Long Now

The Long Now Foundation
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Apr 12, 2016 • 1h 32min

Priyamvada Natarajan: Solving Dark Matter and Dark Energy

## The darkness of dark matter and dark energy ALL THAT WE KNOW of the universe we get from observing photons, Natarajan pointed out. But dark matter, which makes up 90 percent of the total mass in the universe, is called dark because it neither emits nor reflects photons — and because of our ignorance of what it is. It is conjectured to be made up of still-unidentified exotic _collisionless_ particles which might weigh about six times more than an electron. Though some challenge whether dark matter even exists, Natarajan is persuaded that it does because of her research on “the heaviest objects in the universe“ — galaxy clusters of more than 1,000 galaxies. First of all, the rotation of stars within galaxies does not look Keplerian — the outermost stars move far too quickly, as discovered in the 1970s. Their rapid rate of motion only makes sense if there is a vast “halo” of dark matter enclosing each galaxy. And galaxy clusters have so much mass (90 percent of it dark) that their gravitation bends light, “lenses” it. A galaxy perfectly aligned on the far side of a galaxy cluster appears to us — via the Hubble Space Telescope — as a set of multiple arc-shaped (distorted) galaxy images. Studying the precise geometry of those images can reveal some of the nature of dark matter, such as that it appears to be “clumpy.” With the next generation of space telescopes — the James Webb Space Telescope that comes online in 2018 and the Wide-Field Infrared Survey Telescope a few years afterward — much more will be learned. There are also instruments on Earth trying to detect dark-matter particles directly, so far without success. As for dark energy — the _accelerating_ expansion of the universe — its shocking discovery came from two independent teams in 1998–99. Dark energy is now understood to constitute 72 percent of the entire contents of the universe. (Of the remainder, dark matter is 23 percent, and atoms — the part that we know — makes up just 4.6 percent.) When the universe was 380,000 years old (13.7 billion years ago), there was no dark energy. But now “the universe is expanding at a pretty fast clip.” Natarajan hopes to use galaxy-cluster lensing as a tool “to trace the geometry of space-time which encodes dark energy.” These days, she said, data is coming in from the universe faster than theory can keep up with it.” We are in a golden age of cosmology.”
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Mar 15, 2016 • 1h 28min

Jane Langdale: Radical Ag: C4 Rice and Beyond

## Revolutionary rice Feeding the world (and saving nature) in this populous century, Jane Langdale began, depends entirely on agricultural efficiency—the ability to turn a given amount of land and sunlight into ever more food. And that depends on three forms of efficiency in each crop plant: 1) interception efficiency (collecting sunlight); 2) conversion efficiency (turning sunlight into sugars and starch); and 3) partitioning efficiency (maximizing the edible part). Of these, after centuries of plant breeding, only conversion efficiency is far short of the theoretical maximum. Most photosynthesis (called “C3“) is low-grade, poisoning its own process by reacting with oxygen instead of carbon dioxide when environmental conditions are hot and dry. But some plants, such as corn and sugar cane, have a brilliant workaround. They separate the photosynthetic process into two adjoining cells. The outer cell creates a special four-carbon compound (hence “C4“) that is delivered to the oxygen-protected inner cell. In the inner cell, carbon dioxide is released from the C4 compound, enabling drastically more efficient photosynthesis to take place because carbon dioxide is at a much higher concentration than oxygen. Rice is a C3 plant--which happens to be the staple food for half the world. If it can be converted to C4 photosynthesis, its yield would increase by _50%_ while using _half_ the water. It would also be drought-resistant and need far less fertilizer. Langdale noted that C4 plants have evolved naturally 60 times in a variety of plant families, all of which provide models of the transition. “How difficult could it be?” she deadpanned. The engineering begins with reverse-engineering. For instance, the main leaves in corn are C4, but the husk leaves are C3-like, so the genes that affect the two forms of development can be studied. Langdale’s research suggests that the needed structural change in rice can be managed with about 12 engineered genes, and previous research by others indicates that the biochemical changes can be achieved with perhaps 10 genes. How much is needed for the eventual fine tuning will emerge later. When is later? The C4 Rice project began in 2006 at the International Rice Research Institute in the Philippines, funded by the Bill & Melinda Gates Foundation. The research is on schedule, and engineering should begin in 2019, with the expectation that breeding of delicious, fiercely efficient C4 rice could be complete by 2039. It is the kind of thing that highly focussed multi-generation science can accomplish.
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Feb 10, 2016 • 1h 25min

Stephen Pyne: Fire Slow, Fire Fast, Fire Deep

### Ecological wildfire “We are uniquely fire creatures,” Pyne began, “on a uniquely fire planet.” Life itself is a form of slow metabolic combustion—which eventually created oxygen and burnable vegetation that allowed fast combustion, ignited by lightning. Humans came along and mastered fire for warmth, food preparation, and managing the landscape, and that made us a keystone species. Humanity’s ecological signature on the world is fire. Then we made fire the all-purpose catalyst for craft (clay, glass, metal) and eventually industry, shifting to the vast geological resource of fossil fuels. That “pyric transition” made humans dominant on the earth, even to the point of affecting climate. We used fire to clear much of the world’s forest for agriculture. Then came a century of misdirection about wildfire. The forests of Europe are mostly too wet to burn, but by the late 19th century the leading foresters in world came from there and taught their ignorance to foresters in North America and India, where the land depends on seasonal fire for ecological health. National governments set about suppressing all wildfire, with catastrophic success. In the absence of the usual occasional local fires, massive fuel loads built up, and destructive megafires became the norm. There was an alternative theory of a “restoration strategy” to manage wildfire in way that would emulate how lightning and native American burning kept the landscape ecologically healthy, but it has been applied haltingly and fractionally, and megafires still rule. “The real argument for fire is that it does ecological work that nothing else does,” Pyne concluded. “Charismatic megaflora” like redwoods need fire. An ecologically rich mosaic of forest, savannah, and meadows needs fire. Healthy prairie needs fire or it gets taken over by invasive woody plants. People trained only as foresters are blind to all that. Wildfire practice now works best when it is guided by wildlife biologists who insist that red cockaded woodpeckers need fire-dependent longleaf pines, that grizzly bears need the berries that grow in recent burns, that pheasants need grassland burned free of invasive eastern red cedar. The techniques for prescribed burns for a bioabundant natural landscape are now well honed. They need to be applied much more widely. When in doubt how to proceed, ask the ecologists, who will ask the animals.
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Jan 12, 2016 • 1h 28min

Eric Cline: 1177 B.C.: When Civilization Collapsed

### When chaos overwhelmed civilization Archaeologist Cline began by declaring that the time he would most like to be transported to is the Late Bronze Age in the Mediterranean—the five centuries between 1700 and 1200 B.C. In those centuries eight advanced societies were densely connected—Egyptians, Assyrians, Babylonians, Canaanites, Hittites, Cypriots, Minoans, and Mycenaeans. They grew to power over two millennia, but they collapsed simultaneously almost overnight. What happened? The density of their connection can be learned from trade goods found in shipwrecks, from Egyptian hieroglyphs and wall paintings, and from countless well-preserved clay-tablet letters written between the states. The tin required for all that bronze (tin was the equivalent of oil today) came from Afghanistan 1,800 miles to the east. It was one of history’s most globalized times. In the 12th Century B.C. everything fell apart. For Cline the defining moment was the battle in 1177 B.C. (8th Year of Ramses III) when Egypt barely defeated a mysterious army of “Sea Peoples.” Who were they? Do they really explain the general collapse, as historians long assumed? Cline thinks the failure was systemic, made of a series of cascading calamities in a highly interdependent world. There were indeed invasions—they might have been soldiers, or refugees, or civil war, or all three. But the violence was probably set in motion by extensive drought and famine reported in tablet letters from the time. Voices in the letters: “There is famine in our house. We will all die of hunger.” “Our city is sacked. May you know it!” In some regions there were also devastating earthquakes. The interlinked collapses played out over a century as central administrations failed, elites disappeared, economies collapsed, and whole populations died back or moved elsewhere. In the dark centuries that followed the end of the Bronze Age, romantic myths grew of how wondrous the world had once been. Homer sang of Achilles, Troy, and Odysseus. Those myths inspired the Classical Age that eventually emerged. Cline wonders, could the equivalent of the Bronze Age collapse happen in our current Age?
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Nov 24, 2015 • 1h 35min

Philip Tetlock: Superforecasting

Philip Tetlock, an academic and author known for leading the Good Judgment Project, dives into the art of forecasting. He reveals how amateur 'superforecasters' outperformed seasoned intelligence officers by applying rigorous scoring techniques. Tetlock discusses balancing cognitive errors and teamwork to achieve better predictions. He also critiques the certainty often seen in intelligence assessments and emphasizes the need for probabilistic thinking. Lastly, he proposes using forecasting methods to enhance public debates and tackle complex policy issues.
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Oct 7, 2015 • 1h 21min

James Fallows: Civilization's Infrastructure

### Infrastructure investment tricks All societies under-invest in their infrastructure—in the systems that allow them to thrive. There is hardware infrastructure: clean water, paved roads, sewer systems, airports, broadband; and, Fallows suggested, software infrastructure: organizational and cultural practices such as education, safe driving, good accounting, a widening circle of trust. China, for example, is having an orgy of hard infrastructure construction. It recently built a hundred airports while America built zero. But it is lagging in soft infrastructure such as safe driving and political transition. Infrastructure always looks unattractive to investors because the benefits: 1) are uncertain; 2) are delayed; and 3) go to others—the public, in the future. And the act of building infrastructure can be highly disruptive in the present. America for the last forty years has starved its infrastructure, but in our history some highly controversial remarkable infrastructure decisions got through, each apparently by a miracle—the Louisiana Purchase, the Erie Canal, the Gadsden Purchase, the Alaska Purchase, National Parks, Land Grant colleges, the GI Bill that created our middle class after World War II, and the Interstate highway system. In Fallows’ view, the miracle that enabled the right decision each time was either an _emergency_ (such as World War II or the Depression), _stealth_ (such as all the works that quietly go forward within the military budget or the medical-industrial complex), or a _story_ (such as Manifest Destiny and the Space Race). Lately, Fallows notes, there is a little noticed infrastructure renaissance going in some mid-sized American cities, where the political process is nonpoisonous and pragmatic compared to the current national-level dysfunction. By neglecting the long view, Fallows concluded, we overimagine problems with infrastructure projects and underimagine the benefits. But with the long view, with the new wealth and optimism of our tech successes, and expanding on the innovations in many of our cities, there is compelling story to be told. It might build on the unfolding emergency with climate change or on the new excitement about space exploration. Responding to need or to opportunity, we can tell a tale that inspires us to reinvent and build anew the systems that make our society flourish.
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Sep 22, 2015 • 1h 42min

Saul Griffith: Infrastructure and Climate Change

## Green infrastructure Griffith began with an eyeroll at the first round of responses in the US to reducing greenhouse gases, a program he calls “peak Al Gore.” Some activities feel virtuous —becoming vegetarian, installing LED lights, avoiding bottled water, reading news online, using cold water detergent, and “showering less in a smaller, colder house”—but they demand constant attention and they don’t really add up to what is needed. Griffith’s view is that we deal best with greenhouse gases by arranging our infrastructure so we don’t have to think about climate and energy issues every minute. Huge energy savings can come from designing our buildings and cars better, and some would result from replacing a lot of air travel with “video conferencing that doesn’t suck.“ Clean energy will mostly come from solar, wind, biofuels (better ones than present), and nuclear. Solar could be on every roof. The most fuel-efficient travel is on bicycles, which can be encouraged far more. Electric cars are very efficient, and when most become self-driving they can be lighter and even more efficient because “autonomous vehicles don’t run into each other.” Sixty percent of our energy goes to waste heat; with improved design that can be reduced radically to 20 percent. Taking the infrastructure approach, in a few decades the US could reduce its total energy use by 40 percent, while eliminating all coal and most oil and natural gas burning, with no need to shower less.
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Aug 11, 2015 • 1h 22min

Sara Seager: Other Earths. Other Life.

## To find living exoplanets Thanks to recent exoplanet research, Seager began, we now know that nearly all of our galaxy’s 300 billion stars are accompanied by planets, and a unexpectedly high number of them are rocky like Earth, and many of those orbit in a “habitable” range—meaning that they could harbor liquid water and perhaps life. How can we detect that life? (To learn about the 4,700-plus planets so far discovered, Seager recommended an exciting dynamic map and encyclopedia from NASA called “[Eyes on Exoplanets](http://eyes.jpl.nasa.gov/eyes-on-exoplanets.html).” Seager predicts that “If an Earth 2.0 exists, we have the capability to find and identify it by the 2020s.”) The way to discover life from a distance is to search for spectrographic evidence of “biosignature gases” such as oxygen or methane in the planetary atmosphere. To do that we have to acquire direct imaging of the rocky planets, but we can’t because our telescopes are blinded by the brilliance of the planet’s star, a billion times brighter than the planet. “It’s like looking for a firefly next to a searchlight, from thousands of miles away,” Seager said. Even the next planet-discovery telescope, called TESS (Transiting Exoplanet Survey Satellite), which is coming in 2018, will not be able to study exoplanet atmospheres. The solution that Seager has been working on is called [Starshade](http://planetquest.jpl.nasa.gov/video/15). To perfectly occult a star with a perfectly dark, hard-edged shadow, it will be deployed tens of thousands of kilometers from its telescope. It will be a disk 15 to 20 meters in diameter, with a perimeter of exotically shaped “petals” to defeat the effect of light diffracting around the edges of the disk. The edges have to be geometrically exact and machined to razor sharpness. The Starshade would fly in formation with a telescope located at the stable Lagrange point called L2, a million miles from Earth in the direction away from the Sun. The cost, including launch, will be about $650 million—not currently budgeted by NASA. Now that we know planets are extremely common, one of the profoundest questions is whether life is also common in our galaxy, or is it extremely rare? Seager thinks that life abounds out there, and we will be able to point to examples in this century.
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8 snips
Jul 23, 2015 • 1h 27min

Ramez Naam: Enhancing Humans, Advancing Humanity

### Enhancing humans and humanity Beginning with the accelerating pace of biotech tools for human health and enhancement, Naam noted that health issues such as disease prevention will be drastically easier to implement than enhancement. Preventing some hereditary diseases can be done with a single gene adjustment, whereas enhancement of traits like intelligence or longevity entails the fine tuning of hundreds of genes. He favors moving ahead with human germline engineering to totally eliminate some of our most horrific diseases. Over time he expects that human gene editing will lead in the opposite direction from the enforced conformity depicted in _Brave New World_ and the film “Gattaca.” Instead people will relish exploring variety, and the plummeting costs of the technology will mean that the poor will benefit as well as the rich. Naam’s brain discussion began with the Sergey Brin quote, “We want Google to be the third half of your brain.” Brain interface tools are proliferating. There are already 200,000 successful cochlear implants which feed sound directly into the nervous system. There is a digital eye that feeds pretty good visual data directly to the brain via a jack in the side of the user’s head. There is a hippocampus chip that can restore brain function in a rat. Rat brains have been linked so that what one rat learns, the other rat knows. The paper on that work was titled “Meta-organism of Two Rats on the Internet.” Humans also have been linked brain to brain at a distance to share function. Zebrafish have been lit up to show all their neurons firing in real time. Coming soon is the deployment of “neural dust” that can provide ultrasonic communications with tens of thousands of neurons at a time. How profound are the ethical issues? Naam observed that we already have many of the attributes of telepathy in our cell phones and smart phones. They came so rapidly and cheaply that they erased most of the concerns about a “digital divide.” Half of the world is now on the Internet, with the rest coming fast. And rather than a divider, the technology proved to be an equalizer and a connector, fostering economic growth and the rapid spread and sifting of ideas. Digital connectivity, he argued, is widening everyone’s “circle of empathy.” A viral video started the Arab Spring. Viral videos are changing how everyone thinks about race in America. These technologies, he concluded, are making humans more humane. One question from the audience inquired about the origin of so much reference in the Nexus series to group meditation as the epitome of mind sharing. Naam noted that Buddhists, including the Dalai Lama, are highly interested in brain science, and his own experiences of the ecstacy of mind sharing were at a rave at Burning Man and a ten-day Vipassana Meditation Retreat in Thailand. I asked if he agreed with the current round of panic about superintelligent artificial intelligence posing an existential threat to humanity. He said no. The dark scenarios imagine an AI so smart it implements new and grotesquely harmful pathways to solve a poorly contextualized problem. Naam pointed out that “Software almost never does anything well by accident.” (A flock of Tweets burst from the theater with that line.) And the dark scenarios imagine an isolated rogue super-capable AI. In reality nothing really capable is developed in isolation.
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Jun 10, 2015 • 1h 43min

Neil Gaiman: How Stories Last

## How stories last Stories are alive. The ones that last, Gaiman said, outcompete other stories by changing over time. They make it from medium to medium—from oral to written to film and beyond. They lose uninteresting elements but hold on to the most compelling bits or even add some. The most popular version of the Cinderella story (which may have originated long ago in China) has kept the gloriously unlikely _glass_ slipper introduced by a careless French telling. “Stories,” Gaiman said, “teach us how the world is put together and the rules of living in the world, and they come in an attractive enough package that we take pleasure from them and want to help them propagate.” Northwest coast native Americans have a tale about a beautiful woman and young man whose forbidden love was punished by the earth shaking, and black ash on snow, and finally fire coming from a mountain, killing many people. It stopped only when the beautiful woman was thrown into the burning mountain. That is important information-- solid-seeming mountains can suddenly erupt, and early warnings of that are earthquakes and ash. As pure information it won’t last beyond three generations. But add in beauty and forbidden love and tragic death, and the story will be told as long as people live in the mountains. The first emperor of China died 2,300 years ago. He was so powerful that he was able to totally conceal the location of his tomb, and all that was left was stories about the fabulous treasures buried with him. There was said to a whole army of terracotta warriors and ships floating on lakes of mercury. A few years ago a terracotta warrior was dug up in a field in China, and then a whole army of them. Archaeologists figured out where the emperor’s mausoleum must be buried, but first they did something not normally done at archeological digs. They checked if there might be any incredibly poisonous mercury around. There is. Gaiman said he learned something important about stories from his cousin Helen Fagin, a Holocaust survivor who taught class in a Polish ghetto during the Nazi occupation. Books were forbidden on pain of death, but Helen had a Polish translation of _Gone With the Wind_ she read at night, and she told its story to her entranced students by day. “The magic of escapist fiction,” Gaiman said, “is that it can offer you escape from an otherwise intolerable situation, and it can furnish you with armor, knowledge, weapons, and other tools you can take back into your life to make it better.” “‘Once upon a time,’ Gaiman said, “is code for ‘I’m lying to you.’ We experience stories as lies and truth at the same time. We learn to empathize with real people via made-up people. The most important thing that fiction does is it lets us look out through other eyes, and that teaches us empathy—that behind every pair of eyes is somebody like us.“ Stories have their own form of life, Gaiman concluded. “You can view people as this peculiar byproduct that stories use for breeding and transmission. They are symbiotic with us. They are the thing that we have used since the dawn of humanity to become more than just one person.“

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