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Venus May Have Been Habitable, Says NASA (sciencedaily.com)
EzInKy writes: Science Daily has an article speculating that Venus may have been habitable which is suggested by NASA climate modeling, which proposes that Venus may have had a shallow liquid-water ocean and habitable surface temperatures for up to two billion years of its early history. Talk about global climate change run amok. Venus may represent a near Earth example of what is in store for the future of our world if we don't make it a number one priority to address. Science Daily reports: "Venus today is a hellish world. It has a crushing carbon dioxide atmosphere 90 times as thick as Earth's. There is almost no water vapor. Temperatures reach 864 degrees Fahrenheit (462 degrees Celsius) at its surface. Scientists have long theorized that Venus formed out of ingredients similar to Earth's, but followed a different evolutionary path. Measurements by NASA's Pioneer mission to Venus in the 1980s first suggested Venus originally may have had an ocean. However, Venus is closer to the sun than Earth and receives far more sunlight. As a result, the planet's early ocean evaporated, water-vapor molecules were broken apart by ultraviolet radiation, and hydrogen escaped to space. With no water left on the surface, carbon dioxide built up in the atmosphere, leading to a so-called runaway greenhouse effect that created present conditions."
And transmitted images digitally from the surface, in 1975. Cold War was a gift to mankind, that pissing match was legendary.
No, that's not "about it". The things that are earthlike include:
* Temperature
* Pressure
* Gravity
* Radiation shielding (compared to other destinations)
* Sunlight levels
* Atmospheric turbulence
The environment is amazingly earthlike, except for the chemistry. And concerning the chemistry....
The phrase "full of sulfuric acid" gives completely the wrong impression. The sulfuric acid mists in the cloud deck at reasonable heights (~54km., give or take a couple km) are on the order of half a dozen ppm. They're not much higher than the OSHA standards for breathing sulfuric acid mists during an 8 hour shift. Now, Venus's H2SO4 mists are a higher concentration than those on Earth, and there are also anhydrous acidic components. But comparisons to a bath in sulfuric acid are totally inappropriate. It's more like a bad smog or vog (in fact, it is a bad vog).
When you're talking about plastics (were you actually thinking that one would make a blimp's skin out of steel?), sulfuric acid is well tolerated by a large number, if not the majority of plastics. Organic solvents are much more concerning - I'd have much greater concerns for a blimp on Titan. Some fluoropolymers, like FEP and PTFE, are so chemical resistant that they're easier much defined by what does hurt them than what doesn't.
Realistic flight envelopes are not a single component. You generally will have an outer anti-corrosion layer (generally a fluoropolymer... the least fluorinated that provides the desired properties; ECTFE or PCTFE would be excellent), with one or more layers for permeation resistance and strength (generally biaxially-oriented when strength is of concern, like BoPET); for extra permeation resistance, something like EVOH or PVDC), optionally an inner layer (condensation control, anti-fouling, melt-through lamination, etc), optionally adhesive layers (such as EVA-based), and fiber reinforcement (vectran is popular for Venus proposals, although would be somewhat difficult for local production; on the opposite end of the spectrum, the easiest possibility for local production would be UHMWPE, but you'd need to ensure proper UV resistance and that the film components are compatible with the inevitable creep... though to be fair vectran also needs UV control) (there are countless fibers in-between with varying tensile, UV, chemical, creep, etc properties).
Beyond the basic skin you also need ballonets; most likely an additional phase-change envelope for altitude stability; catenary curtains and cables to distribute the weight to hanging structures; and in some cases, where objects need to be kept a minimum distance away from the envelope (such as propulsion), collapsible trusses. You also need mist collection for local propellant production (there are many different architectures, but they're all built around the fact that all of Venus's mists are highly hydrophilic and thus readily condense into water (through membranes or exposed) and onto hydrophilic surfaces. Lastly, if you use a ballute approach (for any combination of reentry, atmospheric deceleration, and/or initial inflation), you need a burble fence (which could potentially double as mist collection, depending on the architecture).
In cases where you might have exposed metal - such as propulsion motors (although even that isn't an inherent requirement) - there are a lot of alloys considered to be fine in Venus-conditions, and indeed which have been used on Venus probes in the past. An example includes Hastelloy C22. You may have noticed that here on Earth, metals in industry are frequently exposed to extremely corrosive chemical production environments for very long times. You design to your environment. A more
No, she's fine. My associate is vomiting for a totally unrelated reason.