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doogly wrote:On a scale of Mr Rogers to Fascism, how mean do you think we're being?
Belial wrote:My goal is to be the best brain infection any of you have ever had.
allegedly...Jessica wrote:we found
++$_ wrote:Liquid ammonia is probably the most likely candidate to replace water, since it is readily formed and can dissolve a lot of things. There are other solvents, like acetone, but they are less likely to be present naturally, so I don't see how you would accumulate enough of them on a planet to form an ocean, at least without living things creating them first. Maybe you can have a planet with "second-generation" acetone oceans, having been pumped out as waste by a previous generation of water-based life, or something.
Either type of ocean would be much less compatible with atmospheric oxidizing gases than water. Maybe a lower concentration of oxygen would work, or perhaps another gas like nitrous oxide or chlorine would have to be used instead.
As for fluorine: No, probably not. It is scarce in the universe compared to oxygen, and it will react instantly with almost anything other than fluorine, fluorides, platinum-group metals, or noble gases. If you were to pump some fluorine into the atmosphere of an ordinary planet, it would quickly be used up oxidizing the rocks. In this video a brick is lit on fire using fluorine.
ATCG wrote:I had to chuckle after reading this, then noticing your location. Surely you risk being burned at the stake as a heretic.Tass wrote:Nice to see another person sharing my views of quantum mechanics. Use Occam's razor, cut out the wavefunction collapse.
The Piper Encyclopedia wrote:Niflheim
Niflheim is the 4th planet of Nu Puppis. It's about 5 AU from its primary, with about 1g surface gravitation and one atmosphere of pressure. Ambient temperature is about -60C. It was discovered by the Terran Federation Space Navy. The atmosphere is 4-5% free fluorine with some inert components. The bulk of the atmosphere is the result of the reaction of fluorine with other materials: CF4, BF3, SiF4, PF5, SF6 and others. There is also a little free oxygen. The planet's rocks are weak and consist exclusively of fluorides. The only free liquid on the surface was liquid hydrofluoric acid (HF). It is rich in uranium.
Niflheim's native plants and animals metabolize fluorine. Their harder tissues are long-chain fluorocarbons (e.g., Teflon). Trees are described as "topped with huge ragged leaves, looking like hundred-foot stalks of celery." Other plants as "a mat of wormlike colorless or pastel sprouts". Animals are described as "Little round things, four inches across, gnawing at the vegetation, and bigger things, two feet long, with articulated shell-armor and sixteen legs which fed on the smaller herbivores."
Probably the most surprising and interesting thing about the Twayne edition is the essay that forms the introduction to that volume, and is reprinted here. The essay is by Dr. John D. Clark, an eminent scientist of the forties and fifties and one of the discoverers of sulfa, the first "miracle drug." It describes in great detail the planetary system of the star Beta Hydri, and gives the names of those planets: Uller and Niflheim. A publisher's note states that Clark's essay was written first, and given to the contributors as background material for a novel they would then write.
The fans of H. Beam Piper seem to owe a great debt to Dr. Clark. Uller Uprising became the foundation of Piper's monumental Terro-Human Future History; the first story where we encounter the Terran Federation. In it we learn about Odin, the planet that will one day be the capital of the First Galactic Empire; and humble Niflheim, which in more decadent times will become a common expletive, a word meaning hell.
madd0ct0r wrote:how to get such a concentration of flourine though?
Oxygen is far more common, slightly less reactive and also slightly heavier. hmmm
A planet has flourine and oxygen, with the flourine getting bound up in salts on the surface and driving the oxygen off.
Along comes a nova shockwave (or something) and strips the atmosphere off. Bye Bye oxygen.
Over time, the flourine salts slowly separate (how? photosynthesis?) and flourine becomes a larger component of the atmosphere again.
Wikipedia wrote:From the perspective of cosmology, fluorine is relatively rare with 400 ppb in the universe. Within stars, any fluorine that is created is rapidly eliminated through nuclear fusion: either with hydrogen to form oxygen and helium, or with helium to make neon and hydrogen. The presence of fluorine at all—outside of temporary existence in stars—is somewhat of a mystery because of the need to escape these fluorine-destroying reactions.
Three theoretical solutions to the mystery exist. In type II supernovae, atoms of neon are hit by neutrinos during the explosion and converted to fluorine. In Wolf-Rayet stars (blue stars over 40 times heavier than the Sun), a strong solar wind blows the fluorine out of the star before hydrogen or helium can destroy it. In asymptotic giant branch (a type of red giant) stars, fusion reactions occur in pulses and convection lifts fluorine out of the inner star. Only the red giant hypothesis has supporting evidence from observations.
Waffles to space = 100% pure WIN.
What do you mean when you say oxygen is slightly heavier than fluorine?madd0ct0r wrote:how to get such a concentration of flourine though?
Oxygen is far more common, slightly less reactive and also slightly heavier. hmmm
Waffles to space = 100% pure WIN.
oxoiron wrote:What do you mean when you say oxygen is slightly heavier than fluorine?madd0ct0r wrote:how to get such a concentration of flourine though?
Oxygen is far more common, slightly less reactive and also slightly heavier. hmmm
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