Space mining economics

By Thomas Wood (@advanced-eschatonics.com)
Published:

SpinLaunch: Hype or Future of Aerospace?

So I saw an article on Spinlaunch and they're using a centrifuge to get a rocket up to 5000 mph before release and I'm like what are the forces on the projectile when it hits atmosphere? So I asked o3 and here's its response:

1 What the vehicle experiences the instant it meets the outside air

When the dart-shaped launch vehicle punches through the very thin Mylar membrane that seals the centrifuge, the surrounding pressure jumps from ~0 Pa (hard vacuum) to ~101 kPa (sea-level air) in less than a millisecond. At 5 000 mph (≈ 2 240 m s⁻¹, ≈ Mach 6.5) the key numbers are:

• Dynamic pressure q = ½ ρ V² ≈ ½ (1.225 kg m⁻³)(2 240 m s⁻¹)² ≈ 3.1 MPa ≈ 30 atm For comparison, the “max-q” a Falcon 9 sees is ~40–50 kPa; SpinLaunch’s dart must shrug off ~60× higher aerodynamic loads.

• Stagnation temperature rise ΔT = V²/(2 cp ) ≈ 2 240² /(2 · 1 005) ≈ 2 500 K. The nose momentarily sees > 2 700 K, hotter than steel’s melting point, so the tip must be a refractory metal or an ablative.

• Initial drag deceleration (ballistic-coefficient β = m/(Cd A) ≈ 10 000 kg m⁻² for the 200 kg, 0.35 m-diameter dart SpinLaunch describes) a = q C_d A /m ≈ 3.1 MPa × 0.2 × 0.096 m² / 200 kg ≈ 30–40 g Because air density falls roughly exponentially, the peak lasts only a few-tens of milliseconds; within the first second the vehicle has climbed ~1 km and q has dropped by roughly a factor of two.

2 Does that destroy the vehicle?

• Structure A 200-kg tungsten-nose, carbon-fiber body could be built strong enough for 3 MPa loads; the internal electronics already have to survive 50 000–100 000 g during the 30-min spin-up . • Heating The heat pulse is short. Total heat load (ρ V³ Δt) over the first 0.1 s is similar to what a re-entry vehicle sees high in the atmosphere; an ablative or copper-alloy nose tip and a thin cork or PICA sleeve are probably sufficient. • Guidance/booster SpinLaunch avoids fragile liquid plumbing; the second-stage solid booster lights ~60 km up, after the dart has coasted for ~80 s when dynamic pressure has fallen below ordinary rocket values .

3 Why “it’s still really hard”

BigThink’s review lists the main hurdles: surviving the 25-fold higher impact on the rupture disk, unprecedented peak drag forces, and the need for all-solid propulsion . None of those are show-stoppers individually, but together they make the engineering margin razor-thin; a tiny manufacturing flaw (foam on Columbia’s wing is the cautionary tale) can liberate tens of kilojoules at these speeds.

4 Bottom line

The dart does not instantly vaporize, but it is smacked by roughly 30 atmospheres of dynamic pressure and a 2 500 K stagnation shock for a few-tens of milliseconds, then rapidly climbs into thinner air. With extreme materials and careful shaping this is survivable, yet it is far beyond the aerodynamic load envelope of any current launch vehicle. Whether SpinLaunch can turn that “barely survivable” transient into day-in, day-out reliability remains the open—and very expensive—question.

So it is feasible

I was like well damn then okay. Next question: what does this mean for asteroid miners?

The response:

Can SpinLaunch-style launches work for asteroid-mining robots?

Short answer: Yes, in principle you could fire very rugged, compact mining robots or robot sub-assemblies with a centrifuge, but the concept forces you into extreme design choices—tiny payload mass (<200 kg each), 10 000–20 000 g loads, no liquids, very high drag/heating at exit, and you still need an upper-stage rocket to finish orbit insertion and then an interplanetary transfer stage. For most foreseeable asteroid-mining architectures those constraints erase much of the cost benefit over a conventional small-launch vehicle.


1 The centrifuge’s intrinsic limits

| Item | Typical SpinLaunch number | Consequence for mining robots | |------|--------------------------|--------------------------------| |Tip speed | 2.2 km s⁻¹ (≈5 000 mph) | Only ~⅓ of the ≈7.8 km s⁻¹ needed for LEO, so a kick-stage is mandatory.| |Peak radial acceleration| 10 000–20 000 g during spin-up | Any mechanism must be purely solid-state or flexure-based; bearings, solder joints, batteries and optical components must be specially ruggedized.| |Payload envelope | ≈ 2 m × 0.4 m dia, ≤200 kg | Drives you toward “micro-crawler” or “lego-brick” style robots that self-assemble later.| |Exit environment | 3 MPa dynamic pressure, 2 500 K stagnation T for ~10 ms | Outer structure must be ablative or tungsten-tipped; no fragile antennas or solar wings can be exposed.| |Vacuum launch tube | Cannot contain propellants or cryogens | Upper stage must be solid rocket or sealed pressure-fed monoprop.|

These numbers are heroic even for defense projectiles; for comparison, the NASA Robotic Asteroid Prospector study assumed a conventional launch and gentle 6–10 g loads .


2 What parts of a mining architecture survive 10 000 g?

• Electronics & sensors – modern silicon dies and MEMS gyros actually tolerate 20 000 g if potted; flash memory survives >50 000 g in artillery shells. • Actuators – brushless DC motors withstand the load provided the rotor is radially pre-loaded; harmonic drives or cycloidal gears outperform ball screws. • Energy storage – Li-ion cells rupture above ~6 000 g unless they’re tiny; primary Li-SOCl₂ cells in metal cans fare better. Super-capacitors are even sturdier. • Propulsion tanks – pressure vessels with nitrous oxide, hydrogen peroxide or solid propellant grains are fine; cryogenic tanks are impossible. • Delicate mechanisms (deployable solar wings, sample-handling arms) must launch as nested, crush-packed parts to be assembled robotically after orbit, much like CubeSat deployables.

The upshot: a “seed factory” concept—lots of billiard-ball-strong parts that re-assemble into a larger miner at an L1 staging point—fits far better than firing a finished ̶m̶o̶b̶i̶l̶e̶ ̶e̶x̶c̶a̶v̶a̶t̶o̶r̶.


3 Mass economics versus conventional rides

A small dedicated rocket such as Rocket Lab’s Electron currently charges ≈US$7 M for 200 kg to LEO (≈$35 k kg⁻¹). SpinLaunch’s goal is “sub-$500 kg⁻¹” for the first 200 kg, but:

If your asteroid-mining business plan needs hundreds or thousands of identical launches per year, those fixed-cost penalties can be amortized; if you’re flying a few dozen precursor robots (e.g., Asteroid Mining Corporation’s 20 kg SCAR-E prospectors ), a conventional microlauncher is cheaper and lower risk.


4 Trajectory implications

A centrifuge throw gives Δv ≈ 2.2 km s⁻¹ horizontally. After the solid kick-stage circularises LEO, you still need another 2–3 km s⁻¹ of high-Isp Δv to rendezvous with a near-Earth asteroid. Electric propulsion packages (Hall thrusters or electrospray) survive g-loads well and can be fired later. In fact, Lewis and co-authors highlighted self-refueling electric tugs as the key mass lever for asteroid mining.

So the SpinLaunch leg saves only ~2 km s⁻¹ out of a 10–12 km s⁻¹ end-to-end delta-v chain. That is helpful but not revolutionary.


5 Bottom line

• SpinLaunch can, in theory, loft very rugged, component-level hardware for an asteroid-mining enterprise. • Anything with fluids, large deployables or precision mechanisms must be redesigned or launched the old-fashioned way. • The business case closes only if you plan factory-scale launch cadence and are willing to pay the upfront engineering premium for 10 000-g survivability.

For early prospecting and first-generation off-world manufacturing, ordinary small rockets remain the saner path; a centrifuge launcher might become attractive later, when the goal is to toss out hundreds of identical “nuts-and-bolts” packages once a mature space-mining infrastructure already exists.


So yeah

It's pretty cool. Some very hard constraints on the kind of payloads you can put in orbit, but potentially a game changer, especially if existing orbital manufacturing infrastructure already exists and you're just shipping up whatever can't be sourced upstairs.