Mini-golfing our way through the cosmos

August 11, 2009 | 3:51 pm

We rocketed up and out of the tunnel and into the open air; my fellow traveler and I sailed above Queens, watching as Manhattan grew smaller in the distance. As the train launched us further into the outer limits, we noticed the vast expanse of space above us. Landing at our final destination, we begin our adventure in the cosmos.

Our long ride took us to Flushing Meadows, Queens and home of the New York Hall of Science, built in 1964 as part of the World’s Fair.

Rocket Golf. Photo courtesy of NYHOS.

Rocket Park Mini Golf. Photo courtesy of NYHOS.

The place was thriving when we arrived–crawling with kids and adults, and full of stuff to play with and climb on. My companion–who is not a science nerd–unpaid and giving up a Saturday, would serve as my litmus test for the Hall’s true entertainment value. We were there for their newest attraction: Rocket Park Mini Golf.

The course sits next to the Hall’s Rocket Park, which displays two breathtaking replicas of the Mercury and Gemini space capsules, plus actual Atlas and Titan II rocket boosters. These majestic structures alone got “wows” from Unpaid Companion and made my own heart skip a beat.

We were the only two people without kids dangling off us, and probably the only people taking careful note of the physics placards placed beside all nine holes of the course. The design of the course models a rocket launch–taking golfers on a journey from takeoff, through orbit, to reentry. Some of the holes actually proved too challenging for the six-year-old girls in front of us, but kept the two of us entertained. Around the fifth hole, Unpaid Companion turned to me and said, “I’m actually having a lot of fun right now!”

As for the physics, here are the nine holes we played:

1.       Launch Window. Putt yourself into orbit when the moon and other planets are aligned in such a way as to maximize your use of fuel and time. Getting the ball through a little hole that opens for only three seconds at a time stumped the two adults in front of us.

2.       Escape Velocity. To get away from Earth’s gravitational pull, hit your rocket with just enough force. Too much and it’ll shoot into space (and a booming voice over a speaker will announce “Mission Failure!”). Putt it too lightly and it’ll fall back down to Earth. A successful launch yields a blast-off sound effect.

3.       Zero Gravity. Putt a loop-the-loop around Earth with just enough force and you’ll demonstrate how a rocket orbiting around the Earth is still falling, but is going fast enough that it falls around the Earth instead of into it.

Earth's Orbit; Photo Courtesy of NYHOS

Earth's Orbit. Courtesy of NYHOS.

4.       Earth’s Orbit. Choose the best path to orbit around Earth. The right path leads your ball to a large funnel where your rocket goes around and around. At this point in the course, Unpaid Companion and I are tied.

5.       Space Docking. Join up with a space station in space; this is another hole emphasizing that timing is everything. Putt carefully into the orbiting rocket ships, but don’t miss and shoot off into space! Unpaid Companion flies off into an asteroid and I pull ahead.

6.       Space Junk. More than a million pieces of space junk, left over from previous missions and satellites, still orbit the Earth at 20,000 miles per hour. The sign reads, “At that speed, a screwdriver could put a hole in your ship.” Unpaid Companion takes a shameful number of strokes to get through the junk.

7.       Gravity Whip. Whip around Mars to get to Jupiter. This is one of the holes with really expert construction. With enough of a push straight down the green, the ball takes a curved path all the way around Mars, and is slung back in the other direction. It provided a nice demonstration of the concept, and once again tested the determination of the girls in front of us.

8.       Re-entry Angle. Another well-crafted hole that rewards subtlety over strength. Give your rocket enough oomph to get up a slight incline, but just enough that it falls back down to the Earth.

9.       Splash Down. Time to come back to Earth, where a rescue boat is waiting for you.

At the end of the day, the space junk hole sealed unpaid companion’s fate and I won the game. But we did leave feeling like we’d sailed through the cosmos.

The New York Times ran an article on the golf course, in which the writer did far more preparation than I and brought along two children and an astrophysicist. He concludes that the course did teach the kids a little about physics, and wonders what other kinds of science could be taught through mini golf.

Calla Cofield

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Starving baby black holes?

August 10, 2009 | 11:52 am

A simulation shows a black hole, white, interacting with gas, blue, about 200 million years after the big bang. Image courtesy of Marcelo Alvarez, John H. Wise and Tom Abel.

A black hole, in white, interacts with gas, in blue, about 200 million years after the big bang. Click image to see simulation, both courtesy of Marcelo Alvarez, John H. Wise and Tom Abel.

In the infant universe there were no stars.  Less than a billion years later, stars not only existed, but some had also collapsed into supermassive black holes, with a million to a billion times the mass of our sun.

Astrophysicists have long assumed that the first black holes quickly put on weight as they gobbled up surrounding gas.  But supercomputer simulations at the Kavli Institute for Particle Astrophysics and Cosmology suggest otherwise.

From a press release in SLAC Today

In the simulation, clouds of gas left over from the Big Bang slowly coalesced under the force of gravity, and eventually formed the first stars. These massive, hot stars burned bright for a short time, emitting so much energy in the form of starlight that they pushed nearby gas clouds far away. Yet these stars could not sustain such a fiery existence for long, and they soon exhausted their internal fuel. This caused one of the stars in the simulation to collapse under its own weight, forming a black hole located in a pocket of emptiness. With very little matter in the near vicinity, this black hole was essentially “starved” of food on which to grow.

“Quasars [extremely strong sources of radiation] powered by black holes a billion times more massive than our sun have been observed in the early universe, and we have to explain how these behemoths could have grown so big so fast,” said [Marcelo] Alvarez. “Their origin remains among the most fundamental unanswered questions in astrophysics.”

One explanation for the existence of supermassive black holes in the early universe postulates that the first black holes were “seeds” that grew into much larger black holes by gravitationally attracting and then swallowing matter. But in their simulation, Alvarez, Abel and Wise found that such growth was negligible, with the black hole in the simulation growing by less than one percent of its original mass over the course of a hundred million years.

Glennda Chui

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Muons at the science fair

August 7, 2009 | 9:33 am

Katrina Korman was only 15 years old when she started working with physicist Alec Habig on a science fair project.  She knew almost nothing about particle physics and computer programming when she began. Yet she dared to take on the challenge of analyzing the steady stream of muons that bombards Earth.

Katrina Korman

Katrina Korman

Korman isn’t a physics whiz kid, says Habig. Google her name and you’ll find more references to her pitching abilities than anything else. During her high school years, the Minnesota native filled her spare time with softball, tennis, volleyball, and hockey, two musical instruments, and activities with the National Honors Society.

When Korman entered her sophomore year, she was already a regular at the yearly science fair.  Twice she had presented the results of her experiments on how life in outer space might affect the growth of soybean plants. “At the time I think I wanted to work for NASA,” she says. “That was my dream job.”

Craving another project dealing with the cosmos, she asked her teacher Cynthia Welsh for a suggestion; Welsh set up a meeting with Habig, the director of graduate studies at the University of Minnesota Physics Department.

Habig, who regularly conducts outreach activities with nearby high schools, does research with a handful of physics experiments, including the Main Injector Neutrino Oscillation Search.  The MINOS experiment uses two giant particle detectors, one located at Fermi National Accelerator Laboratory in Illinois and the other at the Soudan mine in northern Minnesota, to study neutrinos.

The MINOS detector at Soudan is buried more than a half mile underground, where rock shields it from cosmic rays that hit Earth continuously. Nevertheless, some high-energy muons still manage to reach the detector, where they create significant static in the MINOS neutrino data.

But does the stream of muons vary over the course of a year?

Data gathered by many other particle physics experiments had hinted at seasonal fluctuations in the rate at which cosmic muons strike the Earth. Few scientists, however, had done a complete analysis to prove the existence of the effect or examined the fluctuations quantitatively.

This was the first time one of Habig’s science-fair students would approach a real-life particle physics problem, providing results that he and his colleagues could use. Habig felt that the analysis of MINOS data would offer the right skill level for a high school student like Korman. Because he was fairly certain the analysis would have a positive result, he thought it would also prove fun and rewarding.

Starting from square one, Korman spent most of her summer learning how to write computer code while Habig taught her particle physics. He and her high school teacher offered support and assistance as Korman wrote a computer program to sift through MINOS data to look for seasonal muon fluctuations.

For Korman, this science fair project was a big departure from growing plants and watching their progress over weeks.

“With the soybeans you grow the plants and you take the measurements yourself and you put them in the graphs. With [the MINOS] project it’s less hands-on,” she says. “You feel like you’re not getting anywhere until you see the results and then you’re like, ‘Oh! That’s neat!’”

Habig says Korman’s greatest strength was simply her determination to finish the project.

“The thing that made it work very well was [Katrina] was very motivated and diligent and willing to sit down and learn apparently irrelevant stuff like programming and statistics,” Habig says. “She’s different from many physics majors who come in thinking a lot of stuff is really neat, and they are really surprised that it’s a lot of work. So as a result, physics programs lose maybe half of declared majors. She wasn’t necessarily a big fan of physics, but there was a project that was interesting and she wanted to do it and was willing to sit down and do the work to get it done.”

The MINOS particle detector, located a half mile underground in the Soudan Underground Laboratory in Minnesota, weighs 6000 tons.

The MINOS particle detector, located a half mile underground in the Soudan Underground Laboratory in Minnesota, weighs 6000 tons.

The project gave Korman a close-up look at what particle physicists are doing. Habig took Korman on a tour of the MINOS detector at Soudan, and she and her father watched the launch of a weather balloon carrying instruments to measure atmospheric conditions to associate with the MINOS data on muons. These were the project’s biggest highlights, she says.

Korman took her project to the regional science fair that fall and moved on to the state competition that spring. She’d successfully shown that there is indeed a fluctuation in the muon rate as the seasons change and the atmospheric conditions change.

After that year’s science fair, the project was over for Korman. But her analysis became the basis for a Ph.D. thesis by Eric Grashorn, a graduate student working under Habig. He took Korman’s work and went deeper, finding a way to calculate the quantitative fluctuations in muon showers during the year. To honor the work she’d done to get the ball rolling, the scientists included Korman as a coauthor on the paper.  (For more on this work and its significance, see “Cosmic Weather Gauges” in the March 09 issue of symmetry.)

Habig says he’ll definitely consider doing a similar project with another student in the future. In the meantime, his work with Korman will provide a valuable example in his upcoming outreach efforts.

“When I’m talking to classes of undergraduates or high school students I try to put in a slide with pictures of students like them who have done work with neutrinos or cosmic rays in the past. And that makes [the new students] feel like this stuff is not off on another planet,” Habig says. “Giving them some tangible evidence that other students like them have understood this stuff in the past makes them want to try harder to understand it.”

And, as Habig points out, the project still achieved the ultimate goal of increasing one student’s scientific literacy.

“Even if Katrina has nothing to do with science for the rest of her life, 20 years from now she’ll pick up a newspaper and read a science story and she’ll have a framework for it,” Habig says.

Now, as Katrina prepares for her freshman year of college, she still isn’t sure if science is the path she’ll take. Even if she doesn’t follow in Habig’s footsteps and become a physicist, she thinks the experience taught her a great deal about her own abilities and where her interests lie. As part of her resume, the MINOS project even may have helped Katrina get into a good school.  This fall she’ll attend the University of St. Thomas in St. Paul, Minnesota.

“The funny thing is, I’ve done all these science projects and I still just feel like I’m in over my head,” says Korman. Would she recommend a science project such as this one to other high school students?  “Yes and no,” she says. “You obviously have to know what you’re getting into. You have to be prepared to feel like you don’t know what’s going on. But I think it would be good for kids to learn.”

Calla Cofield

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New round of stimulus funds includes $327M for DOE science

August 4, 2009 | 5:31 pm

From today’s US Department of Energy press release:

Of the $327 million in Recovery Act funding announced today, $107.5 million is slated to go to universities, nonprofit organizations, and private firms, generally on a competitive, peer-reviewed basis. The remaining $220 million will go to U.S. Department of Energy National Laboratories for a range of research, instrumentation, and infrastructure projects, including $164.7 million for projects already allocated as follows:

Fermi National Accelerator Laboratory; Batavia, IL$60.2 million, including $52.7 million for research on next-generation particle accelerator technologies; and $7.5 for neutrino research in collaboration with Brookhaven National Laboratory.

Lawrence Berkeley National Laboratory; Berkeley, CA$ 37.8 million, including $13.1 million to upgrade equipment at the DOE Joint Genome Institute; $11 million for fusion energy research; $8.8 million for equipment improvements at the Advanced Light Source; $4 million for new instrumentation at the DOE Joint BioEnergy Institute, one of three DOE Bioenergy Research Centers; and $875,000 for mathematical analysis related to the development of Smart Grid technology.

SLAC National Accelerator Laboratory; Stanford, CA$21.8 million, including $20 million for an experimental end station at the Linac Coherent Light Source to study high energy density plasmas; and $1.8 million for improvements at the Stanford Synchrotron Radiation Lightsource.

Princeton Plasma Physics Laboratory; Princeton, NJ$13.8 million, including $8.8 million for a variety of initiatives in fusion energy research and $5 million for infrastructure improvements at the laboratory.

Brookhaven National Laboratory; Upton, NY$9.5 million, including $3 million for improvements at the National Synchrotron Light Source; and $6.5 million for neutrino research.

Oak Ridge National Laboratory; Oak Ridge, TN$8.7 million, including $5.4 million for equipment at the DOE BioEnergy Science Center, a DOE Bioenergy Research Center; $3.2 million to seed development of computerized knowledgebase to integrate masses of data flowing from DOE-supported genomics and systems biology research; and $180,000 for fusion energy research.

Pacific Northwest National Laboratory; Richland, WA$5.7 million, including $4.9 million for integrated assessment modeling for climate; and $867,000 for mathematical analysis related to the development of Smart Grid.

Argonne National Laboratory; Argonne, IL$5.6 million for improvements at the Advanced Photon Source.

Lawrence Livermore National Laboratory; Livermore, CA$810,000 for fusion energy research.

Sandia National Laboratories; Sandia, NM, and Sandia, CA$800,000, including $688,000 for mathematical analysis related to the development of Smart Grid; and $75,000 for fusion energy research.

In March Secretary Chu announced $1.2 billion in DOE Office of Science Recovery Act projects. In July, DOE announced a new Office of Science Early Career Research Program to be funded with $85 million in Recovery Act funds. With this third and final round of projects, the Obama Administration has now approved projects covering the full $1.6 billion that the DOE Office of Science received from Congress under the Recovery Act.

 We’ll bring you details as they become available.   In the meantime, here’s some background on how the first round of stimulus funding is being put to work at SLAC, Fermilab, Lawrence Berkeley lab, Argonne, and Brookhaven.

Glennda Chui

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Happy birthday to charm!

August 3, 2009 | 3:35 pm

 

Shawne Workman reports in SLAC Today:

Today, charm turns 45. Sheldon Glashow and James Bjorken coined the term “charm” for a theoretical new particle, the charm quark, in a paper published in Physical Review Physics Letters on August 1, 1964. The paper is available full-text, online [subscription required for full text] from SPIRES-HEP database: Elementary Particles and SU(4)

 

Thanks to SLAC archivist Jean Deken for passing along along this gem.

 

So what’s the perfect gift for a middle-aged yet still mysteriously alluring particle?  A charm plushie comes to mind:

 

 

 

 

 

As for allure, check out “Chasing Charm in China” from the May 2009 issue of symmetry, which describes how the quest to understand charm quarks and related particles has lured American scientists to the newly upgraded Beijing Electron Positron Collider.

 

Glennda Chui

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Sir Isaac Newton bags a counterfeiter

August 3, 2009 | 5:00 am

Now here’s a bit of physics-related lore I didn’t know: After leaving Cambridge, Sir Isaac Newton was appointed Warden of the English Mint, where he got involved in some very nasty business.

From a review of Newton and the Counterfeiter: The Unknown Detective Career of the World’s Greatest Scientist, on TheScientist.com:

The greatest mind of the 17th (or arguably any) century found himself in a position to use his superior mental powers to study and rectify the problems of England’s Mint. Once he’d improved the manufacture of the King’s coin by adding eight new rolling mills and five new coin presses to the Mint, his attention turned to the country’s counterfeiters. This is when Newton morphed into a master sleuth, building a network of spies and informers in London’s underworld, never hesitating to wade into unsavory, dangerous territory. His mania for detail helped him in matching wits with one of the most inventive criminals of the age, one William Chaloner.

Reviewer Margaret Guthrie writes that author Thomas Levenson’s pace and timing

…rival those of the best crime story authors. He has written a real page-turner, perfect for a long afternoon’s engagement with the hammock or whiling away a long airport layover.

Apparently Newton left detailed records of the case he built against Chaloner; the author also had the benefit of a 17th-century biography of the master criminal.  So now we can indulge in a bit of true-crime reading while nobly boning up on the history of physics — sort of.

Glennda Chui

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LHC Update: July 31, 2009

July 31, 2009 | 9:54 am

This week’s issue of the CERN Bulletin reports on the suspected cause of two vacuum leaks discovered in mid-July that have pushed the LHC restart date until at least November. The likely culprit is a flexible hose in the liquid helium transport circuits. The same type of hose caused a vacuum leak in another LHC sector two years ago, which was fixed by replacing the flexible hose with a smaller, solid tube. If the flexible hose is confirmed as the cause of the new leaks, it will be repaired using the same technique.

In other LHC repair news, Science magazine reports today that more bad connections between superconducting magnets may reduce the maximum energy for the LHC’s first run, or further delay the restart.

Katie Yurkewicz

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In the works: a movie starring subatomic particles and two Star Trek captains

July 31, 2009 | 5:00 am

Dave the Photon Courtesy of Jupiter 9 Productions.

Dave the Photon (Image from the Jupiter 9 Productions Web site.)

TrekMovie.com has posted an interesting review of a new movie that highlights the study of space and touches on particle physics in a unique and fun way.

Quantum Quest: A Cassini Space Odyssey blends education and entertainment though the use of 3D computer-generated animation and footage from seven NASA space missions, including the Cassini Huygens mission to Saturn.

Audience members will get a tour of the outer planets and moons of our solar system while meeting the movie’s cast of characters, which includes a photon, neutrino, proton and an evil genius, The Void, who represents “nothingness” and seems to have traits similar to dark matter and dark energy.  A number of celebrities lend their voices to characters, including former Star Trek captain William Shatner as The Core, a figure that represents the sun and knowledge, and, arguably, all visible matter.

From a press release:

The full voice cast includes Chris Pine (Captain Kirk in J.J. Abrams’
upcoming “Star Trek XI” feature film), Samuel L. Jackson (”The Spirit,”
“Pulp Fiction,” “Star Wars”), Hayden Christensen (”Jumper,” “Star Wars”),
Amanda Peet (”X-Files Movie 2,” “The Whole Nine Yards”), Robert Picardo
(”Stargate Atlantis”), Jason Alexander (”Seinfeld”), Tom Kenny (voice of
“Sponge Bob Squarepants,” “Transformers”), Sandra Oh (”Sideways,” “Grey’s
Anatomy”), Brent Spiner (”Independence Day,” “Star Trek: Next
Generation”), James Earl Jones (”Star Wars”), William Shatner (”Boston
Legal,” “Star Trek”), Mark Hamill (”Star Wars”), Neil Armstrong, Doug
Jones (”Pan’s Labyrinth,” “Abe Sabien – Hell Boy”), Abigail Breslin
(”Little Miss Sunshine,” “Kit Kittredge: An American Girl”), Spencer
Breslin (”The Happening”), Gary Graham (”Alien Nation,” “Enterprise”),
and Janina Gavankar (”The L Word”).

The movie features the voices of two Captain Kirks (veteran William
Shatner and Chris Pine, star of JJ Abrams’ upcoming “Star Trek” movie)
and two Darth Vaders (James Earl Jones and Hayden Christensen) — a first
for Hollywood and a first for the galaxy.

The movie is expected to appear in theaters worldwide sometime in 2010 in IMAX and conventional 3D format. It is the brainchild of Jupiter 9 Productions producer Harry Kloor, who has Ph.D.s in physics and chemistry and has written for the Star Trek franchise.

The movie was initiated by NASA’s Jet Propulsion Laboratory as part of the outreach program for the Cassini Huygens space mission in 1996.  About once a week for the nine months leading up to the film’s release, its creators will post video clips and supplemental educational material on the film’s Web site.

The main Web site has limited movie clips available so far, but computer-generated images posted with the TrekMovie.com story look amazing. It doesn’t look anything like your typical education-based film, and the story definitely seems worth a read.

Tona Kunz

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Tiny droplets carry proteins, viruses into the paths of bright x-ray imagers

July 30, 2009 | 5:00 am

John Spence, a physicist at Arizona State University, is a longtime user of the Advanced Light Source at Lawrence Berkeley National Laboratory, where he has contributed to major advances in lensless imaging. It’s a particularly apt propensity for someone who works with x-rays, since they can’t be focused with ordinary lenses.

As new light sources evolve to produce brighter x-rays in faster pulses, lensless imaging becomes ever more critical for science. Among the promises of superbright, ultrafast x-ray pulses is the ability to solve the structure of the complicated molecules from which our bodies are made. All living things are made of proteins and nucleic acids, but relatively few of the atomic structures of the thousands, perhaps millions, of varieties of proteins are known.

The Linac Coherent Light Source (LCLS) will soon begin operation at the SLAC National Accelerator Laboratory in Menlo Park, California, using energetic electrons from a linear accelerator to produce coherent x-rays with an instrument called a free electron laser (FEL). The x-rays will be delivered 120 times a second in pulses only a tenth of a trillionth of a second long – about the time it takes light to travel the width of a human hair. These brief, bright pulses offer a novel approach to the problem of protein structure.

Unfolding the origami

Proteins begin as strings of amino acids that fold themselves into an amazing variety of origami-like structures, whose bumps and crannies and distribution of electrical charges determine how they act individually or fit together to form complex molecular machines. Simple organisms like viruses often consist of a few proteins fitted together to enclose a thread of DNA or RNA.

Proteins are usually large molecules containing many thousands of atoms. Drug molecules are much smaller, and do their work by attaching themselves to the larger protein molecules. A knowledge of the arrangement of a protein’s atoms is therefore a great help to drug designers, who like to understand how a drug molecule will dock with a protein to promote or inhibit its activity, or cripple the organism of which it is a part.

Until now, the best way to solve the structure of a protein or virus has been with x ray crystallography. The crystal consists of many copies of the protein or virus arranged in regular order. As the crystal rotates in the x-ray beam, x-rays scatter off the atoms and reveal – once these complex diffraction patterns have been converted into a 3-D image by computers – how the electrons, and thus the atoms, are arranged.

But many proteins can’t be crystallized at all, and others are so difficult to crystallize it’s virtually impossible to obtain crystals large enough to use in today’s light sources.

Ultrafast, ultrabright x-rays offer a way past this dilemma. The idea is that a quick pulse of tightly focused x-rays can be diffracted from a microcrystal or even a single protein or virus in solution. The pulse is so brief that it comes and goes before any of the atoms can move, freezing their orientation like a strobe light. Just as important, a sufficiently brief pulse may terminate before radiation damage effects can start. In this way it can outrun radiation damage, always one of the fundamental limitations to imaging in biology.

Another quick pulse could be diffracted from another copy of the protein in a different orientation. As the process is repeated, diffractions from different angles give the overlapping views needed for the computer to construct a 3-D image of the structure.

It’s a great idea, but as Spence notes, there are a few problems. “So as not to scatter, the x-ray beam has to be in a high vacuum, but a protein or virus in its natural state is usually wet. As in T. S. Eliot’s Wasteland, water is life. How do we maintain the protein or virus in an aqueous environment inside the vacuum?”

Shot from a microcannon

The answer was what Spence calls a “particle gun, like an ink-jet printer,” designed to inject a beam of water droplets across the tightly focused x-ray beam in single file, each droplet so small it contains only a single protein or virus. He and colleagues Bruce Doak and Uwe Weierstall of ASU designed a nozzle that can fire liquid droplets, each less than a millionth of a meter in diameter (one micrometer), faster than hundreds of thousands of times a second. The sample jet is designed to shoot droplets right through a pulsed beam of x-rays a billion times brighter than any ever created in a light source before.

It wasn’t easy. Nozzles made of solid material like glass invariably clog up, limiting droplets to at best 20 micrometers across. What Spence and his colleagues wanted was a jet of particles less than a micrometer in size. ASU postdoc Dan DePonte has done most of the recent hard work needed to make it all function.

The frequency at which droplets emerge is controlled by an acoustic trigger, which can be tuned so that each droplet containing a protein or virus meets an incoming pulse of x rays.

The frequency at which droplets emerge is controlled by an acoustic trigger, which can be tuned so that each droplet containing a protein or virus meets an incoming pulse of x-rays.

Back in 1878 Lord Rayleigh, a professor of experimental physics at Cambridge University, discovered that a smooth, cylindrical jet of liquid emerging from an orifice spontaneously breaks up to form a train of spherical droplets. In the late 1990s, physicist Alfonso Gañán-Calvo of the University of Seville found a way to surround the streaming liquid with pressurized gas to make a co-flowing liquid sheath. By adjusting gas and liquid pressure and other parameters, he was able to create a “virtual nozzle” that could shrink the diameter of the liquid jet to a thread so small it would not clog the physical aperture of the tube. In effect, the gas sheath acts to focus the liquid stream.

Spence and his colleagues needed a true microthread of liquid, however, one that produced droplets sized a millionth of a meter or less. In their nozzle, liquid flows through a narrow capillary inside the tube through which the gas flows; the liquid issues from the capillary some distance from the opening in the outer tube, so the gas surrounds it, then increases speed and pressure as it approaches the opening, squeezing and accelerating the thin stream of liquid until it is so small that the proteins or viruses dissolved in the liquid can only fit into the droplets one at a time.

And the nozzle won’t clog, because even a particle bigger than the sample protein or virus – bigger than the stream of liquid itself – can still fly through the glass nozzle without hitting the walls and getting stuck.

The frequency at which the droplets emerge can be controlled by an oscillator the researchers call an “acoustic trigger.” Tuning the acoustic trigger adjusts the frequency so that each droplet containing a protein or virus meets an incoming pulse of x-rays.

The entire device – which the researchers call a gas dynamic virtual nozzle (GDVN) – is only about a millimeter in diameter (not counting feed lines and cables) and fits to the side of the beamline’s vacuum chamber. After passing through the beam, the liquid droplets and the gas (typically carbon dioxide) freeze in a trap opposite the injection point, without significantly reducing the vacuum.

The liquid flows through a narrow capillary, issuing some distance from the opening in the outer tube through which the gas flows. Approaching the narrow opening, gas pressure and speed increase, focusing the thin stream of liquid until it is so small only a single protein or virus can fit into each droplet.

The liquid flows through a capillary, issuing some distance from the opening in the outer tube through which the gas flows. Approaching the narrow opening, gas pressure and speed increase, focusing the thin stream of liquid until it is so small only a single protein or virus can fit into each droplet.

In 2008 Spence and his colleagues, including Berkeley Lab’s David Shapiro, successfully tested the GDVN on the Advanced Light Source beamline 9.0.1, managed by Berkeley Lab’s Stefano Marchesini. The test was done with protein microcrystals extracted from the fluid in which researchers were attempting to grow larger crystals. These are the smallest protein nanocrystals from which diffraction patterns have ever been obtained, and the first from membrane protein nanocrystals – among the most resistant to crystallization.

Although the microcrystals weren’t individual protein specimens, and while the 9.0.1’s x-ray beams aren’t as bright or as rapidly pulsed as SLAC’s LCLS will be, the experiment demonstrated the jet technique’s high potential for speeds and exposures that won’t subject the samples to radiation damage. Some of the patterns the researchers obtained come from nanocrystals just a few molecules on a side, with a width of about 100 billionths of a meter (100 nanometers). At SLAC, the researchers plan to steadily reduce the nanocrystal size down to single molecules.

The corresponding reduction in scattered intensity will hasten and improve lensless imaging. The first step in lensless imaging is scattering the beam from the sample; the second step is constructing the image by interpreting and combining the data from the diffracted x-rays.

In order to merge the different views (projections) of an object, which is subsequently vaporized in this “diffract-and-destroy” mode, it is important that they all be identical. In biology, that leaves only molecules like proteins and viruses. DNA or RNA inside a virus is often packed differently in each virus, and cells are not identical at the molecular level, so cannot be studied in 3-D by this method.

Besides identical particles, successful data-merging also depends partly on knowing how the sample was oriented in the beam – easy to do with a large crystal, not so easy to do with a sample inside a drop of liquid whizzing across the beam. It may be possible to orient flying droplets by optical methods such as polarized laser beams or with specially shaped nozzles.

Perhaps simpler is to use the ever-increasing power of the computer – which for a lensless imaging system is where most of the functions of a lens reside. Computer systems have been developed that infer the orientation of the sample from the diffraction pattern itself, even when as few as four percent of the pixels in the detector light up. It does take a lot of diffraction patterns to derive an image this way – as many as 10 million – which will take the LCLS a few hours until better ways of orienting the droplets can be devised.

Nevertheless, Spence’s group recently obtained excellent diffraction patterns of MS2 virus capsids at the ALS by subtracting the diffraction “noise” of the liquid jet itself. These capsids, made in Mat Francis’s lab at the University of California at Berkeley, are the shells of the virus lacking its RNA genome and have the regular shape of buckyballs. Eventually the LCLS will be able to get a good diffraction pattern from a target like this with a single ultrabright pulse. In this case, however, computer processing was able to derive an excellent pattern by averaging diffraction from a series of samples.

DePonte will soon install Spence and Doak’s ultrafine, ultrafast “inkjet printer,” tested at the ALS, on the powerful new SLAC machine. It will be the first step into a bold new future for investigating the biological universe, one big molecule at a time.

Additional information

X-ray imaging beyond the limits,” by Henry N. Chapman, appeared in Nature Materials, April, 2009.

Powder diffraction from a continuous microjet of submicrometer protein crystals,” by D. A. Shapiro, H. N. Chapman, D. DePonte, R. B. Doak, P. Fromme, G. Hembree, M. Hunter, S. Marchesini, K. Schmidt, J. Spence, D. Starodub, and U. Weierstall, appeared in the Journal of Synchrotron Radiation, November, 2008.

Gas dynamic virtual nozzle for generation of microscopic droplet streams,” by D. P. DePonte, U. Weierstall, K. Schmidt, J. Warner, D. Starodub, J. C. H. Spence, and R. B. Doak, appeared in the Journal of Physics D: Applied Physics, 19 September, 2008.

By Paul Preuss

This article first appeared on July 28, 2009 on the Berkeley Lab News Center.

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The CERN Courier's 50th anniversary issue

July 29, 2009 | 5:00 am

Issue one of the Cern Courier

Issue one of the CERN Courier

For those who enjoy a nostalgic look back, the CERN Courier has posted a treat:  The very first issue of the Courier, which started as an in-house newsletter and now reaches 25,000 subscribers around the world.

Writing in the July/August issue, CERN Director-General Rolf Heuer notes that both the European lab and the Courier have changed beyond recognition since the first issue came out 50 years ago:

One thing that has stayed the same, however, is the magazine’s openness to the world. Issue number 1 reported not only on progress towards starting up the PS [Proton Synchrotron], but also carried news of the City of Hamburg’s purchase of a 40 MeV linac for a new lab known as the Deutsches Elektronen Synchrotron. Back then, the Courier felt the need to spell out the DESY acronym. There was also news from the US, including bold ambitions for linear accelerator developments at Stanford University. CERN’s mission of bringing nations together for peaceful collaboration is witnessed by a report from a trip to the USSR, precursor to a long and fruitful collaboration with the Joint Institute for Nuclear Research at Dubna.

The anniversary issue highlights five decades of science from the Courier archives, from the 1959 announcement of the first beam in the Proton Synchrotron (news so fresh that the issue had to be made over at the last minute to fit it in) to accelerator milestones, particle discoveries, Nobel Prizes, the invention of the World Wide Web and the startup of the Large Hadron Collider. 

As someone who loves browsing through old postcards and magazines — and who owns a 55-year-old issue of Life magazine from the month I was born — I have to say I love this stuff:  The typefaces, then so modern and now so charmingly retro; the pastel pages; the thought of how much harder it was back then to put out a publication like this one; and the language of a dynamic, yet more genteel time, as in this request for suggestions from page 8 of issue one:

You don’t have to sign them. If you believe you might blush in seeing your name in print in our next issue, or if modesty prevents you from being further associated with your idea, then just drop us a note “incognito.”  You may be sure your appeal will always receive due consideration, even if it is not so tender to us.  Editors are — and should be — rugged people…

That, at least, has not changed!

We wish the Courier  a very happy anniversary and many exciting reports ahead.

Glennda Chui

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