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Thursday, May 28, 2009

Planet-Hunting Method Succeeds at Last

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

J.D. Harrington 202-358-5241
NASA Headquarters, Washington
jharring@nasa.gov

NEWS RELEASE: 2009-090 May 28, 2009

Planet-Hunting Method Succeeds at Last

PASADENA, Calif. -- A long-proposed tool for hunting planets has netted its first catch -- a Jupiter-like
planet orbiting one of the smallest stars known.

The technique, called astrometry, was first attempted 50 years ago to search for planets outside our
solar system, called exoplanets. It involves measuring the precise motions of a star on the sky as an
unseen planet tugs the star back and forth. But the method requires very precise measurements over
long periods of time, and until now, has failed to turn up any exoplanets.

A team of two astronomers from NASA's Jet Propulsion Laboratory, Pasadena, Calif., has, for the
past 12 years, been mounting an astrometry instrument to a telescope at the Palomar Observatory near
San Diego. After careful, intermittent observations of 30 stars, the team has identified a new
exoplanet around one of them -- the first ever to be discovered around a star using astrometry.

"This method is optimal for finding solar-system configurations like ours that might harbor other
Earths," said astronomer Steven Pravdo of JPL, lead author of a study about the results to be
published in the Astrophysical Journal. "We found a Jupiter-like planet at around the same relative
place as our Jupiter, only around a much smaller star. It's possible this star also has inner rocky planets.
And since more than seven out of 10 stars are small like this one, this could mean planets are more
common than we thought."

The finding confirms that astrometry could be a powerful planet-hunting technique for both ground-
and space-based telescopes. For example, a similar technique would be used by SIM Lite, a NASA
concept for a space-based mission that is currently being explored.

The newfound exoplanet, called VB 10b, is about 20 light-years away in the constellation Aquila. It is
a gas giant, with a mass six times that of Jupiter's, and an orbit far enough away from its star to be
labeled a "cold Jupiter" similar to our own. In reality, the planet's own internal heat would give it an
Earth-like temperature.

The planet's star, called VB 10, is tiny. It is what's known as an M-dwarf and is only one-twelfth the
mass of our sun, just barely big enough to fuse atoms at its core and shine with starlight. For years,
VB 10 was the smallest star known -- now it has a new title: the smallest star known to host a planet.
In fact, though the star is more massive than the newfound planet, the two bodies would have a
similar girth.

Because the star is so small, its planetary system would be a miniature, scaled-down version of our
own. For example, VB 10b, though considered a cold Jupiter, is located about as far from its star as
Mercury is from the sun. Any rocky Earth-size planets that might happen to be in the neighborhood
would lie even closer in.

"Some other exoplanets around larger M-dwarf stars are also similar to our Jupiter, making the stars
fertile ground for future Earth searches," said Stuart Shaklan, Pravdo's co-author and the SIM Lite
instrument scientist at JPL. "Astrometry is best suited to find cold Jupiters around all kinds of stars,
and thus to find more planetary systems arranged like our home."

Two to six times a year, for the past 12 years, Pravdo and Shaklan have bolted their Stellar Planet
Survey instrument onto Palomar's five-meter Hale telescope to search for planets. The instrument,
which has a 16-megapixel charge-coupled device, or CCD, can detect very minute changes in the
positions of stars. The VB 10b planet, for instance, causes its star to wobble a small fraction of a
degree. Detecting this wobble is equivalent to measuring the width of a human hair from about three
kilometers away.

Other ground-based planet-hunting techniques in wide use include radial velocity and the transit
method. Like astrometry, radial velocity detects the wobble of a star, but it measures Doppler shifts in
the star's light caused by motion toward and away from us. The transit method looks for dips in a
star's brightness as orbiting planets pass by and block the light. NASA's space-based Kepler mission,
which began searching for planets on May 12, will use the transit method to look for Earth-like
worlds around stars similar to the sun.

"This is an exciting discovery because it shows that planets can be found around extremely light-
weight stars," said Wesley Traub, the chief scientist for NASA's Exoplanet Exploration Program at
JPL. "This is a hint that nature likes to form planets, even around stars very different from the sun."

JPL is a partner with the California Institute of Technology in Pasadena in the Palomar Observatory.
Caltech manages JPL for NASA. More information about exoplanets and NASA's planet-finding
program is at http://planetquest.jpl.nasa.gov . More information about the Palomar Observatory is at
http://www.astro.caltech.edu/palomar/ .

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Wednesday, May 27, 2009

NASA Selects Student's Entry as New Mars Rover Name

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 1-818-354-5011
http://www.jpl.nasa.gov

Alan Buis/Carolina Martinez 1-818-354-0474/9382
Jet Propulsion Laboratory, Pasadena, Calif.
Alan.buis@jpl.nasa.gov/carolina.martinez@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

NEWS RELEASE: 2009-089 May 27, 2009

NASA Selects Student's Entry as New Mars Rover Name

PASADENA, Calif. – NASA's Mars Science Laboratory rover, scheduled for launch in 2011, has a
new name, thanks to a sixth-grade student from Kansas. Twelve-year-old Clara Ma from the
Sunflower Elementary school in Lenexa submitted the winning entry, "Curiosity." As her prize, Ma
wins a trip to NASA's Jet Propulsion Laboratory in Pasadena, Calif., where she will be invited to sign
her name directly onto the rover as it is being assembled.

A NASA panel selected the name following a nationwide student contest that attracted more than
9,000 proposals via the Internet and mail. The panel primarily took into account the quality of
submitted essays. Name suggestions from the Mars Science Laboratory project leaders and a non-
binding public poll also were considered.

"Students from every state suggested names for this rover. That's testimony to the excitement Mars
missions spark in our next generation of explorers," said Mark Dahl, the mission's program executive
at NASA Headquarters in Washington. "Many of the nominating essays were excellent and several of
the names would have fit well. I am especially pleased with the choice, which recognizes something
universally human and essential to science."

Ma decided to enter the rover-naming contest after she heard about it at her school.

"I was really interested in space, but I thought space was something I could only read about in books
and look at during the night from so far away," Ma said. "I thought that I would never be able to get
close to it, so for me, naming the Mars rover would at least be one step closer."

"Curiosity is an everlasting flame that burns in everyone's mind. It makes me get out of bed in the
morning and wonder what surprises life will throw at me that day," Ma wrote in her winning essay.
"Curiosity is such a powerful force. Without it, we wouldn't be who we are today. Curiosity is the
passion that drives us through our everyday lives. We have become explorers and scientists with our
need to ask questions and to wonder."

The naming contest was conducted in partnership with Disney-Pixar's animated film "WALL-E." The
activity invited ideas from students 5 - 18 years old enrolled in a U.S. school. The contest started in
November 2008. Entries were accepted until midnight Jan. 25.

Walt Disney Studios Motion Pictures supplied the prizes for the contest, including 30 for semifinalists
related to "WALL-E." Nine finalists have been invited to provide messages to be placed on a
microchip mounted on Curiosity. The microchip also will contain the names of thousands of people
around the world who have "signed" their names electronically via the Internet. Additional electronic
signatures still are being accepted via the Internet.

"We have been eager to call the rover by name," said Pete Theisinger, who manages the JPL team
building and testing Curiosity. "Giving it a name worthy of this mission's quest means a lot to the
people working on it."

Curiosity will be larger and more capable than any craft previously sent to land on the Red Planet. It
will check to see whether the environment in a selected landing region ever has been favorable for
supporting microbial life and preserving evidence of life. The rover also will search for minerals that
formed in the presence of water and look for several chemical building blocks of life.

The Mars Science Laboratory project is managed by JPL for NASA's Science Mission Directorate in
Washington.

For more information about the mission and the contest winner, visit: http://www.nasa.gov/msl .

To send your name on the rover microchip, visit:
http://marsprogram.jpl.nasa.gov/msl/participate/sendyourname .

JPL is managed for NASA by the California Institute of Technology in Pasadena.

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Thursday, May 21, 2009

NASA Rover Sees Variable Environmental History at Martian Crater

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Gay Hill 818-354-0344
Jet Propulsion Laboratory, Pasadena, Calif.
gay.y.hill@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

NEWS RELEASE: 2009-088 May 21, 2009

NASA Rover Sees Variable Environmental History at Martian Crater

PASADENA, Calif. -- One of NASA's two Mars rovers has recorded a compelling saga of
environmental changes that occurred over billions of years at a Martian crater.

The Mars rover, Opportunity, surveyed the rim and interior of Victoria Crater on the Red Planet
from September 2006 through August 2008. Key findings from that work, reported in the May
22 edition of the journal Science, reinforce and expand what researchers learned from
Opportunity's exploration of two smaller craters after landing on Mars in 2004.

The rover revealed the effects of wind and water. The data show water repeatedly came and left
billions of years ago. Wind persisted much longer, heaping sand into dunes between ancient
water episodes. These activities still shape the landscape today. At Victoria, steep cliffs and
gentler alcoves alternate around the edge of a bowl about 0.8 kilometers (half a mile) in diameter.
The scalloped edge and other features indicate the crater once was smaller than it is today, but
wind erosion has widened it gradually.

"What drew us to Victoria Crater is the thick cross-section of rock layers exposed there," said
Steve Squyres of Cornell University in Ithaca, N.Y. Squyres is the principal investigator for the
science payloads on Opportunity and its twin rover, Spirit. "The impact that excavated the crater
millions of years ago provided a golden opportunity, and the durability of the rover enabled us to
take advantage of it."

Imaging the crater's rim and interior, Opportunity inspected layers in the cliffs around the crater,
including layered stacks more than 10 meters (30 feet) thick. Distinctive patterns indicate the
rocks formed from shifting dunes that later hardened into sandstone, according to Squyres and
33 co-authors of the findings.

Instruments on the rover's arm studied the composition and detailed texture of rocks just outside
the crater and exposed layers in one alcove called "Duck Bay." Rocks found beside the crater
include pieces of a meteorite, which may have been part of the impacting space rock that made
the crater.

Other rocks on the rim of the crater apparently were excavated from deep within it when the
object hit. These rocks bear a type of iron-rich small spheres, or spherules, that the rover team
nicknamed "blueberries" when Opportunity first saw them in 2004. The spherules formed from
interaction with water penetrating the rocks. The spherules in rocks deeper in the crater are larger
than those in overlying layers, suggesting the action of groundwater was more intense at greater
depth.

Inside Duck Bay, the rover found that, in some ways, the lower layers differ from overlying
ones. The lower layers showed less sulfur and iron, more aluminum and silicon. This composition
matches patterns Opportunity found earlier at the smaller Endurance Crater, about 6 kilometers
(4 miles) away from Victoria, indicating the processes that varied the environmental conditions
recorded in the rocks were regional, not just local.

Opportunity's first observations showed interaction of volcanic rock with acidic water to produce
sulfate salts. Dry sand rich in these salts blew into dunes. Under the influence of water, the
dunes hardened to sandstone. Further alteration by water produced the iron-rich spherules,
mineral changes and angular pores left when crystals dissolved away.

A rock from space blasted a hole about 600 meters (2,000 feet) wide and 125 meters (400 feet)
deep. Wind erosion chewed at the edges of the hole and partially refilled it, increasing the
diameter by about 25 percent and reducing the depth by about 40 percent.

Since leaving Victoria Crater about eight months ago, Opportunity has been on its way to study a
crater named Endeavour that is about 20 times bigger than Victoria. The rover has driven about
one-fifth of what could be a 16-kilometer (10-mile) trek to this new destination.

The twin rovers, Spirit and Opportunity, continue to produce scientific results while operating far
beyond their design life. The mission, designed to last 90 days, celebrated its fifth anniversary in
January. Both rovers show signs of aging but are still capable of exploration and scientific
discovery.

NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the Mars rovers for NASA's
Science Mission Directorate in Washington.

More information about Spirit and Opportunity is at
http://www.nasa.gov/rovers .

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Wednesday, May 20, 2009

Hubble Educator Conference to Cap an Amazing May

Hubble Educator Conference to Cap an Amazing May

Although you would have to be somewhat attentive to the goings-on in space, the month of May 2009 has been
quite remarkable. This message is a reminder to join us at JPL at the end of the month for our celebration of the
biggest news, upgrades to NASA's Hubble Space Telescope by astronauts on space shuttle Atlantis.

During five spectacular space walks over five straight days, astronauts turned Hubble into a brand new telescope
with new equipment and instruments onboard, enabling it to get an even better view of the universe. Our
conference will look at Hubble's last 19 years and at what's ahead and include highlights from the servicing mission.
We'll also have a look into the 2009 International Year of Astronomy.

The registration form is below. For complete conference details, please visit:
http://education.jpl.nasa.gov/events/conf-20090530.html

And in case you missed any of this, in May...
* Shuttle Atlantis (STS-125) successfully launched and completed Hubble Servicing Mission-4.
* Astronomical observatory satellites Herschel and Planck were successfully launched by a European Ariane 5
booster.
* A Russian supply spacecraft arrives at the International Space Station (ISS).
* At the end of the month a Russian Soyuz will bring three more astronauts/cosmonauts to ISS to join the three
onboard for the first crew of six. The station will be truly international with a crew of two Russians, an American, a
Canadian, a Japanese and a European Space Agency astronaut (from Belgium).
* The Spitzer Space Telescope, one of the "Great Observatories" like Hubble, used up the last of its coolant as
expected, and began its "warm mission" to look at near-Earth objects and extrasolar planets.
* Astronaut Dr. Scott Parazynski, five-time space flyer, reached the summit of Mt. Everest. (But he is on vacation
time so it isn't really a NASA event!)



To register for this conference please send a check postmarked by Friday, May 22, 2009, for $40.00 payable to "Jet
Propulsion Laboratory" to:

Hubble Educator Conference
Attn: Mary Kay Kuehn
Jet Propulsion Laboratory
M/S 180-109
4800 Oak Grove Drive
Pasadena CA 91109

Please register by Friday, May 22, 2009. The $40 registration fee includes continental breakfast and breaks both
days and a box lunch on Saturday.
For registration questions please call the JPL Education Office at 818-393-0561 or e-mail mary.k.kuehn@jpl.nasa.gov

For updates and information visit the JPL Education Gateway at http://education.jpl.nasa.gov/.

Name________________________________________
Title_________________________________________
Organization/School_________________________________________________
Address_______________________________________ State____ Zip________
Grade(s) Taught/Enrolled_____________________________________________
Subject(s) Taught/Enrolled____________________________________________
Contact info for confirmation & last minute changes:
E-mail: ________________________________
Phone: ________________________________

$40 Registration Fee Enclosed? Check # ____________

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Monday, May 18, 2009

Mars and Earth Activities Aim to Get Spirit Rolling Again

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
Guy.Webster@jpl.nasa.gov

Mars Exploration Rover Mission Status Report May 18, 2009

Mars and Earth Activities Aim to Get Spirit Rolling Again

PASADENA, Calif. -- NASA's rover project team is using the Spirit rover and other
spacecraft at Mars to begin developing the best maneuvers for extracting Spirit from the
soft Martian ground where it has become embedded.

A diagnostic test on May 16 provided favorable indications about Spirit's left middle
wheel. The possibility of the wheel being jammed was one factor in the rover team's May 7
decision to temporarily suspend driving Spirit after that wheel stalled and other wheels had
dug themselves about hub-deep into the soil. The test over the weekend showed electrical
resistance in the left middle wheel is within the expected range for a motor that has not
failed.

"This is not a full exoneration of the wheel, but it is encouraging," said John Callas of
NASA's Jet Propulsion Laboratory, Pasadena, Calif., project manager for Spirit and its
twin rover, Opportunity. "We're taking incremental steps. Next, we'll command that wheel
to rotate a degree or two. The other wheels will be kept motionless, so this is not expected
to alter the position of the vehicle."

Another reason to suspend driving is the possibility that the wheels' digging into the soil
may have lowered the body of the rover enough for its belly pan to be in contact with a
small mound of rocks. The rover team is using Opportunity to test a procedure for possible
use by Spirit: looking underneath the rover with the microscopic imager camera that is
mounted on the end of the rover's arm. This might be a way to see whether Spirit is, in fact,
touching the rocks beneath it.

NASA's Mars Odyssey orbiter is also aiding in the Spirit recovery plan. As a result of
winds blowing dust off Spirit's solar panel four times in the past month, Spirit now has
enough power to add an extra communication session each day. The Odyssey project has
made the orbiter available for receiving extra transmissions from Spirit. The transmissions
include imaging data from Spirit's examinations of soil properties and ground geometry.

Rover team members are using that data and other information to construct a simulation of
Spirit's situation in a rover testing facility at JPL. The team is testing different materials to
use as soil that will mimic the physical properties of the Martian soil where Spirit is
embedded. Later, the team will test maneuvers to get the rover free. Weeks of testing are
anticipated before any attempt to move Spirit.

JPL, a division of the California Institute of Technology in Pasadena, manages the Mars
Exploration Rover project for NASA's Science Mission Directorate, Washington.

#2009-087


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Friday, May 15, 2009

NASA's Spitzer Begins Warm Mission

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

Spitzer Space Telescope Mission Status May 15, 2009

NASA's Spitzer Begins Warm Mission

PASADENA, Calif. -- After more than five-and-a-half years of probing the cool cosmos, NASA's
Spitzer Space Telescope has run out of the coolant that kept its infrared instruments chilled. The
telescope will warm up slightly, yet two of its infrared detector arrays will still operate successfully.
The new, warm mission will continue to unveil the far, cold and dusty universe.

Spitzer entered standby mode at 3:11 p.m. Pacific Time (6:11 p.m. Eastern Time or 22:11 Universal Time),
May 15, as result of running out of its liquid helium coolant. Scientists and engineers will spend the
next few weeks recalibrating the instrument at the warmer temperature, and preparing it to begin
science operations.

Additional information, including the following items, is at:
http://www.nasa.gov/mission_pages/spitzer/news/spitzer-warm.html .
--A full news release about Spitzer's warm mission and past accomplishments
--A mock interview titled "If Spitzer Could Talk: An Interview with NASA's Coolest Space
Mission"
--A video about the Spitzer mission
--An article about the late astronomer Lyman Spitzer, the mission's namesake

Detailed information about the Spitzer mission at http://www.spitzer.caltech.edu/spitzer and
http://www.nasa.gov/spitzer

Who's Who of the Spitzer mission:
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer mission for NASA's
Science Mission Directorate in Washington, D.C. Science operations are conducted at the Spitzer
Science Center at the California Institute of Technology in Pasadena. Lockheed Martin Space
Systems in Denver, and Ball Aerospace & Technologies Corp., in Boulder, Colo., support mission
and science operations. NASA's Goddard Space Flight Center in Greenbelt, Md., built Spitzer's
infrared array camera; the instrument's principal investigator was Giovanni Fazio of the Harvard-
Smithsonian Center for Astrophysics in Cambridge, Mass. Ball Aerospace & Technologies Corp.
built Spitzer's infrared spectrograph; its principal investigator was Jim Houck of Cornell University
in Ithaca, N.Y. Ball Aerospace & Technologies Corp. and the University of Arizona in Tucson,
built the multiband imaging photometer for Spitzer; its principal investigator was George Rieke of
the University of Arizona.

#2009-086


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Thursday, May 14, 2009

Herschel and Planck on Way to Study our Cosmic Roots

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

NEWS RELEASE: 2009-085 May 14, 2009

Herschel and Planck on Way to Study our Cosmic Roots

The Herschel and Planck spacecraft successfully blasted into space at 6:12 a.m. Pacific Time
(9:12 a.m. Eastern Time) on May 14 from the Guiana Space Centre in French Guiana.

The European Space Agency missions, with significant participation from NASA, hitched a ride
together on an Ariane 5 rocket, but now have different journeys before them. Herschel will
explore, with unprecedented clarity, the earliest stages of star and galaxy birth in the universe; it
will help answer the question of how our sun and Milky Way galaxy came to be. Planck will
look back to almost the beginning of time itself, gathering new details to help explain how our
universe came to be.

"These two missions have spent a lot of time together," said Ulf Israelsson, NASA project
manager for both Herschel and Planck at NASA's Jet Propulsion Laboratory, Pasadena, Calif.
"But now they are going their separate ways, each ready to do what it does best."

JPL contributed key technology to both missions. NASA team members will play an important
role in data analysis and science operations.

Herschel separated from its Ariane 5 rocket 26 minutes after launch, followed by Planck about
two minutes later. The spacecraft are traveling on separate trajectories to a point in the Earth-sun
system called the second Lagrangian point, four times farther away than the moon's orbit, or an
average distance of 1.5 million kilometers (930,000 miles) from Earth. They will spend the rest
of their missions independently orbiting this point -- located on the other side of Earth from the
sun -- as they make their way around the sun every year. See animations at
http://www.esa.int/esa-
mmg/mmg.pl?b=b&type=VA&mission=Herschel&single=y&start=10
and
http://www.esa.int/esa-mmg/mmg.pl?b=b&type=VA&mission=Planck&single=y&start=10
.

Herschel will start preparing for science operations while en route toward its operational orbit,
which will be reached in about two months. Four months later, the science mission will begin
and is expected to last more than three-and-a-half years. Planck will reach a similar orbit in
roughly two months, with science observations beginning one month later. The mission's science
operations are scheduled to last a minimum of 15 months, with the possibility of an extension.

Both observatories are designed to see light that our human eyes cannot. Herschel will detect
light that has gone largely unexplored until now, with wavelengths in the infrared and
submillimeter range. It will make the most detailed measurements yet of the cold and dark
wombs where the embryos of stars and galaxies have just begun to grow.

Herschel will also be able to detect key elements and molecules involved in a star's life, tracing
their evolution from atoms to potentially life-forming materials. One of these molecules is water;
astronomers say Herschel will provide a greatly improved measurement of how much water
there is in space.

"Using Herschel is like opening a dirty window and getting a clear view of stars and galaxies,"
said Paul Goldsmith, the NASA Herschel project scientist at JPL.

Planck will see longer wavelength light, from the submillimeter to microwave range. It will work
like the ultimate time capsule, to see light that has traveled billions of years from the newborn
universe to reach us. This light, called the cosmic microwave background, contains information
about the Big Bang that created space and time itself.

"Our previous images of the baby universe were like fuzzy snapshots -- now we'll have the
cleanest, deepest and sharpest images ever made of the early universe," said Charles Lawrence,
the NASA Planck project scientist at JPL.

In order to do their jobs, the instruments on both spacecrafts will be icy cold. Liquid helium will
cool the coldest of Herschel's detectors to just 0.3 Kelvin (minus 459 degrees Fahrenheit), or 0.3
degrees above the coldest temperature theoretically attainable in the universe. Planck's coldest
detectors, which are chilled by cutting-edge coolers developed in part by JPL, will reach a frosty
0.1 Kelvin.

Herschel is a European Space Agency mission, with science instruments provided by a
consortium of European-led institutes, and with important participation by NASA. NASA's
Herschel Project Office is based at JPL. JPL contributed mission-enabling technology for two of
Herschel's three science instruments. The NASA Herschel Science Center, part of the Infrared
Processing and Analysis Center at the California Institute of Technology in Pasadena, supports
the United States astronomical community. Caltech manages JPL for NASA. More information
is online at http://www.nasa.gov/herschel and http://www.herschel.caltech.edu/ and
http://www.esa.int/herschel .

Planck is a European Space Agency mission, with significant participation from NASA.
NASA's Planck Project Office is based at JPL. JPL contributed mission-enabling technology
for both of Planck's science instruments. European, U.S. and NASA Planck scientists will
work together to analyze the Planck data. More information is online at
http://www.nasa.gov/planck and http://www.esa.int/planck .

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Wednesday, May 13, 2009

Let the Planet Hunt Begin

Media RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

Michael Mewhinney 650-604-3937
NASA's Ames Research Center, Moffett Field, Calif.
michael.s.mewhinney@nasa.gov

Kepler Mission Status Report May 13, 2009

Let the Planet Hunt Begin

NASA's Kepler spacecraft has begun its search for other Earth-like worlds. The mission,
which launched from Cape Canaveral, Fla., on March 6, will spend the next three-and-a-
half years staring at more than 100,000 stars for telltale signs of planets. Kepler has the
unique ability to find planets as small as Earth that orbit sun-like stars at distances where
temperatures are right for possible lakes and oceans.

"Now the fun begins," said William Borucki, Kepler science principal investigator at
NASA's Ames Research Center, Moffett Field, Calif. "We are all really excited to start
sorting through the data and discovering the planets."

Scientists and engineers have spent the last two months checking out and calibrating the
Kepler spacecraft. Data have been collected to characterize the imaging performance as
well as the noise level in the measurement electronics. The scientists have constructed the
list of targets for the start of the planet search, and this information has been loaded onto
the spacecraft.

"If Kepler got into a staring contest, it would win," said James Fanson, Kepler project
manager at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "The spacecraft is ready
to stare intently at the same stars for several years so that it can precisely measure the
slightest changes in their brightness caused by planets." Kepler will hunt for planets by
looking for periodic dips in the brightness of stars -- events that occur when orbiting
planets cross in front of their stars and partially block the light.

The mission's first finds are expected to be large, gas planets situated close to their stars.
Such discoveries could be announced as early as next year.

Kepler is a NASA Discovery mission. NASA Ames Research Center, Moffett Field,
Calif., is the home organization of the science principal investigator, and is responsible for
the ground system development, mission operations and science data analysis. JPL
manages the Kepler mission development. Ball Aerospace & Technologies Corp. of
Boulder, Colo., is responsible for developing the Kepler flight system and supporting
mission operations.

For more information about the Kepler mission, visit:
http://www.nasa.gov/kepler and http://www.kepler.nasa.gov .

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Spitzer Catches Star Cooking Up Comet Crystals

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
Whitney.clavin@jpl.nasa.gov

NEWS RELEASE: 2009-083 May 13, 2009

Spitzer Catches Star Cooking Up Comet Crystals

Scientists have long wondered how tiny silicate crystals, which need sizzling high
temperatures to form, have found their way into frozen comets, born in the deep freeze of
the solar system's outer edges. The crystals would have begun as non-crystallized silicate
particles, part of the mix of gas and dust from which the solar system developed.

A team of astronomers believes they have found a new explanation for both where and
how these crystals may have been created, by using NASA's Spitzer Space Telescope to
observe the growing pains of a young, sun-like star. Their study results, which appear in
the May 14 issue of Nature, provide new insight into the formation of planets and
comets.

The researchers from Germany, Hungary and the Netherlands found that silicate appears
to have been transformed into crystalline form by an outburst from a star. They detected
the infrared signature of silicate crystals on the disk of dust and gas surrounding the star
EX Lupi during one of its frequent flare-ups, or outbursts, seen by Spitzer in April 2008.
These crystals were not present in Spitzer's previous observations of the star's disk during
one of its quiet periods.

"We believe that we have observed, for the first time, ongoing crystal formation," said
one of the paper's authors, Attila Juhasz of the Max-Planck Institute for Astronomy in
Heidelberg, Germany. "We think that the crystals were formed by thermal annealing of
small particles on the surface layer of the star's inner disk by heat from the outburst. This
is a completely new scenario about how this material could be created."

Annealing is a process in which a material is heated to a certain temperature at which
some of its bonds break and then re-form, changing the material's physical properties. It is
one way that silicate dust can be transformed into crystalline form.

Scientists previously had considered two different possible scenarios in which annealing
could create the silicate crystals found in comets and young stars' disks. In one scenario,
long exposure to heat from an infant star might anneal some of the silicate dust inside the
disk's center. In the other, shock waves induced by a large body within the disk might
heat dust grains suddenly to the right temperature to crystallize them, after which the
crystals would cool nearly as quickly.

What Juhasz and his colleagues found at EX Lupi didn't fit either of the earlier theories.
"We concluded that this is a third way in which silicate crystals may be formed with
annealing, one not considered before," said the paper's lead author, Peter Abraham of the
Hungarian Academy of Sciences' Konkoly Observatory, Budapest, Hungary.

EX Lupi is a young star, possibly similar to our sun four or five billion years ago. Every
few years, it experiences outbursts, or eruptions, that astronomers think are the result of
the star gathering up mass that has accumulated in its surrounding disk. These flare-ups
vary in intensity, with really big eruptions occurring every 50 years or so.

The researchers observed EX Lupi with Spitzer's infrared spectrograph in April 2008.
Although the star was beginning to fade from the peak of a major outburst detected in
January, it was still 30 times brighter than when it was quiet. When they compared this
new view of the erupting star with Spitzer measurements made in 2005 before the
eruption began, they found significant changes.

In 2005, the silicate on the surface of the star's disk appeared to be in the form of
amorphous grains of dust. In 2008, the spectrum showed the presence of crystalline
silicate on top of amorphous dust. The crystals appear to be forsterite, a material often
found in comets and in protoplanetary disks. The crystals also appear hot, evidence that
they were created in a high-temperature process, but not by shock heating. If that were
the case, they would already be cool.

"At outburst, EX Lupi became about 100 times more luminous," said Juhasz. "Crystals
formed in the surface layer of the disk but just at the distance from the star where the
temperature was high enough to anneal the silicate--about 1,000 Kelvin (1,340 degrees
Fahrenheit)--but still lower than 1,500 Kelvin (2,240 degrees Fahrenheit). Above that, the
dust grains will evaporate." The radius of this crystal formation zone, the researchers note,
is comparable to that of the terrestrial-planet region in the solar system.

"These observations show, for the first time, the actual production of crystalline silicates
like those found in comets and meteorites in our own solar system," said Spitzer Project
Scientist Michael Werner of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "So
what we see in comets today may have been produced by repeated bursts of energy when
the sun was young."

JPL manages the Spitzer Space Telescope mission for NASA's Science Mission
Directorate, Washington. Science operations are conducted at the Spitzer Science Center
at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA.

More information about Spitzer is at http://www.spitzer.caltech.edu/spitzer and
http://www.nasa.gov/spitzer .

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Monday, May 11, 2009

Soft Ground Puts Spirit in Danger Despite Gain in Daily Energy

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
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http://www.jpl.nasa.gov

Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif. May 11, 2009
Guy.Webster@jpl.nasa.gov

MARS EXPLORATION ROVER MISSION STATUS REPORT

Soft Ground Puts Spirit in Danger Despite Gain in Daily Energy

PASADENA, Calif. -- The five wheels that still rotate on NASA's Mars Exploration Rover
Spirit have been slipping severely in soft soil during recent attempts to drive, sinking the
wheels about halfway into the ground.

The rover team of engineers and scientists has suspended driving Spirit temporarily while
studying the ground around the rover and planning simulation tests of driving options with
a test rover at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

"Spirit is in a very difficult situation," JPL's John Callas, project manager for Spirit and its
twin rover, Opportunity, said Monday. "We are proceeding methodically and cautiously. It
may be weeks before we try moving Spirit again. Meanwhile, we are using Spirit's scientific
instruments to learn more about the physical properties of the soil that is giving us trouble."

Both Spirit and Opportunity have operated more than five years longer than their originally
planned missions of three months on Mars and have driven much farther than designed.
The rover team has so far developed ways to cope with various symptoms of aging on both
rovers.

Spirit has been driving counterclockwise from north to south around a low plateau called
"Home Plate" for two months. The rover progressed 122 meters (400 feet) on that route
before reaching its current position.

In the past week, the digging-in of Spirit's wheels has raised concerns that the rover's belly
pan could now be low enough to contact rocks underneath the chassis, which would make
getting out of the situation more difficult. The right-front wheel on Spirit stopped working
three years ago. Driving with just five powered wheels while dragging or pushing an
immobile wheel adds to the challenge of the situation.


Favorably, three times in the past month, wind has removed some of the dust accumulated
on Spirit's solar panels. This increases the rover's capability for generating electricity.

"The improved power situation buys us time," Callas said. "We will use that time to plan
the next steps carefully. We know that dust storms could return at any time, although the
skies are currently clear."

Behavioral problems that Spirit exhibited in early April -- episodes of amnesia, computer
resets and failure to wake for communications sessions -- have not recurred in the past three
weeks, though investigations have yet to diagnose the root causes.

JPL, a division of the California Institute of Technology in Pasadena, manages the Mars
Exploration Rover project for NASA's Science Mission Directorate, Washington.

#2009-082
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Sunday, May 10, 2009

Hubble Photographs a Planetary Nebula to Commemorate Decommissioning of Super Camera

DC Agle 818-393-9011
NASA's Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov

JD Harrington/Dwayne Brown
NASA Headquarters, Washington
202-358-5241/1726
j.d.harrington@nasa.gov /dwayne.c.brown@nasa.gov

Cheryl Gundy 410-338-4707
Space Telescope Science Institute, Baltimore, Md.
gundy@stsci.edu

News release: 2009-081 May 10, 2009

Hubble Photographs a Planetary Nebula to Commemorate Decommissioning of Super Camera

The Hubble community bids farewell to the soon-to-be decommissioned Wide Field and Planetary
Camera 2 onboard NASA's Hubble Space Telescope. In tribute to Hubble's longest-running optical
camera, which was developed and built by NASA's Jet Propulsion Laboratory, Pasadena, Calif., a
planetary nebula has been imaged as the camera's final "pretty picture."

This planetary nebula is known as Kohoutek 4-55 (or K 4-55). It is one of a series of planetary nebulae
that were named after their discoverer, Czech astronomer Lubos Kohoutek. A planetary nebula
contains the outer layers of a red giant star that were expelled into interstellar space when the star
was in the late stages of its life. Ultraviolet radiation emitted from the remaining hot core of the star
ionizes the ejected gas shells, causing them to glow.

In the specific case of K 4-55, a bright inner ring is surrounded by a bipolar structure. The entire
system is then surrounded by a faint red halo, seen in the emission by nitrogen gas. This multi-shell
structure is fairly uncommon in planetary nebulae.

This Hubble image was taken by the Wide Field and Planetary Camera 2 on May 4, 2009. The colors
represent the makeup of the various emission clouds in the nebula: red represents nitrogen, green
represents hydrogen, and blue represents oxygen. K 4-55 is nearly 4,600 light-years away in the
constellation Cygnus.

The Wide Field and Planetary Camera 2 instrument, which was installed in 1993 to replace the original
Wide Field/Planetary Camera, will be removed to make room for Wide Field Camera 3 during the
upcoming Hubble Servicing Mission.

During the camera's amazing, nearly 16-year run, the Wide Field and Planetary Camera 2 provided
outstanding science and spectacular images of the cosmos. Some of its best-remembered images are
of the Eagle Nebula pillars, Comet P/Shoemaker-Levy 9's impacts on Jupiter's atmosphere, and the
1995 Hubble Deep Field -- the longest and deepest Hubble optical image of its time.

The scientific and inspirational legacy of the camera will be felt by astronomers and the public alike, for
as long as the story of the Hubble Space Telescope is told.

For images and more information about planetary nebula K 4-55, visit:
http://hubblesite.org/news/2009/21 . For more information about the Wide Field and Planetary
Camera 2, visit: http://www.jpl.nasa.gov/wfpc2/

The Hubble Space Telescope is a project of international cooperation between NASA and the
European Space Agency and is managed by NASA's Goddard Space Flight Center in Greenbelt, Md.
The Space Telescope Science Institute conducts Hubble science operations. The institute is operated
for NASA by the Association of Universities for Research in Astronomy, Inc., Washington, D.C.

The Space Telescope Science Institute is an International Year of Astronomy 2009 program partner.
JPL is managed for NASA by the California Institute of Technology in Pasadena.

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The Camera That Saved Hubble… Twice JPL's Wide Field and Planetary Camera 2

The Camera That Saved Hubble… Twice JPL's Wide Field and Planetary Camera 2

First motion is almost always a big event in the world of space exploration. Whether the first motion is
of a wheel beginning to rotate or a rocket lifting off the pad, first motion means things are definitely
changing. On day four of the upcoming shuttle servicing mission of the Hubble Space Telescope,
there will be another such significant first motion. It will begin when a bolt that has been frozen in place
for a decade and a half completes its 20th counterclockwise rotation.

"When that happens, that will be the first time in 15-and-a-half years that our instrument will have
moved over one one-millionth of an inch from its position aboard the Hubble Space Telescope," said
John Trauger of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "That is when the mission of
the camera that saved Hubble will come to an end."

Certainly, the Wide Field and Planetary Camera 2 (WFPC2, as many scientists call it) is not your
normal, everyday camera -- it is the size of a baby grand piano. But then again, Hubble does just
about everything big. Orbiting 353 miles up, the school bus-sized Hubble is one of NASA's premiere
eyes on the universe. When light from a distant galaxy enters the telescope, it arrives untouched by
the light-scattering vagaries of Earth's atmosphere.

What happens next to this pristine, extra-terrestrial light is the reason the first motion of WFPC2 in 15-
plus years is so significant. Because what happens next is -- as with all telescopes-- these photons of
light bounce off the telescope's primary mirror. In Hubble's case, when light first bounced off its 8-foot
(2.4-meter) diameter primary mirror, it bounced off in a way Hubble scientists and engineers did not
expect -- and did not plan for. Another problem -- by the time they realized Hubble's mirror might be
flawed, it was already in orbit.

"Hubble launched aboard space shuttle Discovery in April 1990," said Trauger. "Discovery was already
safely down on the ground before we recognized there was a problem, and that it would severely
affect what science we could with the Hubble observatory."

Ed Weiler is the associate administrator for NASA's Science Mission Directorate. Back then he was
Hubble's program scientist. After the first images came down from Hubble on May 20, his outlook took
a turn for the worse. "It was like climbing to the top of Mount Everest and then suddenly, within a
couple of months, sinking to the bottom of the Dead Sea -- the lowest point on Earth."

We figured out it was a problem we couldn't fix and we decided to do a press conference on June 27,
1990, and announce to the world that the pictures we promised, the science we promised, wouldn't be
delivered by the Hubble Space Telescope."

The theories on what caused the problem were plentiful and some more than a little wild. While
theories were bandied about, there was a toll taken on the team.

"It was a very sad, very difficult time," said Dave Leckrone, senior project scientist at NASA's Goddard
Space Flight Center in Greenbelt, Md. "Astronomers had planned very detailed scientific programs that
would take full advantage of this wonderful image quality that Hubble was to provide. They became
very, very discouraged when they saw the images coming back from the telescope. Some of them left
the program in disgust."

The theories on what exactly happened to Hubble flew fast and furious. The main problem with
proving any of them was that much of the evidence was located 350 miles straight up. NASA
appointed JPL's director, Lew Allen, to chair a board to investigate what had happened to Hubble. But
investigative boards are thorough and take time to get it right. Answers and action were needed now,
and it was someone else from JPL who provided Weiler and the Hubble team some hope.

"Around the time of that (June 27) briefing, John Trauger cornered me in a hallway outside the space
telescope science working group meeting and said, 'Ed, I think we have a way to fix with the Wide
Field and Planetary Camera 2,'" said Weiler. "You cannot believe how down every astronomer on the
Hubble team was that day because we didn't have the telescope we thought. So, John gave me this
one ray of hope. It was one little ray of hope and I glommed onto it."

The beginning of the heroic fix of the Hubble Space Telescope began even before a problem was
known to exist. Even before the telescope hit the cold, dark, unforgiving blackness of space. It was
back in 1985 that Weiler moved heaven and Earth to make sure Hubble's universe had a spare Wide
Field and Planetary Camera on hand.

"A number of people in the science working group, but in particular Ed Weiler, the program scientist,
drew the conclusion that the Hubble is all about imagery," said Dave Leckrone. "It is all about taking
clear, sharp, beautiful pictures of the sky and doing fantastic science with those images (see
companion article: "A Universal Art Form"), and it is unthinkable that Hubble should ever go blind. That
was the mantra. We could never allow Hubble to go blind, so let's build a replica of WFPC."

By the time Discovery deposited Hubble in orbit, the Wide Field and Planetary Camera 2 was well
underway. A few days after the first image from Hubble hit the cover of the New York Times, JPL
scientists Aden and Marjorie Mienel dropped by the camera team's offices at JPL. The Mienels had a
lifetime of experience with astronomical telescopes and they smelled a rat. It was perhaps the first
time one of the most dreaded terms in all of astronomy was uttered in reference to Hubble: "spherical
aberration."

"Spherical aberration happens when the primary mirror is polished incorrectly," said Trauger. You can
think of the mirror as a very shallow bowl. With spherical aberration it's just a little too shallow, a little
too flat."

Later, the investigative board chaired by JPL's Lew Allen would trace the source of Hubble's spherical
aberration to faulty test equipment used to define and measure the primary mirror's curvature. But
now, JPL's Hubble camera team was concerned with what could be done about it. Aden Mienel had
suggested that the space telescope's optical issues could be worked out by reworking the optics of
their new, still to be completed camera – WFPC2.

"Norm Page, a JPL optical engineer, was the custodian of our optical prescription for Hubble," said
Trauger. "I went down to the lab with and we played with our model of our new Wide Field Camera.
We soon realized that Aden was right, that we could correct for Hubble's mirror by replacing four small
mirrors, each the size of a nickel, inside our new camera.

It was only when armed with that information that Trauger approached Weiler with the proposed fix
prior to the first media briefing about Hubble's imaging problem. And Weiler told the world about it
during the briefing. That there was a date in mind for a repair mission and that the spare Wide Field
Camera would play a big role. But few in the media noticed.

"I announced… in three years, by December of 1993, we would launch the clone, the wide field clone,
and we would fix the problem," said Weiler. "Nobody believed us, that we would do it, and that we
could do it. So it was a disaster in the press for many months thereafter and suddenly in the press was
born the term "Hubble trouble." One thing we learned from that is never name a telescope after
someone who rhymes with trouble."

The bad press kept coming and Hubble's troubles became the fodder for more than one late-night
comedian. Hubble and failure had become part of the American Zeitgeist.

"I remember giving a talk to some kindergarten kids about the wonders of Hubble," said Trauger. I said
the words Hubble Telescope and everybody laughed. They didn't know what it meant but they knew it
was funny. Back then, everything about Hubble was funny all of a sudden.

Trauger, the Wide Field and Planetary Camera 2 project managers, Dave Rogers and Larry Simmons,
and a team that at times exceeded more than 100 engineers and scientists, learned what it was like to
live life in a fishbowl. Everything mattered, and everything aboard their 610-pound camera had to be
right, checked and double checked and then checked again. If they needed any further reminding,
they got it the day NASA Administrator Dan Goldin paid them a visit.

"Goldin came to the cleanroom where we were doing some testing and asked what was going on,"
said Trauger. "Larry Simmons said – 'well, we are here to fix the Hubble Telescope.' Goldin's response
was – 'no, you are here to save the agency.'"

Everyone working on the camera knew the score. Not only its importance to NASA's future, but the
open questions that would not be answered until their camera was on orbit and firing back images,
because they had never done anything like this before.

We purposefully made the mirrors in our camera out of focus, said Trauger. "The inverse of, and just
as profoundly out of focus as, the Hubble telescope was. And that was not easy to measure in a
laboratory because you can't just look for a sharp focus, you have to look for something you think
exists aboard Hubble."

Trauger and his team delivered the Wide Field and Planetary Camera 2 to the Goddard Space Flight
Center ahead of schedule. They ushered it through final testing and watched as on December 2, 1993,
space shuttle Atlantis carried the hopes and dreams of so many into space.

"Off it goes and you can only imagine what it would be like to be an astronaut in the midst of that
violence," said Trauger. "But what I couldn't help thinking was we spent the last couple of years
aligning the optics of this delicate camera and everything has to be so perfectly aligned to work, and
here it is just getting shaken all over the place."

Sixteen days later, Trauger, Weiler, Leckrone and several other members of the Hubble Science team
were crowded around a monitor in the basement of the Space telescope Science Institute in Baltimore
to see if the camera's optics would prove them right -- or wrong.

"We were all holding our breath, crossing our fingers and doing a lot of praying and hoping that things
were going to look at lot better this time," said Leckrone. The images that came down were so sharp
we knew we had succeeded. There was just intense joy, people slapping others backs. I'm sure there
were tears in more than a few eyes."

"It was a huge relief," said Trauger. We knew this was the beginning and not an end, that Hubble's
science program could now kick into high gear."

On Thursday Jan 13, 1994, NASA released its first images from the new Hubble. Among them a
"before and after" picture taken of spiral galaxy M100. The difference in picture quality was startling.
The picture would appear the next day in papers around the world. It was taken by the Wide field and
Planetary Camera 2. It indicated to the American people and the world that "the trouble with Hubble"
was now over.

Over the next decade-and-a-half, JPL's Wide Field and Planetary Camera 2 would take over 135,000
observations of the universe. It images would go on to adorn posters, album covers, screen savers
and science text books throughout the world. And in 2007, Hubble's workhorse camera would once
again "save Hubble" when the Advanced Camera for Surveys, a more technologically advanced
camera than WFPC2, failed. Having been placed aboard Hubble in 2002, the advanced camera had
been in orbit five years.

"When the Advanced Camera for Surveys failed, there was good old WFPC2 still chugging along,"
said Dave Leckrone. "Just amazing to have gone all of these years, that camera is still working very
well. And I think that is a huge credit to the engineers at JPL who designed and built it. Just an
amazing instrument."

Trauger, the principal investigator for the Wide Field and Planetary Camera 2 during its entire lifetime,
has fond memories of the camera and the team that made it work – so very well. But he also knows its
time in the spotlight is drawing to a close, and like a good scientist, he looks forward to the discoveries
to come.

"As the only instrument to remain in service since the repair mission in 1993, it certainly has served its
mission," said Trauger. "But WFPC2 is the grandpa of Hubble now. It is old and tired and it's time for it
to be brought home.

"And what is going to replace it is going to be even better. It has newer technology and it's going to
renew the whole mission."

Hubble's new Wide Field Camera 3 not only looks like JPL's original WFPC and the veteran WFPC2, it
carries its heritage into space with it. The Wide Field Camera 3's housing, radiator and other
components came from the original WFPC which returned to Earth at the conclusion of the first Hubble
servicing mission.

On the morning of the fourth day of the final Hubble servicing mission, rest assured the men and
women who lived through "the trouble with Hubble" will be watching as astronaut Andy Feustel turns
that bolt for the 20th time, and the Wide Field and Planetary Camera 2 begins to stir.

"You know, JPL promised a lifetime of only three years when we launched it in 1993. It is still working
today, over 15 years later," said Weiler. "It is going to be a tough moment when it comes out of the
Hubble because I remember exactly the moment it was placed in the Hubble. I can still see the
astronauts slowly pushing it in and hoping upon hope that we got the prescription for the thing correct.
I will always remember that moment when it was coming in. I am sure I will remember the moment
when it is coming down.

"But I really look forward to the moment when I get to walk up to it and touch it someday in the
Smithsonian and say, 'that is the camera that saved Hubble.'"

The Wide Field and Planetary Camera 2 was proudly designed and built by NASA's Jet Propulsion
Laboratory, Pasadena, Calif.

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Thursday, May 7, 2009

NASA Releases Interactive 3-D Views of Space Station, New Mars Rover

Guy Webster 1-818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Michael Mewhinney 1-650-604-3937
Ames Research Center, Moffett Field, Calif.
michael.s.mewhinney@nasa.gov

John Yembrick 1-202-358-1100
Headquarters, Washington
john.yembrick-1@nasa.gov

News release: 2009-080 May 7, 2009

NASA Releases Interactive 3-D Views of Space Station, New Mars Rover

PASADENA, Calif. -- NASA released an interactive, 3-D photographic collection of internal and
external views of the International Space Station and a model of the next Mars rover on
Thursday, May 7.

NASA and Microsoft's Virtual Earth team developed the online experience with hundreds of
photographs and Microsoft's photo imaging technology called Photosynth. Using a click-and-
drag interface, viewers can zoom in to see details of the space station's modules and solar
arrays or zoom out for a more global view of the complex.

"Photosynth brings the public closer to our spaceflight equipment and hardware," said Bill
Gerstenmaier, associate administrator for Space Operations at NASA Headquarters in
Washington. "The space station pictures are not simulations or graphic representations but actual
images taken recently by astronauts while in orbit. Although you're not flying 220 miles above the
Earth at 17,500 miles an hour, it allows you to navigate and view amazing details of the real
station as though you were there."

The software uses photographs from standard digital cameras to construct a 3-D view that can
be navigated and explored online.

"This stunning collection of photographs using Microsoft's Photosynth interactive 3-D imaging
technology provides people around the world with an exciting new way to explore the space
station and learn about NASA's upcoming Mars Science Laboratory mission," said S. Pete
Worden, director of NASA's Ames Research Center in Moffett Field, Calif. "This collaboration
with Microsoft offers the public the opportunity to participate in future exploration using this
innovative technology."

The Mars rover imagery gives viewers an opportunity to preview the hardware of NASA's Mars
Science Laboratory, currently being assembled for launch to the Red Planet in 2011.

"We are making this enhanced viewing experience available from the Mars Science Laboratory
project because we're eager for the public to share in the excitement that's building for this
mission," said Fuk Li, manager of NASA's Mars Exploration Program at NASA's Jet Propulsion
Laboratory in Pasadena, Calif.

NASA's Photosynth collection can be viewed at http://www.nasa.gov/photosynth .

The NASA images also can be viewed on Microsoft's Virtual Earth Web site at
http://www.microsoft.com/virtualearth .

While roaming through different components of the station, the public also can join in a
scavenger hunt. NASA has a list of items that can be found in the Photosynth collection. These
items include a station crew patch, a spacesuit and a bell that is traditionally used to announce
the arrival of a visiting spacecraft. Clues to help in the hunt will be posted on NASA's Facebook
page and @NASA on Twitter. To access these sites, visit http://www.nasa.gov/collaborate .

NASA astronaut Sandra Magnus took the internal images of the space station during the 129
days she lived aboard the complex. She photographed the station's exterior while aboard the
space shuttle Discovery, which flew her back to Earth in March. The rover images were taken of
a full-scale model in a Mars-simulation testing area at JPL. Photosynth has multiple potential
benefits for NASA. Engineers can use it to examine hardware, and astronauts can use it for
space station familiarization training.

Photosynth software allows the combination of up to thousands of regular digital photos of a
scene to present a detailed 3-D model of a subject, giving viewers the sensation of smoothly
gliding around the scene from every angle. A collection can be constructed using photos from a
single source or multiple sources. The NASA Photosynth collection also includes shuttle
Endeavour preparing for its STS-118 mission in August 2008.

For more information about the space station, visit http://www.nasa.gov/station . For more
information about the Mars Science Laboratory, visit http://mars.jpl.nasa.gov/msl . JPL, a
division of the California Institute of Technology, Pasadena, manages the Mars Science
Laboratory Project for the NASA Science Mission Directorate, Washington.

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Wednesday, May 6, 2009

NASA Wins Two Webby Awards for Internet Excellence

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Carolina Martinez 818-354-9382
Jet Propulsion Laboratory, Pasadena, Calif.
carolina.martinez@jpl.nasa.gov

Michael Cabbage 202-358-1600
Headquarters, Washington
mcabbage@nasa.gov

NEWS RELEASE: 2009-079 May 6, 2009

NASA Wins Two Webby Awards for Internet Excellence

PASADENA, Calif. – NASA has received two Webby awards for excellence on the Internet.
NASA's main Web site, http://www.nasa.gov, won the People's Voice award for best
government Web site. The Cassini mission Web site, http://saturn.jpl.nasa.gov, received a Webby
award for best science site.

The People's Voice award is the second for NASA's Web site, which also won in 2003. More
than 500,000 people cast votes this year.

"We're extremely happy to be honored by the Internet community this way," said Brian Dunbar,
the content manager for http://www.nasa.gov at NASA Headquarters in Washington. "We've
always tried to focus the site on giving the public what they're looking for in an engaging and
compelling way. Combined with some of the highest customer-satisfaction ratings in the
government, this award tells us we're on the right track."

Judges from the International Academy of Digital Arts and Sciences, which sponsors the
Webbys, selected the Cassini site for the top honor in the science category.

"The Cassini Web site is the door to the science and technology of the mission to Saturn,
contained in hundreds of thousands of pages," said Alice Wessen, manager of Cassini public
engagement at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "The site houses all the latest
news, science findings and images Cassini returns as it orbits Saturn. The public can see every
picture within eight hours after it's beamed down from the spacecraft."

NASA's Web site, which received 120 million visits in 2008, offers the public the latest news,
mission coverage and multimedia from the agency's scientific research, technology development
and exploration efforts. Visitors can surf thousands of images from throughout the universe,
watch live video from the International Space Station or read more than a dozen blogs written by
agency employees.

In the last year, the NASA Web team has expanded its presence into social media, creating an
official NASA channel on YouTube at http://www.youtube.com/nasatelevision, multiple Twitter
feeds led by @NASA, and mission pages on Facebook and MySpace. Since NASA astronaut
Mike Massimino began twittering via @Astro_Mike on April 3, he has gained more than 175,000
followers. NASA was recognized in February with a Shorty award for its @marsphoenix Twitter
presence, which was written in the "voice" of the spacecraft.

For a list of NASA missions providing updates on social media Web sites, visit
http://www.nasa.gov/collaborate.

NASA's Web team also was among the honorees for Rich Media/Advertising for its multimedia
commemoration of NASA's 50th anniversary, http://www.nasa.gov/50years. The feature, hosted
by the robot Automa, includes an interactive news conference with the original Mercury
astronauts, music from across the decades and an "appearance" by renowned astronomer Carl
Sagan.

On Feb. 2, NextGov.com cited NASA's popular homepage as one of five federal government
agencies employing best practices in Web 2.0. Socialgovernment.com also recognized the agency
as among the best in federal government using Twitter, YouTube and social media.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and
the Italian Space Agency. JPL manages the Cassini-Huygens mission for NASA's Science
Mission Directorate, and designed, developed and assembled the orbiter. JPL is managed for
NASA by the California Institute of Technology in Pasadena.

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NASA's Spitzer Telescope Warms up to New Career

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

NEWS RELEASE: 2009-078 May 6, 2009

NASA's Spitzer Telescope Warms up to New Career

PASADENA, Calif. -- The primary mission of NASA's Spitzer Space Telescope is about to end
after more than five-and-a-half years of probing the cosmos with its keen infrared eye. Within
about a week of May 12, the telescope is expected to run out of the liquid helium needed to chill
some of its instruments to operating temperatures.

The end of the coolant will begin a new era for Spitzer. The telescope will start its "warm"
mission with two channels of one instrument still working at full capacity. Some of the science
explored by a warm Spitzer will be the same, and some will be entirely new.

"We like to think of Spitzer as being reborn," said Robert Wilson, Spitzer project manager at
NASA's Jet Propulsion Laboratory, Pasadena, Calif. "Spitzer led an amazing life, performing
above and beyond its call of duty. Its primary mission might be over, but it will tackle new
scientific pursuits, and more breakthroughs are sure to come."

Spitzer is the last of NASA's Great Observatories, a suite of telescopes designed to see the
visible and invisible colors of the universe. The suite also includes NASA's Hubble and Chandra
space telescopes. Spitzer has explored, with unprecedented sensitivity, the infrared side of the
cosmos, where dark, dusty and distant objects hide.

For a telescope to detect infrared light -- essentially heat -- from cool cosmic objects, it must have
very little heat of its own. During the past five years, liquid helium has run through Spitzer's
"veins," keeping its three instruments chilled to -456 degrees Fahrenheit (-271 Celsius), or less
than 3 degrees above absolute zero, the coldest temperature theoretically attainable. The cryogen
was projected to last as little as two-and-a-half years, but Spitzer's efficient design and careful
operations enabled it to last more than five-and-a-half years.

Spitzer's new "warm" temperature is still quite chilly at -404 degrees Fahrenheit (-242 Celsius) --
much colder than a winter day in Antarctica when temperatures sometimes reach -75 degrees
Fahrenheit (-59 Celsius). This temperature rise means two of Spitzer's instruments -- its longer
wavelength multiband imaging photometer and its infrared spectrograph -- will no longer be cold
enough to detect cool objects in space.

However, the telescope's two shortest-wavelength detectors in its infrared array camera will
continue to function perfectly. They will still pick up the glow from a range of objects: asteroids
in our solar system, dusty stars, planet-forming disks, gas-giant planets and distant galaxies. In
addition, Spitzer still will be able to see through the dust that permeates our galaxy and blocks
visible-light views.

"We will do exciting and important science with these two infrared channels," said Spitzer
Project Scientist Michael Werner of JPL. Werner has been working on Spitzer for more than 30
years. "Our new science program takes advantage of what these channels do best. We're focusing
on aspects of the cosmos that we still have much to learn about."

Since its launch from Cape Canaveral, Fla., on Aug. 25, 2003, Spitzer has made countless
breakthroughs in astronomy. Observations of comets both near and far have established that the
stuff of comets and planets is similar throughout the galaxy. Breathtaking photos of dusty stellar
nests have led to new insights into how stars are born. And Spitzer's eye on the very distant
universe, billions of light-years away, has revealed hundreds of massive black holes lurking in the
dark.

Perhaps the most revolutionary and surprising Spitzer findings involve planets around other stars,
called exoplanets. Exoplanets are, in almost all cases, too close to their parent stars to be seen
from our Earthly point of view. Nevertheless, planet hunters continue to uncover them by looking
for changes in the parent stars. Before Spitzer, everything we knew about exoplanets came from
indirect observations such as these.

In 2005, Spitzer detected the first light, or photons, from an exoplanet. In a clever technique,
now referred to as the secondary-eclipse method, Spitzer was able to collect the light of a hot,
gaseous exoplanet and learn about its temperature. Further detailed spectroscopic studies later
revealed more about the atmospheres, or "weather," on similar planets. More recently, Spitzer
witnessed changes in the weather on a wildly eccentric gas exoplanet -- a storm of colossal
proportions brewing up in a matter of hours before quickly settling down.

"Nobody had any idea Spitzer would be able to directly study exoplanets when we designed it,"
Werner said. "When astronomers planned the first observations, we had no idea if they would
work. To our amazement and delight, they did."

These are a few of Spitzer's achievements during the past five-and-a-half years. Data from the
telescope are cited in more than 1,500 scientific papers. And scientists and engineers expect the
rewards to keep on coming during Spitzer's golden years.

Some of Spitzer's new pursuits include refining estimates of Hubble's constant, or the rate at
which our universe is stretching apart; searching for galaxies at the edge of the universe; assessing
how often potentially hazardous asteroids might impact Earth by measuring the sizes of
asteroids; and characterizing the atmospheres of gas-giant planets expected to be discovered soon
by NASA's Kepler mission. As was true during the cold Spitzer mission, these and the other
programs are selected through a competition in which scientists from around the world are
invited to participate.

JPL manages the Spitzer mission for NASA's Science Mission Directorate in Washington.
Science operations are conducted at the Spitzer Science Center at the California Institute of
Technology in Pasadena. Lockheed Martin Space Systems in Denver, and Ball Aerospace &
Technologies Corp. in Boulder, Colo. support mission and science operations. NASA's Goddard
Space Flight Center in Greenbelt, Md., built Spitzer's infrared array camera; the instrument's
principal investigator is Giovanni Fazio of the Harvard-Smithsonian Center for Astrophysics in
Cambridge, Mass. Ball Aerospace & Technology Corp. built Spitzer's infrared spectrograph; its
principal investigator is Jim Houck of Cornell University in Ithaca, N.Y. Ball Aerospace &
Technology Corp. and the University of Arizona in Tucson, built the multiband imaging
photometer for Spitzer; its principal investigator is George Rieke of the University of Arizona.

More information about Spitzer is online at http://www.nasa.gov/spitzer and
http://www.spitzer.caltech.edu/spitzer .

-end-

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Tuesday, May 5, 2009

Corrected Title - A Universal Art Form: NASA's Wide Field and Planetary Camera 2

A Universal Art Form: NASA's Wide Field and Planetary Camera
2

Designed and built by JPL, the Wide Field and Planetary Camera 2
has been the workhorse camera on NASA's Hubble Space
telescope's since it was added to the observatory in December of 1993.
The camera has produced most of the stunning images that have been
released by Hubble during its 15-plus years of service. Its high image resolution
and quality are some of the reasons the camera became the
space telescope's most requested instrument. Throughout history, humanity has
been moved by the work of the great artists of their age. Wielding brush, chisel or
baton, these masters of expression have been able to interpret the environment around
them in innovative ways, providing their public new avenues to explore their own senses
and emotions. But as with so many career fields, the role and tools of the artisan are
changing.

NASA's Wide Field and Planetary Camera 2 is one such new tool of artistic expression.
The name may be unfamiliar to you, but more likely than not, you know of -- and have
been moved by -- its iconic tableaus. For this camera is the implement by which humans
first bore witness to some of the most inspiring and thought provoking vistas in the known
universe.

"I cannot tell you how many times I have heard people tell me how much this picture or
that image has meant to them," said John Trauger, principal investigator of the Wide Field
and Planetary Camera 2 at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "After
a while, I began to realize what we have achieved reached beyond the scope of pure
science and became something more."

Born as a clone, a safeguard, to be used only in the most dire circumstances, the Wide
Field and Planetary Camera 2, or WFPC2, as it's known to the team, was employed
under exactly those conditions. Since its arrival aboard NASA's Hubble Space Telescope
15-and-a-half years ago, the baby grand piano-sized camera has been collecting and
analyzing the photons of deep space, and redefining our cosmos.

"The WFPC2 image I remember most is of the Eagle Nebula," said Ed Weiler, acting
assistant administrator for NASA's Science Mission Directorate in Washington. "It has
these pillars of gas and dust that are trillions of miles long. You know there are new stars
and planets being formed in there, and the colors are just so intriguing. But what really got
me was not my reaction to the picture, but the reaction of the American public."

Imaged by the camera on April 1, 1995, the Eagle Nebula, 7,000 light-years away, is
composed of dense, towering clusters of interstellar hydrogen, oxygen and sulfur.
Emerging from these towers of cosmic material can be seen newborn stars. It is, in
essence, an interstellar nursery.

"After we released the image during a press conference, CNN continued to cover the
story live," said Weiler. "People felt compelled to call in with their reactions to this one
picture. They were seeing the faces of famous people. One person thought he saw Elvis.
Others called it the pillars of creation. I mean this picture touched Americans in a way I
have never seen an astronomical picture do."

Another famous portrait by the camera reached out and touched people by peering back
almost to the very beginning of the universe itself.

"The original Hubble Deep Field was the deepest image mankind had ever taken out
across the universe, literally back in time," said Dave Leckrone, senior project scientist at
NASA Goddard Space Flight Center, Greenbelt, Md. "That was the first time we really
drove the Hubble Space Telescope to its limits in terms of its ability to see extremely faint
objects extremely far away."

Over 10 consecutive days in December 1995, Hubble and the Wide Field and Planetary
Camera 2 stared at a speck of sky no bigger than a grain of sand held at arm's length.
Soaking in the paltry traces of light (four-billion times fainter than can be seen by the
human eye), the camera generated 342 separate images. When all 342 were combined,
the resulting image pulled back the curtain on a part of the universe no one had seen
before and few had imagined.

"You have got to appreciate that the Hubble Deep Field was taken of a part of the sky
that was purposefully chosen to be as empty as people could imagine," said Leckrone.
"Astronomers looked at ground-based images of that little part of the sky and said it was
basically black - there wasn't anything there. And then you take this Hubble Deep Field
and suddenly you see that it is not empty at all. It is filled with thousands of galaxies of
every kind imaginable.

"It was just so beautiful," Leckrone added. It produced an emotional response in people
saying we are part of something bigger, and more complicated and more beautiful than
we ever thought before as human beings."

"One of my personal favorites is of a planetary nebula called MyCn18," said Trauger.
"This image has been widely reproduced in settings as diverse as the cover of National
Geographic [April 1997] and the cover of Pearl Jam's "Binaural" CD.

The hourglass-shaped nebula has an intricate pattern of "etchings" in its walls. A
planetary nebula is the glowing relic of a dying, sun-like star. Scientists theorize the
hourglass-shape of this particular nebula is produced by the expansion of a fast stellar
wind within a slowly expanding cloud of interstellar gas, which is denser near its equator
than its poles.

While the star in one of Trauger's favorite images may be dying, the camera itself is not.
With more than 185,000 images of the cosmos under its belt, the Wide Field and
Planetary Camera 2 is providing the kind of art astronomers, scientists and other people
around the world love, right up to the end. And as much as he values his camera's time in
the spotlight, the principal investigator knows when to put the brushes away.

"That camera is the grandpa, the oldest, longest-lasting instrument aboard Hubble," said
John Trauger. "But with all that history comes its fair share of radiation damage and plain
old obsolescence. It is tired, it is time for it to be brought home."

The camera replacing it, the Wide Field Camera 3, is equipped with state-of-the-art
detectors and optics. The new imager is expected to improve Hubble's discovery
efficiency and extend its outstanding imaging performance.

"We can only guess what that new camera will discover," said Trauger. "But history tells
us that every increase in our reach will uncover new wonders. We will learn still more
about the life cycles of galaxies, stars and planetary systems, and the unique
astronomical setting of our Earth, and to me that means a lot. WFPC2 helped us see the
light."

The Wide Field and Planetary Camera 2 was designed and built by NASA's Jet
Propulsion Laboratory.

-end-


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If Spitzer Could Talk: An Interview with NASA's Coolest Space Telescope

Feature May 5, 2009

A Universal Art Form - NASA's Wide Field and Planetary Camera 2


Throughout history, humanity has been moved by the work of the great artists of
their age. Wielding brush, chisel or baton, these masters of expression have
been able to interpret the environment around them in innovative ways,
providing their public new avenues to explore their own senses and emotions.
But as with so many career fields, the role and tools of the artisan are changing.

NASA's Wide Field and Planetary Camera 2 (WFPC2) is one such new tool of
artistic expression. The name may be unfamiliar to you, but more likely than not,
you know of -- and have been moved by -- its iconic tableaus. For this camera is
the implement by which humans first bore witness to some of the most inspiring
and thought provoking vistas in the known universe.

"I cannot tell you how many times I have heard people tell me how much this
picture or that image has meant to them," said John Trauger, principal
investigator of the Wide Field and Planetary Camera 2 at NASA's Jet Propulsion
Laboratory in Pasadena, Calif. "After a while, I began to realize what we have
achieved reached beyond the scope of pure science and became something
more."

Born as a clone, a safeguard, to be used only in the most dire circumstances,
WFPC2 was employed under exactly those conditions. Since its arrival aboard
NASA's Hubble Space Telescope 15-and-a-half years ago, the baby grand
piano-sized camera has been collecting and analyzing the photons of deep
space, and redefining our cosmos.

"The WFPC2 image I remember most is of the Eagle Nebula," said Ed Weiler,
associate administrator for NASA's Science Mission Directorate in Washington.
"It has these pillars of gas and dust that are trillions of miles long. You know
there are new stars and planets being formed in there, and the colors are just so
intriguing. But what really got me was not my reaction to the picture, but the
reaction of the American public."

Imaged by WFPC2 on April 1, 1995, the Eagle Nebula, 7,000 light-years away, is
composed of dense, towering clusters of interstellar hydrogen, oxygen and
sulfur. Emerging from these towers of cosmic material can be seen newborn
stars. It is, in essence, an interstellar nursery.

"After we released the image during a press conference, CNN continued to
cover the story live," said Weiler. "People felt compelled to call in with their
reactions to this one picture. They were seeing the faces of famous people. One
person thought he saw Elvis. Others called it the pillars of creation. I mean this
picture touched Americans in a way I have never seen an astronomical picture
do."

Another famous WFPC2 portrait reached out and touched people by peering
back almost to the very beginning of the universe itself.

"The original Hubble Deep Field was the deepest image mankind had ever
taken out across the universe, literally back in time," said Dave Leckrone, senior
project scientist at the Space Telescope Science Institute, Baltimore, Md. "That
was the first time we really drove the Hubble Space Telescope to its limits in
terms of its ability to see extremely faint objects extremely far away."

Over 10 consecutive days in December 1995, Hubble and WFPC2 stared at a
speck of sky no bigger than a grain of sand held at arm's length. Soaking in the
paltry traces of light (four-billion times fainter than can be seen by the human
eye), WFPC2 generated 342 separate images. When all 342 were combined,
the resulting image pulled back the curtain on a part of the universe no one had
seen before and few had imagined.

"You have got to appreciate that the Hubble Deep Field was taken of a part of
the sky that was purposefully chosen to be as empty as people could imagine,"
said Leckrone. "Astronomers looked at ground-based images of that little part of
the sky and said it was basically black - there wasn't anything there. And then
you take this Hubble Deep Field and suddenly you see that it is not empty at all.
It is filled with thousands of galaxies of every kind imaginable.

"It was just so beautiful," Leckrone added. It produced an emotional response in
people saying we are part of something bigger, and more complicated and more
beautiful than we ever thought before as human beings."

"One of my personal favorites is of a planetary nebula called MyCn18," said
Trauger. "This WFPC2 image has been widely reproduced in settings as
diverse as the cover of National Geographic [April 1997] and the cover of Pearl
Jam's "Binaural" CD.

The hourglass-shaped nebula has an intricate pattern of "etchings" in its walls.
A planetary nebula is the glowing relic of a dying, sun-like star. Scientists
theorize the hourglass-shape of this particular nebula is produced by the
expansion of a fast stellar wind within a slowly expanding cloud of interstellar
gas, which is denser near its equator than its poles.

While the star in one of Trauger's favorite images may be dying, the camera
itself is not. With more than 185,000 images of the cosmos under its belt,
WFPC2 is providing the kind of art astronomers, scientists and other people
around the world love, right up to the end. And as much as he values his
camera's time in the spotlight, the principal investigator for WFPC2 knows when
to put the brushes away.

"That camera is the grandpa, the oldest, longest-lasting instrument aboard
Hubble," said John Trauger. "But with all that history comes its fair share of
radiation damage and plain old obsolescence. It is tired, it is time for it to be
brought home."

The camera replacing WFPC2, the Wide Field Camera 3, is equipped with state-
of-the-art detectors and optics. The new imager is expected to improve Hubble's
discovery efficiency and extend its outstanding imaging performance.

"We can only guess what that new camera will discover," said Trauger. "But
history tells us that every increase in our reach will uncover new wonders. We
will learn still more about the life cycles of galaxies, stars and planetary systems,
and the unique astronomical setting of our Earth, and to me that means a lot.
WFPC2 helped us see the light."

The Wide Field and Planetary Camera 2 was designed and built by NASA's Jet
Propulsion Laboratory.

-end-


1

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