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posted by martyb on Monday April 24 2017, @04:18AM   Printer-friendly
from the power-to-the-lander dept.

On Wednesday, April 19th, in a seminar titled "An Air-Breathing Metal-Combustion Power Plant for Venus in situ Exploration", NASA engineer Michael Paul presented a novel idea where existing technology could be used to make longer-duration missions to Venus.

To recap the history of Venus exploration, very few probes have ever been able to explore its atmosphere or surface for long. Not surprising, considering that the atmospheric pressure on Venus is 92 times what it is here on Earth at sea level. Not to mention the fact that Venus is also the hottest planet in the solar system – with average surface temperatures of 737 K (462 °C; 863.6 °F).

Hence why those few probes that actually explored the atmosphere and surface in detail – like the Soviet-era Venera probes and landers and NASA's Pioneer Venus multiprobe – were only able to return data for a matter of hours. All other missions to Venus have either taken the form of orbiters or consisted of spacecraft conducting flybys while en route to other destinations.

[...] "What can you do with other power systems in places where the Sun just doesn't shine? Okay, so you want to get to the surface of Venus and last more than a couple of hours. And I think that in the last 10 or 15 years, all the missions that [were proposed] to the surface of Venus pretty much had a two-hour timeline. And those were all proposed, none of those missions were actually flown. And that's in line with the 2 hours that the Russian landers survived when they got there, to the surface of Venus."

The solution to this problem, as Paul sees it, is to employ a Stored-Chemical Energy and Power System (SCEPS), also known as a Sterling[sic] engine. This proven technology relies on stored chemical energy to generate electricity, and is typically used in underwater systems. But repurposed for Venus, it could provide a lander mission with a considerable amount of time (compared to previous Venus missions) with which to conduct surface studies.

For the power system Paul and his colleagues are envisioning, the Sterling[sic] engine would take solid-metal lithium (or possibly solid iodine), and then liquefy it with a pyrotechnic charge. This resulting liquid would then be fed into another chamber where it would combined with an oxidant. This would produce heat and combustion, which would then be used to boil water, spin turbines, and generate electricity.

Such a system is typically closed and produces no exhaust, which makes it very useful for underwater systems that cannot compromise their buoyancy. On Venus, such a system would allow for electrical production without short-lived batteries, an expensive nuclear fuel cell, and could function in a low solar-energy environment.

Stirling engines could extend the mission durations.


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  • (Score: 2) by VLM on Monday April 24 2017, @04:58PM

    by VLM (445) Subscriber Badge on Monday April 24 2017, @04:58PM (#498944)

    There's a lot of indoctrination in the USA about the trivia fact (which is true) that the surface of Venus is hotter than the surface of Mercury due to the greenhouse gas effect. If normies know anything about Venus, they know its hot. So a layer of high altitude atmosphere at a low but survivable pressure that's kinda cold by earth standards is a bit of cognitive dissonance to "all I know is its the hottest surface temp in the solar system". It probably varies by country and education system.

    Its an interesting trivial pursuit problem of another sort to wander thru the solar system and find locations where the temp and pressure are simultaneously human survivable. There's aren't many places off the earth other than that 55 KM level of atmosphere in Venus.

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