Tuesday, March 31, 2015
Reading List: Living Among Giants
- Carroll, Michael. Living Among Giants. Cham, Switzerland: Springer International, 2015. ISBN 978-3-319-10673-1.
- In school science classes, we were taught that the solar system, our home in the galaxy, is a collection of planets circling a star, along with assorted debris (asteroids, comets, and interplanetary dust). Rarely did we see a representation of either the planets or the solar system to scale, which would allow us to grasp just how different various parts of the solar system are from another. (For example, Jupiter is more massive than all the other planets and their moons combined: a proud Jovian would probably describe the solar system as the Sun, Jupiter, and other detritus.) Looking more closely at the solar system, with the aid of what has been learned from spacecraft exploration in the last half century, results in a different picture. The solar system is composed of distinct neighbourhoods, each with its own characteristics. There are four inner “terrestrial” or rocky planets: Mercury, Venus, Earth, and Mars. These worlds huddle close to the Sun, bathing in its lambent rays. The main asteroid belt consists of worlds like Ceres, Vesta, and Pallas, all the way down to small rocks. Most orbit between Mars and Jupiter, and the feeble gravity of these bodies and their orbits makes it relatively easy to travel from one to another if you're patient. Outside the asteroid belt is the domain of the giants, which are the subject of this book. There are two gas giants: Jupiter and Saturn, and two ice giants: Uranus and Neptune. Distances here are huge compared to the inner solar system, as are the worlds themselves. Sunlight is dim (at Saturn, just 1% of its intensity at Earth, at Neptune 1/900 that at Earth). The outer solar system is not just composed of the four giant planets: those planets have a retinue of 170 known moons (and doubtless many more yet to be discovered), which are a collection of worlds as diverse as anywhere else in the domain of the Sun: there are sulfur-spewing volcanos, subterranean oceans of salty water, geysers, lakes and rain of hydrocarbons, and some of the most spectacular terrain and geology known. Jupiter's moon Ganymede is larger than the planet Mercury, and appears to have a core of molten iron, like the Earth. Beyond the giants is the Kuiper Belt, with Pluto its best known denizen. This belt is home to a multitude of icy worlds—statistical estimates are that there may be as many as 700 undiscovered worlds as large or larger than Pluto in the belt. Far more distant still, extending as far as two light-years from the Sun, is the Oort cloud, about which we know essentially nothing except what we glean from the occasional comet which, perturbed by a chance encounter or passing star, plunges into the inner solar system. With our present technology, objects in the Oort cloud are utterly impossible to detect, but based upon extrapolation from comets we've observed, it may contain trillions of objects larger than one kilometre. When I was a child, the realm of the outer planets was shrouded in mystery. While Jupiter, Saturn, and Uranus can be glimpsed by the unaided eye (Uranus, just barely, under ideal conditions, if you know where to look), and Neptune can be spotted with a modest telescope, the myriad moons of these planets were just specks of light through the greatest of Earth-based telescopes. It was not until the era of space missions to these worlds, beginning with the fly-by probes Pioneer and Voyager, then the orbiters Galileo and Cassini, that the wonders of these worlds were revealed. This book, by science writer and space artist Michael Carroll, is a tourist's and emigrant's guide to the outer solar system. Everything here is on an extravagant scale, and not always one hospitable to frail humans. Jupiter's magnetic field is 20,000 times stronger than that of Earth. and traps radiation so intense that astronauts exploring its innermost large moon Io would succumb to a lethal dose of radiation in minutes. (One planetary scientist remarked, “You need to have a good supply of grad students when you go investigate Io.”) Several of the moons of the outer planets appear to have oceans of liquid water beneath their icy crust, kept liquid by tidal flexing as they orbit their planet and interact with other moons. Some of these oceans may contain more water than all of the Earth's oceans. Tidal flexing may create volcanic plumes which inject heat and minerals into these oceans. On Earth, volcanic vents on the ocean floor provide the energy and nutrients for a rich ecosystem of life which exists independent of the Sun's energy. On these moons—who knows? Perhaps some day we shall explore these oceans in our submarines and find out. Saturn's moon Titan is an amazing world. It is larger than Mercury, and has an atmosphere 50% denser than the Earth's, made up mostly of nitrogen. It has rainfall, rivers, and lakes of methane and ethane, and at its mean temperature of 93.7°K, water ice is a rock as hard as granite. Unique among worlds in the solar system, you could venture outside your space ship on Titan without a space suit. You'd need to dress very warmly, to be sure, and wear an oxygen mask, but you could explore the shores, lakes, and dunes of Titan protected only against the cold. With the dense atmosphere and gravity just 85% of that of the Earth's Moon, you might be able to fly with suitable wings. We have had just a glimpse of the moons of Uranus and Neptune as Voyager 2 sped through their systems on its way to the outer darkness. Further investigation will have to wait for orbiters to visit these planets, which probably will not happen for nearly two decades. What Voyager 2 saw was tantalising. On Uranus's moon Miranda, there are cliffs 14 km high. With the tiny gravity, imagine the extreme sports you could do there! Neptune's moon Triton appears to be a Kuiper Belt object captured into orbit around Neptune and, despite its cryogenic temperature, appears to be geologically active. There is no evidence for life on any of these worlds. (Still, one wonders about those fish in the dark oceans.) If barren, “all these worlds are ours”, and in the fullness of time we shall explore, settle, and exploit them to our own ends. The outer solar system is just so much bigger and more grandiose than the inner. It's as if we've inhabited a small island for all of our history and, after making a treacherous ocean voyage, discovered an enormous empty continent just waiting for us. Perhaps in a few centuries residents of these remote worlds will look back toward the Sun, trying to spot that pale blue dot so close to it where their ancestors lived, and remark to their children, “Once, that's all there was.”
Friday, March 20, 2015
Partial Solar Eclipse: 2015-03-20
Click image to enlarge.
Here is the solar eclipse of March 20th, 2015, taken at maximum eclipse, around 09:35 UTC. Although this was a total eclipse, from my location (47°4' N 7°3' E) the Sun was only about 70% obscured. The sky was milky/murky, but the Sun was clearly visible through the solar filter.
Wednesday, March 18, 2015
Reading List: Rocket Ship Galileo
- Heinlein, Robert A. Rocket Ship Galileo. Seattle: Amazon Digital Services, [1947, 1974, 1988] 2014. ASIN B00H8XGKVU.
- After the end of World War II, Robert A. Heinlein put his wartime engineering work behind him and returned to professional writing. His ambition was to break out of the pulp magazine ghetto in which science fiction had been largely confined before the war into the more prestigious (and better paying) markets of novels and anthologies published by top-tier New York firms and the “slick” general-interest magazines such as Collier's and The Saturday Evening Post, which published fiction in those days. For the novels, he decided to focus initially on a segment of the market he understood well from his pre-war career: “juveniles”—books aimed a young audience (in the case of science fiction, overwhelmingly male), and sold, in large part, in hardcover to public and school libraries (mass market paperbacks were just beginning to emerge in the late 1940s, and had not yet become important to mainstream publishers). Rocket Ship Galileo was the first of Heinlein's juveniles, and it was a tour de force which established him in the market and led to a series which would extend to twelve volumes. (Heinlein scholars differ on which of his novels are classified as juveniles. Some include Starship Troopers as a juvenile, but despite its having been originally written as one and rejected by his publisher, Heinlein did not classify it thus.) The plot could not be more engaging to a young person at the dawn of the atomic and space age. Three high school seniors, self-taught in the difficult art of rocketry (often, as was the case for their seniors in the era, by trial and [noisy and dangerous] error), are recruited by an uncle of one of them, veteran of the wartime atomic project, who wants to go to the Moon. He's invented a novel type of nuclear engine which allows a single-stage ship to make the round trip, and having despaired of getting sclerotic government or industry involved, decides to do it himself using cast-off parts and the talent and boundless energy of young people willing to learn by doing. Working in their remote desert location, they become aware that forces unknown are taking an untoward interest in their work and seem to want to bring it to a halt, going as far as sabotage and lawfare. Finally, it's off to the Moon, where they discover the dark secret on the far side: space Nazis! The remarkable thing about this novel is how well it holds up, almost seventy years after publication. While Heinlein was writing for a young audience, he never condescended to them. The science and engineering were as accurate as was known at the time, and Heinlein manages to instill in his audience a basic knowledge of rocket propulsion, orbital mechanics, and automated guidance systems as the yarn progresses. Other than three characters being young people, there is nothing about this story which makes it “juvenile” fiction: there is a hard edge of adult morality and the value of courage which forms the young characters as they live the adventure. At the moment, only this Kindle edition and an unabridged audio book edition are available new. Used copies of earlier paperback editions are readily available.
Friday, February 20, 2015
Reading List: A Force of Nature
- Reeves, Richard. A Force of Nature. New York: W. W. Norton, 2008. ISBN 978-0-393-33369-5.
- In 1851, the Crystal Palace Exhibition opened in London. It was a showcase of the wonders of industry and culture of the greatest empire the world had ever seen and attracted a multitude of visitors. Unlike present-day “World's Fair” boondoggles, it made money, and the profits were used to fund good works, including endowing scholarships for talented students from the far reaches of the Empire to study in Britain. In 1895, Ernest Rutherford, hailing from a remote area in New Zealand and recent graduate of Canterbury College in Christchurch, won a scholarship to study at Cambridge. Upon learning of the award in a field of his family's farm, he threw his shovel in the air and exclaimed, “That's the last potato I'll ever dig.” It was. When he arrived at Cambridge, he could hardly have been more out of place. He and another scholarship winner were the first and only graduate students admitted who were not Cambridge graduates. Cambridge, at the end of the Victorian era, was a clubby, upper-class place, where even those pursuing mathematics were steeped in the classics, hailed from tony public schools, and spoke with refined accents. Rutherford, by contrast, was a rough-edged colonial, bursting with energy and ambition. He spoke with a bizarre accent (which he retained all his life) which blended the Scottish brogue of his ancestors with the curious intonations of the antipodes. He was anything but the ascetic intellectual so common at Cambridge—he had been a fierce competitor at rugby, spoke about three times as loud as was necessary (many years later, when the eminent Rutherford was tapped to make a radio broadcast from Cambridge, England to Cambridge, Massachusetts, one of his associates asked, “Why use radio?”), and spoke vehemently on any and all topics (again, long afterward, when a ceremonial portrait was unveiled, his wife said she was surprised the artist had caught him with his mouth shut). But it quickly became apparent that this burly, loud, New Zealander was extraordinarily talented, and under the leadership of J.J. Thomson, he began original research in radio, but soon abandoned the field to pursue atomic research, which Thomson had pioneered with his discovery of the electron. In 1898, with Thomson's recommendation, Rutherford accepted a professorship at McGill University in Montreal. While North America was considered a scientific backwater in the era, the generous salary would allow him to marry his fiancée, who he had left behind in New Zealand until he could find a position which would support them. At McGill, he and his collaborator Frederick Soddy, studying the radioactive decay of thorium, discovered that radioactive decay was characterised by a unique half-life, and was composed of two distinct components which he named alpha and beta radiation. He later named the most penetrating product of nuclear reactions gamma rays. Rutherford was the first to suggest, in 1902, that radioactivity resulted from the transformation of one chemical element into another—something previously thought impossible. In 1907, Rutherford was offered, and accepted a chair of physics at the University of Manchester, where, with greater laboratory resources than he had had in Canada, pursued the nature of the products of radioactive decay. By 1907, by a clever experiment, he had identified alpha radiation (or particles, as we now call them) with the nuclei of helium atoms—nuclear decay was heavy atoms being spontaneously transformed into a lighter element and a helium nucleus. Based upon this work, Rutherford won the Nobel Prize in Chemistry in 1908. As a person who considered himself first and foremost an experimental physicist and who was famous for remarking, “All science is either physics or stamp collecting”, winning the Chemistry Nobel had to feel rather odd. He quipped that while he had observed the transmutation of elements in his laboratory, no transmutation was as startling as discovering he had become a chemist. Still, physicist or chemist, his greatest work was yet to come. In 1909, along with Hans Geiger (later to invent the Geiger counter) and Ernest Marsden, he conducted an experiment where high-energy alpha particles were directed against a very thin sheet of gold foil. The expectation was that few would be deflected and those only slightly. To the astonishment of the experimenters, some alpha particles were found to be deflected through large angles, some bouncing directly back toward the source. Geiger exclaimed, “It was almost as incredible as if you fired a 15-inch [battleship] shell at a piece of tissue paper and it came back and hit you.” It took two years before Rutherford fully understood and published what was going on, and it forever changed the concept of the atom. The only way to explain the scattering results was to replace the early model of the atom with one in which a diffuse cloud of negatively charged electrons surrounded a tiny, extraordinarily dense, positively charged nucleus (that word was not used until 1913). This experimental result fed directly into the development of quantum theory and the elucidation of the force which bound the particles in the nucleus together, which was not fully understood until more than six decades later. In 1919 Rutherford returned to Cambridge to become the head of the Cavendish Laboratory, the most prestigious position in experimental physics in the world. Continuing his research with alpha emitters, he discovered that bombarding nitrogen gas with alpha particles would transmute nitrogen into oxygen, liberating a proton (the nucleus of hydrogen). Rutherford simultaneously was the first to deliberately transmute one element into another, and also to discover the proton. In 1921, he predicted the existence of the neutron, completing the composition of the nucleus. The neutron was eventually discovered by his associate, James Chadwick, in 1932. Rutherford's discoveries, all made with benchtop apparatus and a small group of researchers, were the foundation of nuclear physics. He not only discovered the nucleus, he also found or predicted its constituents. He was the first to identify natural nuclear transmutation and the first to produce it on demand in the laboratory. As a teacher and laboratory director his legacy was enormous: eleven of his students and research associates went on to win Nobel prizes. His students John Cockcroft and Ernest Walton built the first particle accelerator and ushered in the era of “big science”. Rutherford not only created the science of nuclear physics, he was the last person to make major discoveries in the field by himself, alone or with a few collaborators, and with simple apparatus made in his own laboratory. In the heady years between the wars, there were, in the public mind, two great men of physics: Einstein the theoretician and Rutherford the experimenter. (This perception may have understated the contributions of the creators of quantum mechanics, but they were many and less known.) Today, we still revere Einstein, but Rutherford is less remembered (except in New Zealand, where everybody knows his name and achievements). And yet there are few experimentalists who have discovered so much in their lifetimes, with so little funding and the simplest apparatus. Rutherford, that boisterous, loud, and restless colonial, figured out much of what we now know about the atom, largely by himself, through a multitude of tedious experiments which often failed, and he should rightly be regarded as a pillar of 20th century physics. This is the thousandth book to appear since I began to keep the reading list in January 2001.
Wednesday, February 18, 2015
Reading List: Tools for Survival
- Rawles, James Wesley. Tools for Survival. New York: Plume, 2014. ISBN 978-0-452-29812-5.
- Suppose one day the music stops. We all live, more or less, as part of an intricately-connected web of human society. The water that comes out of the faucet when we open the tap depends (for the vast majority of people) on pumps powered by an electrical grid that spans a continent. So does the removal of sewage when you flush the toilet. The typical city in developed nations has only about three days' supply of food on hand in stores and local warehouses and depends upon a transportation infrastructure as well as computerised inventory and payment systems to function. This system has been optimised over decades to be extremely efficient, but at the same time it has become dangerously fragile against any perturbation. A financial crisis which disrupts just-in-time payments, a large-scale and protracted power outage due to a solar flare or EMP attack, disruption of data networks by malicious attacks, or social unrest can rapidly halt the flow of goods and services upon which hundreds of millions of people depend and rely upon without rarely giving a thought to what life might be like if one day they weren't there. The author, founder of the essential SurvivalBlog site, has addressed such scenarios in his fiction, which is highly recommended. Here the focus is less speculative, and entirely factual and practical. What are the essential skills and tools one needs to survive in what amounts to a 19th century homestead? If the grid (in all senses) goes down, those who wish to survive the massive disruptions and chaos which will result may find themselves in the position of those on the American frontier in the 1870s: forced into self-reliance for all of the necessities of life, and compelled to use the simple, often manual, tools which their ancestors used—tools which can in many cases be fabricated and repaired on the homestead. The author does not assume a total collapse to the nineteenth century. He envisions that those who have prepared to ride out a discontinuity in civilisation will have equipped themselves with rudimentary solar electric power and electronic communication systems. But at the same time, people will be largely on their own when it comes to gardening, farming, food preservation, harvesting trees for firewood and lumber, first aid and dental care, self-defence, metalworking, and a multitude of other tasks. As always, the author stresses, it isn't the tools you have but rather the skills between your ears that determine whether you'll survive. You may have the most comprehensive medical kit imaginable, but if nobody knows how to stop the bleeding from a minor injury, disinfect the wound, and suture it, what today is a short trip to the emergency room might be life-threatening. Here is what I took away from this book. Certainly, you want to have on hand what you need to deal with immediate threats (for example, firefighting when the fire department does not respond, self-defence when there is no sheriff, a supply of water and food so you don't become a refugee if supplies are interrupted, and a knowledge of sanitation so you don't succumb to disease when the toilet doesn't flush). If you have skills in a particular area, for example, if you're a doctor, nurse, or emergency medical technician, by all means lay in a supply of what you need not just to help yourself and your family, but your neighbours. The same goes if you're a welder, carpenter, plumber, shoemaker, or smith. It just isn't reasonable, however, to expect any given family to acquire all the skills and tools (even if they could afford them, where would they put them?) to survive on their own. Far more important is to make the acquaintance of like-minded people in the vicinity who have the diverse set of skills required to survive together. The ability to build and maintain such a community may be the most important survival skill of all. This book contains a wealth of resources available on the Web (most presented as shortened URLs, not directly linked in the Kindle edition) and a great deal of wisdom about which I find little or nothing to disagree. For the most part the author uses quaint units like inches, pounds, and gallons, but he is writing for a mostly American audience. Please take to heart the safety warnings: it is very easy to kill or gravely injure yourself when woodworking, metal fabricating, welding, doing electrical work, or felling trees and processing lumber. If your goal is to survive and prosper whatever the future may bring, it can ruin your whole plan if you kill yourself acquiring the skills you need to do so.
Monday, February 9, 2015
Reading List: The Testament of James
- Suprynowicz, Vin. The Testament of James. Pahrump, NV: Mountain Media, 2014. ISBN 978-0-9670259-4-0.
- The author is a veteran newspaperman and was arguably the most libertarian writer in the mainstream media during his long career with the Las Vegas Review-Journal. He earlier turned his hand to fiction in 2005's The Black Arrow (May 2005), a delightful libertarian superhero fantasy. In the present volume he tells an engaging tale which weaves together mystery, the origins of Christianity, and the curious subculture of rare book collectors and dealers. Matthew Hunter is the proprietor of a used book shop in Providence, Rhode Island, dealing both in routine merchandise but also rare volumes obtained from around the world and sold to a network of collectors who trust Hunter's judgement and fair pricing. While Hunter is on a trip to Britain, an employee of the store is found dead under suspicious circumstances, while waiting after hours to receive a visitor from Egypt with a manuscript to be evaluated and sold. Before long, a series of curious, shady, and downright intimidating people start arriving at the bookshop, all seeking to buy the manuscript which, it appears, was never delivered. The person who was supposed to bring it to the shop has vanished, and his brothers have come to try to find him. Hunter and his friend Chantal Stevens, ex-military who has agreed to help out in the shop, find themselves in the middle of the quest for one of the most legendary, and considered mythical, rare books of all time, The Testament of James, reputed to have been written by James the Just, the (half-)brother of Jesus Christ. (His precise relationship to Jesus is a matter of dispute among Christian sects and scholars.) This Testament (not to be confused with the Epistle of James in the New Testament, also sometimes attributed to James the Just), would have been the most contemporary record of the life of Jesus, well predating the Gospels. Matthew and Chantal seek to find the book, rescue the seller, and get to the bottom of a mystery dating from the origin of Christianity. Initially dubious such a book might exist, Matthew concludes that so many people would not be trying so hard to lay their hands on it if there weren't something there. A good part of the book is a charming and often humorous look inside the world of rare books, one with which the author is clearly well-acquainted. There is intrigue, a bit of mysticism, and the occasional libertarian zinger aimed at a deserving target. As the story unfolds, an alternative interpretation of the life and work of Jesus and the history of the early Church emerges, which explains why so many players are so desperately seeking the lost book. As a mystery, this book works superbly. Its view of “bookmen” (hunters, sellers, and collectors) is a delight. Orthodox Christians (by which I mean those adhering to the main Christian denominations, not just those called “Orthodox”) may find some of the content blasphemous, but before they explode in red-faced sputtering, recall that one can never be sure about the provenance and authenticity of any ancient manuscript. Some of the language and situations are not suitable for young readers, but by the standards of contemporary mass-market fiction, the book is pretty tame. There are essentially no spelling or grammatical errors. To be clear, this is entirely a work of fiction: there is no Testament of James apart from this book, in which it's an invention of the author. A bibliography of works providing alternative (which some will consider heretical) interpretations of the origins of Christianity is provided. You can read an excerpt from the novel at the author's Web log; continue to follow the links in the excerpts to read the first third—20,000 words—of the book for free.
Friday, January 30, 2015
Reading List: The Case of the Displaced Detective Omnibus
- Osborn, Stephanie. The Case of the Displaced Detective Omnibus. Kingsport, TN: Twilight Times Books, 2013. ASIN B00FOR5LJ4.
- This book, available only for the Kindle, collects the first four novels of the author's Displaced Detective series. The individual books included here are The Arrival, At Speed, The Rendlesham Incident, and Endings and Beginnings. Each pair of books, in turn, comprises a single story, the first two The Case of the Displaced Detective and the latter two The Case of the Cosmological Killer. If you read only the first of either pair, it will be obvious that the story has been left in the middle with little resolved. In the trade paperback edition, the four books total more than 1100 pages, so this omnibus edition will keep you busy for a while. Dr. Skye Chadwick is a hyperspatial physicist and chief scientist of Project Tesseract. Research into the multiverse and brane world solutions of string theory has revealed that our continuum—all of the spacetime we inhabit—is just one of an unknown number adjacent to one another in a higher dimensional membrane (“brane”), and that while every continuum is different, those close to one another in the hyperdimensional space tend to be similar. Project Tesseract, a highly classified military project operating from an underground laboratory in Colorado, is developing hardware based on advanced particle physics which allows passively observing or even interacting with these other continua (or parallel universes). The researchers are amazed to discover that in some continua characters which are fictional in our world actually exist, much as they were described in literature. Perhaps Heinlein and Borges were right in speculating that fiction exists in parallel universes, and maybe that's where some of authors' ideas come from. In any case, exploration of Continuum 114 has revealed it to be one of those in which Sherlock Holmes is a living, breathing man. Chadwick and her team decide to investigate one of the pivotal and enigmatic episodes in the Holmes literature, the fight at Reichenbach Falls. As Holmes and Moriarty battle, it is apparent that both will fall to their death. Chadwick acts impulsively and pulls Holmes from the brink of the cliff, back through the Tesseract, into our continuum. In an instant, Sherlock Holmes, consulting detective of 1891 London, finds himself in twenty-first century Colorado, where he previously existed only in the stories of Arthur Conan Doyle. Holmes finds much to adapt to in this often bewildering world, but then he was always a shrewd observer and master of disguise, so few people would be as well equipped. At the same time, the Tesseract project faces a crisis, as a disaster and subsequent investigation reveals the possibility of sabotage and an espionage ring operating within the project. A trusted, outside investigator with no ties to the project is needed, and who better than Holmes, who owes his life to it? With Chadwick at his side, they dig into the mystery surrounding the project. As they work together, they find themselves increasingly attracted to one another, and Holmes must confront his fear that emotional involvement will impair the logical functioning of his mind upon which his career is founded. Chadwick, learning to become a talented investigator in her own right, fears that a deeper than professional involvement with Holmes will harm her own emerging talents. I found that this long story started out just fine, and indeed I recommended it to several people after finishing the first of the four novels collected here. To me, it began to run off the rails in the second book and didn't get any better in the remaining two (which begin with Holmes and Chadwick an established detective team, summoned to help with a perplexing mystery in Britain which may have consequences for all of the myriad contunua in the multiverse). The fundamental problem is that these books are trying to do too much all at the same time. They can't decide whether they're science fiction, mystery, detective procedural, or romance, and as they jump back and forth among the genres, so little happens in the ones being neglected at the moment that the parallel story lines develop at a glacial pace. My estimation is that an editor with a sharp red pencil could cut this material by 50–60% and end up with a better book, omitting nothing central to the story and transforming what often seemed a tedious slog into a page-turner. Sherlock Holmes is truly one of the great timeless characters in literature. He can be dropped into any epoch, any location, and, in this case, anywhere in the multiverse, and rapidly start to get to the bottom of the situation while entertaining the reader looking over his shoulder. There is nothing wrong with the premise of these books and there are interesting ideas and characters in them, but the execution just isn't up to the potential of the concept. The science fiction part sometimes sinks to the techno-babble level of Star Trek (“Higgs boson injection beginning…”). I am no prude, but I found the repeated and explicit sex scenes a bit much (tedious, actually), and they make the books unsuitable for younger readers for whom the original Sherlock Holmes stories are a pure delight. If you're interested in the idea, I'd suggest buying just the first book separately and see how you like it before deciding to proceed, bearing in mind that I found it the best of the four.
Saturday, January 10, 2015
Reading List: Enlightening Symbols
- Mazur, Joseph. Enlightening Symbols. Princeton: Princeton University Press, 2014. ISBN 978-0-691-15463-3.
Sometimes an invention is so profound and significant yet apparently
obvious in retrospect that it is difficult to imagine how people
around the world struggled over millennia to discover it, and how
slowly it was to diffuse from its points of origin into general use.
Such is the case for our modern decimal system of positional
notation for numbers and the notation for algebra and other
fields of mathematics which permits rapid calculation and
transformation of expressions. This book, written with the extensive source citations
of a scholarly work yet accessible to any reader familiar with
arithmetic and basic algebra, traces the often murky origins of
this essential part of our intellectual heritage.
From prehistoric times humans have had the need to count things,
for example, the number of sheep in a field. This could be
done by establishing a one-to-one correspondence between the
sheep and something else more portable such as
one's fingers (for a small flock), or pebbles kept in a sack.
To determine whether a sheep was missing, just remove a
pebble for each sheep and if any remained in the sack,
that indicates how many are absent. At a slightly more abstract
level, one could make tally marks on a piece of bark or clay
tablet, one for each sheep. But all of this does not imply
number as an abstraction independent of individual items of
some kind or another. Ancestral humans don't seem to have
required more than the simplest notion of numbers: until the
middle of the 20th century several tribes of Australian
aborigines had no words for numbers in their languages at all,
but counted things by making marks in the sand. Anthropologists
discovered tribes in remote areas of the Americas, Pacific
Islands, and Australia whose languages had no words for numbers
greater than four.
With the emergence of settled human populations and the
increasingly complex interactions of trade between villages
and eventually cities, a more sophisticated notion of numbers
was required. A merchant might need to compute how many
kinds of one good to exchange for another and to keep records
of his inventory of various items. The earliest known
written records of numerical writing are Sumerian cuneiform clay
tablets dating from around 3400 B.C.
These tablets show number symbols formed from two distinct
kinds of marks pressed into wet clay with a stylus. While
the smaller numbers seem clearly evolved from tally marks,
larger numbers are formed by complicated combinations of the
two symbols representing numbers from 1 to 59. Larger numbers
were written as groups of powers of 60 separated by spaces.
This was the first known instance of a positional number system,
but there is no evidence it was used for complicated calculations—just
as a means of recording quantities.
Ancient civilisations: Egypt, Hebrew, Greece, China, Rome, and the
Aztecs and Mayas in the Western Hemisphere all invented
ways of writing numbers, some sophisticated and capable of
representing large quantities. Many of these systems were
additive: they used symbols, sometimes derived from
letters in their alphabets, and composed numbers by writing
symbols which summed to the total. To write the number 563,
a Greek would write
γ=3. By convention, numbers were
written with letters in descending order of the value they
represented, but the system was not positional. This made
the system clumsy for representing large numbers, reusing
letters with accent marks to represent thousands and an
entirely different convention for ten thousands.
How did such advanced civilisations get along using number systems
in which it is almost impossible to compute? Just imagine a
Roman faced with multiplying MDXLIX by XLVII
(1549 × 47)—where do you start?
You don't: all of these civilisations used some form of
mechanical computational aid: an abacus, counting rods, stones
in grooves, and so on to actually manipulate numbers. The
Zi Suan Jing, dating from fifth century China, provides
instructions (algorithms) for multiplication, division, and
square and cube root extraction using bamboo counting sticks
(or written symbols representing them). The result of the
computation was then written using the numerals of the language.
The written language was thus a way to represent numbers, but
not compute with them.
Many of the various forms of numbers and especially computational
tools such as the abacus came ever-so-close to stumbling on the
place value system, but it was in India, probably before the
third century B.C. that a positional
decimal number system including zero as a place holder, with
digit forms recognisably ancestral to those we use today
emerged. This was a breakthrough in two regards. Now, by
memorising tables of addition, subtraction, multiplication,
and division and simple algorithms once learned by schoolchildren
before calculators supplanted that part of their brains, it was
possible to directly compute from written numbers. (Despite
this, the abacus remained in common use.) But, more profoundly,
this was a universal representation of whole numbers.
Earlier number systems (with the possible exception of that
invented by Archimedes in
The Sand Reckoner
[but never used practically]) either had a limit on the largest number
they could represent or required cumbersome and/or lengthy conventions
for large numbers. The Indian number system needed only ten symbols
to represent any non-negative number, and only the single
convention that each digit in a number represented how many of that
power of ten depending on its position.
Knowledge diffused slowly in antiquity, and despite India being on
active trade routes, it was not until the 13th century
introduced the new number system, which had been transmitted
via Islamic scholars writing in Arabic, to Europe in
Abaci. This book not only introduced the new number
system, it provided instructions for a variety of practical
computations and applications to higher mathematics. As revolutionary
as this book was, in an era of hand-copied manuscripts, its
influence spread very slowly, and it was not until the
16th century that the new numbers became almost universally used.
The author describes this protracted process, about which a great deal
of controversy remains to the present day.
Just as the decimal positional number system was becoming established
in Europe, another revolution in notation began which would
transform mathematics, how it was done, and our understanding of
the meaning of numbers. Algebra, as we now understand it, was known
in antiquity, but it was expressed in a rhetorical way—in words.
For example, proposition 7 of book 2 of Euclid's Elements
If a straight line be cut at random, the square of the whole is equal to the squares on the segments and twice the rectangle contained by the segments.Now, given such a problem, Euclid or any of those following in his tradition would draw a diagram and proceed to prove from the axioms of plane geometry the correctness of the statement. But it isn't obvious how to apply this identity to other problems, or how it illustrates the behaviour of general numbers. Today, we'd express the problem and proceed as follows:
“Here lies Diophantus,” the wonder behold.Oh, go ahead, give it a try before reading on! Today, we'd read through the problem and write a system of two simultaneous equations, where x is the age of Diophantus at his death and y the number of years his son lived. Then:
Through art algebraic, the stone tells how old;
“God gave him his boyhood one-sixth of his life,
One twelfth more as youth while whiskers grew rife;
And then one-seventh ere marriage begun;
In five years there came a bounding new son.
Alas, the dear child of master and sage
After attaining half the measure of his father's life chill fate took him.
After consoling his fate by the science of numbers for four years, he ended his life.”
Friday, January 2, 2015
Reading List: The Strangest Man
- Farmelo, Graham. The Strangest Man. New York: Basic Books, 2009. ISBN 978-0-465-02210-6.
- Paul Adrien Maurice Dirac was born in 1902 in Bristol, England. His father, Charles, was a Swiss-French immigrant who made his living as a French teacher at a local school and as a private tutor in French. His mother, Florence (Flo), had given up her job as a librarian upon marrying Charles. The young Paul and his older brother Felix found themselves growing up in a very unusual, verging upon bizarre, home environment. Their father was as strict a disciplinarian at home as in the schoolroom, and spoke only French to his children, requiring them to answer in that language and abruptly correcting them if they committed any faute de français. Flo spoke to the children only in English, and since the Diracs rarely received visitors at home, before going to school Paul got the idea that men and women spoke different languages. At dinner time Charles and Paul would eat in the dining room, speaking French exclusively (with any error swiftly chastised) while Flo, Felix, and younger daughter Betty ate in the kitchen, speaking English. Paul quickly learned that the less he said, the fewer opportunities for error and humiliation, and he traced his famous reputation for taciturnity to his childhood experience. (It should be noted that the only account we have of Dirac's childhood experience comes from himself, much later in life. He made no attempt to conceal the extent he despised his father [who was respected by his colleagues and acquaintances in Bristol], and there is no way to know whether Paul exaggerated or embroidered upon the circumstances of his childhood.) After a primary education in which he was regarded as a sound but not exceptional pupil, Paul followed his brother Felix into the Merchant Venturers' School, a Bristol technical school ranked among the finest in the country. There he quickly distinguished himself, ranking near the top in most subjects. The instruction was intensely practical, eschewing Latin, Greek, and music in favour of mathematics, science, geometric and mechanical drawing, and practical skills such as operating machine tools. Dirac learned physics and mathematics with the engineer's eye to “getting the answer out” as opposed to finding the most elegant solution to the problem. He then pursued his engineering studies at Bristol University, where he excelled in mathematics but struggled with experiments. Dirac graduated with a first-class honours degree in engineering, only to find the British economy in a terrible post-war depression, the worst economic downturn since the start of the Industrial Revolution. Unable to find employment as an engineer, he returned to Bristol University to do a second degree in mathematics, where it was arranged he could skip the first year of the program and pay no tuition fees. Dirac quickly established himself as the star of the mathematics programme, and also attended lectures about the enigmatic quantum theory. His father had been working in the background to secure a position at Cambridge for Paul, and after cobbling together scholarships and a gift from his father, Dirac arrived at the university in October 1923 to pursue a doctorate in theoretical physics. Dirac would already have seemed strange to his fellow students. While most were scions of the upper class, classically trained, with plummy accents, Dirac knew no Latin or Greek, spoke with a Bristol accent, and approached problems as an engineer or mathematician, not a physicist. He had hoped to study Einstein's general relativity, the discovery of which had first interested him in theoretical physics, but his supervisor was interested in quantum mechanics and directed his work into that field. It was an auspicious time for a talented researcher to undertake work in quantum theory. The “old quantum theory”, elaborated in the early years of the 20th century, had explained puzzles like the distribution of energy in heat radiation and the photoelectric effect, but by the 1920s it was clear that nature was much more subtle. For example, the original quantum theory failed to explain even the spectral lines of hydrogen, the simplest atom. Dirac began working on modest questions related to quantum theory, but his life was changed when he read Heisenberg's 1925 paper which is now considered one of the pillars of the new quantum mechanics. After initially dismissing the paper as overly complicated and artificial, he came to believe that it pointed the way forward, dismissing Bohr's concept of atoms like little solar systems in favour of a probability density function which gives the probability an electron will be observed in a given position. This represented not just a change in the model of the atom but the discarding entirely of models in favour of a mathematical formulation which permitted calculating what could be observed without providing any mechanism whatsoever explaining how it worked. After reading and fully appreciating the significance of Heisenberg's work, Dirac embarked on one of the most productive bursts of discovery in the history of modern physics. Between 1925 and 1933 he published one foundational paper after another. His Ph.D. in 1926, the first granted by Cambridge for work in quantum mechanics, linked Heisenberg's theory to the classical mechanics he had learned as an engineer and provided a framework which made Heisenberg's work more accessible. Scholarly writing did not come easily to Dirac, but he mastered the art to such an extent that his papers are still read today as examples of pellucid exposition. At a time when many contributions to quantum mechanics were rough-edged and difficult to understand even by specialists, Dirac's papers were, in the words of Freeman Dyson, “like exquisitely carved marble statues falling out of the sky, one after another.” In 1928, Dirac took the first step to unify quantum mechanics and special relativity in the Dirac equation. The consequences of this equation led Dirac to predict the existence of a positively-charged electron, which had never been observed. This was the first time a theoretical physicist had predicted the existence of a new particle. This “positron” was observed in debris from cosmic ray collisions in 1932. The Dirac equation also interpreted the spin (angular momentum) of particles as a relativistic phenomenon. Dirac, along with Enrico Fermi, elaborated the statistics of particles with half-integral spin (now called “fermions”). The behaviour of ensembles of one such particle, the electron, is essential to the devices you use to read this article. He took the first steps toward a relativistic theory of light and matter and coined the name, “quantum electrodynamics”, for the field, but never found a theory sufficiently simple and beautiful to satisfy himself. He published The Principles of Quantum Mechanics in 1930, for many years the standard textbook on the subject and still read today. He worked out the theory of magnetic monopoles (not detected to this date) and speculated on the origin and possible links between large numbers in physics and cosmology. The significance of Dirac's work was recognised at the time. He was elected a Fellow of the Royal Society in 1930, became the Lucasian Professor of Mathematics (Newton's chair) at Cambridge in 1932, and shared the Nobel Prize in Physics for 1933 with Erwin Schrödinger. After rejecting a knighthood because he disliked being addressed by his first name, he was awarded the Order of Merit in 1973. He is commemorated by a plaque in Westminster Abbey, close to that of Newton; the plaque bears his name and the Dirac equation, the only equation so honoured. Many physicists consider Dirac the second greatest theoretical physicist of the 20th century, after Einstein. While Einstein produced great leaps of intellectual achievement in fields neglected by others, Dirac, working alone, contributed to the grand edifice of quantum mechanics, which occupied many of the most talented theorists of a generation. You have to dig a bit deeper into the history of quantum mechanics to fully appreciate Dirac's achievement, which probably accounts for his name not being as well known as it deserves. There is much more to Dirac, all described in this extensively-documented scientific biography. While declining to join the British atomic weapons project during World War II because he refused to work as part of a collaboration, he spent much of the war doing consulting work for the project on his own, including inventing a new technique for isotope separation. (Dirac's process proved less efficient that those eventually chosen by the Manhattan project and was not used.) As an extreme introvert, nobody expected him to ever marry, and he astonished even his closest associates when he married the sister of his fellow physicist Eugene Wigner, Manci, a Hungarian divorcée with two children by her first husband. Manci was as extroverted as Dirac was reserved, and their marriage in 1937 lasted until Dirac's death in 1984. They had two daughters together, and lived a remarkably normal family life. Dirac, who disdained philosophy in his early years, became intensely interested in the philosophy of science later in life, even arguing that mathematical beauty, not experimental results, could best guide theorists to the best expression of the laws of nature. Paul Dirac was a very complicated man, and this is a complicated and occasionally self-contradictory biography (but the contradiction is in the subject's life, not the fault of the biographer). This book provides a glimpse of a unique intellect whom even many of his closest associates never really felt they completely knew.
Wednesday, December 31, 2014
Books of the year: 2014Here are my picks for the best books of 2014, fiction and nonfiction. These aren't the best books published this year, but rather the best I've read in the last twelvemonth. The winner in both categories is barely distinguished from the pack, and the runners up are all worthy of reading. Runners up appear in alphabetical order by their author's surname.
- The Martian by Andy Weir
- Miss Leavitt's Stars by George Johnson