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As the answer to this thread states, cooling superconductors in spacecraft is necessary because of waste heat from secondary systems and thermal radiation of the sun. The application in which superconductors are the most interesting to me is magnetically shielding spaceships from solar wind and galactic cosmis rays to reduce the radiation risks for manned spaceflight.

What I'm thinking about is getting rid of anything superfluous, making the system as simple as possible and just shooting it away from the ship with a conductive tether connected to the superconductive coil, which is itself connected to a large and thin reflective film that blocks heat from the sun. After positioning the solar shade, the coil should slowly radiate away energy and eventually become superconductive (at 10 Kelvin for conventional niobium-titanium alloy), right? You could then gradually add current to the coil until the magnetic field is strong enough to block harmful radiation.

Problems I see with this approach:

1) Orienting the solar shade

You can never let the coil heat beyond its critical temperature, so the solar shade has to stay in front of the coil at all times. This probably requires thrusters and a computer, which makes the solar shade a kind of mini satellite in itself.

2) Tethers, secondary systems and waste heat

The electrical energy comes from the conductive tether which is not a superconductor itself, so there'll be waste heat. Deflecting charged particles will also take energy, you constantly have to add new current to the coil. On top of that you probably also need a computer and something to monitor and regulate the coil, producing even more waste heat.

3) Magnetic field strength

The farther the magnetic shield is from the spacecraft the smaller is the amount of protection you'll get. If you get too close to the ship, thermal radiation from it might heat up your superconductor and the magnetic field will affect metal inside of it. Does the required distance from the craft give you enough protection to make this worthwhile?

4) Shutting the coil off

You can let it heat beyond the critical temperature, but the superconducting material will quench and release a lot of heat, which might damage it.

All in all, is this actually a feasible idea compared to just using active cooling?

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  • $\begingroup$ I think it would take some one familiar with the heat loads placed on super conducting materials, hence my comment rather than answer. But one potential concern is the poor cooling properties of objects in space. Without air currents to convect heat away, you're left with radiation only so it may be difficult to maintain superconducting temperatures without active cooling. $\endgroup$
    – Saiboogu
    Jun 25 '18 at 18:14
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    $\begingroup$ The JWST is a good model. That cools parts of the telescope to.39K passively. Other parts need active cooling to get down to 7K . So you could have a cuprate superconducting magnet passively cooled, but not a metal one. That's in a more or less ideal setting, with, sun, earth and moon always on the same side of the spaceship $\endgroup$
    – Steve Linton
    Jun 26 '18 at 8:52
  • $\begingroup$ "Shielding Space Explorers From Cosmic Rays" (Prof Eugene Parker) suggests that the magnetic field strength necessary to deflect particles would do biological harm of its own. $\endgroup$
    – Foo Bar
    Jun 27 '18 at 18:13
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A lot depends on the temperature requirements for your superconductors. That in turn depends on how much magnetic field you need, your mass budget for the coils, and how exotic a material you can afford.

There's a nice summary of (mostly active) space cryogenics here. Passive cooling to 50K has already flown on Planck (they were planning 60K, but did better), and the JWST is planning 40K.

The environment matters a lot. "Cooling" comes from radiating to space at ~5k (averaging over star flux in the local area of the Galaxy); heating comes from any local object. The more and larger shields you need for Sun, Earth, Moon, etc, the less solid angle you have to radiate to the rest of the sky.

JWST's 5-layer shield was designed to meet the requirement of no more than 2W passed flux, which in turn could be radiated to space for a telescope instrument temperature of 40K. Because flux goes like $T^4$, keeping all things the same, you'd need to drop the flux by a factor of $4^4 = 256$ to get to 10K. If everything was perfect, this would just require 2 (maybe 3) more layers.

But it's hard to keep such a shield perfect, and even a defect at the 0.1% level could let through enough heat flux to overwhelm the passive cooling by radiation. At some point, the requirement for perfection becomes too expensive.

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Deflecting charged particles will also take energy, you constantly have to add new current to the coil.

No, magnets do not change the energy of the particle, just their momentum. Otherwise permanent magnets wouldn't work constantly. But the momentum is transferred to the magnet, so you need active station keeping for it as well.

After positioning the solar shade, the coil should slowly radiate away energy and eventually become superconductive at 10 Kelvin

Yes, it will cool down, but likely not as much: There are crates close to the poles of the Moon that never receive sunlight. They have a temperature of about 100 Kelvin.

But, a solar shield doesn't protect you from all the heat the Sun delivers: Your solar shield will heat up and due to thermal conduction its backside will get warm as well. You can add more insulation in the shield, but this will not prevent the heat transfer, just making it slower. Once the shield is warm, it will radiate heat by itself and thus heat up the magnet coil. You will need some active cooling to keep the backside cold enough.

Also note that the distance of the shield doesn't matter: The closer it is, the smaller it can be. The amount of radiation the coil receives depends on the angular size (coverage of the hemisphere) of the shield, not its distance nor size.

Without doing the calculations: To reach such low temperatures, I assume you need, besides active cooling, a shield to protect the coil from radiation coming from Earth and possibly even the Moon.

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    $\begingroup$ The vacuum multi-layer insulation approach to a heat shield can reduce the thermal flux by $10^6$ or more. Each layer reflects part of the flux "upstream", and is cooler than the last. This is how the Webb Telescope will passively cool parts below 30K. There's some more info here: cas.web.cern.ch/sites/cas.web.cern.ch/files/lectures/… $\endgroup$
    – Bob Jacobsen
    Jun 27 '18 at 5:48
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    $\begingroup$ Maybe my assumptions are a bit too pessimistic, but I doubt that 10 K can be reached with any justifiable effort. $\endgroup$
    – asdfex
    Jun 27 '18 at 13:59
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To my knowledge the short answer is no probably not. You can assign a "temperature" to space which is the temperature at which the radiation from a perfect black body, matches the radiation striking the object. It is key to note here that an object will not radiate as much as a perfect black body so the equivalent temperature of the coil would be larger than the temperature assigned to space. I can't find any average estimates on what that temperature is in LEO, but we can assume that temperature is far above the operating temperature of a conventional superconductor. The lowest known equivalent temperature is 2.7 K far from any galaxy. If you were to place a solar shield out in front, or even completely enclose the exposed surfaces of the superconductor, eventually that shield/the entire craft would reach that equivalent temperature. That being said, that would likely take a long time. Additionally, shielding just the solar radiation would not be enough since we sit inside a galaxy. Based on what I've learned about heat transfer, without an active cooling system, this is not feasible. However, your idea may be able to significantly reduce the necessary amount of active cooling. Much of the details of this possibility HEAVILY revolve around the craft design, and exact orbits of the craft but based on my preliminary analysis, the best bet is that this could be used to increase the effectiveness of any cooling system implemented.

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    $\begingroup$ "It is key to note here that an object will not radiate as much as a perfect black body so the equivalent temperature of the coil would be larger than the temperature assigned to space." I don't believe this is correct at all. Objects will always eventually reach radiative equilibrium with their surroundings, and if their surroundings are nothing but 2.7 K CMB, they will inevitably hit 2.7 K themselves, whether they're composed of polished aluminum or pure graphite. $\endgroup$
    – Nathan Tuggy
    Jun 28 '18 at 15:11
  • $\begingroup$ @Nathan Tuggy I was under the impression that no matter radiates in the expected spectrum distribution of a black body and that it tends to be less emissive than expected, but if there's justification for that, I'll change it in my answer. That being said, my answer isn't that great anyways as it's for of a blob of my thought process looking back $\endgroup$
    – Gigaboggie
    Jun 28 '18 at 15:15
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    $\begingroup$ It's absolutely true that all matter radiates less than a black body because its spectrum is different, even radically different. But since emissive and absorptive spectra must be the same, an object in a single-temperature environment will always reach equilibrium at that temperature because the incoming radiation, which is the only ongoing source of heat, will eventually match outgoing. The time taken for this can vary wildly depending on emissivity, but it will always happen eventually. $\endgroup$
    – Nathan Tuggy
    Jun 28 '18 at 15:24

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