
What is unknown is the buttress of what is known. If you focus upon what you know then you can become an expert in it, if you focus upon what we collectively find enigmatic then you become an experienced enigmatist. When your boots are a little too big try these for size.
Is time an illusion?What’s at Earth’s Core?How does a fertilized egg become a human?What happened to the Neanderthals?Why do we sleep?Where did life come from?How can observation affect the outcome of an experiment?How do entangled particles communicate?Why do placebos work?What is the universe made of?
Astronomers scouring the heavens with powerful telescopes can see objects that are billions of trillions of miles away. These observations have proven essential to piecing together a fairly refined picture of the history and evolution of the cosmos. Nevertheless, a gaping hole remains in our understanding of a basic question: What is the universe made of? For more than 100 years we’ve known about atoms, and over the past century or so we’ve gone further and identified atomic constituents like electrons and quarks, as well as their exotic cousins - neutrinos, muons, and the like. But there is now convincing evidence that these ingredients are a cosmic afterthought. Current data shows that if you weighed everything in existence, these familiar particles would amount to about 5 percent of the total. Most of the universe is composed of other stuff, which, with all of science’s deep insights, we’ve yet to identify.How do we know this? Well, over the course of many decades, astronomers studied the motion of galaxies and the stars within them, and found that the gravity exerted by this luminous matter was insufficient to account for the way these heavenly bodies moved. Only by positing large amounts of additional matter that doesn’t give off light (visible, x-ray, infrared, or any other kind) and is thus invisible to telescopes, could the data be explained. Through detailed cosmological measurements, scientists also discovered that this so-called dark matter couldn’t be made of the same electrons, protons, and neutrons that make up everything with which we are familiar.Then, in the late 1990s, two groups of astronomers, one led by Saul Perlmutter of the Lawrence Berkeley National Laboratory, the other by Brian Schmidt of the Australian National University, found something even stranger. Through observation of distant supernovas, these astronomers measured how the expansion rate of the universe has changed over time. Because of gravity’s relentless pull, most everyone expected that the expansion would be slowing. But the data from both groups showed the opposite. The expansion of the universe is speeding up. Something must be pushing outward, and luckily Einstein’s general theory of relativity provides a ready-made candidate: A uniform, diffuse energy spread throughout space can act as an antigravity force. Since this energy gives off no light, it’s called dark energy.Collectively, the observations establish that about 23 percent of the universe is dark matter and about 72 percent is dark energy. Everything else is squeezed into the remaining few percent.Several experiments are now under way to identify dark matter. Scientists are searching for what they suspect is an exotic species of particle. Some studies are looking for clues by analyzing particles bombarding Earth from space; others, like the Large Hadron Collider, will analyze collisions between extremely fast-moving protons that have the potential to create dark matter in the lab. We are guardedly optimistic that we’ll be able to identify dark matter soon. By contrast, the question of dark energy is wide open. What is its origin? What determined its quantity? Does the amount stay constant or vary? These are critical questions. Calculations show that if the amount of dark energy had been slightly larger, the universe would have blown apart so quickly that life as we know it could not exist.
- Brian Greene, author of The Elegant UniverseWhat is the purpose of noncoding DNA?Will forests slow global warming - or speed it up?What happens to information in a black hole?
Inside a black hole, gravity is so intense that neither matter nor energy can escape. But in 1975, Cambridge physicist Stephen Hawking said that something does escape: random particles now known as “Hawking radiation.” So if black holes eat organized matter - chock-full of information - and then spit out random noise, where does the information go?Hawking said it gets locked up inside as the black hole eventually evaporates, destroying the information in the process. Which creates a paradox. Because the rules of physics say information, like matter and energy, can’t be destroyed.Hawking was confident. He convinced his super-genius counterpart at Caltech, physicist Kip Thorne, that he was right - but Thorne’s colleague John Preskill remained skeptical. So they made a bet: Hawking and Thorne said the singularity at the heart of a black hole destroyed information; Preskill said “nuh-uh.” Then, in 2004, Hawking reversed his position and decided that things that fall into a singularity aren’t lost; their information does leak out, though no one, except maybe Hawking himself, can explain why or how. He presented Preskill with a baseball encyclopedia from which, presumably, information can be retrieved at will. Preskill accepted only grudgingly. “Even if you’re Stephen Hawking, it’s possible to be wrong twice,” he says.
- Erin BibaWhat causes ice ages?
Scientists know that small-scale ice ages occur every 20,000 to 40,000 years and that massive ones happen every 100,000 years or so. They just don’t know why. The current working theory - first proposed in 1920 by Serbian engineer Milutin Milankovitch - is that irregularities in Earth’s orbit change how much solar energy it absorbs, resulting in sudden (well, geologically speaking) cooling. While this neatly fits the timing of short-term events, there’s still a big problem. Over the past few decades, studies have shown that orbital fluctuations affect solar energy by 1 percent or less - far too little to produce massive climate shifts on their own. “The mystery is, what is the amplification factor?” says University of Michigan geologist and climatologist Henry Pollack. “What takes a small amount of solar energy change and produces a large amount of glaciation?”Studies of ice and seabed cores reveal that temperature rise and fall is heavily correlated with changes in greenhouse-gas concentrations. But it’s a chicken-and-egg problem. Are CO2 rises and falls a cause of climate change or an effect? If they are a cause, what initiates the change? Figuring this out could tell us a great deal about the current global warming problem and how it might be solved. But as Matthew Saltzman, a geologist at Ohio State puts it, “We need to know why greenhouse gases fluctuated in prehuman times, and we just don’t.”
- John Hockenberry, WIRED contributing editorWhy do the poles reverse?
Almost 800,000 years ago, compasses would have pointed south. A little further back, they would have pointed north. Evidence for such reversals comes from lava flows and cracks in the ocean floor, places where newly formed rock makes a record of the magnetic polarity. We know that as Earth spins, the liquid metal in its molten core churns, generating an electro-magnetic field. We also know that shifts in the movement of the core can alter the polarity of that field and that it takes about 7,000 years for the orientation to flip-flop once the process of reversal begins - something that happens on average two or three times every million years. But no one knows how it works. Some scientists believe the poles migrate slowly from one end to the other; some theorize that the magnetic field shuts down and then reemerges with opposite polarity. As for what triggers the event, experts have suggested that a huge impact - say, a giant meteor - could create a disturbance in the core. But research by Gary Glatzmaier, a planetary science professor at UC Santa Cruz, shows that a violent catalyst isn’t needed. So why does pole reversal occur? “That’s like asking, why do hurricanes start?” he says. “Well, they’re always trying to, and sometimes the conditions are just right.”
- Geoffrey Gagnon Why do we die when we do?
When asked why things die, physicists don’t hesitate: It’s the second law of thermodynamics. Everything, be it mineral, plant, or animal, a Lexus or a mitral valve or a protein in a cell wall, eventually breaks down. What that looks like in humans - what exactly it is that makes us age - is a question for biologists. It’s DNA damage by free radicals, maybe, or shrinkage of the caps on chromosomes. Telomeres, as they’re called, get smaller with each cell division. When they hit a certain length: apoptosis, or cell death. But for the best explanation of the when of our mortality, you have to ask the ecologists. They have a rough way of calculating life span. Basically, the larger the species, the slower its energy-delivery systems (all that internal tubing, all that complicated traffic); the lower the metabolic rate, the longer the life. Animals can live fast or burn slow. “If you’ve ever picked up a little mouse, it’s effectively vibrating, its heart is beating so fast,” says Brian Enquist, an ecologist at the University of Arizona. “A blue whale’s heart is like a slow metronome or the ringing of a church bell, a very slow bong… bong… bong.” Yet both get roughly the same number of beats - 100 million and change, spread over two years for the mouse and roughly 80 years for the whale. “There’s this beautiful invariant: All living creatures have about the same amount of energetic life,” Enquist says. Yet while many animals outmass us humans, few outlive us. Why the long life for us lightweights? Like the hide of a rhinoceros or the claws of a tiger, human cleverness makes us tough to kill. That means random longevity-enhancing genes have a pretty good shot at evading natural selection. A bird that gets eaten in its second month of life never passes on whatever fluke mutation might have given it - and its progeny - an extra year or two. As for the ecologists’ neat mathematical equation, “primates are a little different,” Enquist concedes. “For the number of heartbeats we have in our lives, we live a little longer than we should, and it’s a big mystery why that is.” He speculates that the difference for us outliers will be explained by brain size - or, rather, by how much time and energy humans spend growing their brains relative to the rest of their bodies. Why lavishing that extra energy on brainmaking translates into disproportionately long lives, Enquist isn’t sure (and at 37, he has only about 36 more years to figure it out). Luckily, the same biological aberration that allows people to contemplate their own mortality is responsible, albeit indirectly, for delaying it.
- Susan Dominus, writer for The New York Times MagazineWhy do we still have big questions?
Information is expanding 10 times faster than any product on this planet - manufactured or natural. According to Hal Varian, an economist at UC Berkeley and a consultant to Google, worldwide information is increasing at 66 percent per year - approaching the rate of Moore’s law - while the most prolific manufactured stuff - paper, let’s say, or steel - averages only as much as 7 percent annually. By this rough metric, knowledge is growing exponentially. Indeed, the current pace of discovery is accelerating so rapidly that it seems as if we’re headed for that rapture of enlightenment known as the Singularity. In fact, we may be nearly there. A decade ago, author John Horgan interviewed prestigious scientists in many fields and concluded in his book The End of Science that all the big questions had been answered. The world of science has been roughly mapped out - structure of atoms, nature of light, theories of relativity and evolution, and so on - and all that remains now is to color in the details. So why do we still have so many unanswered questions? Take the current state of physics: We don’t know what 96 percent of the universe is made of. We call it “dark matter,” a euphemism for our ignorance. Yet it is also clear that we know far more about the universe than we did a century ago, and we have put this understanding to practical use - in consumer goods like GPS receivers and iPods, in medical devices like MRI scanners, and in engineered materials like photovoltaic cells and carbon nanotubes. Our steady and beneficial progress in knowledge comes from steady and beneficial progress in tools and technology. Telescopes, microscopes, fluoroscopes, and oscilloscopes allow us to see in new ways and to know more about the universe. The paradox of science is that every answer breeds at least two new questions. More answers mean even more questions, expanding not only what we know but also what we don’t know. Every new tool for looking farther or deeper or smaller allows us to spy into our ignorance. Future technologies such as artificial intelligence, controlled fusion, and quantum computing (to name a few on the near horizon) will change the world - that means the biggest questions have yet to be asked.
- Kevin Kelly, author of Cool Tools