Thursday, May 3

NASA Assigns Washington, D.C., Native to Upcoming Shuttle Mission

May 3, 2007

Katherine Trinidad
Headquarters, Washington
202-358-3749

James Hartsfield
Johnson Space Center, Houston
281-483-5111

RELEASE: 07-99

NASA ASSIGNS WASHINGTON, D.C., NATIVE TO UPCOMING SHUTTLE MISSION

WASHINGTON - NASA astronaut and Air Force Col. Benjamin Alvin Drew
will join the crew of the STS-118 space shuttle mission, targeted for
launch Aug. 9.

Drew, born in Washington, will take a seat that opened when astronaut
Clayton Anderson was moved to shuttle Atlantis' STS-117 flight, which
is targeted to launch June 8. Anderson will begin a long-duration
mission on the International Space Station, and current station crew
member Suni Williams will return to Earth aboard Atlantis.

Shuttle Endeavour will carry Drew on his first spaceflight. He will
serve as a mission specialist during STS-118, which will deliver
another segment to continue building the station by 2010. Navy Cmdr.
Scott Kelly will serve as STS-118's commander, and Marine Corps Lt.
Col. Charles Hobaugh will be the pilot. Mission specialists are Tracy
Caldwell, Ph.D., Rick Mastracchio, Barbara Morgan, the first educator
astronaut, and Canadian Space Agency astronaut Dr. Dave Williams.

Drew received bachelor's degrees in astronautical engineering and
physics from the United States Air Force Academy, Colorado Springs,
Colo., in 1984; a master's degree in aerospace science from Embry
Riddle University, Daytona Beach, Fla., in 1995; and a master's
degree in strategic studies in political science from the Air Force
Air University, Maxwell Air Force Base, Ala., in 2006. He received
his commission as a second lieutenant in the Air Force in May 1984.
He completed helicopter pilot training and flew combat missions in
operations Just Cause, Desert Shield, Desert Storm and Provide
Comfort. Drew was selected as an astronaut in 2000.

Training video of Drew will air on NASA TV's Video File. For downlink
and scheduling information and links to streaming video, visit:

http://www.nasa.gov/ntv


For more about the STS-118 crew and mission, visit:

http://www.nasa.gov/shuttle


www.nasa.gov/shuttle



-end-

To subscribe to the list, send a message to:
hqnews-subscribe@mediaservices.nasa.gov
To remove your address from the list, send a message to:
hqnews-unsubscribe@mediaservices.nasa.gov

Wednesday, May 2

NASA Supports Train-Derailment Recovery in Alabama

May 2, 2007

Katherine Trinidad
Headquarters, Washington
202-358-3749

Kyle Herring
Johnson Space Center, Houston
281-483-5111

RELEASE: 07-97

NASA SUPPORTS TRAIN-DERAILMENT RECOVERY IN ALABAMA

WASHINGTON - Officials from NASA and ATK Launch Systems, Edina, Minn.,
are assisting the Federal Railroad Administration during its
investigation of a train derailment Wednesday morning near
Pennington, Ala. The train was carrying space shuttle reusable solid
rocket motor segments from the ATK Launch Systems manufacturing site
in Brigham City, Utah, to NASA's Kennedy Space Center, Fla.

"Several members of the NASA family were injured in this serious
accident. Today our prayers are for those who have been injured and
their families. Our employees work in hazardous jobs every day, and
it is our goal to keep them safe," said NASA's Space Shuttle Program
Manager Wayne Hale.

The special train carrying only solid rocket motor segments and a
passenger car to monitor their transportation was crossing a bridge
or a trestle, which collapsed under the locomotives. Six people were
injured when the two locomotives and the passenger car dropped about
10 feet and turned on their sides.

One of the cars carrying a solid rocket motor segment is also on its
side. The remaining cars containing seven solid rocket motor segments
and two aft exit cone segments are upright.

The hardware was intended for use on shuttle Discovery's STS-120
mission in October and shuttle Atlantis's STS-122 mission in
December. These segments are interchangeable, and ATK Launch Systems
has replacement units that could be used for the shuttle flights, if
necessary.

Each segment weighs approximately 300,000 lbs. and is protected by a
white or yellow colored fiberglass cover during shipment. The
condition of the rocket motor segments will be assessed as soon as
teams conduct a full inspection. Solid Rocket Motor segments have
been transported across country by rail for more than 26 years with
an excellent record of safe transportation. For information about the
Space Shuttle Program, visit:

www.nasa.gov/shuttle



-end-

To subscribe to the list, send a message to:
hqnews-subscribe@mediaservices.nasa.gov
To remove your address from the list, send a message to:
hqnews-unsubscribe@mediaservices.nasa.gov

NASA to Announce Extraordinary Stellar Discovery

May 2, 2007

Grey Hautaluoma
Headquarters, Washington
202-358-0668

Megan Watzke
Chandra X-ray Center, Cambridge, Mass.
617-496-7998

MEDIA ADVISORY: M07-46

NASA TO ANNOUNCE EXTRAORDINARY STELLAR DISCOVERY

WASHINGTON - At a NASA Science Update Monday, May 7, at 2 p.m. EDT,
astronomers will announce new findings about a record-breaking
stellar event discovered using NASA's Chandra X-ray Observatory. The
event will be held in the auditorium at NASA Headquarters, 300 E St.,
S.W., in Washington and will be broadcast live on NASA Television and
streamed at http://www.nasa.gov.

Media at participating NASA centers will have the opportunity to ask
questions.

The Chandra X-ray Observatory is the world's most powerful X-ray
telescope. Chandra is designed to observe X-rays from high-energy
regions of the universe, such as the remnants of exploded stars.
Along with the Hubble Space Telescope, the Spitzer Space Telescope,
and the now de-orbited Compton Gamma Ray Observatory, Chandra is one
of NASA's "Great Observatories."

The Smithsonian Astrophysical Observatory in Cambridge, Mass., is
responsible for the day-to-day ?ight operations and science
activities for Chandra from the Operations Control Center and Chandra
X-ray Center facilities.

For more information about NASA TV, streaming video, downlink and
schedule information, visit:

http://www.nasa.gov/ntv

For more information about the Chandra X-ray Observatory, visit:

http://www.nasa.gov/chandra


-end-

To subscribe to the list, send a message to:
hqnews-subscribe@mediaservices.nasa.gov
To remove your address from the list, send a message to:
hqnews-unsubscribe@mediaservices.nasa.gov

New Technologies for James Webb Space Telescope Approved Early

May 2, 2007

Grey Hautaluoma
Headquarters, Washington
202-358-0668

Rob Gutro
Goddard Space Flight Center, Greenbelt, Md.
301-286-4044

RELEASE: 07-96

NEW TECHNOLOGIES FOR JAMES WEBB SPACE TELESCOPE APPROVED EARLY

WASHINGTON - More than a year ahead of schedule, a team of independent
experts has approved all ten new technologies developed for NASA's
James Webb Space Telescope. Many of the technologies are
revolutionary and have never before been used on any satellite or
space telescope. The early approval can reduce the risk of increased
costs and schedule delays before the program is approved for further
development.

NASA commissioned the team of engineers, scientists and project
managers to conduct the technical review. The group evaluated the
telescope's near and mid-infrared detectors, sunshield materials,
lightweight cryogenic mirrors, microshutter arrays, cryogenic
detector readout application-specific integrated circuits, cryogenic
heat switches, a large precision cryogenic structure, a cryocooler
for the mid-infrared instrument, and wavefront sensing and control.
They determined the technologies were tested successfully in a
space-like environment and are mature enough to include on the
telescope's upcoming mission.

The actual hardware and software that will fly on the telescope now
can be engineered from working prototypes. These technologies will
allow the observatory to peer back in time to about 400 million years
after the Big Bang, enabling scientists to study the first generation
of stars and galaxies.

"The technology non-advocate review was our attempt to address one
common problem that NASA missions encounter that leads to cost
growth," said Eric Smith, Webb program scientist at NASA
Headquarters, Washington. "That problem is late maturation of
technology in a program's life-cycle. By conducting an external
review of our technologies more than a year ahead of the Preliminary
Design Review - when they are traditionally examined - we hope to
better manage that aspect of the program's costs."

Two examples of the new technologies are the microshutter arrays and
wavefront sensing and control.

Microshutters are tiny doorways, the width of a few hairs, that will
allow scientists to remotely and systematically block out unwanted
light and view the most distant stars and galaxies ever seen. The
telescope will be the first project to employ this technology.

Through a process called wavefront sensing and control, a set of
algorithms and software programs, the optimum position of each of the
telescope mirrors will be computed, and the positions will be
adjusted as necessary, causing the individual mirrors to function as
one very sensitive telescope.

"At the inception of the James Webb Space Telescope program, NASA
adopted a strategy of making significant, early investments in the
development of the diverse and challenging new technologies needed to
conduct the mission," said Phil Sabelhaus, project manager at
Goddard. "Receiving the review board's confirmation that we have met
the goal more than a year early for all of our new technologies is a
major accomplishment for our team and a tribute to the benefits of
the early investment strategy," Sabelhaus said.

Northrop Grumman Corporation, Redondo Beach, Calif.; Ball Aerospace
Corporation, Boulder, Colo.; Teledyne Imaging Systems, Thousand Oaks,
Calif.; Utah State University's Space Dynamics Lab, North Logan,
Utah; Raytheon Vision Systems, Santa Barbara, Calif.; Alliant
Techsystems, Magna, Utah; and Sheldahl, Northfield, Minn., worked
with NASA Goddard Space Flight Center, Greenbelt, Md., on these and
other technologies.

The James Webb Space Telescope is expected to launch in 2013. The
telescope is a joint project of NASA, the European Space Agency and
the Canadian Space Agency.

For more information about the James Webb Space Telescope, visit:

http://www.jwst.nasa.gov

For related images on this story, visit:

http://www.nasa.gov/vision/universe/starsgalaxies/webb_technologies.html

-end-


-end-

To subscribe to the list, send a message to:
hqnews-subscribe@mediaservices.nasa.gov
To remove your address from the list, send a message to:
hqnews-unsubscribe@mediaservices.nasa.gov

NASA Briefing at Full-Sized James Webb Space Telescope Model

May 2, 2007

Grey Hauatluoma
Headquarters, Washington
202-358-0668

MEDIA ADVISORY: M07-45

NASA BRIEFING AT FULL-SIZED JAMES WEBB SPACE TELESCOPE MODEL

WASHINGTON - Media are invited to a briefing about NASA's James Webb
Space Telescope on Thursday, May 10 from 10-11 a.m. EDT. Attendees
will have an opportunity to see a full-scale model of NASA's
next-generation space telescope and examine its hexagonal mirror and
five-layer sunshield. The briefing will take place next to the
telescope model on display at the National Mall, between the
Smithsonian National Air and Space Museum and the National Gallery of
Art, Washington.

Experts will discuss the telescope's mission in deep space, its role
in NASA's space exploration program and current construction
progress. Participants are:

Edward Weiler, director, NASA's Goddard Space Flight Center,
Greenbelt, Md.

Matt Mountain, director, Space Telescope Science Institute, Baltimore

Martin Mohan, Webb Telescope program manager, Northrop Grumman Space
Technology, Redondo Beach, Calif.

To attend, contact Grey Hautaluoma, NASA Headquarters, Washington,
202-358-0668, grey.hautaluoma-1@nasa.gov or Sally Koris, Northrop
Grumman Space Technology, 310-812-4721, sally.koris@ngc.com.

The James Webb Space Telescope is a 21st century space observatory
that will peer back nearly 13 billion years in time to understand the
evolution of our own solar system and the formation of galaxies,
stars and planets. It is expected to launch in 2013. The telescope is
a joint project of NASA, the European Space Agency and the Canadian
Space Agency.

The model is on display in conjunction with Public Service Recognition
Week, sponsored by the Council for Excellence in Government.

For more information about the James Webb Space Telescope, visit:

http://www.jwst.nasa.gov


-end-

To subscribe to the list, send a message to:
hqnews-subscribe@mediaservices.nasa.gov
To remove your address from the list, send a message to:
hqnews-unsubscribe@mediaservices.nasa.gov

Tuesday, May 1

On Trip to Mars, NASA Must Rethink Death

Mars


On Trip to Mars, NASA Must Rethink Death from PhysOrg.com

(AP) -- How do you get rid of the body of a dead astronaut on a three-year mission to Mars and back????

Pluto-Bound New Horizons Provides New Look at Jupiter System

May 1, 2007

Dwayne Brown
Headquarters, Washington
202-358-1726

Michael Buckley
Johns Hopkins University Applied Physics Laboratory, Laurel, Md.
240-228-7536

RELEASE: 07-95

PLUTO-BOUND NEW HORIZONS PROVIDES NEW LOOK AT JUPITER SYSTEM

WASHINGTON - NASA's New Horizons spacecraft has provided new data on
the Jupiter system, stunning scientists with never-before-seen
perspectives of the giant planet's atmosphere, rings, moons and
magnetosphere.

These new views include the closest look yet at the Earth-sized
"Little Red Spot" storm churning materials through Jupiter's cloud
tops; detailed images of small satellites herding dust and boulders
through Jupiter's faint rings; and of volcanic eruptions and circular
grooves on the planet's largest moons.

New Horizons came to within 1.4 million miles of Jupiter on Feb. 28,
using the planet's gravity to trim three years from its travel time
to Pluto. For several weeks before and after this closest approach,
the piano-sized robotic probe trained its seven cameras and sensors
on Jupiter and its four largest moons, storing data from nearly 700
observations on its digital recorders and gradually sending that
information back to Earth. About 70 percent of the expected 34
gigabits of data has come back so far, radioed to NASA's largest
antennas over more than 600 million miles. This activity confirmed
the successful testing of the instruments and operating software the
spacecraft will use at Pluto.

"Aside from setting up our 2015 arrival at Pluto, the Jupiter flyby
was a stress test of our spacecraft and team, and both passed with
very high marks," said Science Mission Directorate Associate
Administrator and New Horizons Principal Investigator Alan Stern,
NASA Headquarters, Washington. "We'll be analyzing this data for
months to come; we have collected spectacular scientific products as
well as evocative images."

Images include the first close-up scans of the Little Red Spot,
Jupiter's second-largest storm, which formed when three smaller
storms merged during the past decade. The storm, about half the size
of Jupiter's larger Great Red Spot and about 70 percent of Earth's
diameter, began turning red about a year before New Horizons flew
past it. Scientists will search for clues about how these systems
form and why they change colors in their close observations of
materials spinning within and around the nascent storm.

"This is our best look ever of a storm like this in its infancy," said
Hal Weaver, New Horizons project scientist from the Johns Hopkins
University Applied Physics Laboratory (APL), Laurel, Md. APL built
and operates the New Horizons spacecraft. "Combined with data from
telescopes on and around Earth taken at the same time New Horizons
sped past Jupiter, we're getting an incredible look at the dynamics
of weather on giant planets."

Under a range of lighting and viewing angles, New Horizons also
grabbed the clearest images ever of the tenuous Jovian ring system.
In them, scientists spotted a series of unexpected arcs and clumps of
dust, indicative of a recent impact into the ring by a small object.
Movies made from New Horizons images also provide an unprecedented
look at ring dynamics, with the tiny inner moons Metis and Adrastea
appearing to shepherd the materials around the rings.

"We're starting to see that rings can evolve rapidly, with changes
detectable during weeks and months," said Jeff Moore, New Horizons
Jupiter Encounter science team lead from NASA Ames Research Center,
Moffett Field, Calif. "We've seen similar phenomena in the rings of
Saturn."

Of Jupiter's four largest moons, the team focused much attention on
volcanic Io, the most geologically active body in the solar system.
New Horizons' cameras captured pockets of bright, glowing lava
scattered across the surface; dozens of small, glowing spots of gas;
and several fortuitous views of a sunlit umbrella-shaped dust plume
rising 200 miles into space from the volcano Tvashtar, the best
images yet of a giant eruption from the tortured volcanic moon.

The timing and location of the spacecraft's trajectory also allowed it
to spy many of the mysterious, circular troughs carved onto the icy
moon Europa. Data on the size, depth and distribution of these
troughs, discovered by the Jupiter-orbiting Galileo mission, will
help scientists determine the thickness of the ice shell that covers
Europa's global ocean.

Already the fastest spacecraft ever launched, New Horizons reached
Jupiter 13 months after lifting off from Cape Canaveral Air Force
Station, Fla., in January 2006. The flyby added 9,000 miles per hour,
pushing New Horizons past 50,000 miles per hour and setting up a
flight by Pluto in July 2015.

The number of observations at Jupiter was twice that of those planned
at Pluto. New Horizons made most of these observations during the
spacecraft's closest approach to the planet, which was guided by more
than 40,000 separate commands in the onboard computer.

"We can run simulations and take test images of stars, and learn that
things would probably work fine at Pluto," said John Spencer, deputy
lead of the New Horizons Jupiter Encounter Science Team, Southwest
Research Institute, Boulder, Colo. "But having a planet to look at
and lots of data to dig into tells us that the spacecraft and team
can do all these amazing things. We might not have explored the full
capabilities of the spacecraft if we didn't have this real planetary
flyby to push the system and get our imaginations going."

More data are to come, as New Horizons completes its unprecedented
flight down Jupiter's long magnetotail, where it will analyze the
intensities of sun-charged particles that flow hundreds of millions
of miles beyond the giant planet.

New Horizons is the first mission in NASA's New Frontiers Program of
medium-class spacecraft exploration projects. Stern leads the mission
and science team as principal investigator; APL manages the mission
for NASA's Science Mission Directorate. The mission team also
includes Ball Aerospace Corp., Boulder, Colo; the Boeing Company,
Chicago; NASA's Goddard Space Flight Center, Greenbelt, Md.;NASA's
Jet Propulsion Laboratory, Pasadena, Calif.; Stanford University,
Palo Alto, Calif.; KinetX, Inc., Simi Valley, Calif.; Lockheed Martin
Corp.; Denver; University of Colorado, Boulder; the U.S. Department
of Energy, Washington; and a number of other firms, NASA centers, and
university partners.

To view the new images visit:

www.nasa.gov/newhorizons



-end-

To subscribe to the list, send a message to:
hqnews-subscribe@mediaservices.nasa.gov
To remove your address from the list, send a message to:
hqnews-unsubscribe@mediaservices.nasa.gov