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STS-132 LAUNCH L-3 FINAL PAYLOAD BAY DOOR CLOSURE FOR FLIGHT 2010-3239

KENNEDY SPACE CENTER, Fla. -- Resting inside Atlantis’s payload bay are the Joint Airlock Module (bottom) and pallet containing the high pressure gas assembly (above). Both are heading for the International Space Station on mission STS-104, scheduled to be launched July 12. The module, which comprises a crew lock and an equipment lock, will be connected to the starboard (right) side of Node 1 Unity. Once installed and activated, the Airlock becomes the primary path for Space Station spacewalk entry and departure for U.S. spacesuits, which are known as Extravehicular Mobility Units, or EMUs. In addition, the Joint Airlock is designed to support the Russian Orlan spacesuit for EVA activity. The high pressure gas assembly will support future spacewalk operations from the Space Station and augment the Service Module gas resupply system KSC-01pp1228

SCALING TEST NATIONAL ADVISORY COUNCIL FOR AERONAUTICS 0012 AIR FOIL 10.5 INCH CHORD

History of Hubble Space Telescope (HST)

LDEF (Prelaunch), M0002-01 : Trapped-Proton Energy Spectrum Determination, Tray G12

The fly away saturation system dive bell moves from the deck of a barge into the water where U.S. Navy saturation divers conduct pierside training operations.

16-antenna array (16589934569)

NBL Experimental Photographic Support

BOEING DELTA 4 SHROUD SEPARATION TEST IN SPACE POWER FACILITY AT NASA PLUM BROOK STATION

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KENNEDY SPACE CENTER, FLA. -In the RTG Facility at Kennedy Space Center, Jim Wojciechowski and Dan Brunson lower a metal canister over the radioisotope thermoelectric generator (RTG). The canister will protect the RTG when it is moved. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2440

KENNEDY SPACE CENTER, FLA. - In the RTG Facility at Kennedy Space Center, Jim Wojciechowski and Dan Brunson install a clamping ring onto the radioisotope thermoelectric generator (RTG). Watching at right is Steve Killian. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2438

KENNEDY SPACE CENTER, FLA. - In the RTG Facility at Kennedy Space Center, Tim Hoyle and Mervin Smith check the cable on the radioisotope thermoelectric generator (RTG). The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2433

KENNEDY SPACE CENTER, FLA. - Inside the RTG facility at Kennedy Space Center, Dave Nobles oversees the operation as the container is lifted away from the radioisotope thermoelectric generator (RTG). The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2425

KENNEDY SPACE CENTER, FLA. - In the RTG Facility at Kennedy Space Center, officials check the radioisotope thermoelectric generator (RTG) after being lowered onto a transporter. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2437

KENNEDY SPACE CENTER, FLA. - n the RTG Facility at Kennedy Space Center, Jim Wojciechowski and Dan Brunson move a metal canister toward the radioisotope thermoelectric generator (RTG). The canister will protect the RTG when it is moved. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2439

KENNEDY SPACE CENTER, FLA. - In the RTG Facility at Kennedy Space Center, Steve Killian, Jim Wojciechowski and Dan Brunson tilt the radioisotope thermoelectric generator (RTG) to a horizontal position. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2431

KENNEDY SPACE CENTER, FLA. - In the RTG Facility at Kennedy Space Center, Dan Brunson and Jim Wojciechowski lower the radioisotope thermoelectric generator (RTG) onto a transporter. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2436

KENNEDY SPACE CENTER, FLA. - In the Payload Hazardous Servicing Facility, engineers move the radioisotope thermoelectric generator (RTG) away from NASA’s New Horizons spacecraft. The RTG is being returned to the RTG facility after completing a fit check with the spacecraft. The RTG is the baseline power supply for the New Horizons, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2470

KENNEDY SPACE CENTER, FLA. - In the RTG Facility at Kennedy Space Center, the radioisotope thermoelectric generator (RTG) rests in a horizontal position. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015. KSC-05pd2432

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KENNEDY SPACE CENTER, FLA. - In the RTG Facility at Kennedy Space Center, the radioisotope thermoelectric generator (RTG) rests in a horizontal position. The RTG is the baseline power supply for the NASA’s New Horizons spacecraft, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. As it approaches Pluto, the spacecraft will look for ultraviolet emission from Pluto's atmosphere and make the best global maps of Pluto and Charon in green, blue, red and a special wavelength that is sensitive to methane frost on the surface. It will also take spectral maps in the near infrared, telling the science team about Pluto's and Charon's surface compositions and locations and temperatures of these materials. When the spacecraft is closest to Pluto or its moon, it will take close-up pictures in both visible and near-infrared wavelengths. It is expected to reach Pluto in July 2015.

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kennedy space center rtg rtg facility radioisotope generator baseline power baseline power new horizons spacecraft nasa new horizons spacecraft pluto moon charon approaches approaches pluto emission atmosphere maps wavelength methane frost methane frost surface science team science team compositions surface compositions locations temperatures materials close up pictures close up pictures energy generation high resolution nasa
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Date

05/11/2005
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NASA
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https://images.nasa.gov/
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label_outline Explore Rtg Facility, Baseline Power, Approaches Pluto

The a cappella group, Wavelength, performs a song arranged by the Pentatonix during a concert at Riverside Brookfield High School.

KENNEDY SPACE CENTER, FLA. - After being raised to a vertical position, the first stage of an Atlas V rocket is being moved into the Vertical Integration Facility to begin preparations for launch on Launch Complex 41 at Cape Canaveral Air Force Station. The Lockheed Martin Atlas V is the launch vehicle for the New Horizons spacecraft, which is designed to make the first reconnaissance of Pluto and Charon - a "double planet" and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 2007, and reach Pluto and its moon, Charon, in July 2015. KSC-05pd2268

BASELINE GAS TURBINE ENGINE, NASA Technology Images

KENNEDY SPACE CENTER, FLA. - New Horizons arrives at the Vertical Integration Facility at Complex 41 on Cape Canaveral Air Force Station where buildup of its Lockheed Martin Atlas V launch vehicle is complete. New Horizons carries seven scientific instruments that will characterize the global geology and geomorphology of Pluto and its moon Charon, map their surface compositions and temperatures, and examine Pluto's complex atmosphere. After that, flybys of Kuiper Belt objects from even farther in the solar system may be undertaken in an extended mission. New Horizons is the first mission in NASA's New Frontiers program of medium-class planetary missions. The spacecraft, designed for NASA by the Johns Hopkins University Applied Physics Laboratory in Laurel, Md., will launch aboard a Lockheed Martin Atlas V rocket and fly by Pluto and Charon as early as summer 2015. KSC-05pd2637

Members of the United States Geological Survey measuring a baseline near Fort Wingate, N.M., 1883

Office of the Administrator (Stephen L. Johnson) - 11th Annual Landfill Methane Outreach Program (LMOP) Conference and Project Expo [412-APD-349-2008-01-09_LandfillMethane_001.jpg]

KENNEDY SPACE CENTER, FLA. - In the communications room above the Atlas V Spaceflight Operations Center on Cape Canaveral Air Force Station, NASA Public Information Officer George Diller rehearses his role for the upcoming launch of the New Horizons spacecraft. Behind him are Tiffany Nail, with the Launch Services Program at Kennedy Space Center, and Bob Summerville, a Lockheed Martin console system software engineer. Members of the New Horizons team are taking part in a dress rehearsal for the launch scheduled in mid-January. New Horizons carries seven scientific instruments that will characterize the global geology and geomorphology of Pluto and its moon Charon, map their surface compositions and temperatures, and examine Pluto's complex atmosphere. After that, flybys of Kuiper Belt objects from even farther in the solar system may be undertaken in an extended mission. New Horizons is the first mission in NASA's New Frontiers program of medium-class planetary missions. The spacecraft, designed for NASA by the Johns Hopkins University Applied Physics Laboratory in Laurel, Md., will launch aboard a Lockheed Martin Atlas V rocket and fly by Pluto and Charon as early as summer 2015. KSC-05pd2616

The fast attack submarine USS Louisville (SSN 724) moored at Submarine Base New London, is surrounded by ice during below average cold temperatures.

STAY SHARP - SOF BRAIN HEALTH - AFSOC The Comprehensive

A technician gives radioisotope treatment to a patient at Gorgas Army Hospital

Neptune False Color Image of Haze

KENNEDY SPACE CENTER, FLA. — Photographers and spectators watch NASA’s New Horizons spacecraft, trailing fire and smoke from the Atlas V rocket that propels it, as it roars into the cloud-scattered sky. Liftoff was on time at 2 p.m. EST from Complex 41 on Cape Canaveral Air Force Station in Florida. This was the third launch attempt in as many days after scrubs due to weather concerns. The compact, 1,050-pound piano-sized probe will get a boost from a kick-stage solid propellant motor for its journey to Pluto. New Horizons will be the fastest spacecraft ever launched, reaching lunar orbit distance in just nine hours and passing Jupiter 13 months later. The New Horizons science payload, developed under direction of Southwest Research Institute, includes imaging infrared and ultraviolet spectrometers, a multi-color camera, a long-range telescopic camera, two particle spectrometers, a space-dust detector and a radio science experiment. The dust counter was designed and built by students at the University of Colorado, Boulder. The launch at this time allows New Horizons to fly past Jupiter in early 2007 and use the planet’s gravity as a slingshot toward Pluto. The Jupiter flyby trims the trip to Pluto by as many as five years and provides opportunities to test the spacecraft’s instruments and flyby capabilities on the Jupiter system. New Horizons could reach the Pluto system as early as mid-2015, conducting a five-month-long study possible only from the close-up vantage of a spacecraft. Photo credit: NASA/George Shelton KSC-06pd0089

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kennedy space center rtg rtg facility radioisotope generator baseline power baseline power new horizons spacecraft nasa new horizons spacecraft pluto moon charon approaches approaches pluto emission atmosphere maps wavelength methane frost methane frost surface science team science team compositions surface compositions locations temperatures materials close up pictures close up pictures energy generation high resolution nasa