Hydrogen Fuel Quotes

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In other words, a star is a nuclear furnace, burning hydrogen fuel and creating nuclear "ash" in the form of waste helium. A star is also a delicate balancing act between the force of gravity, which tends to crush the star into oblivion, and the nuclear force, which tends to blow the star apart with the force of trillions of hydrogen bombs. A star then matures and ages as it exhausts its nuclear fuel.
Michio Kaku (Hyperspace: A Scientific Odyssey Through Parallel Universes, Time Warps, and the Tenth Dimension)
I thought I was far enough from the explosion but no, not even close. Chunks of twisted metal bashed my boulder while smaller bits of wreckage rained from above. “Oh, right,” I said. I’d forgotten to account for the other explosive in there: the hydrogen fuel-cell battery. All that hydrogen had met the oxygen at high temperature and they’d had a brief chat.
Andy Weir (Artemis)
Not because of the perfect landing, but because he left so much fuel behind. Hundreds of liters of unused hydrazine. Each molecule of hydrazine has four hydrogen atoms in it.
Andy Weir (The Martian)
for every kilogram of hydrogen you bring to Mars, you can make thirteen kilograms of fuel. It’s a slow process, though. It takes twenty-four months to fill the tank.
Andy Weir (The Martian)
Eventually, however, the star will run out of its hydrogen and other nuclear fuels. Paradoxically, the more fuel a star starts off with, the sooner it runs out. This is because the more massive the star is, the hotter it needs to be to balance its gravitational attraction.
Stephen W. Hawking (A Brief History of Time)
Ethanol is a volatile, flammable, colourless liquid with a slight chemical odour. It is used as an antiseptic, a solvent, in medical wipes and antibacterial formulas because it kills organisms by denaturing their proteins. Ethanol is an important industrial ingredient. Ethanol is a good general purpose solvent and is found in paints, tinctures, markers and personal care products such as perfumes and deodorants. The largest single use of ethanol is as an engine fuel and fuel additive. In other words, we drink, for fun, the same thing we use to make rocket fuel, house paint, anti-septics, solvents, perfumes, and deodorants and to denature, i.e. to take away the natural properties of, or kill, living organisms. Which might make sense on some level if we weren’t a generation of green minded, organic, health-conscious, truth seeking individuals. But we are. We read labels, we shun gluten, dairy, processed foods, and refined sugars. We buy organic, we use natural sunscreen and beauty products. We worry about fluoride in our water, smog in our air, hydrogenated oils in our food, and we debate whether plastic bottles are safe to drink from. We replace toxic cleaning products with Mrs. Myers and homemade vinegar concoctions. We do yoga, we run, we SoulCycle and Fitbit, we go paleo and keto, we juice, we cleanse. We do coffee enemas and steam our yonis, and drink clay and charcoal, and shoot up vitamins, and sit in infrared foil boxes, and hire naturopaths, and shamans, and functional doctors, and we take nootropics and we stress about our telomeres. These are all real words. We are hyper-vigilant about everything we put into our body, everything we do to our body, and we are proud of this. We Instagram how proud we are of this, and we follow Goop and Well+Good, and we drop 40 bucks on an exercise class because there are healing crystals in the floor. The global wellness economy is estimated to be worth $4 trillion. $4 TRILLION DOLLARS. We are on an endless and expensive quest for wellness and vitality and youth. And we drink fucking rocket fuel.
Holly Whitaker (Quit Like a Woman: The Radical Choice to Not Drink in a Culture Obsessed with Alcohol)
[08:41] MAV: You fucking kidding me? [09:55] HOUSTON: Admittedly, they are very invasive modifications, but they have to be done. The procedure doc we sent has instructions for carrying out each of these steps with tools you have on hand. Also, you’ll need to start electrolyzing water to get the hydrogen for the fuel plant. We’ll send you procedures for that shortly. [09:09] MAV: You’re sending me into space in a convertible. [09:24] HOUSTON: There will be Hab canvas covering the holes. It will provide enough aerodynamics in Mars’s atmosphere. [09:38] MAV: So it’s a ragtop. Much better.
Andy Weir (The Martian)
Professor J. B. S. Haldane was one of the most celebrated scientists in Britain. A pioneering and broad-ranging thinker, he developed a mathematical theory of population genetics, predicted that hydrogen-producing windmills would replace fossil fuel, explained nuclear fission, and suffered a perforated eardrum while testing a homemade decompression chamber: “Although one is somewhat deaf,” he wrote, “one can blow tobacco smoke out of the ear in question, which is a social accomplishment.
Ben Macintyre (Operation Mincemeat: How a Dead Man and a Bizarre Plan Fooled the Nazis and Assured an Allied Victory)
For the Earth, the future lies in fire. In five or so billion years we will have the last nice day on our home planet, then the sun will exhaust its hydrogen fuel and expand into a red giant star. Eventually the sun will set the sky on fire. The oceans will boil and the mountains will melt. The Earth will be engulfed by the sun, and will orbit like a burnt-out cinder within its fiery atmosphere. There is a biblical reference that says, from ashes to ashes, dust to dust. Physicists say, from stardust we came, to stardust we will return.
Michio Kaku (The Future of Humanity: Terraforming Mars, Interstellar Travel, Immortality, and Our Destiny BeyondEarth)
[08:41] MAV: You fucking kidding me? [09:55] HOUSTON: Admittedly, they are very invasive modifications, but hey have to be done. The procedure doc we sent has instructions for carrying out each of these steps with tools you have on hand. Also, you'll need to start electrolyzing water to get the hydrogen for the fuel plant. We'll send you procedures for that shortly. [09:09] MAV: You're sending me into space in a convertible. [09:24] HOUSTON: There will be Hab canvas covering the holes. It will provide enough aerodynamics in Mars's atmosphere. [09:38] MAV: So it's a ragtop. Much better.
Andy Weir (The Martian)
Nearly, my friend.” “And what will they burn instead of coal?” “Water,” replied Harding. “Water!” cried Pencroft, “water as fuel for steamers and engines! water to heat water!” “Yes, but water decomposed into its primitive elements,” replied Cyrus Harding, “and decomposed doubtless, by electricity, which will then have become a powerful and manageable force, for all great discoveries, by some inexplicable laws, appear to agree and become complete at the same time. Yes, my friends, I believe that water will one day be employed as fuel, that hydrogen and oxygen which constitute it, used singly or together, will furnish an inexhaustible source of heat and light, of an intensity of which coal is not capable. Some day the coalrooms of steamers and the tenders of locomotives will, instead of coal, be stored with these two condensed gases, which will burn in the furnaces with enormous calorific power.
Jules Verne (The Mysterious Island)
Stars are bright, hot, rotating masses of gas which emit large quantities of light and heat as a result of nuclear reactions. Most newly-forming large stars begin to collapse under the weight of their own gravitational pull. That means that their centres are hotter and denser. When the matter in the centre of the star is sufficiently heated-when it reaches at least 10 million degrees Celsius (18 million degrees Fahrenheit)-nuclear reactions begin.56 What happens inside a star is that with enormous energy (fusion), hydrogen turns into helium. Nuclear fusion takes the particles that make up hydrogen and sticks them together to make helium (1 helium atom is made from 4 hydrogen atoms). In order to make the protons and neutrons in the helium stick together, the atom gives off tremendous energy. The energy released in the process is radiated from the surface of the star as light and heat. When the hydrogen is consumed, the star then begins to burn with helium, in exactly the same way, and heavier elements are formed. These reactions continue until the mass of the star has been consumed. However, since oxygen is not used in these reactions inside stars, the result is not ordinary combustion, such as that takes place when burning a piece of wood. The combustion seen as giant flames in stars does not actually derive from fire. Indeed, burning of just this kind is described in the verse. If one also thinks that the verse refers to a star, its fuel and combustion without fire, then one can also think that it is referring to the emission of light and mode of combustion in stars. (Allah knows best.)
Harun Yahya (Allah's Miracles in the Qur'an)
At that moment, remarkably, there was a man in the expansive reactor hall of Unit 4 who witnessed all this.121 Night Shift Chief of the Reactor Shop Valeriy Perevozchenko saw the top of the reactor - a 15-meter-wide disk comprised of 2000 individual metal covers which cap safety valves - begin to jump up and down. He ran. The reactor’s uranium fuel was increasing power exponentially, reaching some 3,000°C, while pressure rose at a rate of 15 atmospheres per second. At precisely 01:23:58, a mere 18 seconds after Akimov pressed the SCRAM button, steam pressure overwhelmed Chernobyl’s incapacitated fourth reactor. A steam explosion blew the 450-ton, 3-meter-thick upper biological shield clear off the reactor before it crashed back down, coming to rest at a steep angle in the raging maw it left behind. The core was exposed.122 A split second later, steam and inrushing air reacted with the fuel’s ruined zirconium cladding to create a volatile mixture of hydrogen and oxygen, which triggered a second, far more powerful explosion.123 Fifty tons of vaporised nuclear fuel were thrown into the atmosphere, destined to be carried away in a poisonous cloud that would spread across most of Europe. The mighty explosion ejected a further 700 tons of radioactive material - mostly graphite - from the periphery of the core, scattering it across an area of a few square kilometers. This included the roofs of the turbine hall, Unit 3, and the ventilation stack it shared with Unit 4, all of which erupted into flames. The reactor fuel’s extreme temperature, combined with air rushing into the gaping hole, ignited the core’s remaining graphite and generated an inferno that burned for weeks. Most lights, windows and electrical systems throughout the severely damaged Unit 4 were blown out, leaving only a smattering of emergency lighting to provide illumination.124
Andrew Leatherbarrow (Chernobyl 01:23:40: The Incredible True Story of the World's Worst Nuclear Disaster)
For unknown ages after the explosive outpouring of matter and energy of the Big Bang, the Cosmos was without form. There were no galaxies, no planets, no life. Deep, impenetrable darkness was everywhere, hydrogen atoms in the void. Here and there, denser accumulations of gas were imperceptibly growing, globes of matter were condensing-hydrogen raindrops more massive than suns. Within these globes of gas was kindled the nuclear fire latent in matter. A first generation of stars was born, flooding the Cosmos with light. There were in those times, not yet any planets to receive the light, no living creatures to admire the radiance of the heavens. Deep in the stellar furnaces, the alchemy of nuclear fusion created heavy elements from the ashes of hydrogen burning, the atomic building blocks of future planets and lifeforms. Massive stars soon exhausted their stores of nuclear fuel. Rocked by colossal explosions, they returned most of their substance back into the thin gas from which they had once condensed. Here in the dark lush clouds between the stars, new raindrops made of many elements were forming, later generation of stars being born. Nearby, smaller raindrops grew, bodies far too little to ignite the nuclear fire, droplets in the interstellar mist on their way to form planets. Among them was a small world of stone and iron, the early Earth. Congealing and warming, the Earth released methane, ammonia, water and hydrogen gases that had been trapped within, forming the primitive atmosphere and the first oceans. Starlight from the Sun bathed and warmed the primeval Earth, drove storms, generated lightning and thunder. Volcanoes overflowed with lava. These processes disrupted molecules of the primitive atmosphere; the fragments fell back together into more and more complex forms, which dissolved into the early oceans. After a while the seas achieved the consistency of a warm, dilute soup. Molecules were organized, and complex chemical reactions driven, on the surface of clay. And one day a molecule arose that quite by accident was able to make crude copies of itself out of the other molecules in the broth. As time passed, more elaborate and more accurate self replicating molecules arose. Those combinations best suited to further replication were favored by the sieve of natural selection. Those that copied better produced more copies. And the primitive oceanic broth gradually grew thin as it was consumed by and transformed into complex condensations of self replicating organic molecules. Gradually, imperceptibly, life had begun. Single-celled plants evolved, and life began generating its own food. Photosynthesis transformed the atmosphere. Sex was invented. Once free living forms bonded together to make a complex cell with specialized functions. Chemical receptors evolved, and the Cosmos could taste and smell. One celled organisms evolved into multicellular colonies, elaborating their various parts into specialized organ systems. Eyes and ears evolved, and now the Cosmos could see and hear. Plants and animals discovered that land could support life. Organisms buzzed, crawled, scuttled, lumbered, glided, flapped, shimmied, climbed and soared. Colossal beasts thundered through steaming jungles. Small creatures emerged, born live instead of in hard-shelled containers, with a fluid like the early ocean coursing through their veins. They survived by swiftness and cunning. And then, only a moment ago, some small arboreal animals scampered down from the trees. They became upright and taught themselves the use of tools, domesticated other animals, plants and fire, and devised language. The ash of stellar alchemy was now emerging into consciousness. At an ever-accelerating pace, it invented writing, cities, art and science, and sent spaceships to the planets and the stars. These are some of the things that hydrogen atoms do, given fifteen billion years of cosmic evolution.
Carl Sagan (Cosmos)
A metallic hydrogen rocket!” she explained. “We reached 995,000 kilometers per hour after escaping Earth’s gravity and still had enough fuel to decelerate before reaching the new Port of Entry. You were right about the G-forces, by the way
Erasmo Acosta (K3+)
Actions Summary The following list of new institutions, policies and actions is my best effort at envisaging what is required for Australia to survive the climate emergency. • A National Target and Plan for 95% or more of electricity to be supplied by renewables by 2030. • State plans to electrify all transport, beginning with the swift retirement of non-electric buses and including a plan for 50% of all new car sales to be EVs by 2030. • Implement planned changes to how we work and live so as to minimise unnecessary travel. • A plan for clean hydrogen to replace bunker fuel in shipping. • A plan for the adoption of e-fuels for aviation, with an aim to have all domestic flights running on e-fuel by 2030. • A National Commission for Climate Adaptation, with a Coastal Defence Fund and a Commission for Primary Production operating under its umbrella. • A National Initiative on Drawdown Innovation to provide leadership in early stage research and fund some on-ground projects. • The Federal Government to help convene a Global Working Group on Geoengineering.
Tim Flannery (The Climate Cure: Solving the Climate Emergency in the Era of COVID-19)
Now, what is jet fuel? That depends. A turbojet has a remarkably undiscriminating appetite, and will run, or can be made to run, on just about anything that will burn and can be made to flow, from coal dust to hydrogen.
John Drury Clark (Ignition!: An informal history of liquid rocket propellants)
In a final energy comeuppance, I came to regret leaving fusion out of my nuclear chapter. Like most, I figured it was too good to be possible—zero mining (the fuel is hydrogen), zero greenhouse gases, zero waste stream, zero meltdown capability, zero weaponization.
Stewart Brand (Whole Earth Discipline: Why Dense Cities, Nuclear Power, Transgenic Crops, Restored Wildlands, and Geoengineering Are Necessary)
2011, I led the Department of Energy’s Quadrennial Technology Review to develop strategies for government support of emerging clean energy technologies. In one town hall meeting, I faced advocates for four different vehicle technologies—internal combustion engines powered by biofuels, compressed natural gas, hydrogen-powered fuel cells, and battery-powered plug-ins. Each of them believed that their technology was the optimal vision for the future, and that all the government had to do was support the development of the appropriate fueling infrastructure. When I reminded them that the country could probably deploy no more than two new fueling technologies at scale, a squabble ensued. There are several reasons I believe that electricity will fuel the passenger vehicles of the future, but one of them is that the existing electrical grid is a good start on the fueling infrastructure. If a widespread transition to plug-in electric cars does come about, systems thinking will be even more important as the electrical and transportation systems would have to work together to accommodate charging millions of vehicles.
Steven E. Koonin (Unsettled: What Climate Science Tells Us, What It Doesn’t, and Why It Matters)
It is well within the capabilities of current technology to create a stratospheric haze via any of a number of methods, including additives to jet fuel or artillery shells that disperse the gas hydrogen sulfide (H2S, which smells like rotten eggs) at high altitude. This would not be a onetime exercise: the haze would have to be refreshed constantly, as the particles settle out over a year or two. The amount of sulfur that would have to be added to the stratosphere each year would be only about one-tenth of that humans currently emit at much lower altitudes, so direct health impacts would be minimal. And projected costs are low enough that a small nation or even a single wealthy individual could carry out the entire project themselves.
Steven E. Koonin (Unsettled: What Climate Science Tells Us, What It Doesn’t, and Why It Matters)