Electric Propulsion Magnets Ready for Space Tests
spectrum.ieee.org
spectrum.ieee.org
Thanks for providing the trigger for my insight.
But it doesn’t apply when you’re collecting energy in situ. The article proposes solar panels. Rocket/wagon equation doesn’t apply.
Break out exhaust velocity.
I get that means zero electrical resistance and stronger magnetic field at rest, but ultimately the engine is doing work accelerating ions, which will be "felt" as resistance in the electrical system. The total energy must be conserved. I would imagine (?) that work done accelerating the ions is far greater than the losses to heat in the magnetic coils.
Or maybe that's not right?
[1] https://www.sciencedirect.com/science/article/pii/S277283072...
The next type of efficiency is how much of the source energy is converted into the energy of the plasma jet. Is it 50%, 90%, 99%. That I don't know, and obviously you want as much as possible.
But this project is addressing a different problem. In order to create this plasma jet, you need a very strong magnetic field to contain the plasma while it is being accelerated. The field itself does not provide the propulsion, it is there only for containment. You don't want to expend a lot of energy maintaining this field. Superconducting magnets are much better than regular electromagnets, so it's no surprise that containing this plasma with superconducting magnets requires a fraction of the power of regular magnets. But someone still needed to do the actual research. What works on paper doesn't translate always in things that work in real life. These guys did just that, and now are ready to send a technology demonstrator in space.
[1] https://en.wikipedia.org/wiki/Magnetoplasmadynamic_thruster
But yes, today’s design space generally prefers as low a power envelope as possible to not have to worry about dissipation.
P = ε * σ * A * T^4
That's the constant, the emissivity of the material, the surface area A, and temperature.
We want to increase the temperature differential above what the natural black body radiation can dissipate for a given device (let's take a space probe) and assume we can't change the material. The only thing we can play with is surface area.
The point of the nitrogen gas is to leverage normal convection / conduction to dissipate into a larger gaseous volume which then naturally also has a larger surface area. This would then give you more surface area to dissipate across. The reason I'm thinking the layering with different pressure gradients might be useful is that it reduces the overall weight because you need less overall gas for a given dissipation profile (i.e. you need high density beside your heat source to transfer energy away quickly but less density further away because there's a larger surface area growing with the square of the distance away from the heat source).
[1] https://en.wikipedia.org/wiki/Stefan%E2%80%93Boltzmann_law
[1] Colgan Mass Optimization [...] Forced-Convection Heat Exchanger for Mars Surface Waste Heat Rejection 2023 https://asset.library.wisc.edu/1711.dl/FYJCG5YME7O4X82/R/fil...
You have to simultaneously solve for power to weight ratio issues on solar panels, power supply, and the actual thruster. The best solutions right now for most purposes are relatively low Isp (low propellant efficiency) Hall thrusters.
In space, heat dissipation is remarkably harder than it is on Earth, so getting to, for example, 97% thermal efficiency rather than 94% would be a big deal in terms of the mass of the heat dissipation system, and I think this and reducing the mass of the actual electromagnet is the advance here, if there is any.
The starship in Avatar got that right. Rest of the film is comic book level and derivative but the ship is good.
https://toughsf.blogspot.com/2019/10/the-expanses-epstein-dr...
This thing would produce more power than all of civilization does today. No radiator could handle it. They use laser fusion, exploding D-He3 fuel pellets well behind the ship, with a giant magnetic nozzle. A tungsten heat shield protects the ship, and reaches an equilibrium temperature without active cooling.
Talking about thermal and propulsive efficiency for a rocket is a little tricky because there are multiple useful metrics, but in this context "waste heat" is anything that doesn't get tossed out the back.
They for sure expect better than the ones currently in use/testing (e.g. the nstar ion thruster)
I'm sure that others, here are far more conversant with the tech, but it's my understanding that one of the attributes of superconducting magnets, is that the very strong field is extremely localized. It doesn't extend too far from the magnet.
Its also for these reasons making a very large nuke is pointless, after some distance the effects are almost 0.
Might just be a manifestation of the Inverse Square Law. Like I said, not my area of expertise.
Sure the biggest ones are comparatively ineffective, thats why the focus on manufacturing was on small/medium yield one, one can produce many more and saturate defenses more easily rather than one/few MOABs.
But heat itself can be imagined as a kind of field. For eg: A candle, the closer you move to the flame, every point closer to flame, the temperature is higher. The farther you move apart the temperature reduces. Same with the Sun.
Take for eg- Sound. The closer you move to the source of it, the louder it sounds, the farther you move from it, the fainter it gets.
Now you could call this a wave. Like the wavelength stretches with distance, also decreasing frequency and amplitude. Another way of looking at this a field. Imagine 3D space with points, like a lattice. Each point has a value, and the values get denser to the center, and move farther apart as move away from center.
If Im not wrong a lot of physical phenomenon exhibit this behaviour. Including thing like light, sound, temperature, gravitation etc.
While you can make a beam of light, I doubt you can make a beam of magnetic field(ray?) or gravity for that matter?
heat: ∂u/∂t = k ∂²u/∂x²
wave: ∂²u/∂t² = c² ∂²u/∂x²
Note the extra time derivative on the wave equation. The heat equation is dissipative, moving towards the average value, spreading energy out over time. The wave equation, on the other hand, allows for solutions that oscillate and maintain their shape while they travel.This means that waves such as electromagnetic (light) or gravitational can in theory be focused and beamed significant distances without much loss. A plane wave solution is lossless, but requires an infinite emitter.
Finally, note that this does not apply to static fields, such as magnetic, electric, or gravitational fields, which if not oscillating will still spread out and dissipate over distance.
Bug normal magnets and superconductor magnets have canceling magnetic charge, the same amount of S and N, so after a few math tricks [1] the field will be inversely proportional to the cube of the distance.
[1] The filed from N decays as 1/r^2 and the field form S as -1/r^2 but they are indifferent places (the r is not the same on both), so the difference is almost like 1/r^3 more details in https://en.wikipedia.org/wiki/Multipole_expansion
Sometimes I wish Xanadu had actually happened. The moment I opened the article I saw something like |R^3. Honestly speaking I don't really know what |R means. And R keeps showing up all over the article.
I will dig more into this using ChatGPT with time.
But I could understand very little from reading the article.
Edit: we also have in there "the coefficients of the multipole expansion can be written as functions of the distance to the origin, r", so it sounds like r in italics is the origin - but that's usually (0, 0, 0), so maybe it's a distance to it. Anyway r in bold is probably a vector, vectors are usually in bold. And you're quite right about Xanadu, I wonder if there's some way to overhaul Wikipedia to put a key to notation in the sidebar of all pages with equations in.
What other space apart from 3 dimensional space exists? And what does that even mean?
https://en.wikipedia.org/wiki/Spatial_gradient
And you could have a gradient (of colors if you like, or salinity or force of whatever) along a line, one dimension, or on a plane, two dimensions, or in space, three dimensions. By extension, just adding components to vectors and iterating over the components when you do stuff with them, you can apply the same logic about higher dimensions. This makes people thin and unhealthy and serves no purpose, but seems to have a compulsive appeal for a certain kind of mind.
You can't always reliably extend some idea to different numbers of dimensions, because the interactions between components can get complicated, sometimes a thing that's valid for certain numbers of dimensions is not in fact valid for other numbers of dimensions, like maybe you have to have a odd number of dimensions to prevent positives and negatives cancelling out or something. Like many people, I knew this stuff for about a month once but forgot the specifics. But a tesseract is kind of fun to look at.
https://en.wikipedia.org/wiki/Tesseract
This is like the next step in the sequence dot, line, square, cube. The animation is a "projection into 3 dimensions", like how the shadow of a cube on a piece of paper is in two dimensions. It can't be shown in four dimensions, due to four dimensions being complete fiction.
(It's squirming like that because it's rotating, but the axis it's rotating around is at some 4D angle.)
Aside from the one and two-dimensional spaces mentioned in a sibling comment (ℝ¹ and ℝ²), there's also spaces with more interesting geometry.
For example, S² is the two-sphere, more conventionally known as "the surface of a ball." On the sphere, the equivalent of straight lines are the great circles. S¹ would be the one-sphere (the circumference of a circle), and S³ would be an interesting, periodic three-dimensional space – kind of like what our universe would be if it were closed rather than (probably) open.
The magnet's geometry and intensity are what define the field, not the material.
There's certainly zero chance that it could be on the moon. It wasn't designed to survive on a surface. It would not be able to support itself.
If we want something in orbit around the moon, it will still be far cheaper to build a new thing designed for that purpose.
Rendezvouzing and pushing or pulling a 900K lb (350K kg) object in orbit has never been demonstrated.
In-orbit outer hull repair on a vessel with occupants has also never been demonstrated?
Are there NEO avoidance plans that do not involve fracturing the object into orbital debris on approach?