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8/3/2019 Caltech_Fall2010
1/48
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
alifornia Boulevard, Pasadena, CA 91125. Annual subscription $20.00 domestic, $30.00 foreign air mail; single copies $5.00.
end subscriptions to Caltech 1-71, Pasadena, CA 91125. Third-class postage paid at Pasadena, CA. All rights reserved.
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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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.
Lf: a rk bwn wo ony lcrod n
7 rcn ydron mxur, nrn frbll.
i no dnrou look xloon
mll. For comron, dnc bwn
lcrod only fw mllmr. t no r
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
Wc slly Bn dcu r
work r of 2010 evrr
Lcur sr.
http://today.caltech.edu/theater/item?story_id=44862http://today.caltech.edu/theater/item?story_id=44862 -
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worldor rr
r Ro-
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d rd bou
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Cludu polmy
georphi.
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
-
8/3/2019 Caltech_Fall2010
9/48
fall 2010 ENGINEERING & SCIENCE
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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,
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frnly colord fluorcn ron,
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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
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wll du-roudd r-
formn ron CsO ,
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.
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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-
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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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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