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Animation Identification Numbers 10300 through 10399



Movie ID Title
Close in as a Neutron Star emits a Gamma Ray Burst.   10300   Neutron Stars - A Closer Perspective:
Ace Spacecraft   10301   ACE - shockwave
Chipsat passes along the equator   10302   Chipsat Spacecraft
Lunar Eclipse   10303   Lunar Eclipse
Gro burns up   10305   Gamma Ray Observatory - Atmospheric Burnup
RHESSI over Earth   10306   RHESSI Spacecraft
Polar Spacecraft in orbit   10307   POLAR Spacecraft in orbit
WMAP heading away from Earth   10308   WMAP Spacecraft
NGTDRS in orbit   10309   Next Generation TDRS Spacecraft
QUIKToms in orbit   10310   QUIKToms Spacecraft
  10311   Spartan 201
A step by step walkthrough of the Boomerang mission from launch to return of the sample capsule   10312   LEX / Boomerang Mission
Lisa - 3 satellites in orbit   10314   Lisa - Print Still Image - Wallpaper
  10315   Cloudsat - Prints Still Images - Wallpaper
Print 1   10316   Calipso - Print Still Images - Wallpaper
Print 1   10317   Aura - Print Still Images - Wallpaper
<b> 1. Hubble Space Telescope Service Mission 4 Animation: </b> A collection of several animations showing the Hubble Space Telescope orbiting Earth and in space shuttle Atlantis cargo bay. All animations depict the Hubble Space Telescope in its current (July 2008) configuration.   10318   HST SM4 Extended Resource Reel v2.0
print1   10320   AIM - Print Still Images - Wallpaper
<b>1. Hubble Space Telescope Service Mission 4 Animation:</b> A collection of several animations showing the Hubble Space Telescope orbiting Earth and in space shuttle Atlantis cargo bay. All animations depict the Hubble Space Telescope in its current (July 2008) configuration.   10321   HST SM4 Resource Reel v2.0
Selected soundbites with Steve Ritz, GLAST Project Scientist (NASA/GSFC)   10322   GLAST Soundbites
NASA's Swift and GLAST satellites will work together to better understand the high energy universe. <p>For complete transcript, click <a href='GLASTcast_Episode3.htm'>here</a>.   10323   GLASTCast Episode 3 - Swift and GLAST
The hopes and anticipations of the GLAST team as they prepare for launch. <p>For complete transcript, click <a href='GLASTcast_Episode4_transcript.htm'>here</a>.   10324   GLASTcast Episode 4: Launching a Spacecraft
Meet the major U.S. players behind the GLAST mission. <p> <p>For complete transcript, click <a href='GLASTcast_Episode5.htm'>here</a>.   10325   GLASTcast Episode 5: Meet the U.S. Team
<b><font size='-1'>A 30 Foot Cable for Laser Ranging</font></b><br/><br/>This fiber optic cable attaches to the back of the Laser Ranging Telescope at the end of the High Gain Antenna boom. It actually has three segments that connect to each other. The first two segments are used to transfer the lights from the back of the telescope to the bottom of the boom. The third segment is used to transfer the light from the bottom of the boom to the LOLA instrument. This cable was carefully handmade at NASA’s Goddard Space Flight Center in Greenbelt, MD.<br/>   10326   Assembly and Testing of the Lunar Reconnaissance Orbiter (LRO)
This animation shows an astronauts gloved hand reaching out and touching the aft shroud area of the Hubble Space Telescope as if to say, “Hello, old friend.”   10327   Astronaut Touches Hubble Animation
<b>Fine Guidance Sensor Installation EVA </b> completed and edited animation sequence.   10328   Fine Guidance Sensor Installation EVA Animation
<b>HST SM4 Rendezvous and Capture </b> completed and edited animation sequence.   10329   HST SM4 Rendezvous and Capture Sequence
<b>HST SM4 New Outer Blanket Layer (NOBL) Installation EVA </b> completed and edited animation sequence.   10330   New Outer Blanket Layer (NOBL) Installation EVA Animation
The Lunar Reconnaissance Orbiter or LRO will give scientists more information about the structure of the Moon’s interior; the types of rock found there, events that shaped it, and the conditions that exist at the surface. LRO will spend one year in a polar orbit collecting this information. LRO's instrument suite will provide the highest resolution and the most comprehensive data set and the most detailed maps ever returned from the moon. It will carry an additional payload called LCROSS. The identification of water is very important to the future of human activities on the Moon. LCROSS will excavate the permanently dark floor of one of the Moon’s polar craters with two heavy impactors to test the theory that ancient ice lies buried there. The impact will eject material from the crater’s surface to create a plume that specialized instruments will be able to analyze for the presence of water (ice and vapor), hydrocarbons and hydrated material. <br/>   10334   Launch, Deploy, and Misson Animation
LRO will be launched via an Atlas V 401 rocket from Cape Canaveral Air Force Station in Florida. It will take approximately four days for the satellite to travel to and then enter the moon's orbit. This video is from the launch of the MOR Mission. The Lunar Reconnaissance Orbiter or LRO will give scientists more information about the structure of the Moon’s interior; the types of rock found there, events that shaped it, and the conditions that exist at the surface.   10335   The Atlas V Rocket Is Readied
<p>The Autonomous Star Trackers provide attitude data and motion rate of the satellite. They are based on a radiation hardened design and proprietary algorithms that ensure accurate and robust 3-axes attitude determination. These same instruments most recently flew onboard NASA's Messenger and Mars Reconnaissance Orbiter missions. For complete transcript, click <a href='script_657_00.html'>here</a>.   10336   StarTrackers Light the Way
Introduction: This gives a brief overview of the concepts behind the Engineering Design Process and outlines the goals of the series.   10341   BEST: Engineering Design Process Professional Development Series
GLAST Prelude<p><p>Celebrating the launch and science of NASA's Gamma-Ray Large Area Space Telescope.   10345   GLASTcast in HD for Apple TV and iTunes
Hubble Space Telescope Servicing Mission 4 is the last time humans will visit Hubble. NASA’s scientists, engineers and astronauts are working together to make Hubble better than it has been before. See what NASA has planned for this last mission to Hubble; from new science instruments, to two challenging and never-done-before instrument repairs, and numerous upgrades.<p><p><p>For complete transcript, click <a href='script_719_01.html'>here</a>.   10346   The Last Mission to Hubble
Orthographic Map<p><p>Astronomers wrapped the Fermi Gamma-ray Space Telescope's first all-sky map over a sphere to produce this view of the gamma-ray universe. The globe in this animation rotates showing the galactic plane and the north galactic pole, then tilts up to show the south galactic pole region.   10347   GLAST First Light All Sky Map
This short video feature describes how LRO's instruments are used collectively to scout for safe landing sites. The crater depicted in this animation is ficticious and only intended for illustrative purposes.<p><p>For complete transcript, click <a href='LRO_Safe_Landings_transcript.htm'>here</a>.   10349   LRO Scouts for Safe Landing Sites
<b>Space Telescope Imaging Spectrograph </b>(STIS), the most versatile spectrograph ever to fly on Hubble, ceased operations in August 2004 due to the failure of its power supply. In order to restore STIS to operational status, astronauts will perform a never-before-attempted on-orbit replacement of an electronics board inside STIS’s main electronics box. On Earth this operation is relatively simple, but in space many challenges confront the astronauts as they work to replace the failed board including working to remove 111 tiny, non-captive screws with astronaut gloves. <p> <b>The Cosmic Origins Spectrograph </b> (COS) that will be added during Servicing Mission 4, and STIS are highly complementary and are very complimentary to each other providing scientists with a full set of spectroscopic tools for astrophysical research. The STIS instrument’s accomplishments include determining the atmospheric composition of an exoplanet as well as spectra and images at ultraviolet and visible wavelengths of the Universe from our solar system out to cosmological distances. </p><p><p><p><p><p>For complete transcript, click <a href='script_725_01.html'>here</a>.   10350   STIS Repair: The Quest for Renewed Exploration
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