In this episode of Brokonomics, I speak to Grant Donoghue, a Planetary Scientist at the University of Liverpool, about the future of the space industry. We discuss the logic behind the logic chain of the supply chain, and how space can become a major contributor to economic growth.
00:00:00.300Hello, and welcome to Brokonomics. Now, as you will know if you followed this show, I'm a tiny bit optimistic about things like AI and robotics and so on.
00:00:10.520Now, you start to follow through the logic of what that does. At the moment, most economic activity is constrained, not so much by the amount of resources,
00:00:20.300but quite literally, it's by the amount of management oversight, the amount of intellectual bandwidth going to something.
00:00:27.460I've worked with many companies over the years, and that ultimately tends to be the restraining factor on a lot of activity.
00:00:35.240After that, you've got the restraining activity, the restraint of the number of workers that you can bring in, people who can actually do the job.
00:00:43.680But with AI and robotics, it's not impossible that we could actually solve those two problems.
00:00:48.780If you do that, then the next logical step is that your constraint becomes the amount of resources available to you.
00:00:55.460And if you do that, then logically, the next major industry that we're not talking about at the moment,
00:01:02.780but we will be on the other side of AI and robotics, is going to be space,
00:01:07.300because that gives you access to the quantity of resources that you need to really take economic growth to an unlimited level.
00:01:14.400So, given that logic chain, I've been wanting to speak to somebody who knows about space.
00:01:20.120And I'm delighted to say that I have found just the man, Grant Donoghue, planetary scientist.
00:01:27.200Thank you so much. I'm very happy to be here.
00:01:29.920Good. Well, can you tell us about yourself? What is a planetary scientist?
00:01:33.940So, planetary science is a subfield of geology, which is an annoying term because geology specifically refers to the Earth.
00:01:40.820But I was trained as a sedimentary petrologist. Professionally, I've worked as both a petroleum and an environmental geologist.
00:01:51.840But more broadly, it means that I study the evolution of systems as the evolution of systems.
00:01:59.480We don't tend to say geology in isolation because we've discovered that there's an enormous amount of interaction between the lithosphere,
00:02:04.800the hydrosphere and the atmosphere, but considering one without the others is simply not reasonable, both on Earth and on other heavenly bodies.
00:02:13.860I see. OK, so you do you do Earth based geology as well.
00:02:17.940I mean, that that is probably helpful because one of the things I was thinking leading into this is how do planetary scientists get jobs?
00:02:24.700Because, you know, there can't be there can't be that much demand for it, given that we're not actually in space yet.
00:02:29.440But if you can do the geology bit as well, I guess that I guess you'll be going to be OK.
00:02:32.460Yes. So there are a number of Ph.D. programs, positions in academia, NASA, for example, who are looking into ISRU,
00:02:43.200a word I'm going to use a lot, in situ resource utilization for whom planetary scientists are of great interest.
00:02:49.100But that would be for someone who's who's more specifically focused on that.
00:02:54.040I I'm a mere mortal and the allure of the petrochemical industry and the greater opportunities there.
00:03:01.300They pay well. Yes. Got it right. But nevertheless, we could we could dream that, you know, 20 years down the line,
00:03:07.680there'll be there'll be real demand for the for the planetary side of your skill set.
00:03:11.160Yes. Getting getting to that point, where do you think we're kind of going to go first in terms of making use of space industry?
00:03:19.740Because I know there is. I mean, there's obviously quite a bit of space industry at the moment with the satellite systems that we have going around.
00:03:25.740And I understand things are getting pushed in that direction more and more.
00:03:28.780So, for example, because there's so much data basically up there in the lower Earth orbit,
00:03:33.360firms are starting to realise that actually it's cheaper to send data centres up into Earth orbit and process the data there than it is to sort of bounce it all backwards and forwards all day.
00:03:43.440And once you start, you know, once you start pushing more and more the value chain up into orbit,
00:03:47.720well, then you've got a growing industry and then it's a natural at some point to go beyond that.
00:03:51.980So what do you think of the sort of key drivers that are going to take us to make this a proper industry?
00:03:58.480Well, so studying there's a wonderful expression in the in geology, which was by Charles Lyon,
00:04:04.560who's along with Hutton, considered the father of geologists.
00:04:07.340He said the present is the key to the past.
00:04:09.900And so what we I think a principle we can extrapolate from that is that if we want to look at how we might expect the industrialisation to play out of space,
00:04:19.860we might it might be useful to examine how industrialisation played out or did not play out in the past.
00:04:25.300And so in that regard, I would say that where we are in space right now is similar to where the Romans were with the area pile,
00:04:32.280you know, the little thing that spun around in that we that the engineering and the technology is there.
00:04:38.620But because of a lack of resources or contravening economic motives, you know, for the Romans,
00:04:44.320it was the fact that they had no real call for labour saving devices.
00:04:48.620Labour was the one thing they had no no shortage of.
00:04:52.600That did much to to halt the advancement of that technology.
00:04:56.220There was no virtuous cycle that led to reinvestment and reinvestment, reinvestment.
00:04:59.980But by contrast, when industrialisation did kick off in the United Kingdom and the Low Countries and eventually the rest of Europe,
00:05:07.340there were a series of factors that drove it most principally when it comes to geology coal.
00:05:13.660England and Wales have the most bountiful resources of anthracite in the world, more or less.
00:05:19.820High quality coal that burns incredibly cleanly and it runs right to the surface.
00:05:24.320And so we we've been extracting coal since the 16th century.
00:05:28.420Railways actually predate the steam engine by 200 years.
00:05:31.060And a lot of people made a lot of money mining coal around southern England.
00:05:34.840But the one of the the interesting things that that affected that was that in Rome and Britain,
00:05:41.560the main thing that limited mining was that you would you wouldn't exhaust the material seams.
00:31:15.000If you were to take a good example of this is seawater.
00:31:18.120There's more gold dissolved in the ocean seawater than has ever been mined on Earth.
00:31:21.780But because the volume of water is enormous, trying to sift it for that concentration isn't economical.
00:31:29.420On the moon, you can find traces of metals pretty easily.
00:31:33.240It's just coming down to are you going to find ores?
00:31:35.960And the trouble with that is that the things that create ores on Earth are a large number of processes that require an atmosphere and a hydrosphere.
00:31:45.340So, again, an example of this is placer deposits.
00:31:48.640A placer deposit is where you get a situation where uranium, most of the uranium on Earth comes from placer deposits where you have water flowing and uranium, small uranium particles, which are present in volcanic rocks.
00:32:55.580And then I'm wondering, OK, well, what about Venus and Mars, which we might reasonably have assumed at some point in the past may have had ocean and a, you know, some proto ecology system.
00:33:25.060Most of our iron comes from something called a banded iron formation, which is where you have microbes on Earth that were taking iron ions and building them up.
00:33:35.080And so you can get these enormous layers, meters and meters thick of iron, chert, iron, chert, iron, chert.
00:33:40.360And these were assembled over millions of years.
00:33:42.720And this is where like 85 percent of our iron ore comes from.
00:33:45.900There are other sources of iron ore that don't need life, but they're much less concentrated, much less common.
00:33:51.280So on the moon and on Mars, the moon and Mars, I'll start with first, we have reason to believe they have a similar geological model, which is called stagnant lid, where the primordial heat trapped by a body is not enough and the radioactive decay is not enough to keep the lid mobile.
00:34:14.100The mantle heat is not producing enough heat that it breaks through and tries to get to the surface, as opposed to Earth, where we have a tectonic lid.
00:34:22.720Is that largely a function of their smaller size?
00:34:37.320And so on Earth, our larger size means that we trapped a lot more heat during formation, primordial heat, and we also have a lot more heavy elements that are undergoing radiometric decay and generating heat inside the planet.
00:34:52.200And so on Earth, that's why we still have active volcanism.
00:34:55.920There isn't active volcanism on Venus.
00:34:57.580There isn't active volcanism on the moon.
00:35:00.800Sorry, there isn't active volcanism on Mars or the moon.
00:35:05.980But on Venus, as of three months ago, we've proved those active volcanism.
00:35:12.080Yes, I understand it's got more volcanoes than anywhere else in the solar system.
00:35:36.540And so we needed to, when we were surveying it, use something that had a high enough wavelength that it wasn't going to interfere with the atmosphere of CO2.
00:35:53.460So if you were to study, for example, a mountain on Venus, that might only be one or two pixels.
00:36:03.620And so we've had a very hard time learning about the surface of Venus.
00:36:07.780And also, since the Soviets went there, we've invested almost nothing in exploring it.
00:36:12.380Venus has been really neglected because people saw it as a hell world, and we said, well, there's not life there.
00:36:16.980It's just a big ball of rock, CO2, basaltic minerals.
00:36:20.600Why would we expect anything to be of value there?
00:36:23.840And so finding out that unlike every other planet in the solar system that we know, it didn't just have historical volcanism, but volcanism is still going on.
00:36:33.840And it's not like Io, where it's driven by tidal heating.
00:36:39.440And that has inspired a lot of active investigation.
00:36:41.660And so my idea that I discussed in that podcast of, well, you just put a cloud city up there, and you float above the clouds, and then you use, again, sort of in-situ 3D printing and robots and stuff.
00:36:53.680You send them down, you stick them under a dome, and you heat-bent it.
00:36:58.820With regards to human habitation, that's probably the only way you would want to try and do it, without the sort of terraforming that you can only do once you've won the game of civilization, once resource scarcity just no longer exists.
00:37:12.740Because at that level, first of all, the delta V to get from the surface of Venus to orbit is three times the delta V to get off the surface of Earth, because of the incredibly thick atmosphere.
00:37:25.300Venus also, because of its incredibly slow and retrograde rotation, it's rotating the wrong way around and incredibly slowly, doesn't give you a gravitational assist getting into an orbit.
00:37:43.880So you'd think that it'd be easier getting off the surface, but the bit of the atmospheric drag, which is a much smaller part on Earth, becomes a hugely significant factor, presumably, than in Venus.
00:37:58.060And also, the other thing you do on Earth is you launch as close as you can to the equator, because that spin of the Earth, it doesn't give you much, but every little helps.
00:38:07.260When you're dealing with that, and that helps you get off.
00:38:09.900But of course, yeah, so Venus has the thick atmosphere, and the spin goes the wrong way, so it doesn't help you at all.
00:38:15.380So everything is, so the surface is a bit of a bitch.
00:38:19.300It absolutely is, but the weird side factor of that is there is a resource on the surface which doesn't need geology to be concentrated, which is very exciting, which is silica.
00:38:32.680Silica, we know that the Venezian crust is rich in silica.
00:38:36.880It's covered in basaltic rock, which can be like 50% to 70% silica by weight, and if you have silica, and you have hydrogen, which you can get from the sulfuric acid clouds, you can make silane, and silane burns in CO2.
00:38:55.700CO2 can be an oxidizer to silane, which means you can get craft, which, a bit like on Earth, when you have a jet engine, unlike a rocket, it doesn't need to also carry an oxidizer.
00:39:10.300On Earth, the reason a plane is more efficient than a rocket is because it can get its oxidizer, oxygen, from the atmosphere, but a rocket needs to carry both.
00:39:20.120Well, if you have a silane-based propulsion system, there's an enormous disadvantage, which is you can probably only use them once, but the advantage is you don't need to carry the oxidizer.
00:39:31.600The reason you probably can only use them once is one of those products is solid.
00:39:38.800It's not clear to me what the useful takeaway from this is.
00:39:42.540I mean, is this going to give you propulsion within the atmosphere of Venus, or more broadly than that?
00:39:47.940It would give you a way to go from your cloud city to low Venusian orbit without spending an arm and a leg.
00:39:53.780You can use a rocket plane, and because of the relative buoyancy, you can float on Venus at 50 kilometers up incredibly easily.
00:40:05.180The CO2 is much denser, and because hydrogen doesn't burn in it, you can get enormous buoyancy forces.
00:40:10.800And so if you take off from 50 kilometers up, you get to avoid the incredibly thick atmosphere.
00:40:14.300In fact, the atmospheric drag is slightly less than Earth, and by not needing to carry an oxidizer, and because of the lower mass, if we can get jet planes working on Earth, that is to say, a craft that can get you to orbit, and then you have a rocket meet it, that's a much cheaper launch.
00:40:33.560And it's easier to get working on Earth.
00:40:58.960But presumably that would be significantly easier on Venus because of the density of the atmosphere.
00:41:04.240It's easier on Venus for a number of reasons.
00:41:09.140First of all, even though Silane has a relatively low specific impulse and you can only use it once, because it can be used at any altitude in the Venusian atmosphere, you can use that to communicate resources from the surface to your sky city and from your sky city to low Earth orbit where it meets with a rocket.
00:41:29.340And then that rocket can go off into the solar system.
00:41:31.640And the reason that's important is because Venus is very good for supporting the second and third stages of space industry because it has abundant sulfur.
00:42:02.880That's actually the term in ore processing.
00:42:04.140Because if you have an asteroid, instead of needing to drill it, imagine if you build a space station that's rotating.
00:42:13.180You know the concept in sci-fi where you generate an artificial gravity by spinning.
00:42:17.340Instead, you have a cylinder and then you spin it and you're on the inside of the cylinder and you stick to the outside.
00:42:25.340Like those old-fashioned fairground rides that spin around and then go up.
00:42:28.180Exactly. You can do the same thing where you fill it, you crush an asteroid, you take big chunks of an asteroid, crush it, and then inject high-temperature CO2.
00:42:36.400And the minerals will simply be, the valuable material will be leached out by the centrifugal forces.
00:42:42.820It will differentially separate because of the higher mass.
00:42:46.160So actually Venus is very, very viable for that phase that we're talking about, which is going to be the key driver, which is the gas station bit.
00:43:02.720That then gets us to Venus and it gives us all of the things you've just talked about that support fleshing out that industry significantly,
00:43:10.220which then enables us to go to the asteroid belt.
00:43:14.280And with the resources that we took from Venus via the moon, via Earth, we can then start, well, basically we have, not unlimited,
00:43:23.040but from our perspective right now, almost unlimited amounts of useful metals and other stuff that if our in-situ,
00:43:30.340our 3D printing is sufficiently developed to that point, I mean, you could start building pretty much anything you want.
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