Thermodynamics and Propulsion
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THERMODYNAMICS: COURSE INTRODUCTION
Course Learning Objectives:
To be able to use the First Law of Thermodynamics to estimate the potential for thermo-mechanical energy conversion in aerospace power and propulsion systems.
- To be able to state the First Law and to define heat, work, thermal efficiency and the difference between various forms of energy. (quiz, self-assessment, PRS)
- To be able to identify and describe energy exchange processes (in terms of various forms of energy, heat and work) in aerospace systems. (quiz, homework, self-assessment, PRS)
- To be able to explain at a level understandable by a high school senior or non-technical person how various heat engines work (e.g. a refrigerator, an IC engine, a jet engine). (quiz, homework, self-assessment, PRS)
- To be able to apply the steady-flow energy equation or the First Law of Thermodynamics to a system of thermodynamic components (heaters, coolers, pumps, turbines, pistons, etc.) to estimate required balances of heat, work and energy flow. (homework, quiz, self-assessment, PRS)
- To be able to explain at a level understandable by a high school senior or non-technical person the concepts of path dependence/independence and reversibility/irreversibility of various thermodynamic processes, to represent these in terms of changes in thermodynamic state, and to cite examples of how these would impact the performance of aerospace power and propulsion systems. (homework, quiz, self-assessment, PRS)
- To be able to apply ideal cycle analysis to simple heat engine cycles to estimate thermal efficiency and work as a function of pressures and temperatures at various points in the cycle. (homework, self-assessment, PRS)
- Detailed lecture notes are available on the web (for viewing and/or downloading). You should download a copy of these and bring them with you to lecture.
- Preparation and participation will be important for learning the material. You will be responsible for studying the notes prior to each lecture. Several reading assignments will be given to help promote this activity (1/3 of participation grade).
- Several active learning techniques will be applied on a regular basis (turn-to-your-partner exercises, muddiest part of the lecture, and ungraded concept quizzes). We will make extensive use of the PRS system (2/3 of participation grade).
- Homework problems will be assigned (approximately one hour of homework per lecture hour). The Unified Engineering collaboration rules apply.
Solar power stations in space could be the answer to our energy needs
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It sounds like science fiction: giant solar power stations floating in space that beam down enormous amounts of energy to Earth. And for a long time, the concept – first developed by the Russian scientist, Konstantin Tsiolkovsky, in the 1920s – was mainly an inspiration for writers. A century later, however, scientists are making huge strides in turning the concept into reality. The European Space Agency has realised the potential of these efforts and is now looking to fund such projects, predicting that the first industrial resource we will get from space is “beamed power”.
Climate change is the greatest challenge of our time, so there’s a lot at stake. From rising global temperatures to shifting weather patterns, the impacts of climate change are already being felt around the globe. Overcoming this challenge will require radical changes to how we generate and consume energy.
Renewable energy technologies have developed drastically in recent years, with improved efficiency and lower cost. But one major barrier to their uptake is the fact that they don’t provide a constant supply of energy. Wind and solar farms only produce energy when the wind is blowing or the sun is shining – but we need electricity around the clock, every day. Ultimately, we need a way to store energy on a large scale before we can make the switch to renewable sources.
A possible way around this would be to generate solar energy in space. There are many advantages to this. A space-based solar power station could orbit to face the Sun 24 hours a day. The Earth’s atmosphere also absorbs and reflects some of the Sun’s light, so solar cells above the atmosphere will receive more sunlight and produce more energy.
But one of the key challenges to overcome is how to assemble, launch and deploy such large structures. A single solar power station may have to be as much as 10 kilometres squared in area – equivalent to 1,400 football pitches. Using lightweight materials will also be critical, as the biggest expense will be the cost of launching the station into space on a rocket.
One proposed solution is to develop a swarm of thousands of smaller satellites that will come together and configure to form a single, large solar generator. In 2017, researchers at the California Institute of Technology outlined designs for a modular power station, consisting of thousands of ultralight solar cell tiles. They also demonstrated a prototype tile weighing just 280 grams per square metre, similar to the weight of card.
Recently, developments in manufacturing, such as 3D printing, are also being looked at for this application. At the University of Liverpool, we are exploring new manufacturing techniques for printing ultralight solar cells on to solar sails. A solar sail is a foldable, lightweight and highly reflective membrane capable of harnessing the effect of the Sun’s radiation pressure to propel a spacecraft forward without fuel. We are exploring how to embed solar cells on solar sail structures to create large, fuel-free solar power stations.
These methods would enable us to construct the power stations in space. Indeed, it could one day be possible to manufacture and deploy units in space from the International Space Station or the future lunar gateway station that will orbit the Moon. Such devices could in fact help provide power on the Moon.
The possibilities don’t end there. While we are currently reliant on materials from Earth to build power stations, scientists are also considering using resources from space for manufacturing, such as materials found on the Moon.
Another major challenge will be getting the power transmitted back to Earth. The plan is to convert electricity from the solar cells into energy waves and use electromagnetic fields to transfer them down to an antenna on the Earth’s surface. The antenna would then convert the waves back into electricity. Researchers led by the Japan Aerospace Exploration Agency have already developed designs and demonstrated an orbiter system which should be able to do this.
There is still a lot of work to be done in this field, but the aim is that solar power stations in space will become a reality in the coming decades. Researchers in China have designed a system called Omega, which they aim to have operational by 2050. This system should be capable of supplying 2GW of power into Earth’s grid at peak performance, which is a huge amount. To produce that much power with solar panels on Earth, you would need more than six million of them.
Smaller solar power satellites, like those designed to power lunar rovers, could be operational even sooner.
Across the globe, the scientific community is committing time and effort to the development of solar power stations in space. Our hope is that they could one day be a vital tool in our fight against climate change.
Can China Break Airbus and Boeing’s Aviation Duopoly ?
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As the COMAC C919 nears its final certification in 2021, it might be interesting to see what we can expect from this aircraft. The C919 features CFM LEAP-1C engines and can seat up to 168 passengers. The narrowbody jet is targeted at ending the duopoly of Boeing 737 and Airbus A320, which overwhelmingly lead the market.
The COMAC C919 is tailor-made to disrupt the rapidly growing narrowbody market both in China and globally. The aircraft has a range of 2,200 nautical miles, enough for most domestic Chinese and regional routes. The C919 can seat 158 to 168 passengers depending on the cabin layout, an important factor for high-demand routes.
Comparing this to the 737 MAX and A320neo, we see some similarities and differences. The former has a range of 3,550nm and the latter 3,400nm, both being far ahead of the 2,200nm offered by the C919. However, all three planes offer a seating capacity of roughly 160 in a two-class layout, making it a competitive option.
The C919 can offer up to 190 seats in a dense cabin configuration, the A320neo offers 194, and the 737 MAX pushes that to over 200 seats. The seating and range likely mean the COMAC jet is destined for more domestic and regional routes. However, the upcoming extended-range version could bring the plane on par with its rivals.
The COMAC C919 hopes to incorporate new technologies to ensure it is as reliable and safe as its counterparts. Indeed, the C919 features the CFM LEAP-1C engines, versions of which are also found on the competing A320neo and 737 MAX. The design is also reminiscent of recent modern jetliners (notice the windshield too). While this does not rule out all safety concerns, it may allay fears over engine issues. The COMAC C919 is designed to be an international airliner with Chinese characteristics. This means an ability to match the quality and safety established by Boeing and Airbus, but also by incorporating the specific needs of the Chinese market: High-density, high-frequency missions with fast turnaround times from airfields with broadly varying levels of development.
While the C919 may have Chinese characteristics, it raises the question of the plane’s success in the global market. Currently, the aircraft reportedly garnered 815 orders from 28 airlines and lessors. This includes airlines like the big three (China Eastern, China Southern, and Air China), Hainan Airlines, Joy Air, and more. GECAS is the only foreign lessor that has placed an order, buying 10 planes with options for 10 more.

The C919 could be certified in 2021 and come into service with launch customer OTT Airlines soon after. However, this date should be taken with a pinch of salt as the program has faced many delays along the way. Assuming all does go well and the C919 enters commercial service, we could see a major shift in the Chinese market.
The Boeing-Airbus rivalry in commercial aerospace has become so engrained in popular culture that it would be easy to forget the duopoly truly started just two decades ago after Boeing bought McDonnell Douglas. Since then, the two companies have been fighting tooth and nail to launch new programs, win customer orders and ramp up their production rates, reaching their peak in 2018, when the two delivered 1,600 aircraft and generated $120 billion in revenues, with both the deliveries and revenues divided pretty evenly between them.
Two Boeing 737 MAX crashes within five months grounded the whole MAX fleet, and quality issues with the Boeing 787 also emerged. At the same time, Airbus announced it would stop producing its A380 jet, which cost more than $15 billion to develop, after selling just 250 units. Meanwhile, orders were drying up for its most recent widebody, the A350, with fewer than 100 new orders tallied in three years. Since then, of course, things have grown much worse, and both companies have been scrambling to mitigate COVID-19 crisis damage.
At first glance, Boeing seems to be in a much worse situation than Airbus. As of November 2020, it had delivered only 118 aircraft for the year, while Airbus delivered 477, giving the European company an unprecedented 80% market share for yearly deliveries (see graph below).

Airbus’ orderbook is now almost 70% larger than Boeing’s. Additionally, Boeing has spent the last two years essentially firefighting, which means it has probably lost some ground in preparing for the next generation of airplanes. In the meantime, Airbus has been carrying on with the development of its A321XLR, which potentially pulls the rug from under Boeing’s work on addressing the “middle of the market” segment.
The two players still will be dominant and compete head-to-head. Beyond the current decade, however, the big question is what the impact of China’s forthcoming entry will be. Indeed, China’s first indigenously developed large commercial airplane—Comac’s narrowbody C919—is expected to come into service within a couple of years. This will mark the country’s official entry into the large commercial aircraft market and a major milestone of a long-term strategic play underpinning colossal geopolitical, industrial and commercial stakes. To succeed, it will need to rely on privileged access to a huge domestic market as well as an aggressive pricing strategy (the C919 could be priced 50% lower than the A320 or 737). But above all, selling commercial airplanes will become part of China’s “soft-power” strategy.
And while European or American airlines likely will not buy a Chinese airplane for some time, carriers in other regions may be enticed more easily. Of course, there are still many hurdles to be overcome for Comac to become a full-fledged competitor to Airbus and Boeing—not the least developing a robust supply chain and an international sales and service network. But in a world where trade wars could become increasingly the norm, China has a lot of assets to put forth.
Whereas the COVID-19 crisis has significantly dented Airbus’ and Boeing’s growth trajectories, it has boosted China’s quest to become an aerospace powerhouse. In the long term, China’s market entry is bound to alter the economics and the politics of the business, if only because it will force Boeing and Airbus to reconsider their global industrial strategy and take more risks on new product development.
Contrary to appearances, the Airbus-Boeing duopoly has never been a long, quiet river. It is certainly far from being one right now, and both players should brace for strong currents and treacherous rapids ahead.
The Math That Makes ‘Paradox-Free’ Time Travel Plausible
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No one has yet managed to travel through time – at least to our knowledge – but the question of whether or not such a feat would be theoretically possible continues to fascinate scientists.
As movies such as The Terminator, Donnie Darko, Back to the Future and many others show, moving around in time creates a lot of problems for the fundamental rules of the Universe: if you go back in time and stop your parents from meeting, for instance, how can you possibly exist in order to go back in time in the first place?
It’s a monumental head-scratcher known as the ‘grandfather paradox’, but in September last year a physics student Germain Tobar, from the University of Queensland in Australia, said he has worked out how to “square the numbers” to make time travel viable without the paradoxes.
“Classical dynamics says if you know the state of a system at a particular time, this can tell us the entire history of the system,” said Tobar back in September 2020.
“However, Einstein’s theory of general relativity predicts the existence of time loops or time travel – where an event can be both in the past and future of itself – theoretically turning the study of dynamics on its head.”
What the calculations show is that space-time can potentially adapt itself to avoid paradoxes.
To use a topical example, imagine a time traveller journeying into the past to stop a disease from spreading – if the mission was successful, the time traveller would have no disease to go back in time to defeat.

Tobar’s work suggests that the disease would still escape some other way, through a different route or by a different method, removing the paradox. Whatever the time traveller did, the disease wouldn’t be stopped.
Tobar’s work isn’t easy for non-mathematicians to dig into, but it looks at the influence of deterministic processes (without any randomness) on an arbitrary number of regions in the space-time continuum, and demonstrates how both closed timelike curves (as predicted by Einstein) can fit in with the rules of free will and classical physics.
“The maths checks out – and the results are the stuff of science fiction,” said physicist Fabio Costa from the University of Queensland, who supervised the research.
The new research smooths out the problem with another hypothesis, that time travel is possible but that time travellers would be restricted in what they did, to stop them creating a paradox. In this model, time travellers have the freedom to do whatever they want, but paradoxes are not possible.
While the numbers might work out, actually bending space and time to get into the past remains elusive – the time machines that scientists have devised so far are so high-concept that for they currently only exist as calculations on a page.
We might get there one day – Stephen Hawking certainly thought it was possible – and if we do then this new research suggests we would be free to do whatever we wanted to the world in the past: it would readjust itself accordingly.
“Try as you might to create a paradox, the events will always adjust themselves, to avoid any inconsistency,” says Costa. “The range of mathematical processes we discovered show that time travel with free will is logically possible in our universe without any paradox.”
How much does Nasa pay its astronauts?
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Astronauts have to risk their lives for the job, so it’s perhaps unsurprising that they get paid pretty well for the work they do. But how much, exactly? Well, you have to remember that astronaut isn’t usually someone’s first job. Often, they’re test pilots – it’s required that any astronaut has logged three years’ professional experience or 1,000 hours flying a jet before they can qualify. They’re also required to have degrees in science, engineering or maths and have to pass a rigorous selection process that’s much harder than getting into any university you care to name.
Once they make it though, they get paid a lot for their work. Nasa pays employees on a scale called the Federal Government’s General Schedule. Astronauts are on so-called ‘grades’ known as GS-12 and GS-13. Within each grade are several ‘steps’ that go form 1 to 10 and are based on performance and years of service.
If you’re a new astronaut on GS-12 step 1, then you’re looking at $66,167 (£54,110) per year. If you move up to GS-12 step 10, then you’re in line for a $86,021 (£70,326) per year. Now, if you’re an excellent astronaut and have served for many years, you may be a GS-13 step 10 earning $102,288 (£83,625) per year, according to Nasa.

Canadian astronaut David Saint-Jacques in spacewalk training at NASA’s Neutral Buoyancy Laboratory in Houston, Texas. (Photo: NASA)
The General Schedule is also just a guide. Astronauts may receive more or less depending on which locations they work in or what missions they’re involved in. Nasa is currently looking at the next generation of astronauts to go back to the moon and eventually to Mars. In a job listing, the space agency listed a salary range of $104,898 to $161,141 per year. Two astronauts, Douglas Hurley and Robert Behnken, are set to earn their paychecks later this month when they take off for the International Space Station aboard a SpaceX Crew Dragon craft for the first time. The launch is set to take place on May 27 from Cape Canaveral in Florida. It will be the first time Nasa has launched astronauts from American soil since 2011. Since retiring the space shuttle, Nasa has relied on Russian rockets to transport crew to the ISS. Next week’s launch will be a huge moment for both Nasa and SpaceX.
‘The Demo-2 mission will be the final major step before NASA’s Commercial Crew Program certifies Crew Dragon for operational, long-duration missions to the space station,’ the space agency said. ‘This certification and regular operation of Crew Dragon will enable NASA to continue the important research and technology investigations taking place onboard the station, which benefits people on Earth and lays the groundwork for future exploration of the Moon and Mars with the agency’s Artemis program.’
The 11th Dimension Theory
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The 11th dimension is a characteristic of space-time that has been proposed as a possible answer to questions that arise in superstring theory. The theory of superstrings involves the existence of nine dimensions of space and one dimension of time (a total of 10 dimensions). According to this notion, we observe only three spatial dimensions and one time dimension because the other six spatial dimensions are “curled up” or “compactified.”
According to superstring theory, all of the elementary particles in the universe are composed of vibrating, one-dimensional mathematical objects known as strings. The theory does not explicitly state what the strings are made of or where they come from; rather, they are proposed as geometric ideals. Each string has a length of only 10-35 meters, many times smaller than the diameter of the nucleus of an atom. Any given subatomic particle (or hadron) is made of a string that vibrates and rotates at the speed of light. A particular hadron gets its unique identity from the manner in which the string rotates and vibrates according to the dynamics of Einstein’s theory of general relativity. The frequency of vibration corresponds to the mass of the particle.
The nagging question remains, “Where do the strings come from?” Also, there are five different versions of superstring theory that explain the way subatomic particles behave. Are all five versions correct, or are some correct and others wrong? In an attempt to answer these questions, some physicists have suggested that there exists an 11th dimension, which is compactified like the other six spatial dimensions we do not directly observe. Superstring theory with the inclusion of the 11th dimension is sometimes called M theory or the theory of everything (TOE).
In the early 1990s, string theory was in a bit of a theoretical pickle. For decades, theorists had poured their hearts and minds into the idea that the fundamental building blocks of reality are tiny, vibrating strings. This was a potentially revolutionary idea, capable of uniting all the forces of nature and all the building blocks of matter into a single, harmonious picture.
The pickle, however, was that there were five independent candidates for string theory, each one looking radically different than the others. Which one was right?
Five’s company
The five different string theories had a few commonalities. For one, they all involved strings. They also all required our universe to have 10 total dimensions: the usual three spatial dimensions, one for time and six more compact dimensions that are tiny and curled up on themselves at submicroscopic scales.
And in all the theories, the ways strings vibrate give rise to the richness of our physical world, from the forces of nature to the building blocks of matter to physical constants themselves. But when it comes to physical theories, details matter, and the five competing string models differed in the details. Some theories only had closed loops of strings, while others allowed open, wiggling strings. Some theories only allowed vibrations to travel in one direction on the strings, while others allowed both. And some theories were combinations of other theories.
For reference, in case you’re curious, the names of the five string theories are: Type 1, Type IIA, Type IIB, SO(32) heterotic, and E8xE8 heterotic.
They obviously couldn’t all be correct descriptions of nature, but which one was the “real” string theory, and which were the phonies? The problem was (and still is today) that string theory isn’t complete — there’s no such thing as the final equations of string theory, something that could be printed on a t-shirt, that describes the theory in the same way that we have the Einstein equations for gravity or the Maxwell equations for electromagnetism.
We only have approximations that we hope — but can’t prove — are close to the actual theory. And so the five string theories represent five different approximations, with no way of being able to decide which one is best.
And then 1995 happened, when prominent theoretical physicist Edward Witten gave a talk at the annual string theory conference. In the talk, he offered a radical suggestion: perhaps the five string theories weren’t so different after all.
It turns out that there are interesting connections, called dualities or symmetries, among the five theories. For example, something we don’t know about strings is how strongly they like to interact. But if you take, say, Type 1 string theory and ramp up its interaction strength, you end up with the weaker version of SO(32) heterotic.
And there’s more. Sometimes strings can wind around a tiny, curled-up dimension a certain number of times with a certain momentum, but the duality of that has the number of windings and the momentum flipped. Type IIA and Type IIB string theories are related by such a duality.
These dualities suggest that the five string theories are all related, somehow, and are probing something much, much deeper. That deeper thing can be guessed at by following all the dualities. By attempting both dualities on the five string theories, sometimes you get links to one of the other five, and sometimes you get dualities to somewhere new.
What is that “somewhere new”? Edward Witten suggested calling it “M-theory”, with the “m” open to interpretation (e.g., “mother,” “mystery” or “membrane”) until such time as we actually understand it.
Big branes
M-theory is like an uber-theory of strings, showing how all five string theories are really just small corners of a much larger, and much more mysterious, theory. We used to think of the five string theories as separate planets, with our theoretical and mathematical explorations confined to little islands on those planets. But M-theory revealed that all those islands actually shared the same, much larger, planet all along.
One curious feature of M-theory (the little that we know about it, that it) is that what we consider string theory appears to be just a low-energy approximation of the real deal. And that real deal requires not 10 but 11 dimensions in our universe.
What’s more, the fundamental object of reality is no longer the string but the d-brane. “Brane” is just a fancy word for multidimensional vibrating things, with the letter “d” signifying the dimension, giving us everything from 1-branes (strings) to 2-branes (sheets) to 3-branes (blobs) and more.
For the most part, these branes lie low and mostly just act like strings, with the eleventh dimension not playing much of a role in the grand cosmic symphony.
Beyond that, there isn’t much known about M-theory. String theorists usually work in one of the five usual regimes, since they’ve been so well studied for decades, and the additional dimension and the introduction of branes makes the already-fiendish mathematics of string theory that much worse. Still, theorists continue to probe at the edges, hoping to someday give a full name to the “m” in M-theory.
Artificial Intelligence Solves Schrödinger Equation For Molecules / Monte Carlo method
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The Schrödinger Equation is a crucial formalism at the center of quantum mechanics. It is used to work out how quantum systems are, and how they evolve. It is also very much a challenge to solve precisely for a system made of more than a few particles, with approximations use in most cases.
Computational methods are used to solve the equation for many systems, and a new study published in Nature Chemistry has put forward a new method. The approach, called PauliNet, is a deep neural network that can get the exact solution for the equation for molecules with up to 30 electrons.
This AI is based on the Monte Carlo method, which uses random sampling to deliver numerical results of a mathematical function. This particular version was built with the knowledge of physical laws, including the important Pauli exclusion principle. The algorithm is named after this law. Watch video below:
Solving the equation can provide insights into the formation and behavior of molecules that several of the current methods can’t provide. This has often been too laborious to be worth it, hence why this method could be a game-changer.
“Escaping the usual trade-off between accuracy and computational cost is the highest achievement in quantum chemistry,” lead author Dr. Jan Hermann of Freie Universität Berlin, said in a statement. “As yet, the most popular such outlier is the extremely cost-effective density functional theory. We believe that deep ‘Quantum Monte Carlo,’ the approach we are proposing, could be equally, if not more successful. It offers unprecedented accuracy at a still acceptable computational cost.”
PauliNet allows for a solution of the Schrödinger Equation to be found for arbitrary molecules. The versatility and strong physical backbone of the software deliver these results. The equation is a mathematical description of the quantum state known as the wave function, and translating this wave function for many electrons into a computer language was not easy.
“Instead of the standard approach of composing the wave function from relatively simple mathematical components, we designed an artificial neural network capable of learning the complex patterns of how electrons are located around the nuclei,” added Professor Frank Noé, who led the team effort.
There are still many kinks to iron out, but the researchers are excited about the possibilities of this algorithm.
“This is still fundamental research,” the authors agree, “but it is a fresh approach to an age-old problem in the molecular and material sciences, and we are excited about the possibilities it opens up.”
Who Will Win the Hypersonic Arms Race? … Russia, China, the U.S.
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The great powers are pursuing hypersonic arms, they are once again locked in an arms race.
The wider world first heard of this type of weaponry in March 2018, when Russian president Vladimir Putin gave a speech describing his country’s plans for a nuclear-powered cruise missile that could fly around the world at blinding speed, then snake around hills and dales to a target. His bold assertions have been questioned, particularly the part about nuclear power. Even so, a year later a nuclear accident killed seven people near a testing range off the northern coast of Russia, and U.S. intelligence officials speculated that it involved hypersonic experiments.
The nature of that accident is still shrouded in mystery, but it’s clear there’s been a huge increase in the research effort in hypersonics. Here’s a roundup of what the superpowers of the 21st century are doing to pursue what is, in fact, an old concept.
The hypersonic missiles in use or in testing in China and Russia can apparently carry either conventional warheads, aimed at ships and other small military targets, or nuclear ones, aimed at cities and government centers. These ship killers could deprive the United States of its preeminence at sea, which is more than enough reason for China, for instance, to develop hypersonics. But a nuclear-armed version that leaves the defender too little time to launch a retaliatory strike would do even more to shift the balance of power, because it would dismantle the painstakingly constructed system of deterrence known as mutually assured destruction, or by the jocular acronym MAD.
“The nuclear side is very destabilizing, which is why the Russians are going after it,” says Christopher Combs, a professor of mechanical engineering at the University of Texas at San Antonio. “But on the U.S. side we see no need for that, so we’re going conventional.”
That is indeed the official U.S. policy. But in August, some months after Combs spoke with IEEE Spectrum, an Aviation Week article pointed out that an Air Force agency charged with nuclear weapons requested that companies submit ideas for a “thermal protection system that can support a hypersonic glide to ICBM ranges.” Soon after that, the request was hastily taken down, and the U.S. Air Force felt compelled to restate its policy not to pursue nuclear-capable hypersonic weapons.
Today’s test vehicles just pick up where the old ones left off, explains Alexander Fedorov, a professor at Moscow Institute of Physics and Technology and an expert on hypersonic flow at the boundary layer, which is right next to the vehicle’s skin. “What’s flying now is just a demonstration of technology—the science is 30 years old,” he says.
Fedorov has lectured in the United States; he even helps U.S. graduate students with their research. He laments how the arms race has stifled international cooperation, adding that he himself has “zero knowledge” about the military project Putin touted two years ago. “But I know that people are working on it,” he adds.
In the new race, Fedorov says, Russia has experience without much money, China has money without much experience, and the United States has both, although it revived its efforts later than did Russia or China and is now playing catch-up. For fiscal 2021, U.S. research agencies have budgeted US $3.2 billion for all hypersonic weapons research, up from $2.6 billion in the previous year.
Other programs are under way in India and Australia; even Israel and Iran are in the game, if on the sidelines. But Fedorov suggests that the Chinese are the ones to watch: They used to talk at international meetings, he says, but now they mostly just listen, which is what you’d expect if they had started working on truly new ideas—of which, he reiterates, there are very few on display. All the competing powers have shown vehicles that are “very conservative,” he says.
One good reason for the rarity of radical designs is the enormous expense of the research. Engineers can learn only so much by running tests on the ground, using computational fluid-flow models and hypersonic wind tunnels, which themselves cost a pretty penny (and simulate only some limited aspects of hypersonic flight). Engineers really need to fly their creations, and usually when they do, they use up the test vehicle. That makes design iteration very costly.
It’s no wonder hypersonic prototypes fail so often. In mere supersonic flight, passing Mach 1 is a clear-cut thing: The plane outdistances the sound waves that it imparts to the air to produce a shock wave, which forms the familiar two-beat sonic boom. But as the vehicle exceeds Mach 5, the density of the air just behind the shock wave diminishes, allowing the wave to nestle along the surface of the vehicle. That in-your-face layer poses no aerodynamic problems, and it could even be an advantage, when it’s smooth. But it can become turbulent in a heartbeat.
“Predicting when it’s going turbulent is hard,” says Wheaton, of Johns Hopkins APL. “And it’s important because when it does, heating goes up, and it affects how control surfaces can steer. Also, there’s more drag.”
The pioneers of hypersonic flight learned about turbulence the hard way. On one of its many flights, in 1967, the U.S. Air Force’s X-15 experimental hypersonic plane went into a spin, killing the pilot, Michael J. Adams. The right stuff, indeed.
Hypersonic missiles come in two varieties. The first kind, launched into space on the tip of a ballistic missile, punches down into the atmosphere, then uses momentum to maneuver. Such “boost-glide” missiles have no jet engines and thus need no air inlets, so it’s easy to make them symmetrical, typically a tube with a cone-shape tip. Every part of the skin gets equal exposure to the air, which at these speeds breaks down into a plume of plasma, like the one that puts astronauts in radio silence during reentry.
Boost-glide missiles are now operational. China appears to have deployed the first one, called the Dongfeng-17, a ballistic missile that carries glide vehicles. Some of those gliders are billed as capable of knocking out U.S. Navy supercarriers. For such a mission it need not pack a nuclear or even a conventional warhead, instead relying on its enormous kinetic energy to destroy its target. And there’s nothing that any country can now do to defend against it.
“Those things are going so fast, you’re not going to get it,” General Mark Milley, chairman of the Joint Chiefs of Staff, said in March, in testimony before Congress.
You might think that you give up the element of surprise by starting with a ballistic trajectory. But not completely. Once the hypersonic missile comes out of its dive to fly horizontally, it becomes invisible to sparsely spaced radars, particularly the handful based in the Pacific Ocean. And that flat flight path can swerve a lot. That’s not because of any AI-managed magic—the vehicle just follows a randomized, preprogrammed set of turns. But the effect on those playing defense is the same: The pizza arrives before they can find their wallets.
The second kind of hypersonic missile gets the bulk of its impulse from a jet engine that inhales air really fast, whirls it together with fuel, and burns the mixture in the instant that it tarries in the combustion chamber before blowing out the back as exhaust. Because these engines don’t need compressors but simply use the force of forward movement to ram air inside, and because that combustion proceeds supersonically, they are called supersonic ram jets—scramjets, for short.
One advantage the scramjet has over the boost-glide missile is its ability to stay below radar and continue to maneuver over great distances, all the way to its target. And because it never enters outer space, it doesn’t need to ride a rocket booster, although it does need some powerful helper to get it up to the speed at which first a ramjet, and then a scramjet, can work.
Another advantage of the scramjet is that it can, in principle, be applied for civilian purposes, moving people or packages that absolutely, positively have to be there quickly. The Europeans have such a project. So do the Chinese, and Boeing has shown a concept. Everyone talks up this possibility because, frankly, it’s the only peaceable talking point there is for hypersonics. Don’t forget, though, that supersonic commercial flight happened long ago, made no money, and ended—and supersonic flight is way easier.
The scramjet has one big disadvantage: It’s a lot harder technically. Any hypersonic vehicle must fend off the rapidly moving air outside, which can heat the leading edges to as high as 3,000 °C. But that heat and stress is nothing like the hellfire inside a scramjet engine. There, the heat cannot radiate away, it’s hard to keep the flame lit, and the insides can come apart second by second, affecting airflow and stability. Five minutes is a long time in this business.
That’s why scramjets, though conceived in the 1950s, still remain a work in progress. In the early 2000s, NASA’s X-43 used scramjets for about 10 seconds in flight. In 2013, Boeing’s X-51 Waverider flew at hypersonic speed for 210 seconds while under scramjet power.
Tests on the ground have fared better. In May, workers at the Beijing Academy of Sciences ran a scramjet for 10 minutes, according to a report in the South China Morning Post. Two years earlier, the leader of the project, Fan Xuejun, told the same newspaper that a factory was being built to construct a variety of scramjets, some supposedly for civilian application. One engine would use a combined cycle, with a turbojet to get off the ground, a ramjet to accelerate to near-hypersonic speed, a scramjet to blow past Mach 5, and maybe even a rocket to top off the thrust. That’s a lot of moving parts—and an ambition worthy of Elon Musk. But even Musk might hesitate to follow Putin’s proposal to use a nuclear reactor for energy.

Photo: Boeing Like Greased Lightning: Boeing’s X-51 Waverider in white is shown slung under the wing of a B-52 bomber, just before a test flight of the hypersonic vehicle in 2012. The B-52 mothership was needed to attain the necessary altitude; a rocket booster on the missile pushed it fast enough into the supersonic range to allow the scramjet to ignite. In 2013, the X-51 flew hypersonically on scramjet power for 210 seconds, the official record.
The cost of developing a scramjet capability is only one part of the economic challenge. The other is making the engine cheap enough to deploy and use in a routine way. To do that, you need fuel you can rely on. Early researchers worked with a class of highly energetic fuels that would react on contact with air, like triethylaluminum.
“It’s a fantastic scramjet engine fuel, but very toxic, a bit like the hydrazine fuels used in rockets nowadays, and this became an inhibitor,” says David Van Wie, of Johns Hopkins APL, explaining why triethylaluminum was dropped from serious consideration.
Next up was liquid hydrogen, which is also very reactive. But it needs elaborate cooling. Worse, it packs a rather low amount of energy into a given volume, and as a cryogenic fuel it is inconvenient to store and transport. It has been and still is used in experimental missiles, such as the X-43.
Today’s choice for practical missiles is hydrocarbons, of the same ilk as jet fuel, but fancier. The Chinese scramjet that burned for 10 minutes—like others on the drawing board around the world—burns hydrocarbons. Here the problem lies in breaking down the hydrocarbon’s long molecular chains fast so the shards can bind with oxygen in the split second when the substances meet and mate. And a split second isn’t enough—you have to do it continuously, one split second after another, “like keeping a match lit in a hurricane,” in the oft-quoted words of NASA spokesman Gary Creech, back in 2004.
Scramjet designs try to protect the flame by shaping the inflow geometry to create an eddy, forming a calm zone not unlike the eye of a hurricane. Flameouts are particularly worrisome when the missile starts jinking about, thus disrupting the airflow. “It’s the ‘unstart’ phenomenon, where the shock wave at the air inlets stops the engine, and the vehicle will be lost,” says John D. Schmisseur, a researcher at the University of Tennessee Space Institute, in Tullahoma. And you really only get to meet such gremlins in actual flight, he adds.
There are other problems besides flameout that arise when you’re inhaling a tornado. One expert, who requested anonymity, puts it this way: “If you’re ingesting air, it’s no longer air; it’s a complex mix of ionized atmosphere,” he says. “There’s no water anymore; it’s all hydrogen and oxygen, and the nitrogen is to some fraction elemental, not molecular. So combustion isn’t air and fuel—it’s whatever you’re taking in, whatever junk—which means chemistry at the inlet matters.”
Simulating the chemistry is what makes hypersonic wind-tunnel tests problematic. It’s fairly simple to see how an airfoil responds aerodynamically to Mach 5—just cool the air so that the speed of sound drops, giving a higher Mach number for a given airspeed. But blowing cold air tells you only a small part of the story because it heads off all the chemistry you want to study. True, you can instead run your wind tunnel fast, hot, and dense—at “high enthalpy,” to use the term of art—but it’s hard to keep that maelstrom going for more than a few milliseconds.
“Get the airspeed high enough to start up the chemistry and the reactions sap the energy,” says Mark Gragston, an aerospace expert who’s also at the UT Space Institute. Getting access to such monster machines isn’t easy, either. “At Arnold Air Force Base, across the street from me, the Air Force does high-enthalpy wind-tunnel experiments,” he says. “They’re booked up three years in advance.”
Other countries have more of the necessary wind tunnels; even India has about a dozen. Right now, the United States is spending loads of money building these machines in an effort to catch up with Russia and China. You could say there is a wind-tunnel gap—one more reason U.S. researchers are keen for test flights.
Another thing about cooling the air: It does wonders for any combustion engine, even the kind that pushes pistons. Reaction Engines, in Abingdon, England, appears to be the first to try to apply this phenomenon in flight, with a special precooling unit. In its less-ambitious scheme, the precooler sits in front of the air inlet of a standard turbojet, adding power and efficiency. In its more-ambitious concept, called SABRE (Synergetic Air Breathing Rocket Engine), the engine operates in combined mode: It takes off as a turbojet assisted by the precooler and accelerates until a ramjet can switch on, adding enough thrust to reach (but not exceed) Mach 5. Then, as the vehicle climbs and the atmosphere thins out, the engine switches to pure rocket mode, finally launching a payload into orbit.
In principle, a precooler could work in a scramjet. But if anyone’s trying that, they’re not talking about it.
Fast forward five years and boost-glide missiles will no doubt be deployed in the service of multiple countries. Jump ahead another 15 or 20 years, and the world’s superpowers will have scramjet missiles.
So what? Won’t these things always play second fiddle to ballistic missiles? And won’t the defense also have its say, by unveiling superfast antimissiles and Buck Rogers–style directed-energy weapons?
Perhaps not. The defense always has the harder job. As President John F. Kennedy noted in an interview way back in 1962, when talking about antiballistic missile defense, what you are trying to do is shoot a bullet with a bullet. And, he added, you have to shoot down not just one but many, including a bodyguard of decoys.
Today there are indeed antimissile defenses that can protect particular targets against ballistic missiles, at least when they’re not being fired in massive salvos. But you can’t defend everything, which is why the great powers still count on deterrence through mutually assured destruction. By that logic, if you can detect cruise missiles soon enough, you can at least make those who launched them wish they hadn’t.
For that to work, we’ll need better eyes in the skies. In the United States, the military wants around $100 million for research on low-orbit space sensors to detect low-flying hypersonic missiles, Aviation Week reported in 2019.
Hardly any of the recent advances in hypersonic flight result from new scientific discoveries; almost all of it stems from changes in political will. Powers that challenge the international status quo—China and Russia—have found the resources and the will to shape the arms race to their benefit. Powers that benefit from the status quo—the United States, above all—are responding in kind. Politicians fired the starting pistol, and the technologists are gamely leaping forward.
How Viruses Spread in Aircraft — and the safest place to sit
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The World Health Organization defines contact with an infected person as being seated within two rows of one another.
But people don’t just sit during flights, particularly ones lasting longer than a few hours. They visit the bathroom, stretch their legs, and grab items from the overhead bins. In fact, during the 2003 coronavirus outbreak of the severe acute respiratory syndrome (SARS), a passenger aboard a flight from Hong Kong to Beijing infected people well outside the WHO’s two-row boundary. The New England Journal of Medicine noted that the WHO criteria “would have missed 45 percent of the patients with SARS.”
Passengers in window seats have the lowest likelihood of coming in contact with an infected person (see figure below).

Inspired in part by that case, a team of public health researchers set out to study how random movements about the airplane cabin might change passengers’ probability of infection.
The “FlyHealthy Research Team” observed the behaviors of passengers and crew on 10 transcontinental U.S. flights of about three and a half to five hours. Led by Emory University’s Vicki Stover Hertzberg and Howard Weiss, they not only looked at how people moved about the cabin, but also at how that affected the number and duration of their contacts with others. The team wanted to estimate how many close encounters might allow for transmission during transcontinental flights.
“Suppose you’re seated in an aisle seat or a middle seat and I walk by to go to the lavatory,” says Weiss, professor of biology and mathematics at Penn State University. “We’re going to be in close contact, meaning we’ll be within a meter. So if I’m infected, I could transmit to you…Ours was the first study to quantify this.”
As the study revealed in 2018, most passengers left their seat at some point—generally to use the restroom or check the overhead bins—during these medium-haul flights. Overall, 38 percent of passengers left their seats once and 24 percent more than once. Another 38 percent of people stayed in their seats throughout the entire flight.
This activity helps pinpoint the safest places to sit. The passengers who were least likely to get up were in window seats: only 43 percent moved around as opposed to 80 percent of people seated on the aisle.
Accordingly, window seat passengers had far fewer close encounters than people in other seats, averaging 12 contacts compared to the 58 and 64 respective contacts for passengers in middle and aisle seats.
Choosing a window seat and staying put clearly lowers your likelihood of coming into contact with an infectious disease. But, as you can see in the accompanying graphic, the team’s model shows that passengers in middle and aisle seats—even those that are within the WHO’s two-seat range—have a fairly low probability of getting infected.
Weiss says that’s because most contact people have on airplanes is relatively short.
“If you’re seated in an aisle seat, certainly there will be quite a few people moving past you, but they’ll be moving quickly,” Weiss says. “In aggregate, what we show is there’s quite a low probability of transmission to any particular passenger.”
The story changes if the ill person is a crew member. Because flight attendants spend much more time walking down the aisle and interacting with passengers, they are more likely to have additional—and longer—close encounters. As the study stated, a sick crew member has a probability of infecting 4.6 passengers, “thus, it is imperative that flight attendants not fly when they are ill.”
What does it mean for the new coronavirus?
As Weiss points out, we don’t know yet the preferred way that the new coronavirus transmits. It could be primarily through respiratory droplets, physical contact with saliva or diarrhea followed by oral consumption of viral material, or perhaps even aerosols.
He notes that this model doesn’t include the transmission of aerosols, though the FlyHealthy team hopes to research this topic in the future. In the study, the researchers also warn that this model cannot be directly extrapolated for long-haul flights or airplanes with more than one aisle.
Landon agrees that we don’t yet know how the coronavirus transmits, but believes the results of this study are applicable. All previous coronaviruses have transmitted through droplets, she notes, so it would be unusual if this new pathogen was different. And indeed, the new coronavirus is behaving much like SARS in many respects. Both are zoonotic, meaning they started in animals before jumping to humans, and both appear to have started in bats. The pair also transmit from human to human and have a long incubation period—up to 14 days for the Wuhan coronavirus, compared to about two for influenza—which means that people might be sick and transmitting the disease before symptoms show up.
With all that in mind, Landon suggests following the CDC guidance for infectious diseases when you’re on an airplane.
That includes washing your hands with regular soap or using an alcohol-based hand sanitizer after touching any surface—especially since there’s evidence that coronaviruses last longer on surfaces than other illnesses, around three to 12 hours.
You should also avoid touching your face and contact with coughing passengers by whatever means possible.
What’s worse, the coronavirus or influenza?
There are many ways to estimate the risk posed by a disease, but let’s focus on two numbers often used by public health researchers: the reproduction number and the case-fatality ratio.
The reproduction number—R0 or “r naught”—simply refers to the number of additional people that an infected person typically makes sick. Maia Majumder, a faculty member at Boston Children’s Hospital and Harvard Medical School, has been tracking exactly that.
Researchers from Germany are to examine the way virus particles spread in the passenger cabins of aircraft and trains using experiments and computer simulations to help fight the Covid-19 pandemic.
The research looking at virus spread in aircraft cabins is soon to start in a new laboratory at the German Aerospace Center (DLR) Institute of Aerodynamics and Flow Technology in Göttingen and is part of an EU project called Advent.
“We can now use the scientific tools that we have developed to research the spread of viruses within passenger cabins.”
The tests introduce a sick passenger into a fully occupied area. They then look at how far exhaled particles are distributed.
Computer simulations of a section of the cabin are first run where the sick passenger’s exhalation or coughing pattern is generated using a program that is usually used to simulate cabin airflow. This is supplemented by the addition of aerosol particles, which then atomize and evaporate.
For coughing, the atomization process has clear parallels with the process of fuel injection into an engine, where strong shear forces cause the droplets to disintegrate, said DLR.
The parameters used, such as the exhaled lung volume of around one to 1.5 litres and the size of the droplets, which range from smaller than one micrometre to several hundreds of micrometres, are derived from studies conducted by the FAA.
The computer program calculates the distribution and range of the particles and provides a graphical representation of their propagation.
Rolf Henke, the DLR executive board member responsible for aeronautics research said, “Aircraft cabins are self-contained systems and already have a high level of air quality control. Our research on virus spread in cabins is intended to help protect passengers from infections and find ways of making flying safe in future.”
At the same time, researchers at the generic train laboratory in Göttingen are replicating a similar situation in an experiment. Here, 24 mannequins fitted with sensors serve as the passengers. A ‘sick’ mannequin releases air with added droplets and a tracer gas from its mouth area. High-speed cameras and gas sensors track the spread of the particles within the cabin. The particles and their concentration are recorded at various points within the space.
The DLR researchers in Göttingen are investigating the spread of physical particles that are analogous to virus-laden droplets. Meanwhile, researchers elsewhere including at the DLR Institute of Aerospace Medicine in Cologne, are studying the infectiousness of the droplets and the effect of aircraft air filters.
Preliminary results from the recently initiated research studies are expected in the coming weeks. However, some of the experiments are set to continue for months. All of the findings will be published and made available to partners in industry, said DLR.
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Tests on Passengers and Safe Distance: How soon can we fly after Covid-19?
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How soon are we going to be allowed to travel freely after COVID-19 is over and what will it look like? Those are the questions everyone is asking in every corner of the globe.
Emirates will have vacant seats in between individual passengers or family groups and won’t allow cabin baggage on flights as the airline seeks to contain the spread of the coronavirus. “Seats are pre-allocated with vacant seats placed between individual passengers or family groups in observance of physical distancing protocols,” a statement from the Dubai-based airline said. Emirates, which grounded most of its passenger flights, is gradually restarting operations that were shut following the coronavirus outbreak. It also started testing passengers before flying out of Dubai.
The statement from the carrier added: “All cabin crew, boarding agents and ground staff in direct contact with passengers will now don personal protective equipment (PPE) which includes a protective disposable gown over their uniforms, and a safety visor, in addition to masks and gloves.”
Other measures include:
– Magazines and other print reading material are temporarily unavailable
– Carry-on items allowed in the cabin are limited to laptop, handbag, briefcase or baby items
– All other items have to be checked in, and Emirates will add the cabin baggage allowance to customers’ check-in baggage allowance
– Passengers have to wear their masks and gloves throughout their journey from check-in until they disembark


At Dubai International Airport, gloves and masks are mandatory for all customers and employees and thermal scanners are being used to monitor the temperatures of all passengers and employees stepping into the airport. Physical distancing indicators have been placed on the ground and at waiting areas to help travellers maintain the necessary distance during check-in and boarding. The airport team has also installed protective barriers at each check-in desk to provide additional safety reassurance to passengers and employees during interaction over the counter.
