This was a favorite book of mine as a child. It was one of the last books that I scanned and uploaded to sciencemadness.org. That's probably for the best, since I was still learning how to make good scans and PDFs with the early books.
When I first started scanning and uploading books, Google Books did not yet exist. The HathiTrust did not yet exist. Project Gutenberg and Distributed Proofreaders did exist, but their focus on perfect text transcription of non-technical writing did not really suit the books that I wanted to share.
I stopped scanning books because the world largely caught up and surpassed what I could do. Between HathiTrust, Library Genesis, and sci-hub, there has never been a better time for doing deep-dive reading from the comfort of one's own living room. But I'm proud that so many people have enjoyed my scan of this book over the years.
You're the source of that PDF? I can't thank you enough for how much I appreciate that! You, plus Dr Clark of course, single-handedly sparked my interest in chemistry, which up until that point I'd considered a boring collection of facts to rote memorize. This book convinced me to take chemistry as my last undergrad lab rather an easier course, which really opened my eyes to the fascinating and complex physics going on down there. Thanks so much for your effort in spreading knowledge of the world!
I'm glad that it was so inspirational for you! If this is the only thing you've ever seen from sciencemadness, you should also check out the other books in the library:
It's kind of a grab-bag of old scanned texts that I compiled from random third party sources in the earlier days of the web plus those that I scanned personally.
Also see the Los Alamos Technical Reports collection if you might be interested in oddball chemistry, physics, and material science publications from America's premiere nuclear weapons laboratory:
Like "Chemistry of Uranium and Plutonium" -- containing both theoretical and practical documentation for the handling, processing, and analysis of plutonium in the laboratory:
So I assume fo "Ignition!" you did the OCR and then reading the text? The font set to Baskerville, and chemical formulas drawn as ASCII, with = and # as double and triple bonds - or there were better solutions?
People do translations of the book and it's usually highly appreciated by those who doesn't read English. Excellent book. The introduction by Asimov is also awesome.
The OCR text beneath the page image is there to make it easier to search. I used ABBYY FineReader for the OCR process. I didn't do any manual reviewing or correcting of the automatically generated OCR text. I ran additional scripted tools of my own to optimize the PDF that I generated from FineReader for small file size.
"If your answer to the first question is that you are thrilled and fascinated by things that burn and explode, and you love to watch fireworks displays, or you simply want to send a rocket higher than the boy next door, then this book is not written for you, and you had better find something less dangerous to amuse you."
I encountered that book when I was 9. Naturally, I had to read the rest of it! What boy could resist?
I didn't realize that one was rare and expensive! I have it sitting on my shelf next to the 1965 Model Rocketry manual from Estes Industries. But it looks like archive.org already has a scan, so I don't need to scan it myself:
I think I was 10 when I found this. The interest in rocketry it kindled has lasted my lifetime. Wonderful book! Wish I still had my copy for old time's sake.
Ah yes, the book that many of the best rocket engineering quotes come from. I've always been partial to this one:
“It is, of course, extremely toxic, but that’s the least of the problem. It is hypergolic with every known fuel, and so rapidly hypergolic that no ignition delay has ever been measured. It is also hypergolic with such things as cloth, wood, and test engineers, not to mention asbestos, sand, and water-with which it reacts explosively. It can be kept in some of the ordinary structural metals-steel, copper, aluminium, etc.-because of the formation of a thin film of insoluble metal fluoride which protects the bulk of the metal, just as the invisible coat of oxide on aluminium keeps it from burning up in the atmosphere. If, however, this coat is melted or scrubbed off, and has no chance to reform, the operator is confronted with the problem of coping with a metal-fluorine fire. For dealing with this situation, I have always recommended a good pair of running shoes.”
This is the passage that taught me the word hypergolic, while the book itself tried its best to teach me how to write about obscure subjects naturally.
It feels like hanging out with him through his career, and you’re glad along with him that he didn’t accidentally breathe in too much red fuming nitric acid. Math be damned, I give this book 11/10
After reading this book (got a reprint from bookdepository), I am yearning for more. Not necessarily on this very topic, but in this vein: slightly technical, but easily followed even when I know very little on the subject, very humorous and personable, hands on.
I would especially love to read something like this on the development of the A bomb and first reactors - like the very fact that the first reactor was called the Chicago Pile, was, well, a pile of graphite, uranium, and uranium oxide bricks, 400 tons of it, under a rafters of the Chicago University stadium, in the heart of Chicago, with zero radiation sheilding and was happily runnuing for 3 months. Wikipedia has a lot, but it's mostly dry description of the basic facts and history - no zest.
I didn't see liquid methane (CH4) during my quick scan, is it covered in the book?
In a victory of worse-is-better, SpaceX is using methane because it makes Starship/Raptor simple, cheap, and more reliable (a passive cooling system is enough to store it, storable for a more extended period than hydrogen, does not leak, does not require insulation on the fuel tank, and rocket design is simpler)
Methane makes in-space refueling easier, and methane can be produced, handled, and stored more readily on Mars. It also makes Starship rapidly reusable (unike Falcon, whose kerosene Merlin engines need to be cleaned between flights to remove soot)
I don't think they were thinking about reusable rocket engines at that point in time. The primary (?) advantage of methane over kerosene is that it doesn't deposit soot on engine parts, which is highly important for SpaceX today, but not really anyone else in history.
Here's one reference to methane-LOX in the book ("nobody could see any point"):
- "The VfR was completely unaware of all of this when they started work. Oberth had originally wanted to use methane as fuel, but as it was hard to come by in Berlin, their first work was with gasoline and oxygen. Johannes Winkler, however, picked up the idea, and working independently of the VfR, was able to fire a liquid oxygen-liquid methane motor before the end of 1930. This work led nowhere in particular, since, as methane has a performance only slightly superior to that of gasoline, and is much harder to handle, nobody could see any point to following it up." (pages 7-8)
There's more references to methane + [exotic oxidizers], because (going off my memory) they were to trying to min-max Isp performance, for interplanetary probes, constrained to a certain cryogenic temperature range. (This predates radioisotope heaters, I believe. Not *electric* generators -- these little heater things [0]). Liquid CH₄ looked like a good match for the deep-space thermal environment.
- "Deep space probes, working at low temperatures, will probably use methane, ethane, and diborane for fuels, although propane is a possibility. The oxidizers will be OF₂, and possibly ONF₃ and NO₂F, while perchloryl fluoride, ClO₃F, would be useful as far out as Jupiter." (page 191)
(If anyone at Google is reading this, could you consider adding search support for numerals in the superscripts and subscripts block [1]; they don't seem to be normalized in a sensible way. ClO₃F and ClO3F are entirely different searches).
"It's only bad habit is that it decomposes exothermically -- and since
the rate of decomposition is accelerated with temperature, this reaction
can run away from you. But that hardly deserves the bad press it's gotten.
LOX will also bite you, quite readily, if you're careless. "Wings" simply
got it wrong. (Even _Ignition!_, while pretty sour on hydrogen peroxide due
to the decomposition hazard, has the facts right, and only the emphasis is
arguable -- I don't understand how someone can cozy up to ClF5 while
considering peroxide dangerous; but that was Clark's position! )"
SpaceX isn't the only one looking at methalox engines for reusability, though they're definitely the farthest along. Blue Origin's BE-4 engines use methalox; New Glenn's planned to be at least partially reusable, and ULA might try to reuse them on Vulcan with SMART engine recovery.
Technically you could synthesize more complex hydrocarbons such as kerosene as well, it's just that it's way more complexity, energy, and infrastructure required.
There are plenty of references to methane, but no in-depth story about systems using it.
The last part of the book, attempting to predict what fuels would be popular, prescribed methane for deep space probes, for many of the same reasons you give, but failed to foresee reusable boosters or other departures from the status quo.
> as methane has a performance only slightly superior
to that of gasoline, and is much harder to handle, nobody could see
any point...
> For the big first-stage space boosters we will continue to use liquid
oxygen and RP-1 or the equivalent. They work and they're cheap —
and Saturn V uses a lot of propellant! Later, we may shift to hydrogen
as a first-stage fuel, but it appears unlikely. The development of a
reusable booster won't change the picture, but if a ram-rocket booster
is developed all bets are off.
> For the upper stages, the hydrogen-oxygen combination of the
J-2 is very satisfactory, and will probably be used for a long time.
Later, as more energy is needed, there may be a shift, for the final
stage, to hydrogen-fluorine or hydrogen-lithium-fluorine...
> Deep space probes, working at low temperatures, will probably use
methane, ethane, and diborane for fuels, although propane is a
possibility. The oxidizers will be OF2, and possibly ONF3 and NO2F...
If you have the slightest interest in rockets, you should read this funny and informative book. You don't need to be a chemist to follow. I have a hardcopy at home and recommend to read it this way, as the contents are sometimes densely explained and you want to look up some additional information on the Internet in parallel.
I bought this as an audiobook, not realizing how dense some of the chapters are. The narrator is actually great, but you need to be ready to hit the 30-second skip button a lot as he gets into the details.
The narrator, Jonathan Todd Ross (just looked him up) was a champ. I listen to a lot of audiobooks and there is a wide range of quality and this guy nailed it. The book is filled with so many insane chemical names it must have been exhausting!
I don't personally care much about rocketry, and chemistry is easily one of my weakest subjects. But this book hooked me early on and I couldn't stop reading. I even learned a little chemistry along the way!
Fascinating insight into a crazy part of industrial engineering history.
Most deep-space probes use storable hypergolics (hydrazines + nitrogen tetroxide). Some of the crazy parts of this book actually came true!
(I don't intuitively understand how the JWST has $10 billion precision optics and hypercorrosive oxidizers right next to each other, and nothing bad happens. Engineering baffles me).
Not just deep-space probes; Dragon, Orion, and I think Starliner all use hypergols. Plenty of satellites do as well, though I think there's a trend towards using various sorts of electric propulsion. Really, the big misprediction of the book (looking at chapter 13, "What Happens Next") is that it doesn't consider missiles (and some upper/deep-space stages) moving to solid propellant; but it's a book about liquid propellants, so I'm not too surprised.
Absolutely! I’m sure they analyzed for that, but backflow to the opposite direction of the nozzle is quite unintuitive but normal in rarefied flow, with propellant deposition next to the nozzle possible and documented [1]. Just because you point it away from the sensitive stuff does not mean it won’t get there and leave nasty traces.
The propellant tanks don’t leak, the combustion products aren’t corrosive.
Designing spacecraft is like “does this material ever outgas anything which might affect other parts? I guess we can’t use it” much less leaky propellant tanks.
Those experiments generally needed to be run to figure out what was possible and what the different realistic options were, though. There's also more uses for propellants than just orbital launchers; propellant for ICBMs (and other strategic missiles), thrusters for attitude control, some of the monopropellants can also be used to power APUs for hydraulics or electricity. But yes, most applications these days go with simpler, more stable fuels, especially for commercial companies that don't want to spend a bunch of extra money wrangling more sensitive fuels for a few extra seconds of Isp.
When I first started scanning and uploading books, Google Books did not yet exist. The HathiTrust did not yet exist. Project Gutenberg and Distributed Proofreaders did exist, but their focus on perfect text transcription of non-technical writing did not really suit the books that I wanted to share.
I stopped scanning books because the world largely caught up and surpassed what I could do. Between HathiTrust, Library Genesis, and sci-hub, there has never been a better time for doing deep-dive reading from the comfort of one's own living room. But I'm proud that so many people have enjoyed my scan of this book over the years.