xpell said:
Summary:: About the possibility of operating a VHTR or similar using the atmosphere of Venus as coolant.
However, I was wondering if a specially-engineered Generation IV high or very high temperature (800-1,000ºC) nuclear reactor could work in Venus using the local atmosphere at 450ºC as "coolant", just like a "typical" reactor operating at 300ºC works on Earth. If not, why not, please?
It is certainly an interesting idea to consider, and worthy of a homework problem in an advanced reactor and power plant course. One points to a domestic LWR with a peak temperature of ~300°C, which rejects heat at ambient temperature, ~25-35°C.
Thermodynamically, it is possible, although the thermodynamic efficiency would be limited. NASA puts the surface temperature at ~880°Fahrenheit (470°Celsius).
https://solarsystem.nasa.gov/planets/venus/in-depth/#otp_surface
One would probably want to use an open Brayton cycle, given that the atmosphere is mostly CO
2, some N
2 and traces of SO
2 (and sulfuric acid). "96.5%
carbon dioxide, 3.5%
nitrogen, and traces of other gases, most notably
sulfur dioxide."
https://en.wikipedia.org/wiki/Atmosphere_of_Venus#Composition
One could consider a direct open Brayton cycle in which the compressed atmospheric gases are passed through the core directly, assuming one could ensure integrity of the fuel in the core. Then there is the matter of leaving the reactor on the surface at the end of the mission, or launching it back to orbit.
Bear in mind, the Russian Venera program had some limited success: "Due to the extreme surface conditions on Venus, the probes could only survive for a short period on the surface, with times ranging from 23 minutes (Venera 7) to ~two hours (127 minutes, Venera 13)."
https://en.wikipedia.org/wiki/Venera
One would require an material with a reasonably high melting temperature. If the peak operating temperature is 1000°C (1273 K), then one would want a melting temperature (assuming an maximum operating homologous temperature of 0.5) of at least 2273°C (2546K), which doesn't leave too many choices. If one can limit the maximum stress in the system, one might be able to use a homologous temperature of 0.6, which would decrease the melting temperature to 1848°C (2126 K). There is usually a tradeoff among creep (based on maximum stress and temperature), maximum temperature and anticipated lifetime (service life, or mission duration).
There there is the matter of find that high temperature material with reasonable resistance to corrosion (thermochemical) degradation. So, one needs a structural material (probably an alloy) with a reasonably high strength at operating temperature and a protective coating that resists the corrosion of the working fluid, i.e., the atmosphere of Venus.
Others have pointed out challenges to electronics, and consequently, control systems.