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Atlantis to hangar
After its safe landing to end mission STS-115, space shuttle Atlantis is towed from the Kennedy Space Center runway to hangar 1 of the Orbiter Processing Facility for post-flight deservicing and the start of preparations leading to its next mission, STS-117.

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STS-115 landing
Space shuttle Atlantis glides to a smooth touchdown on Kennedy Space Center's Runway 33 at 6:21 a.m. to conclude the successful STS-115 mission that restarted construction of the space station.

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Soyuz TMA-9 docking
The Russian Soyuz TMA-9 space capsule carrying the Expedition 14 resident crew and space tourist Anousheh Ansari safely docks to the International Space Station's Zvezda service module.

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Expedition 14 launch
This extended duration movie follows the Soyuz rocket from the final countdown through arrival in orbit with the Expedition 14 crew. The video shows the three-stage rocket's ascent from Baikonur Cosmodrome and includes views of Mike Lopez-Alegria, Mikhail Tyurin and Anousheh Ansari from cameras inside the capsule.

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Mission of Expedition 14
The voyage of Expedition 14 aboard the International Space Station is expected to see major construction activities for the outpost. Learn more about the mission in this narrated mission preview movie.

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STS-31: Opening window to the Universe
The Hubble Space Telescope has become astronomy's crown jewel for knowledge and discovery. The great observatory was placed high above Earth following its launch aboard space shuttle Discovery on April 24, 1990. The astronauts of STS-31 recount their mission in this post-flight film presentation.

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STS-34: Galileo launch
The long voyage of exploration to Jupiter and its many moons by the Galileo spacecraft began on October 18, 1989 with launch from Kennedy Space Center aboard the space shuttle Atlantis. The crew of mission STS-34 tell the story of their flight to dispatch the probe -- fitted with an Inertial Upper Stage rocket motor -- during this post-flight presentation film.

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Planets prefer safe neighborhoods, Spitzer finds
UNIVERSITY OF ARIZONA NEWS RELEASE Posted: October 3, 2006
A star must live in a relatively tranquil cosmic neighborhood to foster planet formation, say astronomers using NASA's Spitzer Space Telescope.

The potential planet-forming disk of a sun-like star is being violently ripped away by the powerful winds of a nearby hot O-type star in this image from Spitzer. At up to 100 times the mass of sun-like stars, O stars are the most massive and energetic stars in the universe. The O star can be seen to the right of the image, as the large orange spot with the white center. To the left, the comet like structure is actually a neighboring solar system that is being destroyed by the O star's powerful winds and intense ultraviolet light. Credit: NASA/JPL-Caltech/Z. Balog (Univ. of Ariz./Univ. of Szeged) Download larger image version here
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A team of scientists from the University of Arizona's Steward Observatory,
Tucson, came to this conclusion after watching intense ultraviolet light and
powerful winds from O-type stars rip away the potential planet-forming
disks, or protoplanetary disks, around stars like our sun. At up to 100
times the mass of the sun, O stars are the most massive and energetic stars
in the universe. They are at least a million times more powerful than the
sun.
According to Zoltan Balog, lead author of the team's paper, the
super-sensitive infrared eyes of Spitzer are ideal for capturing the
"photoevaporation" of these planet-forming disks. In this process, immense
output from the O star heats the disks that are surrounding nearby sun-like
stars so much that gas and dust boil off (much like the evaporation of
boiling water), and the disk can no longer hold together. Photon (or light)
blasts from the O star then blow away the evaporated material, potentially
stripping the sun-like stars of their ability to form planets.
"We can see that these systems take on a cometary structure as they are
being blown away and destroyed," Balog said.
"No other telescope has ever captured the photoevaporation of a
protoplanetary disk in this much detail," added Kate Su, who is a co-author
on Balog's paper.
The photoevaporation process is very similar to the one that forms the tail
of a comet as it swings by the inner solar system, only a lot more violent
and on a far larger scale, Su said.
"Every time a particle of light from the O star hits a dust grain in the
nearby protoplanetary disk, the light particle pushes the dust grain away
from its host star," Su said. "This is very similar to how comet tails
form."
"Unfortunately these sun-like stars just got a little too close to the
fire," UA Regents Professor George Rieke said. Rieke is also a co-author on
the paper and the principal investigator for Spitzer's Multiband Imaging
Photometer (MIPS) instrument, which made the new observations.
Ultimately, the astronomers hope to determine whether all stars have
planets, and if not, how a star loses the ability to form them. The Spitzer
findings will help astronomers understand what regulates the process of
planet formation.
Team members say that originally they were looking for "diskless stars" in
their survey, stars that had ventured too close to an O star and no longer
had any disk left. With so many O stars in the region, they didn't expect
that a protoplanetary disk would survive for very long. However, they found
something different - stars that had recently blundered into the hostile
neighborhood of an O star and were still in the process of losing their
disks.
"To see protoplanetary disks in an area where no one expected to see one is
very exciting," Balog said. "But to see a disk in the process of evaporating
is even more thrilling."
Balog's paper was recently accepted for publication in Astrophysical
Journal. He is currently is at the University of Arizona on leave from the
Department of Optics and Quantum Electronics, University of Szeged, Hungary.
UA astronomers James Muzerolle and Erick T. Young collaborated with Balog,
Rieke and Su in the observations.
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