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    Volume lXXI I I , Number 4, FAll 2010

    N ThIs Issue:

    Volcanoes and Earthquakes Zombies and Celebrities

    Aggression and Fruit Flies

    California Inst i tute of Technology

    http://www.caltech.edu/http://www.caltech.edu/
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    Engineering & Scienceis printed on recycled paper contain

    minimum of 10 percent postconsumer waste. The papers v

    pulp comes from trees grown in the U.S. in accordance wit

    Forest Stewardship Councils sustainability standards.

    Tedx CalTeChJan uary 14, 2011

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    http://tedxcaltech.com/http://dmse.mit.edu/faculty/faculty/belcher/https://researcher.ibm.com/researcher/view.php?person=almaden-eiglerhttps://researcher.ibm.com/researcher/view.php?person=almaden-eiglerhttp://www.ericjhellergallery.com/http://marcuslab.harvard.edu/http://www.jazzreview.com/articledetails.cfm?ID=655http://www.youtube.com/watch?v=TVyyhHFKI8Ehttp://www.bias-inc.com/about/artistProfiles/bRice.phphttp://susskindsblogphysicsforeveryone.blogspot.com/http://susskindsblogphysicsforeveryone.blogspot.com/http://www.sdss.jhu.edu/~szalay/http://www.sykes.easynet.co.uk/http://www.jcvi.org/cms/about/bios/jcventer/http://www.jcvi.org/cms/about/bios/jcventer/http://theory.caltech.edu/~preskill/http://theory.caltech.edu/~preskill/http://www.its.caltech.edu/~kip/http://www.ted.com/speakers/rives.htmlhttp://tedxcaltech.com/http://tedxcaltech.com/http://www.ted.com/speakers/rives.htmlhttp://www.its.caltech.edu/~kip/http://theory.caltech.edu/~preskill/http://www.jcvi.org/cms/about/bios/jcventer/http://www.jcvi.org/cms/about/bios/jcventer/http://www.sykes.easynet.co.uk/http://www.sdss.jhu.edu/~szalay/http://susskindsblogphysicsforeveryone.blogspot.com/http://susskindsblogphysicsforeveryone.blogspot.com/http://www.bias-inc.com/about/artistProfiles/bRice.phphttp://www.youtube.com/watch?v=TVyyhHFKI8Ehttp://www.jazzreview.com/articledetails.cfm?ID=655http://marcuslab.harvard.edu/http://www.ericjhellergallery.com/https://researcher.ibm.com/researcher/view.php?person=almaden-eiglerhttps://researcher.ibm.com/researcher/view.php?person=almaden-eiglerhttp://dmse.mit.edu/faculty/faculty/belcher/http://tedxcaltech.com/
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    ngineering & Science (ISSN 0013-7812) is published quarterly at the California Institute of Technology, 1200 East

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    eproduction of material contained herein forbidden without authorization. 2010, California Institute of Technology.

    ublished by Caltech and the Alumni Association. Telephone: 626-395-3630.

    VoluMe lXXI I I , nuMBer 4, Fall 2010

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    http://eands.caltech.edu/http://eands.caltech.edu/
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    ENGINEERING & SCIENCE fall 20102

    In a marriage o brute orce and milli-

    metric precision, a vital communica-

    tions link in the Deep Space Network

    has just undergone a major repair. The

    giant Mars dishso named because

    its rst job, in 1966, was to track

    Mariner 4 ater its fyby o the redplanethas relayed commands to,

    and data rom, every earthly emissary

    to have ventured beyond the moon.

    As the most sensitive antenna avail-

    able, it was also crucial in bringing the

    Apollo 13 astronauts home. But 44

    years o operationmore than double

    its projected 20-year liespanhave

    taken a toll on the bearings that allow

    it to aim its radio beam precisely at a

    spacecrat the size o a VW Beetle

    more than 10 billion kilometers away.

    Ocially known as Deep Space

    Station 14, the 70-meter antenna sits

    in a shallow valley at JPLs Goldstone

    complex deep in the Mojave des-

    ert between Los Angeles and Las

    Vegas, where it is shielded rom as

    many o humanitys interering radiosignals as possible. The dish and its

    substructure, including the two-story

    corrugated steel building that houses

    the drive motors and some o the

    signal-processing equipment, weighs

    about 3,000 metric tonsmore than a

    herd o 500 elephants.

    The entire assembly, as tall as a

    20-story building, rests on three steel

    support pads. These pads are part o

    the hydrostatic bearing on which the

    antenna rotates, and they glide on

    a quarter-millimeter lm o oil atop a

    24-meter-diameter steel ring called

    the runner. The runner, in turn, sits on

    a 10-meter-tall pedestal. Tiny trickles

    o oil would seep through the runners

    joints and drip o its edges, deterio-

    rating the cement-based grout below.As the grout sotened, the runner

    would develop waves, so a team o

    our technicians would spend eight

    to 10 hours a week inserting shims

    under the runner to keep it level.

    Work began in March to replace

    the runner, the grout, and the eleva-

    tion bearings that allow the dish to

    tilt rom the zenith to the horizon. The

    elevation bearings were done rsta

    sort o warm-up job, as this merely

    involved liting 1,800 tons o dish o

    its mounting. Next, the crew usedthe same hydraulic jacks to raise the

    entire 3,000-ton colossus ve milli-

    metersenough clearance to ease

    out the old components and install

    a thicker runner with tighter joints on

    new oil-resistant, epoxy-based grout.

    As it talks to ar-fung spacecrat,

    the Mars dish also measures the

    distance to them, providing vital data

    to the navigation teams. Changing the

    dishs height by more than a ew milli-

    meters would void these calculations.The new runner is seven inches thick

    to the old runners ve, so, in one nal

    engineering challenge, the hydrostatic

    bearing pads had to be removed and

    machined down to compensate.

    The project, two years in the

    planning, had a set-in-cement

    deadline: the dish had to be back on

    line by early November, in time or

    JPLs rendezvous with comet Hartley

    2. They made it. MW/DS

    random walk

    operation: mars antenna

    http://deepspace.jpl.nasa.gov/dsn/http://deepspace.jpl.nasa.gov/dsn/features/goldstonetours.htmlhttp://deepspace.jpl.nasa.gov/dsn/features/goldstonetours.htmlhttp://deepspace.jpl.nasa.gov/dsn/features/goldstonetours.htmlhttp://deepspace.jpl.nasa.gov/dsn/features/goldstonetours.htmlhttp://deepspace.jpl.nasa.gov/dsn/
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    fall 2010 ENGINEERING & SCIENCE

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    http://www.nasa.gov/mission_pages/epoxi/index.htmlhttp://www.nasa.gov/mission_pages/epoxi/index.html
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    ENGINEERING & SCIENCE fall 20104

    Having a Blast

    In 2007, soon ater landing at Naha

    Airport on the island o Okinawa in

    Japan, a Boeing 737 started spewing

    uel rom a puncture in its right-wing

    tank. As the uel fowed onto the hot

    engine, it ignited, causing several ex-plosions as fames enguled the plane.

    Fortunately, everyone evacuated in

    time and no one was hurt.

    O course, planes, trains, and

    automobiles dont generally burst

    into huge reballs whenever theyre

    near a heat source, whether it be a

    spark or a lit cigarettedespite what

    Hollywood might lead you to believe.

    But clearly, exploding uel is a hazard,

    and understanding how it ignites al-

    lows engineers to develop the proper

    saety regulations to minimize danger.Postdoc Sally Bane (PhD 10),

    working with Joe Shepherd (PhD 81),

    Johnson Proessor o Aeronautics and

    proessor o mechanical engineering,

    is analyzing how a spark can ignite

    fammable gas. Shes discovered that

    these spark-ignited explosions are a

    lot more complicated than previously

    thought, and her results bring much-

    needed updates to saety standards

    that are decades oldand, in some

    cases, based on data that are fat-outwrong.

    For decades, engineers have

    determined the likelihood o a spark-

    ignited explosion in an aircrat by

    using a number called the minimum

    ignition energy (MIE). Each type o

    uel or vapor has its own MIE value,

    and i a sparks energy is below that

    value, then nothing should ignite. The

    problem, however, is that the MIE is

    based on data rom old experiments,

    some rom more than 60 years ago.

    Even though the numbers have been

    updated over the years, no one has

    ever gone back and reevaluated the

    original experiments in depth. The

    original data rom the 1940s are still

    cited today, Bane says.

    As an expert in explosions, Shep-

    herd was recruited in 1996 by the

    National Transportation Saety Boardto help gure out why TWA Flight

    800 crashed into the Atlantic just 12

    minutes ater takeo rom New Yorks

    JFK Airport (see Learning rom a

    Tragedy, E&SNo. 2, 1998). During

    the investigation, some o Shepherds

    experiments showed unoreseen vari-

    ability in spark-ignited explosions

    even with a spark below the MIE, the

    uel sometimes still blew up. However,

    he didnt get a chance to explore the

    issue urther until Bane came to his

    lab as a graduate student in 2005.According to Bane, perorming

    this kind o experiment is dicult and

    time-consuming, and since there

    hadnt been any obvious reason to

    doubt the old MIE data, people were

    content with the existing inormation.

    It took her ve years to design, build,

    and run her experiments, which are

    among the most rigorous ever done.

    Her explosions range rom harmless

    pus to tiny reballs, saely contained

    in a solid-steel vessel weighing 200kilograms. Inside the vessel are two

    pointy tungsten electrodes, separated

    by a couple o millimeters. Charge

    builds up in the electrodes, generat-

    ing a voltage dierence that ionizes

    the gas between them. The ionized

    gas creates a path or electrons to

    travel rom one electrode to the other,

    and in just a ew nanoseconds, you

    get a spark. The spark energies that

    Bane works with are relatively low

    as low as 50 microjoules. You would

    need a million o these sparks to light

    a 50-watt lightbulb or a second.

    A high-speed camera, which can

    take up to several hundred thousand

    rames per second, records the spark

    and any resulting explosion. Bane

    repeated the experiment or dierent

    spark energies and with various mix-

    tures o fammable gases as suggest-ed by the Aerospace Recommended

    Practices, standards developed by

    the Society o Automobile Engineers

    that guide the design and production

    o aircrat parts. The mixtures con-

    tained 5, 6, or 7 percent hydrogen,

    oxygen, and argon.

    Unlike tests that are common in the

    industry, Banes are done in a sealed

    vessel, which means that she knows

    the gass composition, temperature,

    and pressure with a high degree o

    certainty. Furthermore, Bane says, inother setups, theres no camera that

    directly observes the ignition. Instead,

    the only way to tell that theres been

    an explosion is to watch whether a

    piece o oil, which is across an open-

    ing in the vessel, pops upor, i the

    blast is violent enough, bursts open.

    Bane discovered that there isnt a

    single MIE value or a given famma-

    ble mixture; theres no single energy

    that sets the threshold or whether

    an explosion is possible. Instead,she ound, whether or not a certain

    spark ignites the gas is an exercise

    in probabilities, rising and alling with

    the energy o the spark. To be sure, at

    some point, the energy is too low and

    an explosion is impossible. But its

    not as cut and dried as people had

    thought.

    In the case o the 7 percent

    hydrogen mixture, Banes results

    were roughly comparable to the

    http://www.galcit.caltech.edu/~jeshep/http://eands.caltech.edu/articles/Shepherd%20Feature.pdfhttp://eands.caltech.edu/articles/Shepherd%20Feature.pdfhttp://eands.caltech.edu/articles/Shepherd%20Feature.pdfhttp://eands.caltech.edu/articles/Shepherd%20Feature.pdfhttp://eands.caltech.edu/articles/Shepherd%20Feature.pdfhttp://eands.caltech.edu/articles/Shepherd%20Feature.pdfhttp://www.galcit.caltech.edu/~jeshep/
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    fall 2010 ENGINEERING & SCIENCE

    Fr lf: t frm of fr nulfd Bon

    737 wn lkn ful w nd by o nn.

    Forunly, no on w ur.

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    kn 5, 50, 100, 175, nd 250 mcrocond.

    experiments done by Bernard

    Lewis and Guenther von Elbe in the

    1940s, which gave an MIE o 100

    microjoules. She ound that at 100

    microjoules, the gas had a 10 percent

    chance o igniting. But or the 5 per-

    cent hydrogen mixture, the MIE given

    was 200 microjoules, while Bane

    determined that the spark had to be

    at least 780 microjoules beore it evenhad a 10 percent chance o blowing

    up. It turned out that Lewis and von

    Elbe hadnt actually had data or a 5

    percent hydrogen mixture back in the

    1940sthey had just extrapolated

    the MIE rom data or the 7 percent

    gas.

    This variability is likely an inherent

    characteristic o spark ignition, Bane

    says. Even when she kept the condi-

    tions as constant as possible, the

    explosions were never consistent. The

    spark itselthe channel o plasmaconnecting the two electrodesis

    intrinsically irregular, wavering in

    shape and motion. Other complexities

    have been revealed in fuid-dynamic

    simulations that Bane and graduate

    student Jack Ziegler have run o the

    ignition process.

    Bane and Shepherd are now work-

    ing to develop better saety stan-

    dards with Boeing, which unded the

    research. Last summer, she expanded

    her experiments to include kerosene,the type o uel used in most com-

    mercial aircrat. Unlike clean-burning

    hydrogen, kerosene is a dirty uel, so

    ater each trial, Bane dons a protec-

    tive jacket, Kevlar gloves, and goggles

    beore opening the hot vessel to

    swab out the soot and set up the next

    experiment.

    Bane is nding that it doesnt take

    much energy to set o kerosene.

    She was able to ignite kerosene at

    60 degrees Celsius with only 0.65

    microjoules, while in Shepherds

    previous work, it took 40 microjoules

    to ignite the uel at 52 degrees. I

    anticipate that in uture tests Ill be

    able to ignite mixtures with even lower

    energies, she says. The ignition o

    uel vapor is highly sensitive to tem-

    perature change, Bane explains, and

    her experiment used shorter-durationsparksabout a couple hundred

    nanoseconds, which is a more ac-

    curate simulation o an electrostatic

    dischargeso the discrepancy isnt

    a complete surprise. But the act that

    its apparently much easier to ignite

    kerosene than the test mixtures speci-

    ed by the FAA has certainly gotten

    the attention o the olks at Boeing.

    Bane says her data can be applied

    to any situation where theres a tank

    o uel and the possibility o a

    sparkor example, in power plants,in the natural-gas tank that heats your

    house, or when storing hydrogen gas,

    which has garnered interest as a

    clean-burning uel. But as or

    smoldering cigarettes blowing cars to

    kingdom come? That could never

    happen, Bane says. Gasoline needs

    to be extremely hot to ignite, and a

    cigarette just wont cut it. But it sure

    looks cool. MW

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    http://today.caltech.edu/theater/item?story_id=44862http://today.caltech.edu/theater/item?story_id=44862
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    a m of

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    ENGINEERING & SCIENCE fall 20106 ENGINEERING & SCIENCE fall 20106

    on tHe map

    From Neolithic cave painting to

    Google Earth, humans have used

    maps to depict, understand, and navi-

    gate their environment. Now some o

    the Caltech Archives nest treasures

    on the subject o mapping the earth,the skies, and longitude have gone

    on display, many or the rst time,

    on the second foor o Parsons-

    Gates Hall o Administration. The On

    the Map exhibit includes Claudius

    Ptolemys 2nd-century map o the

    known world; Georg Braun and Frans

    Hogenbergs beautiully illustrated

    Civitates Orbis Terrarum, rom the

    latter part o the 16th century; a 1570

    map o Russia by Abraham Ortelius;

    Johannes Bayers 1603 Uranome-tria; Johannes Keplers world map o

    1627; a 17th-century planispheric

    celestial map by Andries van Luchten-

    berg; prints rom Joan Blaeus 1662

    Atlas Maior; and rst editions o

    books by Tycho Brahe, Johannes

    Hevelius, Giovanni Domenico Cassini,

    and Christiaan Huygens.

    Ptolemys map is an early 16th-

    century version reconstituted rom

    his cartography and geography book,

    the Geographia, published in 150

    CE. Ptolemy, a Roman citizen o

    Alexandria, knew that the earth was

    a globethe ancient Greeks had

    worked it out centuries earlierbut

    his view o the world extends only

    rom the zero-degree line o longitude

    o the west coast o Arica (beyond

    which no sailor had returned to tellthe tale) to the 180-degree line

    through China, and rom 60 degrees

    north latitude to 30 degrees south.

    He omitted the three-quarters o

    the globe that was still uncharted, a

    technique that humans still employ

    today when mapping unknown terrain

    such as Saturns moon Titan, currently

    under surveillance by JPLs Cassini

    spacecrat. Cassinis radar views

    a narrow swath o Saturns lunar

    companion with each fyby, and theresulting maps, in which Titans topo-

    graphical eatures are interspersed

    with black regions or which no data

    exists, are in some sense Ptolemys

    intellectual descendantsJPLs car-

    tographers dont ll the empty space

    with creations o their own ancy.

    Cassini will, in all likelihood, map

    Titan more rapidly than humans

    mapped the earth: the Americas,

    ater all, were not discovered by

    Europe until the late 15th century.

    But once the Age o Exploration got

    under way, the exciting accounts o

    new lands brought back by sailors

    sparked a renewed interest in geogra

    phy among prosperous and literate

    Europeans. Printing presses, invented

    a ew decades earlier, ound a lucra-

    tive market in catering to the demandor inormation.

    In 1513, the German cartographer

    Martin Waldseemller, whose large

    map o the world (and the rst map

    to use the name America) had sold

    well a ew years earlier, decided to

    bring out Ptolemys Geographia. For

    centuries the Christian world had

    regarded the ancient geometer as

    a heretic, and the work was hidden

    away and orgotten until its rediscov-

    ery in the 14th century. Waldseeml-ler borrowed a manuscript copy, in

    Greek, rom an Italian monastery. The

    maps were missing, but he reconsti-

    tuted them, including the world map

    in the Caltech display, rom Ptolemys

    extensive topographical lista

    compendium o place names and

    geographical eatures along with their

    latitudes and longitudes. (The list was

    compiled rom travelers reports, and

    many o the longitudes were wrong

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    fall 2010 ENGINEERING & SCIENCE

    Cn md rdr moc of

    surn moon tn. t urfc

    covrd n , nd blu nd blck.

    anyon comrn currn m of Bl w

    1575 vw from Brun nd honbr Civies Orbis

    terrrum(town of World) m nk

    Rn cnd cour ovr yr. Bu w

    rlly cnd our noon m lwy v

    nor o. in 16 cnury, r w no con-

    vnon for m ornon, nd vw from

    nor lookn ou. a com ro o ud vwr

    w lo condrd unmorn.

    fall 2010 ENGINEERING & SCIENCE

    or, at best, very bad guesseswhich

    is why the landorms get increasingly

    distorted the arther one gets rom the

    Mediterranean.)

    In the decades that ollowed, deco-

    rative maps and atlases ound ready

    buyers. Some o the nest were pro-

    duced by the Flemish cartographer

    Abraham Ortelius, who pioneered the

    change rom the woodcut printing omaps to copperplate engraving, with

    italic lettering and rich hand-coloring

    that greatly enhanced the denition

    and beauty o the prints. When his

    Theatrum Orbis Terrarum (Theater o

    the World), the rst true atlas, sold

    well, he encouraged Georg Braun

    and Frans Hogenberg o Cologne to

    produce a companion book o town

    views and history, the Civitates Orbis

    Terrarum (Towns o the World).

    With its rst volume published

    in 1572, Braun and Hogenbergsambitious project took an additional

    45 years to complete, and Caltech is

    ortunate to own our volumes rom

    the six-volume rst edition. Their

    scrupulously detailed town plans

    generally depict buildings and houses

    rom a birds-eye perspective and

    are brought to lie with drawings o

    people in local costume carrying out

    their trades, o animals, and o scenes

    rom history, all accompanied by an

    account in Latin o the towns situa-

    tion, population, history, government,commerce, and traditions.

    Today the armchair traveler has

    morphed into the Google Earther,

    as more and more people turn to

    cyberspace to swoop in on houses

    or the worlds cities. Interestingly,

    Wikipedias city pages provide almost

    the same inormation that Braun and

    Hogenberg did.

    Humans were likely curious about

    the heavens even beore they ex-

    plored the world: ollowing the daily

    course o the sun, moon, stars, andplanets doesnt involve any traveling.

    Early astronomers and geographers

    both used the same surveying instru-

    ments, such as quadrants and astro-

    labes; and both earth and sky maps

    have equators and poles, latitude and

    longitude. (The longitude o a star or

    planet is given by its right ascension,

    while the latitude is given by its dec-

    lination.) For millennia, star tables

    celestial topographical listsplayed

    an indispensible role in predictingimportant events in the calendar such

    as equinoxes, solstices, phases o the

    moon, and eclipses (not to mention

    their use in casting horoscopes!), but

    they were so imprecise that, accord-

    ing to the young Tycho Brahe, There

    are just as many measurements and

    methods as there are astronomers,

    and all o them disagree.

    Accordingly, Tycho (as he is

    commonly known), a Danish noble-

    man, made it his lies work to take

    accurate, systematic observations

    rom a single spot over many years.

    He persuaded King Frederick II oDenmark to give him the small island

    o Hven (modern Ven), in the straits

    between Denmark and Sweden, and

    to build him an observatory there and

    provide him with a generous income

    to und it. Todays astronomers should

    be so ortunate!

    Tycho named his palatial astro-

    nomical research center Uraniborg,

    the Castle o the Heavens. With

    accommodations or up to a hundred

    observers, assistants, and visiting

    scholars, it was not unlike a modernastronomical research center, save or

    the alchemy workshop in the base-

    ment and the utter lack o telescopes

    (Tycho was the last major astronomer

    to survey the skies entirely by naked

    eye.) He later added Stjerneborg,

    the Castle o the Stars, an under-

    ground observatory with a rotating

    dome that sheltered his instruments

    rom the bueting winds that swirled

    around Uraniborgs towers. A series

    o lakes provided waterpower orboth instrument workshops and a mill

    that produced paper or publications.

    Unortunately, ater Fredericks death,

    Tycho argued with his heir and had to

    abandon the island in 1597.

    Uraniborg, Stjerneborg, and the

    lakes can be seen on the map o

    Hven in the Archives displaya

    reproduction o a colored engraving

    by Willem Blaeu rom Joan Blaeus

    Atlas Maior, 1662. The young Willem,

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    a m of tyco

    Br lnd of hvn

    (now Vn) from Jon

    Bluals Miorof

    1662, own ob-

    rvor Urnbor

    nd sjrnbor nd

    lk rovdd

    wrowr.

    a rr nd unuul m of world

    dnd by Klr for 1627 book of

    r bl, tbule Rudolphine.

    ENGINEERING & SCIENCE fall 20108

    Joans ather, had studied astronomy

    and globe-making with Tycho, and he

    went on to run a successul map-

    publishing business in Amsterdam.

    Uraniborg was demolished shortlyater Tychos sudden death in 1601,

    but today we can zoom in on Ven via

    Google Earth and view Uraniborgs

    partially restored gardens, the remains

    o Stjerneborg, and even, aintly, the

    remains o the lakes.

    Tychos assistant, Johannes Kepler,

    who would go on to attain some ame

    in his own right, nished the work by

    preparing a new set o star tables

    based on the Hven observations.

    These he published in 1627 as the

    Tabulae Rudolphinae, or RudolphineTables, in honor o Rudol II o Aus-

    tria, Holy Roman emperor and Tychos

    royal patron at the end o his lie, and

    Keplers patron as

    well. The exhibit

    includes a photo-

    graph o a large

    world map olded

    inside Caltechs

    copy o the Tables.

    The maps unusual

    projection, compris-ing one whole hemi-

    sphere centered on

    Europe and Arica,

    fanked by two hal

    hemispheres, was

    Keplers own

    design. It was

    probably in-

    tended to make

    it easier or navi-

    gators to plot their position by keep-

    ing the most-traveled seaways o the

    Known World contiguous. Keplers

    line o zero longitude is centered on

    Hven. Caltech is ortunate to havethis map, as it is rare: the engraver

    had not nished it when the book was

    published, and ater the astronomers

    death three years later, it lay orgotten

    until rediscovered in 1658.

    Kepler also tackled the problem o

    accurately measuring ones longitude,

    a necessity or any maritime power

    attempting to become a global pres-

    ence. But although his method gave

    useul results on dry land, despite his

    best eorts, it proved impractical on a

    tossing deck. Among those who triedto nd a better way were Giovanni

    Domenico Cassini, Christiaan Huy-

    gens, and Englands rst Astronomer

    Royal, John Flamsteed; books and

    prints refecting their work are also on

    display.

    Nowadays, ships, planes, and even

    cars navigate with the help o

    satellites, and travelers (almost)

    always know exactly where they are.

    Lie is saer and easierbut our

    curiosity about the world around us is

    as strong as ever. BE

    Barbara Ellis is a writer and

    researcher forOn the Map, which is

    curated by Shelley Erwin, head of

    Archives and Special Collections.

    The majority of the books, prints, and

    artifacts on display were collected

    and later donated to Caltech by

    Earnest C. Watson, founder of the

    Watson Lecture Series and professor

    of physics and dean of the faculty at

    Caltech for many years. The Tabulae

    Rudolphinae are from the Rocco Col-lection, purchased by trustee Harry

    Bauer for Caltech in 1955.

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    R: Un Brnbow cnqu,

    n wc nuron r lbld w df-

    frnly colord fluorcn ron,

    rrcr cn m ou nurl crcu

    n zbrf lrv. Bcu lrv

    v rlvly fw nuron nd r

    rnrn, y mk for ood modl

    ornm for udyn nurl nd

    nc ym rul l.

    fall 2010 ENGINEERING & SCIENCE

    WHy do We

    sleep?

    While we can more or less abstain

    rom some basic biological urges

    or ood, drink, and sexwe cant do

    the same or sleep. At some point, no

    matter how much espresso we drink,we just crash. And every animal thats

    been studied, rom the ruit fy to the

    rog, also exhibits some sort o sleep-

    like behavior. (Paul Sternberg, Morgan

    Proessor o Biology, was one o the

    rst to show that even a millimeter-

    long worm called a nematode alls

    into some sort o somnolent state.)

    But why do weand the rest o the

    animal kingdomsleep in the rst

    place?

    We spend so much o our time

    sleeping that it must be doing some-thing important, says David Prober,

    assistant proessor o biology and

    an expert on how genes and neu-

    rons regulate sleep. Yes, we snooze

    in order to rest and recuperate, but

    what that means at the molecular,

    genetic, or even cellular level remains

    a mystery. Saying that we sleep be-

    cause were tired is like saying we eat

    because were hungry, Prober says.

    That doesnt explain why its better to

    eat some oods rather than others andwhat those dierent kinds o oods do

    or us.

    No one knows exactly why we

    slumber, Prober says, but there are

    our main hypotheses. The rst is

    that sleeping allows the body to

    repair cells damaged by metabolic

    byproducts called ree radicals. The

    production o these highly reactive

    substances increases during the day,

    when metabolism is aster. Indeed,

    scientists have ound that the expres-

    sion o genes involved in xing cells

    gets kicked up a notch during sleep.

    This hypothesis is consistent with the

    act that smaller animals, which tend

    to have higher metabolic rates (and

    thereore produce more ree radicals),

    tend to sleep more. For example,

    some mice sleep or 20 hours a day,

    while giraes and elephants only needtwo- to three-hour power naps.

    Another idea is that sleep helps

    replenish uel, which is burned while

    awake. One possible uel is ATP, the

    all-purpose energy-carrying molecule,

    which creates an end product called

    adenosine when burned. So when

    ATP is low, adenosine is high, which

    tells the body that its time to sleep.

    While a postdoc at Harvard, Prober

    helped lead some experiments in

    which zebrash were given drugs that

    prevented adenosine rom latchingonto receptor molecules, causing the

    sh to sleep less. But when given

    drugs with the opposite eect, they

    slept more. He has since expanded

    on these studies at Caltech.

    Sleep might also be a time or your

    brain to do a little housekeeping. As

    you learn and absorb inormation

    throughout the day, youre constantly

    generating new synapses, the junc-

    tions between neurons through which

    brain signals travel. But your skullhas limited space, so bedtime might

    be when superfuous synapses are

    cleaned out.

    And nally, during your daily

    slumber, your brain might be replay-

    ing the events o the day, reinorcing

    memory and learning. Thanos Siapas,

    associate proessor o computation

    and neural systems, is one o several

    scientists who have done experiments

    that suggest this explanation or

    sleep. He and his colleagues looked

    at the brain activity o rats while the

    rodents ran through a maze and then

    again while they slept. The patterns

    were similar, suggesting the rats were

    reliving their day while asleep.

    O course, the real reason or sleep

    could be any combination o these

    our ideas, Prober says. Or perhaps

    only one o these hypotheses mighthave been true in the evolutionary

    past, but as organisms evolved, they

    developed additional uses or sleep.

    Researchers in Probers lab look or

    the genetic and neural systems that

    aect zebrash sleeping patterns by

    tweaking their genes and watching

    them doze o. An overhead camera

    records hundreds o tiny zebrash

    larvae as they swim in an array o

    shallow square dishes. A computer

    automatically determines whether the

    sh are awake or not based onwhether theyre moving or still, and

    whether they respond to various

    stimuli. Prober has identied about

    500 drugs that aect their sleeping

    patterns, and now his lab is searching

    or the relevant genetic pathways. By

    studying the sh, the researchers

    hope to better understand sleep in

    more complex organisms like humans.

    Even i we nd only a ew new

    genes, thatll really open up the eld,

    he says. The uture is promising, headds, and or that, itll be well worth

    staying awake. MW

    http://biology.caltech.edu/Members/Sternberghttp://biology.caltech.edu/Members/Proberhttp://biology.caltech.edu/Members/Proberhttp://biology.caltech.edu/Members/Sternberg
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    ENGINEERING & SCIENCE fall 201010

    tHe mKids are

    alrigHt

    Build CCAT! the decadal survey

    says. Thats the U.S. National

    Research Councils sixth decadal sur-

    vey or astrophysics and astronomy,released in August. These surveys

    predict the greatest scientic oppor-

    tunities and rank proposed research

    projects accordingly. The outlined

    projects oer the best prospects or

    making discoveriesboth anticipated

    and unanticipatedor which the next

    decade will be remembered. CCAT

    a telescope initiated by Caltech, JPL,

    and Cornell that is slated or con-

    struction in the high-altitude Atacama

    Desert in northern Chilewas listed

    as a top priority or its part in thesearch or the rst stars, galaxies, and

    black holes.

    The rst two billion years o the

    universe will open up in the next

    decade, predicts Chuck Steidel (PhD

    90), Caltechs DuBridge Proessor

    o Astronomy. CCAT has a starring

    role: it is the only telescope that can

    survey the dustiest and most luminous

    galaxies in the primordial universe.

    We expect some big surprises.

    Astronomers have wanted a tele-scope like CCAT since the 1980s,

    when the Caltech Submillimeter Ob-

    servatory (CSO) began to reveal dust

    clouds packed with embryonic stars

    in nearby galaxies. These clouds look

    dim or black to optical telescopes, but

    they blaze in the submillimeter- and

    millimeter-wavelength light that the

    CSO and CCAT are designed to see.

    This light alls between radio waves

    on the one side and near-inrared

    and visible light on the other. To see

    well at these wavelengthsjust out

    o the reach o radio and optical

    telescopescompletely new cameras

    and spectrometers had to be devel-

    oped.

    This light may be tough to work

    with, but it holds the key to under-

    standing galaxy ormation. I star-

    orming regions are thick with dust,primeval galaxies may also be hidden

    by the dust and gas o their own

    ormation. CCAT will survey huge

    swaths o sky at great depths, essen-

    tially looking back in time by catching

    photons that have been traveling or

    more than 10 billion years. Its superb

    site and 25-meter dishmore than

    twice as large as the CSOsare big

    actors in its observing power. But the

    real revolution is down in the bowels

    o the telescope.

    It has taken three decades odogged work, alse leads, and lucky

    breaks to develop the technology

    or CCATs wideband spectrometer

    and its large-ormat cameras. E&S

    discussed this journey o a thou-

    sand steps with Jonas Zmuidzinas

    (BS 81)the Kingsley Proessor o

    Physics, Caltechs project scientist

    or CCAT, and a leader in detector

    development.

    So ar, we have gotten just a

    small taste o what there is to learnat submillimeter wavelengths, says

    Zmuidzinas. Studying a submillimeter-

    bright galaxy oten requires three

    telescopes. You need a submillimeter

    telescope to nd the object, a radio

    telescope to pinpoint its location, and

    an optical spectrometer to analyze its

    chemistry and measure its redshit,

    which determines its place on the

    cosmic time-line.

    CCAT will be able to do all o these

    things. Its spectrometer, the next

    generation o an instrument called

    Z-Spec, will have unprecedented

    bandwidth and be able to target

    multiple objects simultaneously. It

    will routinely nd redshits or distant,

    dust-obscured galaxies rich with new

    stars. Its cameras, using microwave

    kinetic inductance detectors (MKIDs)

    are expected to bring the state othe art rom a ew thousand pixels to

    many tens o thousands o pixels and

    beyond. They will capture detailed

    panoramas o the submillimeter sky.

    Caltech and JPL were central to

    development o the new detectors.

    Thats not because o one or two

    peoplequite the opposite. In this

    small community, ideas fy rom under-

    graduates to senior researchers to

    trustees to alumni (dont try to keep

    track o all the characters that ollow!)

    Here, a good idea can generate thenimble collaboration more typical o a

    pro sports teameach player, aware

    o the skills and resources o the oth-

    ers, contributes what he or she can,

    whether its a new method, a better

    production acility, a timely inusion o

    unding, or a novel design.

    SiS openS the Submillimeter

    Our story begins in 1979, when

    Bell Labs Tom Phillipsnow AltairProessor o Physics at Caltechin-

    vented the superconductor-insulator-

    superconductor, or SIS mixer. The

    SIS mixer was crucial to the develop-

    ment o radio-style receivers or the

    submillimeter band, and it is now

    used in nearly all submillimeter- and

    millimeter-wavelength telescopes. It

    made sensitive high-resolution sub-

    millimeter spectroscopy and interer-

    ometry a possibility, says Zmuidzinas.

    t r of colldn lx known

    annn, n by (from

    lf o r) ody vbl, nfrrd,

    nd ubmllmr lco. CCat

    wll du-roudd r-

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    bu w szr l roluon.

    hubbl szr CsO

    http://www.submm.org/http://www.submm.caltech.edu/http://www.submm.caltech.edu/~tgp/http://www.submm.caltech.edu/~tgp/http://www.submm.caltech.edu/http://www.submm.org/
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    fall 2010 ENGINEERING & SCIENCE

    An SIS mixer channels photons to

    a tiny junction made o two layers o

    superconducting metals, each just a

    tenth o a micrometer thick, separated

    by a smear o insulation. Excited by

    the photons, electrons leap across

    the insulator by quantum tunneling,

    generating a measurable current with

    extremely low noise. John Tucker (BS

    66) developed the theory behindthese mixers, predicting that their

    noise levels could be reduced to the

    undamental limits set by quantum

    mechanics.

    Phillips, who had been a visiting as-

    sociate at Caltech, joined the aculty

    that year. Once installed in Caltech

    telescopes, his prototype SIS receiv-

    ers demonstrated antastic potential,

    convincing JPL to dedicate research-

    ers and lab space to the project.

    The CSO also sped aheadits SIS

    receivers caught their rst photonsin 1987. JPL opened its Microde-

    vices Laboratory in 1988, and the

    new acility turned physicists heads

    nationwide.

    One o those physicists was

    Zmuidzinas, then a postdoc in Illinois.

    He was designing ways to orce-eed

    photons to an SIS junction with mini-

    mal losses. He had rened a device

    called a twin-slot mixer, in which two

    antennas collect light and guide it into

    microstrips made with superconduct-ing metals.

    Zmuidzinas returned to Pasadena

    in 1990. Caltech was irresistible.

    The CSO had recently been com-

    pleted. The Microdevices Lab had

    just opened, so there was a beautiul

    acility or doing this work. Today,

    descendents o the twin-slot are used

    in the Herschel Space Observatorys

    spectrometers and in the CSOs

    high-requency instruments.

    SpiderwebS and Sin

    A ew years later, Zmuidzinas

    ocused on the problem o nding

    distant submillimeter-bright galaxies,

    which would require a camera with

    at least a hundred detectorsone

    per pixel. At the time, the workhorse

    detectors were germanium bolom-

    eters. Bolometers, which are used

    in both cameras and spectrometers,absorb incoming photons and convert

    their energy to heat, which an electri-

    cal thermometer then converts to a

    measurable electrical signal. But the

    devices were laboriously assembled

    by hand. Zmuidzinas wanted to solve

    the problem by combining his twin-

    slot antennas with a new bolometer

    based on superconductor-insulator-

    normal (SIN) junctions that had just

    been invented by a UC Berkeley

    student. With this approach, the en-

    tire detector array could be producedby lithographyno hand-assembly

    needed!

    At that time, the late Andrew Lange,

    then a proessor at Berkeley, and his

    student Jamie Bock were developing

    the spiderweb bolometer, a rened

    germanium bolometer in which every-

    thing could be mass-produced except

    the thermometer. The web, less than

    hal the diameter o a dime, was

    photolithographed, gold-coated sili-

    con nitride. The spiderthe thermom-eterwas hand-placed in the middle.

    When the silicon backing material

    was etched away, the spider and web

    hung in ree space, suspended on

    thin guy lines. Lange began a sab-

    batical at Caltech in 1994; when he

    decided to stay, Bock joined JPL as a

    postdoc. JPLs Microdevices Labora-

    tory was just what they needed: They

    had prototyped the device at Berke-

    ley, but they needed good acilities to

    make a go o it, says Zmuidzinas.

    Lange, Bock, and Zmuidzinas

    started down both pathsspider-

    webs and SINbut soon ocused on

    the spiderwebs. They were more o a

    known quantity, and Lange and Bock

    wanted to create a working instru-

    ment quickly or upcoming experi-

    ments. Spiderweb bolometers made

    cameras aster and more accuratethey had more detectors and needed

    ewer photons to produce a measur-

    able signal, and cosmic rays and the

    heat and shaking o nearby equip-

    ment aected them less. The 1998

    BOOMERanG experiment, co-led by

    Lange, used them to provide the rst

    experimental evidence that the uni-

    verse is fat and that the infationary

    theory is correct (see An Ultrasound

    Portrait o the Embryonic Universe, in

    E&S2000, No. 3). Similar bolometers

    are fying on the Herschel and Planckobservatories326 on Herschel and

    52 on Planck. They were also used in

    a 144-pixel camera installed on the

    CSO in 2002.

    the miSSing redShiftS

    In 1998, a UK team at the James

    Clerk Maxwell Telescopelocated

    on the summit o Hawaiis Mauna

    Kea, just a ew hundred yards rom

    the CSOannounced that they hadound distant submillimeter-bright

    galaxies. They had used hand-assem-

    bled, thread-suspended, pre-spider-

    web bolometers. It was a brute-

    orce, inelegant solution, but they got

    there rst, Zmuidzinas says.

    The galaxies proved to be very aint

    and dicult to study at other wave-

    lengths. In particular, their redshits

    usually measured with optical spec-

    troscopyremained largely unknown.

    Jon Zmudz-

    n (Bs 81),

    Knly prof-

    or of pyc

    nd Clc

    rojc cn

    for CCat.

    http://microdevices.jpl.nasa.gov/http://microdevices.jpl.nasa.gov/http://calteches.library.caltech.edu/712/2/Ultrasound.pdfhttp://calteches.library.caltech.edu/712/2/Ultrasound.pdfhttp://calteches.library.caltech.edu/712/2/Ultrasound.pdfhttp://calteches.library.caltech.edu/712/2/Ultrasound.pdfhttp://microdevices.jpl.nasa.gov/http://microdevices.jpl.nasa.gov/
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    ENGINEERING & SCIENCE fall 201012

    Lf: a drwb bolomr on dm.

    R: tnum nrd Mcrowv Knc

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    Zmuidzinas started to think about how

    to make a submillimeter spectrometer

    with enough bandwidth to measure

    redshits or distant galaxies.

    In an optical spectrometer, a grat-

    ing diracts incoming light, bouncing

    it to an array o detectors. The longer

    the light ans out beore it hits the

    detectors, the more the resolution

    improvesbut the instrument alsogets larger. This becomes a serious

    problem in the submillimeter band,

    because the wavelengths are about a

    thousand times longer than in the op-

    tical. Hoping to shrink the instrument

    back down, Zmuidzinas considered

    conning the light in superconduct-

    ing circuitry on a silicon waer, similar

    to an ordinary printed circuit board.

    This would address the problem

    the metal circuitry would conne the

    light vertically and also slow it down,

    reducing the required path lengthsconsiderably. But experiments initi-

    ated by undergraduate Chiyan Luo

    (BS 00) showed that the circuitry

    would lose too many photons.

    Meanwhile, Jamie Bock, by then

    a JPL research scientist, was also

    trying to make a better submillimeter

    spectrometer. He was looking into

    instruments that bounced light the

    old-ashioned way, with mirrors and

    lenses. But they were proving to be

    unmanageably large, so Zmuidzinassuggested a compromise using a

    machined-metal version o the super-

    conducting spectrometer.

    In 2000, Bock and Zmuidzinas

    joined orces to develop a new instru-

    ment that would draw on each o

    their approaches, and they were soon

    joined by Millikan Postdoctoral Fel-

    low Matt Bradord, graduate student

    Bret Naylor (PhD 08), Hien Nguyen

    at JPL, and collaborators at other

    universities.

    In Z-Spec, the resulting spectrome-

    ter that was rst installed on the CSO

    in 2005, eedhorns unnel light into

    the 2.5-millimeter gap between two

    parallel metal plates, each more than

    a oot on a side. The light hits a ac-

    eted, arc-shaped grating, splintering

    o to be caught by 160 bolometers

    variations on the spiderweb concept.Z-Specs bandwidthon par with

    that o optical spectrometersis over

    ten times larger than that o previous

    submillimeter spectrometers. The in-

    strument recently measured redshits

    o several distant, dust-obscured

    star-orming galaxies discovered with

    Herschel.

    of SQuidS and mkidS

    The story doesnt end with the

    smashing success o the spiderwebbolometers and Z-Spec. In act,

    Lange and Bocks progress on the

    bolometers had let one box un-

    checked: We didnt ulll the vision

    o producing large arrays o detectors

    purely by lithography, Zmuidzinas

    says. Its a requent quandarydo you

    spend more time on a new tool that

    can scale up, or do you prioritize the

    ability to do interesting science right

    away? The spiderwebs had mostly

    solved the issue o hand-assembly,but placing the thermometers and

    installing the wiring was still delicate

    and labor-intensive. In the late 90s,

    Zmuidzinas returned to the challenge

    o making a camera with simple wiring

    and thousands o mass-producible

    detectors.

    Kent Irwin (BS 88) had made

    progress on this problem, in the

    meantime, when he ound a simple,

    practical way to make use o super-

    conducting bolometers as a Stanord

    graduate student in 1995. Called

    transition edge sensors, his bolom-

    eters used strips o superconducting

    metal lms as thermometers. Small

    temperature changes in the strips

    reliably yielded measurable changes

    in resistance, once Irwin drew on the

    design o stereo ampliers to keep

    the strips within a working tempera-ture range. Then, in 1999, in his rst

    job, Irwin and collaborators (including

    Erich Grossman, PhD 88) developed

    readout multiplexers using supercon-

    ducting quantum intererence devices

    (SQUIDs) that simplied the wiring

    or large bolometer arrays. Arrays o

    these detectors, incorporating novel

    antennas inspired by Zmuidzinass

    work, are being developed at JPL

    or studying the cosmic microwave

    background and or sensitive spec-

    troscopy rom space.It was a breakthrough, but the

    SQUID multiplexers seemed com-

    plicated to Zmuidzinas. The SQUID

    approach works well or certain

    applications, but it wouldnt scale up

    to the large detector count needed

    or CCATs cameras. He and JPLs

    Rick LeDuc discussed the problem

    at a coee shop near campus. LeDuc

    wondered: Cant we use kinetic

    inductance somehow?

    This was a lightning bolt orZmuidzinas. Back in his oce, he

    scanned the literature. Photons

    absorbed by a superconductor would

    produce quasiparticles. A quasipar-

    ticle population boom would change

    the superconductors inductance,

    which would change the circuits

    resonant requency. Perhaps he and

    LeDuc could design a lithographed

    superconducting resonator and use

    its requency change as the detect-

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    fall 2010 ENGINEERING & SCIENCE

    able response. Each resonance

    would be sharp, occupying a narrow

    range o requencies. You could tack

    resonators next to each other on one

    readout wire, maybe into the thou-

    sands. There was no theoretical ceil-

    ing or the quality o each resonator.

    reSonant interactionSZmuidzinas and LeDuc shared the

    idea with Tom Tombrello, Caltechs

    Kenan Proessor and then chair o

    the Division o Physics, Mathematics

    and Astronomy. Tombrello spoke with

    then provost Steve Koonin, who con-

    nected him with trustee Alex Lidow

    (BS 75)who provided substantial

    seed unding. Lidows git came at

    a critical time or usit allowed us to

    get the equipment we needed and

    get set up to do this in the right way,

    Zmuidzinas says. Prominent research-ers rom Caltech and JPL, as well as

    other universities, signed on to the e-

    ort. Koonin and Tombrello also talked

    with JPLs Jakob van Zyl (PhD 86),

    who helped move the project ahead.

    JPLs Peter Day (PhD 93) sug-

    gested making the resonators using

    a structure called a coplanar wave-

    guide, etched rom a superconduct-

    ing metal lm deposited on a silicon

    waer. In the resulting resonators, the

    distance covered by the microwavesas they bounced back and orth

    totaled more than a kilometer!

    They were getting Qs(a qual-

    ity actor related to path length) o a

    million-plus, says Keith Schwab, an

    applied physicist at Caltech. People

    in quantum computing and applied

    physics couldnt believe it. Its had

    a big impact on our work. And the

    technology is easy to implement.

    Beyond their unanticipated ben-

    ets, the new MKID circuits actually

    work. The team has created a camera

    with 2,304 detectorsit will be in-

    stalled on the CSO in the all o 2011.

    In development are new versions oMKIDs, in which the radiation is ab-

    sorbed in meandering superconduct-

    ing strips that also let energy slosh

    back and orth between inductors and

    capacitors. They will have Qs in the

    tens o millions. These MKIDs rely on

    superconducting titanium-nitride lms,

    a choice suggested by LeDuc. They

    are very simple, dropping costs and

    enabling abrication o extremely large

    cameras or CCAT.

    The invention is also inspiring newapplications: Caltech physicist Sunil

    Golwala is exploring ways to use

    titanium-nitride MKIDs to detect dark

    matter, Ben Mazin (PhD 04) is de-

    veloping optical-wavelength versions

    or astrophysics, and Zmuidzinas and

    Day hope to use the material to make

    a nearly ideal microwave amplier.

    These ongoing eorts are supported

    by the Keck Institute or Space

    Studies and by the Gordon and

    Betty Moore Foundation, which also

    enabled earlier detector work.

    As you can see, you bounce

    around and it takes a while to land on

    the right idea, says Zmuidzinas. Theinstruments at the heart o CCAT will

    bring decades o work to ruition.

    Looking back, Zmuidzinas refects,

    There are always such surprising

    connections. Who would have

    thought that trying to look or

    submillimeter galaxies would spark an

    idea useul in quantum computing?

    But thats how research works. There

    are deep, hidden connections among

    elds. We all learn rom each other.

    AW

    if umn y could ubmllm-

    r l, ow k ovr

    CCat lco would look. CCat wll

    b bul o Crro Cjnnor n Cl

    acm dr n lvon of

    5,612 mr, on of nd

    dr lc on er. t nl,

    wr vor borb ubmllmr

    wv.

    http://www.kschwabresearch.com/http://www.astro.caltech.edu/~golwala/http://www.astro.caltech.edu/~golwala/http://www.kiss.caltech.edu/http://www.kiss.caltech.edu/http://www.moore.org/http://www.moore.org/http://www.moore.org/http://www.moore.org/http://www.kiss.caltech.edu/http://www.kiss.caltech.edu/http://www.astro.caltech.edu/~golwala/http://www.astro.caltech.edu/~golwala/http://www.kschwabresearch.com/
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    Left: Looking like a knight in a chain-mail hood,

    Koch dons an array of electroencephalography (EEG)

    electrodes for a brain-function test.

    Right: Afterward, he appears to have been a ttacked

    by a giant squid, thanks to the arrays suction cups.

    Be Aware of Your Inner ZombieBy Andrew Portereld

    Be Aware of Your Inner ZombieIn the 1968 horror classic Night of the

    Living Dead, terried people trapped in a

    Pennsylvania armhouse try to survive zom-

    bies hungry or human fesh.

    But real zombies arent like that, accord-

    ing to neurobiologist Christo Koch. The

    word zombie is a surprisingly technical

    term, developed in detail by philosopher

    David Chalmers. Zombies are exactly like

    you and me except that they have no eelingor awareness, Koch saysa rather more

    sympathetic view than director George

    Romeros. Chalmerss 1996 book, The

    Conscious Mind, proposed these zombies

    as a thought experiment through which

    we could explore the question o whether a

    creature could exist that displayed the ull

    range o human behavior but lacked con-

    scious sensations. Such a zombie would get

    up, get dressed, and go to work like you and

    me. I you asked it over lunch what its avor-

    ite band was, it might answer, Pink Floyd,

    and perhaps even invite you on a date tosee a local tribute band cover Dark Side

    of the Moon on Saturday. But the zombie

    would not be experiencing the taste o the

    sandwich it was eating, nor would it enjoy

    the music as a human would. Do any natura

    laws prohibit the existence o such beings?

    Chalmers asked.

    In act, its the unconscious, or zom-

    bie, systems in our brains that help us get

    through daily lie, Koch says, and they can

    show us how consciousness really works.

    Koch has been ascinated by the phe-nomenon o consciousness or more than

    two decades, but his interest started not

    with a penchant or horror cinema, but with

    a toothache. I was teaching a course at

    the Marine Biological Laboratory in Woods

    Hole, Massachusetts. So I was lying in bed,

    had this terrible toothache, Im taking aspirin

    but its still persistent. He began to ask

    himsel, Why should that hurt? Where does

    the eeling come rom?

    Koch blends techniques rom psychology,

    Zombies walk among us. In act, we couldnt get along without

    themoperating below the threshold o awareness, zombie

    systems in our brains take care o all sorts o routine tasks

    without any conscious eort on our part. Studying such un-

    conscious processes is beginning to throw light on how the

    conscious mind works.

    http://www.klab.caltech.edu/~koch/http://www.klab.caltech.edu/~koch/
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    In Kochs world, the

    zombies are in our

    brains. In the pop-

    culture world, the

    zombies are out for

    our brains.

    biology, and neurology to attack the unda-

    mental questions o consciousness: What

    is it in the brain that enables us to eel?

    What part o the human and animal brain is

    necessary to be conscious? And how does

    consciousness arise out o matter?

    The debate about whether theres an

    actual place or consciousness in the brain

    goes back millennia. Plato and Aristotle held

    that the mind was entirely divorced rom thephysical bodylike parallel Las Vegases,

    what happened in the body stayed

    in the body; what happened

    in the mind stayed

    in the mind. More

    recently, the French

    philosopher

    Ren Descartes

    argued that the

    mind and the brain

    could infuence each

    other. He proposed that

    the soul resided in thepineal glanda solitary

    lump in the shape o a pine cone (but about

    the size o a grain o rice) that lies almost ex-

    actly in the middle o the brain, surrounded

    by the matched pairs o structures that make

    up the rest o the brain. This glands singular

    nature and central location, he argued,

    clearly marked it as something special, and

    what could be more special than the physi-

    cal seat o what makes us human? (Alas,

    we now know that the pineal gland doesnt

    do much more than help control our cycle o

    waking and sleeping by secreting the hor-

    mone melatonin in response to darkness.)

    a Risky Business

    When Koch entered the eld in 1988, the

    study o consciousness was not consid-

    ered serious science. A mountain climber

    and trail runner, he describes himsel asa risk taker. Even without tenure, I was

    adventuresome, and I was very interested in

    consciousness. But talking about con-

    sciousness was a sign that you were retired,

    or had a Nobel Prize, or were a mystic and

    slept next to crystal pyramids, he laughs. It

    was like talking about sex during Victorian

    timesit was just taboo. Koch paired up

    with the vigorously unretired Nobel laureate

    Francis Crick, the codiscoverer o the

    double-helical structure o DNA, the

    molecule o heredity, who had moved romprobing the workings o genes to contem-

    world beyond the neurobiology community.

    Today, many laboratories study con-

    sciousness, and Descartess intellectual

    descendants are still asking: Where in the

    brain is the mind? Consider a computer,

    Koch says. I you rig a thermometer to a

    computer and put them both next to a heat

    source, the thermometer will transmit the

    ambient temperature to the computer. Once

    the temperature rises above some thresholdthe computer can be set to print out a mes-

    sage. It is too hot. Im in pain. But does the

    computer actually experience pain? I dont

    think so. At this point, its response is noth-

    ing but a programmed instruction, a refex.

    At a certain threshold temperature value,

    some electrons fow onto a gate, a transis-

    tor opens another gate, opens the register,

    records the content, and prints out a state-

    ment. There is no eeling involved.

    Now compare that to the sensation o

    someone stomping on your toe. Again, atrain o electrical impulsesthis time medi-

    When Koch entered the ield in 1988, the study oconsciousness was not considered serious science.

    plating the workings o the brain 15 years

    earlier. The two remained close collabora-

    tors until Cricks death in 2004.Francis had thought or a long time about

    consciousness, and in his view it was a

    scandalous state o aairs that people were

    studying the brain without ever reerring to

    the act that this brain produces conscious-

    ness every day, day in and day out, Koch

    recalls. Together, the duo published about

    two dozen papers; Crick also wrote the

    oreword to Kochs 2004 book, The Quest

    for Consciousness, which introduced the

    notion o zombie agents to the unsuspecting

    ated by calcium, sodium, potassium, and

    other ionsfows rom your oot to your

    brain. I can say this is just biophysicssignals moving about inside the nervous

    system. Theres no pain eeling anywhere.

    But without any doubt youll eel this bad

    thing, pain. So how is it that a physical

    system like a brain can produce a subjec-

    tive state, but another physical system, the

    computer, doesnt? This is the heart o the

    mind-body problem.

    Some headway has been made since the

    days o Descartes, and scientists have dis-

    covered that not all o the brain is involved in

    creating consciousness. The cerebellum, orexample, controls the timing o motor move-

    ments, and it contains hal o the brains

    neurons. I you lose your cerebellar unction

    you will be unable to coordinate your muscle

    movements, a condition called ataxia. You

    might stagger and sway while you walk,

    or instance. You wont be in a rock band,

    you wont be a ballerina or a climber, but

    your visual consciousness will be marginally

    impacted, i at all, Koch notes.

    Nudist Colony of the Dead, 1991 Pirromount Pictures.

    http://www.amazon.com/gp/product/1936221047/ref=pd_lpo_k2_dp_sr_1?pf_rd_p=486539851&pf_rd_s=lpo-top-stripe-1&pf_rd_t=201&pf_rd_i=0974707708&pf_rd_m=ATVPDKIKX0DER&pf_rd_r=1WKZ0FE9AQK56MBMEABPhttp://www.amazon.com/gp/product/1936221047/ref=pd_lpo_k2_dp_sr_1?pf_rd_p=486539851&pf_rd_s=lpo-top-stripe-1&pf_rd_t=201&pf_rd_i=0974707708&pf_rd_m=ATVPDKIKX0DER&pf_rd_r=1WKZ0FE9AQK56MBMEABPhttp://www.amazon.com/gp/product/1936221047/ref=pd_lpo_k2_dp_sr_1?pf_rd_p=486539851&pf_rd_s=lpo-top-stripe-1&pf_rd_t=201&pf_rd_i=0974707708&pf_rd_m=ATVPDKIKX0DER&pf_rd_r=1WKZ0FE9AQK56MBMEABPhttp://www.amazon.com/gp/product/1936221047/ref=pd_lpo_k2_dp_sr_1?pf_rd_p=486539851&pf_rd_s=lpo-top-stripe-1&pf_rd_t=201&pf_rd_i=0974707708&pf_rd_m=ATVPDKIKX0DER&pf_rd_r=1WKZ0FE9AQK56MBMEABP
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    i see, TheRefoRe i am

    Koch attacks the problem o conscious-

    ness through the brains visual system. He

    originally established his laboratorynot

    coincidentally, painted in bright primary

    colorsto study visual perception, trying to

    understand how we ocus on one aspect o

    a scene, and to gure out how this orm o

    selective visual attention could be taught to

    machine-vision systems. This backgroundlent itsel easily to experiments with visual

    consciousness.

    Kochs other longtime collaborator, Itzhak

    Fried, is a proessor o neurosurgery at

    UCLA who implants microelectrodes into

    epilepsy patients whose seizures cannot

    be controlled by nonsurgical means. Fried

    uses these electrodes to nd the abnormal

    brain-cell activity caused by epilepsy; the

    electrodes pinpoint the lesions locations in

    order to guide his scalpel. The electrodes

    as many as a dozen per patient, with each

    one sprouting as many as nine microwireprobes rom its tipshow up nicely in CAT

    scans, which provide their tips three-

    dimensional coordinates to within a ew

    millimeters.

    Even better, rom Kochs point o view,

    each microwire is sensitive enough to pick

    up the musings o a single neuron. As luck

    would have it, some o the deep-brain cen-

    ters involved in recognizing and remember-

    ing people are in brain areas that are most

    oten aected by epilepsy, such as the

    hippocampus. Thus Frieds electrodes giveKoch a window intoor, more accurately,

    a water glass pressed up against the wall

    othose regions o the brain.

    The electrodes remain in the patients

    heads or up to two weeks. Thats a long

    time to spend hanging around in a hospi-

    tal, so the simple video games that Koch

    and his colleagues have designed or their

    experiments oer a welcome distraction.

    As the patients stare at the computer

    screens, the researchers use the electrodes

    to look or neural correlates o conscious-

    ness, or NCCs, which Koch and Crick had

    dened in a 2003 paper called A Frame-

    work or Consciousness. The paper pro-

    posed that visual NCCs are small coalitions

    o nerve cells that collect inormation rom

    the back o the cerebral cortex, where the

    preliminary processing o visual inormation

    is perormed, and establish sets o two-way

    communication links with other parts o thecerebral cortex at the ront o the brain.

    The receiving regions include the medial

    temporal lobe, where Koch, his grad student

    Gabriel Kreiman (MS, PhD 02), and Fried

    had already ound neurons that only red

    when a person was consciously perceiv-

    ing an image. That discovery had been

    made by tting Frieds patients with special

    LCD glasses that were, in eect, separate

    TV screens or each eye. A picture would

    appear on one screen and remain there so

    that the test subjects could clearly see it.

    Then a second, dierent picture would bemomentarily fashed into the other eyea

    technique known as fash suppression,

    because the new picture in the second

    eye would suppress the perception o the

    old image in the rst eye. In other words,

    the resh image wiped the older one rom

    consciousness, even though both were still

    there to be seen. The neurons ring rates

    refected this. Kreiman noticed that, in most

    cases, each neuron being recorded would

    respond to only one specic image, say a

    picture o a smiling girl. When the imagewas fash-suppressed, however, the neuron

    became ar less active, even though its

    preerred picture was still displayed. Those

    neurons, thereore, ollowed whatever was

    in the patients conscious perception. They

    red when the patient saw the image, and

    they didnt re when the patient didnt.

    Wherever the brains representations o

    the suppressed imagesvisible, but not

    consciously seenmight reside, they had to

    be somewhere else.

    seeing JennifeR anisTon

    That some neurons red only in response

    to specic pictures was no big surprise

    ater all, pattern recognition is one o the

    things our brains do best. But in 2005,

    postdoc Rodrigo Quian Quiroga; grad

    student Leila Reddy (PhD 05); Kreiman, by

    then at MIT; Koch; and Fried announced the

    discovery o individual neurons in the medial

    temporal lobes that recognized specicpeople. It didnt matter whether the picture

    presented was ull-ace or in prole, or even

    a line drawing or a caricature; the neuron

    knew who it was looking at.

    The rst neuron we ound behaving this

    way was a Bill Clinton neuron back in 2002,

    Koch recalls. Then, there was a second

    neuron that responded to three dierent

    cartoon images o characters rom The

    Simpsons, and a third selective neuron to

    basketball superstar Michael Jordan. When

    we rst submitted the paper to Nature, the

    reerees didnt believe this unheard-o

    Left: The regions mentioned in this article lie deep

    within your brain. (The brains outer surface is out-

    lined in orange.) Visual processing begins in area V1

    also known as the primary visual cortex. V2 through

    V5 do additional analysis before sending the informa

    tion on to the medial temporal lobe, the hippocampu

    and other areas where consciousness may lurk. V1

    through V5 are on the inner, facing surfaces of the ce

    rebral hemispheres; the hippocampus, the cerebellum

    and the pineal gland straddle the brains midline.

    Far left: A horizontal slice through the temporal lobes

    V3AV3V1/V2V4 (color)Cerebellum

    Face and objectrecognition areas

    V5 (motion)

    Front

    Temporal lobe

    Hippocampus

    Pineal gland

    Medial temporal lobe

    http://www.nature.com/neuro/journal/v6/n2/abs/nn0203-119.htmlhttp://www.nature.com/neuro/journal/v6/n2/abs/nn0203-119.htmlhttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.nature.com/nature/journal/v435/n7045/abs/nature03687.htmlhttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.pnas.org/content/99/12/8378.abstracthttp://www.nature.com/neuro/journal/v6/n2/abs/nn0203-119.htmlhttp://www.nature.com/neuro/journal/v6/n2/abs/nn0203-119.html
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    Your brain wires up groups of cells that respond to things weconstantly encounter. I had no idea who Jennifer Anistonwas before we did these experiments, but presumably I nowhave a set of neurons that respond to Jennifer Aniston,Koch chuckles.

    degree o selectivity, since we only had

    three such neurons. Three neurons dont

    make a discovery. So we went back and

    characterized many more o these remark-

    able cells51 in that 2005 Nature paper,

    and more since then.

    Grad student Stephen Waydo (PhD 08),

    on loan rom control and dynamical systems

    proessor Richard Murray (BS 85), and

    Koch pieced together an explanation or theprocess behind such extreme selectivity.

    Although the world around us presents an

    innite variety o stimuli, Waydo and Koch

    assumed that most o the patterns that

    come to us through our senses are due to

    a small number o causes. For instance,

    when Im at home, most o the visual activity

    in my brain at any given moment is caused

    by me seeing my amily and the urniture in

    the rooms around me, all o which are very

    amiliar to me, Koch says. Working rom this

    premise, Waydo devised a set o machine-

    learning rules that would enable a com-puter to identiy such commonly occurring

    patternsdiscovering or itsel the Platonic

    orm, i you will, o Kochs soaand then

    represent each one as a specic pattern o

    outputs rom a collection o neurons.

    Similarly, says Koch, Your brain wires up

    groups o cells, what we call concept cells,

    that re specically in response to things we

    constantly encounter. To illustrate this, he

    brings up on his computer a session with

    one o Frieds patients. An image o Marilyn

    Monroe appears on the screen: a rapid-

    re trrrppp, trrrppp, trrrppp pours rom the

    speakers. Then, actor Josh Brolin; nothing.

    I had no idea who Jennier Aniston

    was beore we did these experiments, but

    presumably I now have a set o neurons that

    respond to Jennier Aniston, Koch chuck-

    les. Its an ecient way o dealing with the

    world. It allows inants to learn early thelessons that stay with us: rst you learn to

    recognize your parents and your siblings in

    this abstract and invariant matter, and your

    dog, and all the other important people, ani-

    mals, and things that your brain constantly

    encounters. Then when you get older, its

    on to mastering more abstract things, like

    Marcel Proust or e = mc2.

    Concept cells respond to sensory stimuli

    o all kindsin Anistons case, or example,

    not just seeing her, but hearing the sound

    o her voice or even reading her name; this

    set o neurons will activate when exposed toany aspect o the Zen o Jen.

    There are two schools o thought about

    how concept cells work. The distributed-

    population hypothesis invokes a large

    number o neurons, each contributing a little

    bit to encoding the percept. The power o

    this approach lies in the great number o

    distinct objects that can be encoded, and

    in the robustness o their representation

    lose any one neuron, and the percept hardly

    changes. The sparse-coding hypothesis, on

    the other hand, proposes that a small net-

    work o neurons is entirely responsible or

    the encoding. The ultimate sparse network

    would be one consisting o a single cell;

    this reduction to the extreme is known in the

    trade as the grandmother cell hypothesis,

    because it implies that somewhere in your

    brain there lives a cell whose sole duty is to

    recognize your grandmother.At rst blush, the existence o Jennier

    Aniston neurons would seem to support

    the grandmother-cell hypothesis, but there

    is something to both sides, says Koch.

    In 2008, Quian Quiroga, Kreiman, Koch,

    and Fried ound that yet another o Frieds

    patients had a neuron in the hippocampus

    (an interior region o the medial temporal

    lobe) that responded not only to Aniston but

    to her Friends costar Lisa Kudrow. Since

    the two actresses have only one degree o

    separation on the small screen, it seems

    reasonable that their NCCs might share aew cells as well. (Another cell in the para-

    hippocampal cortex o a dierent patient

    red in response to both the Eiel Tower

    and the Leaning Tower o Pisa but not to

    other landmarks, displaying a similar power

    o generalization.) So it appears that the

    networks are indeed sparse, but maybe not

    thatsparsethey contain enough members

    to be both very selective and very abstract

    at the same time.

    A couple of famous people who might be in your head.

    The first concept cell that Kochs team discovered fired in response to pictures of President Clinton.

    If youve watched more than a few episodes of Friends, youve probably got a set of neurons that respond to

    actress Jennifer Aniston.

    Once a network of concept cells has been wired up, it will be activated whenever it recognizes the object of its

    obsession. It doesnt matter whether the image it sees is a grainy black-and-white photo or even a scrawled

    cariacture; nor does it matter if the subject is seen in a full-face view, in profile, or even partly obscured.

    In fact, the stimulus doesnt even have to be visual. Concept cells will react to sounds, smells, and even the

    written wordany sensory stimulus that we associate with that person.

    http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5http://www.cell.com/trends/cognitive-sciences/abstract/S1364-6613(08)00023-5
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    ENGINEERING & SCIENCE fall 201018

    living The ZomBie life

    So what do zombies have to do with

    any o this? More than wed like to admit,

    apparently. In his upcoming book, Con-

    sciousnessConfessions of a Romantic

    Reductionist, Koch recalls a trail-running

    session in which he encountered a rattle-

    snake. Something made me look down. My

    right leg instantly lengthened its stride, or

    my brain had detected a rattlesnake sunningitsel on the stony path where I was about to

    put my oot, he writes. Beore I had seen

    the reptile or experienced any ear . . . I had

    already acted to avoid stepping on it. Had

    he been orced to think about consciously

    adjusting his stride, it would have been too

    late.

    This unconscious, automatic response

    was choreographed by one o our zombie

    systems. While its well known that the ner-

    vous system controls many body unctions

    without conscious eortthings such as

    heartbeat, breathing, and digestionKochestimates that about 90 percent o our ac-

    tivities are the work o unconscious zombies.

    The central insight o Sigmund Freud is

    that youre not conscious o most o the stu

    in your brain. For example, we spend much

    o the day typing. Now, i I ask someone,

    What nger do you type the letter fwith?

    most people wont know. They have to pan-

    tomime the movement to realize that its the

    let index nger. But i you dont consciously

    think about it, your ngers will do the typing

    by themselves. Even activities as seem-

    ingly varied and unstructured as Kochs

    mountain-climbing adventures call on these

    zombie systems most o the time. Nearly all

    o his risky moves up the side o a cli are

    so ingrained that he doesnt give them a

    thought.

    So why isnt all o lie like that? he asks.

    Why not have a completely zombie exis-

    tence? Because lie throws us curve balls,

    thats why. The world is so complex; you

    have to do things that are nonroutine. Letssay there was an earthquake right now. You

    would look rst at the glass window, which

    could shatter and seriously injure you, and

    then you would look around or a sae way

    to get outside. Reacting to an earthquake

    isnt something youve trained or hundreds

    o times. But or repetitive behaviors, even

    very elaborate ones, its a convenient way or

    our brain to handle the situation with minimal

    eort.

    Paying aTTenTion

    But even with an army o zombies at our

    command, we suer rom inormation over-

    load, says Koch. We have to concentrate

    on the essentials; otherwise we wouldnt get

    anything done. Attention is the brains way

    o maintaining ocus. But attention is not

    the same as awareness or consciousness,

    he adds. While consciousness involves the

    general awareness o the world around us,

    or what we think is the world around us, at-

    tention is a spotlight. Attention takes hold o

    one aspect o our environment, whether its

    scanning your DVD collection or the sev-

    enth season o Friends or listening to one

    person in a crowded room. Its a mechanism

    or selecting or urther processing a ew

    rivulets o inormation out o the food that

    inundates our senses, providing the brain

    a way to organize multiple inputs and make

    sense o the world.

    Scientists have long assumed that atten-

    tion and consciousness are the same, or at

    the very least heavily intertwined. This pastMay, biology postdoc Jeroen van Boxtel,

    psychology and neuroscience postdoc

    Naotsugu Tsuchiya, and Koch demonstrated

    that this assumption is wrong. In these

    experiments, members o the campus com-

    munity were asked to xate their eyes, with-

    out any movement, on a dot in the center

    o a computer screen. Then, o to one side

    o one eyes eld o view, a Gabor patcha

    computer-generated blur resembling a smal

    smudgewould appear or our seconds

    and then vanish, leaving an aterimage in

    the eye that had seen it. (Aterimages arethe oldest tools o visual psychologists, as

    they are easy to induce and manipulate in

    reproducible ways.) The volunteers pressed

    a button when the aterimage disappeared.

    At the same time, the participants were

    asked to count the number o times a

    specic symbol appeared among a series o

    symbols that rapidly fashed, one by one, at

    the center o their gaze. In some o the runs,

    the correct symbols were made deliberately

    hard to spota demanding task requiring

    ull attention. In other runs, the task waseasier, mean