This Friday, in honor of my new facebook friend Steven Chu, I'd like to examine his "White Roofs" campaign through a Fermi problem.
Steven Chu has said that we could all save energy simply by painting our roofs white. The idea is the same one behind why I don't wear a black shirt on a sunny day (and white after Labor Day). Black objects absorb light, and with it, heat, while white objects reflect it. So if you're trying to keep your house cool in the summer, it makes sense to have a roof that reflects sunlight instead of absorbing it. Here's the schpiel:
But how much energy do you save, really?
The Fermi Problem:
The solar flux at Earth's atmosphere is about 1360 watts per square meter. About 0.3 of this is reflected back into space, while the rest is absorbed by the earth. Given the square footage of your roof, how much energy (assumed as heat) would a black roof absorb? How much energy would a white roof absorb?
Now, you could give Secretary Chu the benefit of the doubt and assume that black roofs absorb all of the sun's energy, while white roofs reflect it all. But we're talking getting people to actually paint their roofs white. For reals! So we're going above and beyond the Fermi Problem protocol for this week's problem.
How can we test the difference in absorption between light and dark materials? Let's try placing two thermometers in the sunlight. Procure two boxes. Cover one with white paper, and the other with black paper. Put a thermometer in each box. Go inside and reread a few chapters of Dialogue Concerning Two New Sciences. Then check to see which thermometer reads a higher temperature. Let us know what you find out. Now use this information to calculate the energy you will really save by painting your roof white.
On Monday we'll be posting the results from our own experiment. Send us a photo of your experiment to physicscentral@aps.org with your name and a mailing address, and we will mail you something fun for your scientific efforts!
Now, are you going to do with all the money you save from lower electric bills minus the cost of the white paint? Buy Swedish fish, of course.
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Friday, July 31, 2009
Fermi Problem Friday: How much energy do you save by having a white roof?
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Thursday, July 30, 2009
Add Steven Chu on facebook
Chu must be our most popular and recognizable Secretaries of Energy yet. I mean, can anyone even name a former secretary off the top of their heads? Maybe it's because Chu radiates that ineffable rock star aura known as Geek. He's smart, he bicycles, and he's the first Secretary of Energy who's actually a scientist. And not just your test-tube-shuffling, garden-variety boffin; Chu has a Nobel Prize. (And he's still publishing.)

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Wednesday, July 29, 2009
Your comments on jerks and traffic jams

Yesterday's post generated a lot of great conversation, so I thought I'd respond to some of the interesting points brought up in the comments section. First, are platoons (chains of several cars that are traveling close together) really that bad?
Anonymous said...Strangely enough, Dr. Appert-Rolland told me that the specific expressway she was looking at rarely had accidents, though that wasn't the focus of her study. With such long platoons, it seems like rear-end collisions would happen pretty frequently, so maybe there's something to the above comment. I'd be interested to know why accidents don't happen more frequently here. When I asked her what drivers should do about this platoon effect , she mentioned not only obeying the three-second rule, but trying to look ahead if you can, as the comment above suggests. So perhaps you can fine-tune how closely you follow based on how far ahead you can see, meaning the writer of the comment below should probably stay away from bigger cars:
The thing about these "platoons" is that when you're driving that close you're not just watching the car in front of you but the car in front of him. You actually end up monitoring a couple of cars ahead. So if you see something happening to the car 2,3 or 4 cars ahead you start easying off and you have more time to brake when the mud really hits the fan.
That's another issue. I can't see a damn thing from my Ford Focus when any SUV is ahead of me. I end up depending on the SUV driver's reaction time and style, which is, generally speaking, horrid.Obviously the three-second rule is a rough way to keep your distance larger than your reaction time. (One commenter brought up that reaction times are actually less than one second. Anyone have any evidence for that?) But sometimes even that rule needs to be broken, bringing us back to the first paper the article mentions:
the three-second rule means that most people would never be able to enter the highway. If you attempted to merge, you would break everyone else's three second rule behind you and everyone would have to slow down to let you merge. So you can't say "never" because your highway would be at capacity in no time at all.
Yahktoe said...A comment after my own heart: I often wonder whether the proverbial spherical cow eats grass and moos. So here's a bit more detail on the rules of this model world. So we've got our pedestrian-only street, divided into a grid. Each pedestrian is randomly assigned to move either up or down the street, with each square representing a possible move. You try to move forward if you can, but if there's someone in that square, you can move sideways. If you're a good, rule-abiding citizen, you always try to go right first. If that square's occupied too, then you can go left. But if you're a jerk, you're behavior isn't so rigid. You toss a coin to decide whether to go left or right first. You've got more freedom.
For anybody interested in reading Petter Minnhagen's paper (or at least an abstract of it), you can find it here:
Flow improvement caused by agents who ignore traffic rules
I think it's worth noting how stylized the pedestrian rules are in this study. I haven't sprung for the full paper, but I find myself wondering if maybe the rules themselves could have been changed in such a way as to make rule abiding the optimal "solution."
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Tuesday, July 28, 2009
Jerks actually reduce the risk of traffic jams
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Monday, July 27, 2009
Physicists at TED Global Conference

The hallowed halls of Oxford University have been echoing with even more good ideas than usual lately. Last week the venerable institution hosted the 2009 TED Global Conference. A sort of variety show for the mind, the conference featured talks by innovators, thinkers, musicians, artists, architects, scientists, and even British Prime Minister Gordon Brown (warning before you click: his talk is about pretty tough stuff, and includes photos from war zones in the first few minutes.)
If you haven't heard of TED, go right to the website. There you can find videos of talks by anyone from famed primatologist Jane Goodall to engaging string theorist Brian Greene, and former UN director Louise Fresco to aspiring millennium man Ray Kurzweil. The brainchild of WIRED editor-in-chief Chris Anderson, TED stands for Technology, Entertainment, and Design. It's like a mini-YouTube for the most daring, unusual, thought-provoking ideas (and thinkers) out there. Think of it like the Harvard classics, except fast paced—each talk lasts less than twenty minutes—and in living color, often with props and not-your-average PowerPoints.

The theremin-player moves his hands near two antennas. The proximity of the right hand to the vertical antenna changes the electromagnetic field thus changing the pitch of the sound over a six-octave range. Left hand controls the volume.
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Labels: Steven Cowley, TED, TED Global Conference 2009, theramin, William Kamkwamba
Friday, July 24, 2009
Fermi Problem Friday
We recently celebrated the 40th anniversary of the Apollo 11 moon landing, we're airing a special edition of Fermi Problem Friday in honor of Buzz, Neil, and Mike (you know, Michael Collins, the guy who drew the short straw and had to stay in lunar orbit).
Here is the problem:
It took the Apollo 11 crew four days to reach the moon, blasting off from the Kennedy Space Center on July 16, 1969 and arriving at the moon on July 20. What planet would they be closest to today, about 40 years later, if they'd decided to skip the moon and head out into the solar system?
Extra credit: How many Swedish Fish would it take to form a ring around Saturn that the astronauts could see as they flew by, if they made it that far?
Share the problem with friends, try it out on your blind date tonight, and remember, all you need is your common sense, intuition, and a vague idea of how fast our intrepid crew was traveling.
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Thursday, July 23, 2009
Electricity From Salty Water

Extracting clean, fresh water from salty water requires energy. The reverse process—mixing fresh water and salty water—releases energy. Physicists began exploring the idea of extracting energy from mixing fresh and salty waters, a process known as salination, in the 1970s. They found that the energy released by the world’s freshwater rivers as they flowed into salty oceans was comparable to "each river in the world ending at its mouth in a waterfall 225 meters [739 feet] high," according to a 1974 research paper in the journal Science. But those who have chased the salination dream have collided with technological barriers.
Brogioli has developed a new approach to salination, a prototype cell that relies on two chunks of activated carbon, a porous carbon commonly used for water and air filtration. Once he jump starts the cell with electric power, all that is required to produce electricity are sources of fresh and salty water and a pump to keep the water flowing. When the separate streams of salty and fresh water mix, energy is released.
A typical cell would require about three dollars worth of activated carbon, and, given a steady flow of water, the cell could produce enough electricity to meet the needs of a small house. It's the equivalent, in hydroelectric power, of running your appliances from a personal 100 meter (338 feet) high waterfall.
Salination would be an ideal technique for places where fresh and salty waters naturally mix, such as estuaries, according to Brogioli. He said that a coastal community of about a hundred houses could set up a plant with minimal damage to the ecosystem. "A salinity difference plant will be much smaller than a solar plant," he said. The only waste product is slightly brackish water that can be poured directly into the sea or, Brogioli suggested, into ponds that support estuary-friendly flora and fauna.
Instead of using fresh water, an increasingly scarce global resource, a salinity power plant could use water that is polluted or slightly contaminated with salt, giving new life to unusable water, Brogioli said. Seawater could also be mixed with high-salinity water, obtained by evaporating seawater—perfect for a desert community with little fresh water but sunshine to spare.
"Preliminary evaluations confirm that the setup can be scaled up to very big plants suitable for powering whole cities," said Brogioli.
Scientists agree that Brogioli's concept is sound but are cautious to declare it practical on a large scale.
"I don't see any reason why it should not work," said Yury Gogotsi, director of the A.J. Drexel Nanotechnology Institute at Drexel University in Philadelphia. "Capacitor desalination has been demonstrated and commercialized, and this can be called reverse capacitance desalination. It appears to be a logical approach. Of course the challenge is the practical implementation."
George Crabtree, a senior scientist at Argonne National Laboratory in Illinois, said he likes that the device extracts the energy as immediately usable electricity. But he sees difficulties in scaling up from a lab experiment to megawatt plants that could compete with wind turbines or other clean energy sources. Crabtree thinks the water requirements might limit the technology to large river deltas, like the mouth of the Mississippi. The energy it could potentially generate, he said, "is significant ... [but] not enough to solve everyone's problems."
Fred Schlachter, a retired staff scientist at Lawrence Berkeley National Lab in California, is more skeptical. Brogioli’s experiment, says Schlachter, “only demonstrates that it works in concept on [a small] scale." He points out that salt water is very corrosive, which is one reason that renewable energy ideas for harnessing ocean tides rarely get off the ground. "Realistically I've never seen anything involving the ocean work," he said.
Brogioli maintains that his salinity cell could be ramped up faster than other salination approaches and could be made as affordable as solar power in a decade or so. He argues that any new renewable energy source is worth looking into, even if it is only a partial solution to our energy and environmental problems.
"There is no really clean energy source, and none of them can replace fossil fuels alone," he said. "So, it's a matter of compromise: find the best resource for a given region and use many different resources together."
A paper describing Brogioli’s research is due to be published in an upcoming issue of the journal Physical Review Letters.
Brogioli's laboratory cell, which squeezes out a mere 5 microjoules per cycle (better materials, he said, would get a payoff of 1.6 KJ per liter of fresh water) has to operate below 1 volt. Anything higher would cause redox reactions on the electrodes, allowing the salt ions to trade electrons with the carbon, and suddenly your dielectric is a watery conductor. Robert Norman, the author of the original Science article on saline-based energy devices, said he thinks this is a major hangup. Real river water and seawater, he said, might have an even lower tipping point.
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Wednesday, July 22, 2009
Space fever!

July is the month for space nuts. We're in the midst of a wonderful hullaballoo surrounding the 40th anniversary of Apollo 11, giving the younger generation a taste of the original excitement. The Guardian, the New York Times, and almost every other major newspaper is providing tons of Apollo 11 anniversary coverage, although my favorite piece of media so far is a stunning collection of high-resolution photos from the mission, thanks to the Boston Globe's amazing photo essay collection, The Big Picture. There's something timeless about these gigantic photos; one of my favorites is the close-up shot of Neil Armstrong from an earlier mission, where he had to pilot Gemini VIII through the atmosphere and dock it to a vehicle in orbit. He looks wonderfully lost in thought, almost melancholy; my romantic brain thinks it's the expression only a man who's seen earth from space could wear.
JAXA patches for the Kibo installation missions. The third shows the outboard porch.
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Tuesday, July 21, 2009
NASA followers gather for tweetup


With the Smithsonian (@ReliveApollo11) tweeting the 40th anniversary of the Apollo11 mission and current space shuttle mission commander Mark Polansky (@Astro_127) tweeting the crew's work on the International Space Station, no space nut these days can operate without a twitter account. Today NASA took the experiment one step further and held a tweetup. Part of the growing twitter lexicon this term refers to a real-life meetup for tweople (people on twitter, I'm led to believe). Usually this means a dozen or so people in a bar, but in the case of NASA followers, which broke 100,000 today, the auditorium at NASA headquarters did the trick today. A lucky 150 or so people flew in from as far away as Arizona, Vancouver, and even (wow!) Spain, crowded in, turned on their iPhones and laptops, and were treated to a good two hours with the crew of the STS-125 shuttle mission to make repairs to rejuvenate the Hubble space telescope.
We've come a long way since the first TV transmission from space, just 40 years ago yesterday; the entire STS-125 mission was webcast on NASA TV. Viewers watched on tenterhooks as the astronauts, equipped with cameras on their helmets, removed tiny screws from the telescope's housing and replaced batteries the size of a baby grand piano. And during it all, astronaut Mike Massimino was tweeting. The public loved it; Massimino, or @Astro_Mike as he's known on twitter, has 692,564 followers and counting. His tweets were 140-character haikus from earth orbit—funny, thoughtful, and quietly profound:Night pass over Australia, the city lights give stunning signs of life on our planet within the darkness of nighttime
Hard to sleep last night after my spacewalk, images of the work and the views still vivid in my mind.
Eating chocolates in space, floating then in front of me then floating and eating them like I am a fish.

When the seven astronauts walked on stage in their identical blue polos, one woman shouted, "We love you, Mike!" The astronauts talked about the grueling back-to-back spacewalks they underwent to complete the repairs and how they felt when the mission was delayed in October. They played clips from the mission video and gave a sort of live "director's commentary" on scenes such as a tour of the shuttle toilet and the extra days they spent in microgravity waiting "doing astronaut tricks," as mission specialist Megan McArthur put it, while waiting for permission to head home. And they fielded questions about everything from how stars look without the atmosphere in the way (brighter, more colorful, and not twinkling, apparently) to what the crew members were like in middle school.
All in all, the astronauts were "very, very down to earth, warm, friendly, and really funny," said Kathleen Forden, a technology project manager at the University of Phoenix who'd flown in with a co-worker for the event. ("I'm an uber-geek," she explained.) "They seem like they could be their own comedy club based on a space theme."
"The experience of watching everybody tweeting and interacting with each other is also interesting, getting to see what everybody thought was cool rather just than what I thought was cool," said Schwortz, who teaches physics and astronomy at a community college in Massachusetts. She added that she'll be using twitter in the fall with her online and face-to-face classes for discussions, questions, and to facilitate study groups. She said she's part of a growing number of teachers who are using social networking tools to add an extra dimension to learning.
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Monday, July 20, 2009
Where were you when we landed on the moon?

I think I'll always regret not being alive during the moon landing, forty years ago today. If the Beatles form Exhibit A in the case for me being born in the wrong decade, Apollo 11 is exhibit B. I can't remember it, so what I remember is my dad describing the moon landing as a near-psychedelic experience, forever bound to the bad classic rock song he happened to be listening to at the same time. Figures. It was 1969, and he was 21 years old, living in his parents' basement in Queens, which was lined with those slender, acid-yellow paperbacks that formed the Old and New Testaments of his childhood: Heinlein, Kornbluth, Verne, Asimov.
Armstrong: "we could not see any stars out the window" but "I'm looking at the Earth. It's big and bright and beautiful."
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Friday, July 17, 2009
Crazy (in a good way)
Laurie and Brad are two of this summer's Society of Physics Students interns, a group of motivated, physics-lovin' college students who spend nine weeks every summer working on projects ranging from from locating ice under the Martian soil to developing fun hands-on science curriculum. The interns worked at NASA Goddard Space Flight Center, the University of Maryland's Materials Research Science and Engineering Center, the American Institute of Physics, and the American Physical Society. Laurie and Brad worked at the National Institutes of Standards and Technology laboratory in Gaithersburg, Maryland, exploring bendable electronics and spray-on solar cells.

"The kind of crazy it takes to be in science," Laurie explained.
"From the very first night when we went out to eat, we were talking about quantum and Schrödinger's cat," Brad recalls, laughing. "You won't get that anywhere else."
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Thursday, July 16, 2009
'Invisible' Building Design Could Reduce Earthquake Damage

Engineers have been developing earthquake-resistant buildings for years, but a group of physicists now believe it's possible to make an entire building effectively disappear from an earthquake's destructive path, avoiding serious damage. Inspired by the recent development of novel materials that precisely control the flow of light waves around objects, they've shown that the same ideas can work whether the waves make up light, sound or earthquakes.
Earthquakes are some of the most destructive forces in nature. The waves they produce ripple across the earth's surface, much as water waves travel across the ocean. The waves from earthquakes crumple buildings, bridges, and other structures, causing millions of dollars in damage and often death. Despite efforts to understand earthquakes and reinforce buildings against them, damage from the shaking ground is nearly impossible to avoid. But that may not be the case for long, say a team of physicists in France and the United Kingdom.
Recently, physicists have been developing better and better invisibility cloaks, which hide an object from sight by causing incoming light waves to bend around the object, and come together behind the object. Physicists Mohamed Farhat and Stefan Enoch of the Fresnel Institute in Marseille, France, and Sebastien Guenneau of Liverpool University in England wondered if they could use the same principles to hide an object from the destructive waves produced during an earthquake. In a paper to be published this week in the journal Physical Review Letters, the three physicists show that the answer may be "yes."
Guenneau said that it's possible to shield an object, even a building, so that an incoming earthquake wave behaves as if the object weren't there. The building in the path of the wave is like a rock in a fast-flowing river, he said.
"It's the same picture, the wave pattern, as for a water wave that is propagating in a river, and it's bent smoothly around the rock and will be reconstructed around the rock." The object, or building, is "invisible" to the mechanical waves.
A series of concrete rings would surround a building or other structure, forming the shield. The shield would redirect the vibration around the object inside. "Each ring is going to wobble in such a way that the wave will bend around (the object)," Guenneau said.
Earthquake waves come in varying lengths, with many peaks and troughs in a given distance, or just a few. To effectively shield a building from short and long waves that earthquakes generate, several rings could be built around a structure, each "tuned" to a different wavelength.
A 1,000 square foot house, for example, would need a circular shield with a 33-foot radius, which could be built with commercially available concrete. Guenneau suggested that the method might be used to protect a large building like a stadium, where people could seek shelter after an earthquake and be protected by the rings from possible aftershocks.
Guenneau warned that there are some limits to what the cloak can accomplish. He and his colleagues could not find a way to shield a structure from the types of earthquake waves that travel below the earth’s surface. He noted that surface waves are typically the most destructive in an earthquake.
Jim Beck, an earthquake engineering expert at the California Institute of Technology in Pasadena, wondered if the ring would be worth building if it couldn't protect a structure from different types of shaking, not just different wavelengths. The cloak might only work perfectly in special circumstances, he said.
"It sounds like an interesting idea, but I think there's a long way to go before they get to what they would like to see done," he said.
Guenneau said he hopes that others will take the idea and explore its promising applications. Last year, Guenneau and his colleagues made headlines by building a prototype tsunami invisibility cloak that uses ring-shaped channels to redirect water waves around an object. Now they're probing that idea further in a large-scale experiment.
The reality of making buildings seem invisible to the destructive forces of nature, be they the waves from earthquakes or tsunamis, "seems a bit crazy, but it's not science fiction," Guenneau said. "We gave the people the concept, now people can try to improve it to make it more tractable."
By Lauren Schenkman
for Inside Science News Service
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Wednesday, July 15, 2009
"Sixty Symbols"
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Tuesday, July 14, 2009
USA! USA! USA!

Ok, I got that out of my system, but the IPHO, being held this year in Merida Mexico, really is an incredible event. Each year over 65 teams representing countries from around the world vie for the gold. Instead of incredible feats of strength the participants must perform incredible feats of intellect. Through three physics problems and a lab held over the course of eight days from July 12th to the 19th, the teams will duke it out to see who goes home with the gold!
I had the privilege of meeting some of the team members and coaches in May when they were training at the University of Maryland. I was really blown away when I met them; I have never seen a big group of kids who got such a big kick out of science and discovery.
"It's really fun. It's really exciting. You're challenged a lot more than you would be in high school," said Anand Natarajan, who was selected to travel to Mexico.
Getting to the finals was no easy task for the team members. About four thousand students took the first round "F=MA" exam. From there two more tests followed, each getting tougher as they go. I've looked through some of old exams and the actual IPHO questions and they are not simple matters by any stretch.

What struck me most about the team when I visited was even though many of them had only met each other a few days earlier, how close a bond they all seemed to have. Not only were they a team, but they all really seemed like a big group of friends. When everyone ate lunch together they were relaxed and joked around like they had known each other for years and did this every day.
"They can be who they are without being self conscious about being the only kid in the room who likes physics," said Paul Stanley, their head coach.
Even though there were only five who would travel to Mexico and nineteen kids hoping to go, there was no rivalry between them for the coveted slots. Everyone was there doing what they loved to do, physics.
“I never felt that the camp was about fostering competition over the five traveling team spots,” said Marianna Mao who is currently down in Mexico, “Physics is our idea of a good time.”

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Monday, July 13, 2009
Manhattan's grid is a modern-day Stonehenge
{creator and copyright holderManicMaurice, image available on Flickr}

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Friday, July 10, 2009
The numbers are in: people like science
...while almost all of the scientists surveyed accept that human beings evolved by natural processes and that human activity, chiefly the burning of fossil fuels, is causing global warming, general public is far less sure.
Almost a third of ordinary Americans say human beings have existed in their current form since the beginning of time, a view held by only 2 percent of the scientists. Only about half of the public agrees that people are behind climate change, and 11 percent does not believe there is any warming at all.
Rather than merely complaining about the sorry state of scientific literacy, scientists should value the communicators in their ranks - such as the late astronomer Carl Sagan, who was as comfortable in front of a camera as he was in a lab.
One notes that bylines tend to belong to science writers. Science writers can hope to cover science itself with a semblance of objective dispassion. But they have an inbuilt conflict of interest when the topic is the standing and penetration of science as a way to reach conclusions.
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Thursday, July 09, 2009
Putting old particle physics experiments out to pasture
Somewhere in the quintessentially Californian golden hills above Stanford University, a giant physics experiment is quietly rotting. "In" is the operative word here; the behemoth sits in a three-story-deep, concrete-lined hole in the ground, sheltered in a warehouse-sized structure in one of the more deserted reaches of SLAC National Accelerator Laboratory's sprawling campus. Cars and trucks still park in the lot outside, bearing scientists, construction workers, and engineers to the lab's current big project, accessible via two entrances nearby. But this particular piece of physics junk is closed for business.
A hulking steel beast seemingly overgrown with wires, this detector, known as Mark II, was once a microscope that could peer into the most fundamental building blocks of our universe. And it's only a small piece of the much larger experiment that made it happen. Although you can't see them, the two halves of a 2.2-km circular tunnel come together here. If you could turn the clock back about twenty-five years, electrons and positrons would be flying toward the Mark II from either side of the dank tunnel, coming together in a shower of exotic particles and radiation. The intricate family of detectors within Mark II watched and listened, sending data via its millions of wires to physicists who would then meticulously comb through the piles of numbers for some new clue to the universe's puzzle—the lifetime of the tau lepton? The whisper of "I'm here" from a passing selectron?
I was reminded of the Mark II moldering spectacularly in its grave when I saw today's Wired Science photo essay about the death of another old and much-beloved big physics experiment in the Bay Area, Berkeley Lab's once-futuristic Bevatron. It reminded me of how much SLAC, Berkeley, CERN and other labs are massive, physical palimpsests, continuously reinventing themselves. Although perhaps most famous as the proving ground of an incredibly audacious plan to build a two-mile-long accelerator in the early sixties, SLAC's been home to a venerable family tree of acronymic experiments, each building on the infrastructure (tunnels, buildings, technology) and innovations of the previous generation.
Mark-II enjoyed 13 years of use, though it wasn't always here in this underground lair. It started life in the Stanford Positron Electron Accelerating Ring, or SPEAR, in the heart of SLAC's campus, before it was moved* out to the suburbs. SPEAR hasn't just sat there either. It's now a synchrotron, a factory for high-intensity X-rays. It's a hive of activity where a constantly changing cast of biologists, chemists, earth scientists, physicists, and even archaeologists probe the unseen in their fields. And while SLAC's linear accelerator is no longer a powerhouse of particle physics, its new incarnation as an X-ray free-electron laser (or "Giant Laser," as I like to call it, though it's official moniker is the Linac Coherent Light Source), soon to be capable of molecular movies, shows SLAC scientists are still as daring and ambitious as they were in '61.

*"I mean MOVED, seriously," says Brad Plummer, who for the last three years has written about, snapped photos of, and filmed just about every corner of SLAC. "That's a big, delicate piece of hardware to be moving around. The trailer they put it on had 180 wheels." Thanks, Brad for these gorgeous photos of the Mark II and the hilariously retro control room for the SLAC Large Detector. For more of Brad's stuff, including technolust-inspiring snaps of the Giant Laser, er, LCLS, check out his website.
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