of:


Q: What can the atmosphere of a planet with thousands of bars of abiotically produced oxygen oxydize?

A: Anything it wants to.

[identity profile] anzhalyumitethe.livejournal.com 2014-12-04 07:06 am (UTC)(link)
Going up on the Dragon's Gaze next week.

[identity profile] james-nicoll.livejournal.com 2014-12-04 07:11 am (UTC)(link)
Sorry, didn't mean to bigfoot you.

[identity profile] anzhalyumitethe.livejournal.com 2014-12-04 07:54 am (UTC)(link)
oh no worries. 9 & 10 have a bunch of habitability posts going up.

[identity profile] anzhalyumitethe.livejournal.com 2014-12-04 09:02 pm (UTC)(link)
Better make that the 8, 9 & 10th now.

[identity profile] neowolf2.livejournal.com 2014-12-04 11:21 am (UTC)(link)
O2 on Earth is ultimately pulled out by reaction with reduced rocks and volcanic gases. Overall, the Earth is very reduced, with just a (very) thin skin of more oxidized material at the surface. So I wonder how long it would take for a planet to soak up 100-1000s of bars of O2. This might depend on the rate of weathering of the planetary surface and the rate of volcanism.

[identity profile] graydon saunders (from livejournal.com) 2014-12-04 01:56 pm (UTC)(link)
If the authors think there are going to be false positives for "life bearing world" due to an oxygen-rich atmosphere being detected, they must think the hypothesized atmospheres are going to stay oxygen-rich for long periods of time.

[identity profile] neowolf2.livejournal.com 2014-12-04 02:02 pm (UTC)(link)
I think the time constant for absorbing the O2 from Earth's atmosphere is around 10 million years (if all photosynthesis were to end), so the question is how would that rate scale up if O2 partial pressure were much higher. Billions of years isn't out of the question.

[identity profile] graydon saunders (from livejournal.com) 2014-12-04 02:12 pm (UTC)(link)
Earth's crust is about half oxygen, isn't it? 46% or so?

Given the mechanism being proposed, it doesn't seem implausible that a planet with no hydrosphere (because it's all been disassociated away...) and a low rate of volcanism because it doesn't have much plate tectonics (because it doesn't have much of a hydrosphere) would wind up with a completely oxidized surface.

Gotta say this is totally changing my mental images for "oxygen-rich atmosphere", too. From "oh, there's life, how convenient for our protagonist" to "don't land there, you are flammable, protagonist, flammable!"

[identity profile] bruce munro (from livejournal.com) 2014-12-04 04:18 pm (UTC)(link)
1000 bars of oxygen - that's sort of a "concrete burns" scenario, isn't it?
ext_63737: Posing at Zeusaphone concert, 2008 (rockin' zeusaphone)

[identity profile] beamjockey.livejournal.com 2014-12-04 06:58 pm (UTC)(link)
I wonder what Hal Clement might have done with a setting like this.
Edited 2014-12-04 18:58 (UTC)

[identity profile] neowolf2.livejournal.com 2014-12-04 09:00 pm (UTC)(link)
People could live on airships at the 0.3 bar level.

[identity profile] neowolf2.livejournal.com 2014-12-04 08:58 pm (UTC)(link)
Yes, the Earth's crust is something like 46% oxygen; when I say part of the Earth is "reduced" I mean "has some atoms not in highest oxidation states". In particular, I mean there is ferrous iron, sulfur and sulfide, as well as some other transition metals in somewhat reduced oxidation states.

Reaction with oxygen oxidizes (some of the) the ferrous iron to ferric, and the sulfide/sulfur to sulfate. Things like silicon remain in the same oxidation state (+4).

I wonder if extreme high pressure oxygen might lead to formation of unusual compounds, like perchlorates.

EDIT: BotE scribbles make me think perchlorates could be thermodynamically favored at sufficiently high pressure, if the temperature isn't too high. This could place an upper limit on the atmospheric pressure. But the near-surface carbon is going to be in the planet's atmosphere too, as CO2, so the surface is probably going to be toasty.
Edited 2014-12-04 21:14 (UTC)

[identity profile] bunsen-h.livejournal.com 2014-12-07 03:37 am (UTC)(link)
Fond memories...

Capt. Jonathan Archer: I understand there's an inhabited planet a few light years from here.

Lieutenant Malcolm Reed: We've detected it, sir. Sensors show a nitrogen sulfide atmosphere.

Me: You... don't know a lot of chemists, do you?

[identity profile] owlmirror36.livejournal.com 2014-12-04 09:49 pm (UTC)(link)
I wondered how exactly all this oxygen was supposed to have accumulated . . .

The paper says:
M dwarfs are extremely active (Reid & Hawley 2005; Scalo et al. 2007), emitting large fractions of their luminosity in the X-ray and extreme ultraviolet (jointly referred to as XUV, corresponding to wavelengths of roughly 1-1000 Å ). XUV photons are not only biologically harmful, but can drive fast atmospheric escape that leads to the erosion of planetary atmospheres


So your putative protagonist would have to worry about rather severe sunburn/radiation burn as well as catching-on-fire burn.

[identity profile] neowolf2.livejournal.com 2014-12-04 10:52 pm (UTC)(link)
XUV/EUV photons will not make it down to a pressure level people could live at.

[identity profile] w. dow rieder (from livejournal.com) 2014-12-04 10:16 pm (UTC)(link)
Heh. "Captain Daring, what are our protective suits made out of?"
"Kevlar, why?"
"Um, maybe we should talk to a chemist back at Patrol HQ before we land..."
ext_196996: My avatar (Default)

[identity profile] johnreiher.livejournal.com 2014-12-04 05:09 pm (UTC)(link)
I think blocks of quartz burn level...

[identity profile] ilya187.livejournal.com 2014-12-04 05:40 pm (UTC)(link)
Quartz is already an oxide, so no, it won't burn no matter what the pressure is.
Edited 2014-12-04 17:41 (UTC)
ext_196996: My avatar (Default)

[identity profile] johnreiher.livejournal.com 2014-12-04 05:58 pm (UTC)(link)
My bad, I thought quartz was pure silicon.

[identity profile] monte davis (from livejournal.com) 2014-12-04 06:24 pm (UTC)(link)
There's a ClF3 gas giant nearby for that.

[identity profile] tandw.livejournal.com 2014-12-04 07:55 pm (UTC)(link)
I don't know; what does the oxygen activity need to be to make silicon peroxide stable?

[identity profile] owlmirror36.livejournal.com 2014-12-04 09:57 pm (UTC)(link)
Given that the oxygen is supposed to result from XUV radiation interacting with water (per the paper), I wondered how an ozone layer would affect this scenario. The paper doesn't mention ozone at all -- is this an oversight, or is there an obvious reason why ozone wouldn't form or wouldn't provide enough protection to slow or stop the runaway formation of the described super-oxygenated atmosphere?

[identity profile] neowolf2.livejournal.com 2014-12-04 10:53 pm (UTC)(link)
XUV photons are absorbed above the level of an ozone layer, and are absorbed strongly by more ordinary molecules, like water or molecular oxygen. Ozone is important only because it absorbs UV photons that are too low in energy to be absorbed by O2 or N2.

[identity profile] w. dow rieder (from livejournal.com) 2014-12-04 10:28 pm (UTC)(link)
"Welcome to the Thousand Bar Oxygen Bar, where everything's rock, water, or on fire!" 8-)

[identity profile] scott-sanford.livejournal.com 2014-12-08 06:53 am (UTC)(link)
"For this week's exciting installment of Flashpaper Gordon!"