nside the world's largest clean room at NASA's Goddard Space Flight Center in Greenbelt, Md., engineers worked tirelessly to install another essential part of the James Webb Space Telescope - the Near Infrared Camera into the heart of the telescope. To complete this installation, the engineers needed to carefully move NIRCam inside the heart or ISIM, or Integrated Science Instrument Module that will house all of the science instruments. &quot;Installing NIRCam into the center of the structure is nerve wracking because of the tight clearances,&quot; said Marcia J. Rieke, Professor of Astronomy at the University of Arizona, and principal investigator for the NIRCam. &quot;I'm glad nothing bumped, and all the bolts are in place.&quot; NIRCam is a unique machine because in addition to being one of the four science instruments on the Webb, it also serves as the wavefront sensor, which means it will provide vital information for shaping the telescope mirrors and aligning its optics so that they can function properly and see into the distant universe. The NIRCam instrument will operate at very cold temperatures, and will be tested to ensure that it will be able to withstand the environment of space. The NIRCam is Webb's primary imager that will cover the infrared wavelength range 0.6 to 5 microns. It will detect light from the earliest stars and galaxies in the process of formation, the population of stars in nearby galaxies, as well as young stars and exoplanets in the Milky Way. NIRCam is provided by the University of Arizona and Lockheed Martin Advanced Technology Center. Webb is an international project led by NASA with its partners the European Space Agency and the Canadian Space Agency. The James Webb Space Telescope is the successor to NASA's Hubble Space Telescope. It will be the most powerful space telescope ever built. For more information about the Webb telescope, visit: <a href="http://www.jwst.nasa.gov" rel="nofollow">www.jwst.nasa.gov</a> or <a href="http://www.nasa.gov/webb" rel="nofollow">www.nasa.gov/webb</a> Credit: NASA/Goddard/Chris Gunn <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>

This crescent view of Earth Moon in infrared wavelengths comes from a camera test by NASA Mars Reconnaissance Orbiter spacecraft on its way to Mars. This image was taken by taken by the High Resolution Imaging Science Experiment camera Sept. 8, 2005.

Technicians fill SOFIA’s instrument with liquid nitrogen and helium to keep the detectors cold. The now retired instrument was called the First Light Infrared Test Experiment Camera, or FLITECAM. When SOFIA lands after each flight its instruments can be exchanged, serviced or upgraded to harness new technologies. Left: Chris Koerber, right UCLA's Ken Magnone.

This video shows images taken through infrared range cameras during a recovery simulation at the Utah Test and Training Range on Dec 13, 2005. Infrared cameras will track the landing.

Galaxy NGC 4579 was captured by the Spitzer Infrared Nearby Galaxy Survey, or Sings, Legacy project using the Spitzer Space Telescope infrared array camera. I

Astronomers using the Hubble Space Telescope (HST) have identified what may be the most luminous star known; a celestial mammoth that releases up to 10-million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds as our Sun does in one year. The image, taken by a UCLA-led team with the recently installed Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) aboard the HST, also reveals a bright nebula, created by extremely massive stellar eruptions. The UCLA astronomers estimate that the star, called the Pistol Star, (for the pistol shaped nebula surrounding it), is approximately 25,000 light-years from Earth, near the center of our Milky Way galaxy. The Pistol Star is not visible to the eye, but is located in the direction of the constellation Sagittarius, hidden behind the great dust clouds along the Milky Way

This image from NASA Dawn spacecraft shows Dawn visible and infrared spectrometer image, overlain on top of a framing camera image of the same region on asteroid Vesta.

NASA Cassini spacecraft camera looks in near-infrared light at a dramatic view of Saturn, its ringplane and the shadows of a couple of its moons.

NASA 2001 Mars Odyssey Thermal Emission Imaging System THEMIS acquired these images of the Earth using its visible and infrared cameras as it left the Earth.

Color differences in this daytime infrared image taken by the camera on NASA Mars Odyssey spacecraft represent differences in the mineral composition of the rocks, sediments and dust on the surface.

Illustrated in this artist concept are two possible structures for asteroid 2011 MD. NASA Spitzer infrared camera helped reveal that this asteroid consists of about two-thirds empty space.

Taking its first peek at Uranus, NASA Hubble Space Telescope Near Infrared Camera and Multi-Object Spectrometer NICMOS detected six distinct clouds in images taken July 28,1997.

This image of comet 67P/Churymov-Gerasimenko was taken on March 20, 2014, by the wide-angle camera of the Rosetta spacecraft Optical, Spectroscopic and Infrared Remote Imaging System OSIRIS.

This crescent view of Earth Moon in infrared, blue-green, and red wavelengths comes from a camera test by NASA Mars Reconnaissance Orbiter spacecraft on its way to Mars.

Pastel colors swirl across Mars, revealing differences in the composition and nature of the surface in this false-color infrared image taken on May 22, 2009,by the Thermal Emission Imaging System THEMIS camera on NASA Mars Odyssey orbiter.

This image of comet 67P/Churymov-Gerasimenko was taken on March 21, 2014, by the narrow-angle camera of the Rosetta spacecraft Optical, Spectroscopic and Infrared Remote Imaging System OSIRIS.

Straining to make out the surface of Titan through its murky atmosphere, the Cassini spacecraft wide angle camera manages to exploit one of the infrared spectral windows where the particulate smog is transparent enough for a peek

Many craters around the south polar cap contain dune fields on their floors. This is one example of such a crater. This image was taken with the 2001 Mars Odyssey THEMIS infrared camera and shows the warm daytime temperature of the dunes.

NASA Spitzer Space Telescope used its infrared camera to image this beautiful bulb which might look like a Christmas ornament but is the blown-out remains of a stellar explosion, or supernova.

This view in the southern constellation Carina was acquired on December 13, 2007 as part of the characterization tests of the Framing Camera. The false-color view is a composite of images at 430 nm violet, 650 nm red, and 980 nm infrared.

This psychedelic view of Saturn and its rings is a composite made from images taken with the Cassini spacecraft wide-angle camera using spectral filters sensitive to wavelengths of infrared light

These are three different views of the Martian moon Phobos, as seen by NASA's 2001 Mars Odyssey orbiter using its infrared camera, Thermal Emission Imaging System (THEMIS). Each color represents a different temperature range. https://photojournal.jpl.nasa.gov/catalog/PIA23205

SL4-93-153 (February 1974) --- A vertical view of the Birmingham and central Alabama area is seen in this Skylab 4 Earth Resources Experiments Package S190-B (five-inch earth terrain camera) infrared photographed taken from the Skylab space station in Earth orbit. Illustrated here is the utility of color infrared film in depicting distribution of living vegetation in the 3,600 square mile Birmingham region. The Birmingham industrial complex, with a population of nearly 850,000, is the light gray area nestled in the valley between the northeast-trending ridges that are prominent topographic features in the southern Appalachian Mountains. The narrow ridges and adjacent valleys reflect folded and faulted sedimentary rocks, indicating the complex geological history of the region. Two major rivers and several reservoirs are easily distinguished in this photograph. Bankhand Lake, formed by a dam on the Black Warrior River, appears as bright blue west of Birmingham. Two lakes are formed by dams on the Goosa River east of Birmingham. Federal and state highways appear as thin white lines and are easily identified. Interstate 65 to Montgomery is the prominent white line extending southward from Birmingham. Power line clearings are visible in the center of the picture along the Goosa River, and can be traced northwestward to northern parts of Birmingham. The predominant deep red color of the picture is due to the reflections from living vegetation. In contrast are the light tan areas that commonly occur as rectangular patterns in the east part of the photograph and represent mature agricultural crops or grazing lands. Analysis of the photographic data from the earth terrain camera will be conducted by Dr. H. Jayroe of the Marshall Space Flight Center in developing analytical techniques. All EREP photography is available to the public through the Department of Interior's Earth Resources Observations Systems Data Center, Sioux Falls, South Dakota, 57198. Photo credit: NASA

This image of Rabe Crater and the region around it was collected using the IR (infrared) camera. The brighter the material, the warmer the surface is. Most dunes on Mars are dark in visible wavelengths and bright in infrared. The majority of large craters in the southern hemisphere contain dunes on the crater floor. Orbit Number: 67144 Latitude: -46.329 Longitude: 34.079 Instrument: IR Captured: 2017-02-01 12:57 http://photojournal.jpl.nasa.gov/catalog/PIA21519

iss051e037888 (5/4/2017) --- A view of two AstroPi Raspberry Pi computers, one equipped with a Visual camera and the other with an Infrared Camera in the Columbus module aboard the International space Station (ISS).

These are two views of the same observation of the Martian moon Phobos taken in both infrared and visible light by NASA's 2001 Mars Odyssey orbiter using its infrared camera, Thermal Emission Imaging System (THEMIS). The image was taken on April 24, 2019. The top view is what Phobos looked like in the visible light spectrum, as viewed by THEMIS. The bottom view is what it looks like in infrared, which reveals temperature differences. The warmest temperatures are in the center, and the coolest are on the outer edge. A scale bar is provided to reflect the temperatures, which range from 200 to 300 degrees Kelvin, or -100 degrees Fahrenheit (-73 Celsius) to 80 degrees Fahrenheit (27 Celsius). https://photojournal.jpl.nasa.gov/catalog/PIA23206

KENNEDY SPACE CENTER, FLA. - Workers in KSC's Vertical Processing Facility inspect the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) on its handling fixture. NICMOS is one of two new scientific instruments that will replace two outdated instruments on the Hubble Space Telescope (HST). NICMOS will provide HST with the capability for infrared imaging and spectroscopic observations of astronomical targets. The refrigerator-sized NICMOS also is HST's first cryogenic instrument — its sensitive infrared detectors must operate at very cold temperatures of minus 355 degrees Fahrenheit or 58 degrees Kelvin. NICMOS will be installed in Hubble during STS-82, the second Hubble Space Telescope servicing mission. Liftoff is targeted Feb. 11 aboard Discovery with a crew of seven.

KENNEDY SPACE CENTER, FLA. - Workers in KSC's Vertical Processing Facility lower the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) into the Second Axial Carrier. NICMOS is one of two new scientific instruments that will replace two outdated instruments on the Hubble Space Telescope (HST). NICMOS will provide HST with the capability for infrared imaging and spectroscopic observations of astronomical targets. The refrigerator-sized NICMOS is HST's first cryogenic instrument -- its sensitive infrared detectors must operate at very cold temperatures of minus 355 degrees Fahrenheit or 58 derees Kelvin. NICMOS will be installed in Hubble during STS-82, the second Hubble Space Telescope servicing mission. Liftoff is targeted Feb. 11 aboard Discovery with a crew of seven.

KENNEDY SPACE CENTER, FLA. - STS-82 crew members and workers at KSC's Vertical Processing Facility get a final look at the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) in its flight configuration for the STS-82 mission. The crew is participating in the Crew Equipment Integration Test (CEIT). NICMOS is one of two new scientific instruments that will replace two outdated instruments on the Hubble Space Telescope (HST). NICMOS will provide HST with the capability for infrared imaging and spectroscopic observations of astronomical targets. The refrigerator-sized NICMOS also is HST's first cryogenic instrument - its sensitive infrared detectors must operate at very cold temperatures of minus 355 degrees Fahrenheit or 58 degrees Kelvin. NICMOS will be installed in Hubble during STS-82, the second Hubble Space Telescope servicing mission. Liftoff is scheduled Feb. 11 aboard Discovery with a crew of seven.

KENNEDY SPACE CENTER, FLA. - Workers in KSC's Vertical Processing Facility lift the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) prior to its installation in the Second Axial Carrier. NICMOS is one of two new scientific instruments that will replace two outdated instruments on the Hubble Space Telescope (HST). NICMOS will provide HST with the capability for infrared imaging and spectroscopic observations of astronomical targets. The refrigerator-sized NICMOS also is HST's first cryogenic instrument — its sensitive infrared detectors must operate at very cold temperatures of minus 355 degrees Fahrenheit or 58 degrees Kelvin. NICMOS will be installed in Hubble during STS-82, the second Hubble Space Telescope servicing mission. Liftoff is targeted Feb. 11 aboard Discovery with a crew of seven.

KENNEDY SPACE CENTER, FLA. - Workers in KSC's Vertical Processing Facility lower the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) into the Second Axial Carrier. NICMOS is one of two new scientific instruments that will replace two outdated instruments on the Hubble Space Telescope (HST). NICMOS will provide HST with the capability for infrared imaging and spectroscopic observations of astronomical targets. The refrigerator-sized NICMOS also is HST's first cryogenic instrument — its sensitive infrared detectors must operate at very cold temperatures of minus 355 degrees Fahrenheit or 58 degrees Kelvin. NICMOS will be installed in Hubble during STS-82, the second Hubble Space Telescope servicing mission. Liftoff is targeted Feb. 11 aboard Discovery with a crew of seven.

Here we see two different views of the spiral galaxy, Messier 81. On the left is an image taken in blue light, while on the right is a specially-processed version of an image taken with NASA Spitzer infrared array camera at 4.5 microns.

Newborn stars, hidden behind thick dust, are revealed in this image of a section of the Christmas Tree cluster from NASA Spitzer Space Telescope, created in joint effort between Spitzer infrared array camera and multiband imaging photometer instrument

ISS030-E-049629 (21 Jan. 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, works with two still cameras mounted together in the Destiny laboratory of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-175784 (15 Jan. 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, works with two still cameras mounted together in the Destiny laboratory of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-049643 (21 Jan. 2012) --- NASA astronaut Don Pettit, Expedition 30 flight engineer, works with two still cameras mounted together in the Destiny laboratory of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-175780 (15 Jan. 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, is pictured with still cameras and a punch beverage in the Destiny laboratory of the International Space Station. Two of the cameras are mounted together; one being an infrared modified still camera.

ISS030-E-049664 (21 Jan. 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, uses still cameras to photograph the topography of a point on Earth from a window in the Cupola of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-049671 (21 Jan. 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, uses still cameras to photograph the topography of a point on Earth from a window in the Cupola of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-175782 (15 Jan. 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, works with two still cameras mounted together in the Destiny laboratory of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-049636 (21 Jan. 2012) --- NASA astronaut Don Pettit, Expedition 30 flight engineer, works with two still cameras mounted together in the Destiny laboratory of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-175788 (15 Jan. 2012) --- NASA astronaut Don Pettit, Expedition 30 flight engineer, is pictured with two still cameras mounted together in the Destiny laboratory of the International Space Station. One camera is an infrared modified still camera.

ISS030-E-049632 (21 Jan. 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, works with two still cameras mounted together in the Destiny laboratory of the International Space Station. One camera is an infrared modified still camera.

KENNEDY SPACE CENTER, FLA. - In the Orbiter Processing Facility, from left, United Space Alliance workers Ken Tauer and Paul Ogletree set up an infrared camera in front of Discovery’s nose cap while Ross Neubarth checks the monitor. The nose cap will undergo thermography to verify integrity of hardware before flight. This procedure uses high intensity light to heat areas that are immediately scanned with an infrared camera to check for internal flaws. Discovery is the vehicle assigned to the Return to Flight mission, STS-114.

This image from NASA Spitzer Space Telescope, shows the wispy filamentary structure of Henize 206, is a four-color composite mosaic created by combining data from an infrared array camera IRAC. The LMC is a small satellite galaxy gravitationally bound to our own Milky Way. Yet the gravitational effects are tearing the companion to shreds in a long-playing drama of 'intergalactic cannibalism.' These disruptions lead to a recurring cycle of star birth and star death. Astronomers are particularly interested in the LMC because its fractional content of heavy metals is two to five times lower than is seen in our solar neighborhood. [In this context, 'heavy elements' refer to those elements not present in the primordial universe. Such elements as carbon, oxygen and others are produced by nucleosynthesis and are ejected into the interstellar medium via mass loss by stars, including supernova explosions.] As such, the LMC provides a nearby cosmic laboratory that may resemble the distant universe in its chemical composition. The primary Spitzer image, showing the wispy filamentary structure of Henize 206, is a four-color composite mosaic created by combining data from an infrared array camera (IRAC) at near-infrared wavelengths and the mid-infrared data from a multiband imaging photometer (MIPS). Blue represents invisible infrared light at wavelengths of 3.6 and 4.5 microns. Note that most of the stars in the field of view radiate primarily at these short infrared wavelengths. Cyan denotes emission at 5.8 microns, green depicts the 8.0 micron light, and red is used to trace the thermal emission from dust at 24 microns. The separate instrument images are included as insets to the main composite. An inclined ring of emission dominates the central and upper regions of the image. This delineates a bubble of hot, x-ray emitting gas that was blown into space when a massive star died in a supernova explosion millions of years ago. The shock waves from that explosion impacted a cloud of nearby hydrogen gas, compressed it, and started a new generation of star formation. The death of one star led to the birth of many new stars. This is particularly evident in the MIPS inset, where the 24-micron emission peaks correspond to newly formed stars. The ultraviolet and visible-light photons from the new stars are absorbed by surrounding dust and re-radiated at longer infrared wavelengths, where it is detected by Spitzer. This emission nebula was cataloged by Karl Henize (HEN-eyes) while spending 1948-1951 in South Africa doing research for his Ph.D. dissertation at the University of Michigan. Henize later became a NASA astronaut and, at age 59, became the oldest rookie to fly on the Space Shuttle during an eight-day flight of the Challenger in 1985. He died just short of his 67th birthday in 1993 while attempting to climb the north face of Mount Everest, the world's highest peak. http://photojournal.jpl.nasa.gov/catalog/PIA05517

Sensitive to Jupiter's stratospheric temperatures, these infrared images were recorded by the Cooled Mid-Infrared Camera and Spectrograph (COMICS) at the Subaru Telescope on the summit of Mauna Kea, Hawaii. Scientists used red, blue and yellow to infuse this infrared image; regions of the atmosphere that are more yellow and red indicate the hotter areas. This highlights the auroral heating that occurs at Jupiter's poles, where energy from the solar wind and magnetosphere are deposited. This image was captured on Jan. 12, 2017. https://photojournal.jpl.nasa.gov/catalog/PIA22774

Taken on April 24, 2019, this rainbow-colored image shows the Martian moon Phobos, as viewed by NASA's 2001 Mars Odyssey orbiter using its infrared camera, Thermal Emission Imaging System (THEMIS). Each color represents a different temperature range, with the warmest in the center and coolest on the outer edge. This was the first time THEMIS was used to observe Phobos while in a full moon phase, which offers scientists a much better view for studying the composition of the Martian moon. Previous half-moon views, which can be seen here, were better for studying surface textures. https://photojournal.jpl.nasa.gov/catalog/PIA23204

This high-resolution color infrared photograph of the Uncompahgre Plateau area of Colorado was taken by the Multi-spectral Photographic Camera (Skylab EREP Experiment S190A) of the Skylab's Multi-spectral Photographic Facility during the Skylab-3 mission.

KENNEDY SPACE CENTER, FLA. - In the Space Station Processing Facility, technicians with The Boeing Company move an infrared camera into position near the Japanese Experiment Module (JEM) for pre-assembly measurements. Developed by the Japan Aerospace Exploration Agency (JAXA), the JEM will enhance the unique research capabilities of the orbiting complex by providing an additional environment for astronauts to conduct science experiments.

This movie shows the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter on April 24, 2019. It was put together from 19 images taken 1 second apart by Odyssey's infrared camera, Thermal Emission Imaging System (THEMIS). The apparent motion is due to progression of the camera's pointing during the observation. This was the third observation of Phobos by Mars Odyssey. While displayed here in visible-wavelength light, THEMIS also recorded thermal-infrared imagery in the same scan. The distance to Phobos from Odyssey during the observation was about 5,692 miles (9,160 kilometers). Movie available at https://photojournal.jpl.nasa.gov/catalog/PIA23207

This video shows Jupiter as revealed by a powerful telescope and a mid-infrared filter sensitive to the giant planet's tropospheric temperatures and cloud thickness. It combines observations made on Jan. 14, 2017, using the Subaru Telescope in Hawaii. The filter used admits infrared light centered on a wavelength of 8.8 microns. The video includes interpolated frames for smoother apparent motion. The instrument used to take this image is Cooled Mid-Infrared Camera and Spectrometer (COMICS) of the National Astronomical Observatory of Japan's Subaru Telescope on the Maunakea volcano. Animations are available at https://photojournal.jpl.nasa.gov/catalog/PIA21715

A composite image of the Cigar Galaxy (also called M82), a starburst galaxy about 12 million light-years away in the constellation Ursa Major. The magnetic field detected by the High-resolution Airborne Wideband Camera-Plus instrument (known as HAWC+) on SOFIA (the Stratospheric Observatory for Infrared Astronomy), shown as streamlines, appears to follow the bipolar outflows (red) generated by the intense nuclear starburst. The image combines visible starlight (gray) and a tracing of hydrogen gas (red) observed from the Kitt Peak Observatory, with near-infrared and mid-infrared starlight and dust (yellow) observed by SOFIA and the Spitzer Space Telescope. https://photojournal.jpl.nasa.gov/catalog/PIA23010

AS09-26A-3801A (12 March 1969) --- Colored infrared photograph of the Phoenix, Arizona area, taken on March 12, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey (SO65) Experiment. At 11:28 a.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 127 nautical miles, and the sun elevation was 32 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed was 33 degrees 25 minutes north latitude, and 112 degrees 18 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3743A (9 March 1969) --- Color infrared photograph of the Yazoo River Valley, Pearl River, Pearl River Reservoir, and Jackson, Mississippi, area, taken on March 9, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey SO65 Experiment. At 1:08 p.m. (EST) when this photograph was made the Apollo 9 spacecraft was at an altitude of 105 nautical miles, and the sun elevation was at 55 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed was 32 degrees 34 minutes north latitude, and 89 degrees 57 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3792A (11 March 1969) --- Color infrared photograph of the Atlanta, Georgia area taken on March 11, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey (SO-65) experiment. At 11:21 a.m. (EST) when this picture was taken, the Apollo 9 spacecraft was at an altitude of 106 nautical miles, and the sun elevation was 47 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed was 33 degrees 10 minutes north latitude, and 84 degrees and 40 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3802A (12 March 1969) --- Color infrared photograph of the Globe, Arizona area, including Roosevelt Lake and San Carlos Reservoir, taken on March 12, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey SO65 Experiment. At 11:29 a.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 119 nautical miles, and the sun elevation was 38 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed was 33 degrees 42 minutes north latitude, and 103 degrees 1 minute west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3800A (12 March 1969) --- Color infrared photograph of southwestern Arizona, Yuma-Gila Desert-Gila River-Colorado River area, taken on March 12, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey SO65 Experiment. At 11:28 a.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 128 nautical miles, and the sun elevation was 30 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed 33 degrees 19 minutes north latitude, and 113 degrees 45 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3748A (9 March 1969) --- A color infrared photograph of the Salton Sea and Imperial Valley area of Southern California and the Mexicali, Mexico area, taken on March 9, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey S065 Experiment. At 2:36 p.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 103 nautical miles, and the sun elevation was 45 degrees above at which the four-camera combination was aimed was 33 degrees 3 minutes north latitude, and 115 degrees 45 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3728A (8 March 1969) --- Color infrared photograph of the Houston-Galveston-Freeport, Texas Gulf Coast area taken on March 8, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey S065 Experiment. At 3:05 p.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 105 nautical miles, and the sun elevation was 54 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed was 29 degrees 4 minutes north latitude, and 95 degrees 24 minutes west longitude. The three other cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3807A (12 March 1969) --- Color infrared photograph of the Texas-New Mexico border area, between Lubbock and Roswell, taken on March 12, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey (SO65). At 11:30 a.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 119 nautical miles, and the sun elevation was 38 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed was 33 degrees 42 minutes north latitude, and 103 degrees 1 minute west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3816A (12 March 1969) --- Color infrared photograph of the Atlantic coast of Georgia, Brunswick area, taken on March 12, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey SO65 Experiment. At 11:35 a.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 102 nautical miles, and the sun elevation was 51 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed 31 degrees 16 minutes north latitude, and 81 degrees 17 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3808A (12 March 1969) --- Color infrared photograph of the Lubbock, Texas area, taken on March 12, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey SO65 Experiment. At 11:31 a.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 117 nautical miles, and the sun elevation was 38 degrees above the horizon. The location of the point on the surface of Earth at which the four-camera combination was aimed was 33 degrees 41 minutes north latitude, and 101 degrees 29 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

AS09-26A-3793A (12 March 1969) --- Color infrared photograph of the Atlantic Coast of South Carolina, Georgetown-Myrtle Beach-Conway area, taken on March 12, 1969, by one of the four synchronized cameras of the Apollo 9 Earth Resources Survey SO65 Experiment. At 10:00 a.m. (EST) when this picture was made the Apollo 9 spacecraft was at an altitude of 116 nautical miles, and the sun elevation was 39 degrees above the horizon. The location of the point on Earth's surface at which the four-camera combination was aimed was 33 degrees 35 minutes north latitude, and 79 degrees 3 minutes west longitude. The other three cameras used: (B) black and white film with a red filter; (C) black and white infrared film; and (D) black and white film with a green filter.

Galileo has eyes that can see more than ours can. By looking at what we call the infrared wavelengths, the NIMS (Near Infrared Mapping Spectrometer) instrument can determine what type and size of material is on the surface of a moon. Here, 3 images of Ganymede are shown. Left: Voyager's camera. Middle: NIMS, showing water ice on the surface. Dark is less water, bright is more. Right: NIMS, showing the locations of minerals in red, and the size of ice grains in shades of blue. http://photojournal.jpl.nasa.gov/catalog/PIA00500

AST-13-797 (24 July 1975) --- An infrared, near vertical view of the Chesapeake Bay area showing portions of Virginia, Maryland and Delaware, as photographed from the Apollo spacecraft in Earth orbit during the joint U.S.-USSR Apollo-Soyuz Test Project mission. Richmond and Norfolk can be seen in this picture. Tidewater Virginia covers much of this view. The photograph was taken at an altitude of 217 kilometers (135 statute miles) with a 70mm Hasselblad camera using infrared Aerochrome type 2443 Ektachrome film.

The Close Orbiting Propellant Plume Elemental Recognition (COPPER) was developed by students from St. Louis University as a technology demonstration mission whose objective is to test the suitability of a commercially-available compact uncooled microbolometer (tiny infrared camera) array for scientific imagery of Earth in the long-wave infrared range (LWIR, 7-13 microns). Launched by NASA’s CubeSat Launch Initiative on the ELaNa IV mission as an auxiliary payload aboard the U.S. Air Force-led Operationally Responsive Space (ORS-3) Mission on November 19, 2013.

This color infrared view of Houston (29.5N, 95.0W) was taken with a dual camera mount. Compare this scene with STS048-78-034 for an analysis of the unique properties of each film type. Comparative tests such as this aids in determining the kinds of information unique to each film system and evaluates and compares photography taken through hazy atmospheres. Infrared film is best at penetrating haze, vegetation detection and producing a sharp image.

Released 24 June 2004 This pair of images shows a crater and its ejecta. Day/Night Infrared Pairs The image pairs presented focus on a single surface feature as seen in both the daytime and nighttime by the infrared THEMIS camera. The nighttime image (right) has been rotated 180 degrees to place north at the top. Infrared image interpretation Daytime: Infrared images taken during the daytime exhibit both the morphological and thermophysical properties of the surface of Mars. Morphologic details are visible due to the effect of sun-facing slopes receiving more energy than antisun-facing slopes. This creates a warm (bright) slope and cool (dark) slope appearance that mimics the light and shadows of a visible wavelength image. Thermophysical properties are seen in that dust heats up more quickly than rocks. Thus dusty areas are bright and rocky areas are dark. Nighttime: Infrared images taken during the nighttime exhibit only the thermophysical properties of the surface of Mars. The effect of sun-facing versus non-sun-facing energy dissipates quickly at night. Thermophysical effects dominate as different surfaces cool at different rates through the nighttime hours. Rocks cool slowly, and are therefore relatively bright at night (remember that rocks are dark during the day). Dust and other fine grained materials cool very quickly and are dark in nighttime infrared images. Image information: IR instrument. Latitude -9, Longitude 164.2 East (195.8 West). 100 meter/pixel resolution. http://photojournal.jpl.nasa.gov/catalog/PIA06445

Attendees of the USA Science and Engineering Festival observe their infrared images as a NASA Staff member describes the James Webb Space Telescope. It will be a large infrared telescope with a 6.5 meter primary mirror and will study every phase in the history of our Universe ranging from the Big Bang to the formation of our Solar System. The USA Science and Engineering Festival took place at the Washington Convention Center in Washington, DC on April 26 and 27, 2014. Photo Credit: (NASA/Aubrey Gemignani)

An attendee of the USA Science and Engineering Festival observes the infrared image of himself as a NASA Staff member describes the James Webb Space Telescope. It will be a large infrared telescope with a 6.5 meter primary mirror and will study every phase in the history of our Universe ranging from the Big Bang to the formation of our Solar System. The USA Science and Engineering Festival took place at the Washington Convention Center in Washington, DC on April 26 and 27, 2014. Photo Credit: (NASA/Aubrey Gemignani)

An attendee of the USA Science and Engineering Festival observes the infrared image of himself as a NASA staff member describes the James Webb Space Telescope. It will be a large infrared telescope with a 6.5 meter primary mirror and will study every phase in the history of our Universe ranging from the Big Bang to the formation of our Solar System. The USA Science and Engineering Festival took place at the Washington Convention Center in Washington, DC on April 26 and 27, 2014. Photo Credit: (NASA/Aubrey Gemignani)

An attendee of the USA Science and Engineering Festival examines how glass blocks some heat, altering the infrared image of himself. The James Webb Space Telescope will be a large infrared telescope with a 6.5 meter primary mirror and will study every phase in the history of our Universe ranging from the Big Bang to the formation of our Solar System. The USA Science and Engineering Festival took place at the Washington Convention Center in Washington, DC on April 26 and 27, 2014. Photo Credit: (NASA/Aubrey Gemignani)

Artist: Rick Guidice SIRTF Artwork update - cutaway Space Infrared Telescope Facility's will orbit at 900 kilometers aboard a platform-type spacecraft, providing power, pointing, and communications to Earth. The telescope and its infrared instruments, will reside within a cylindrical cryogen tank. The hollow walls of the tank will contain the superfluid helium that cools the telescope to its operating temperature, a few degrees above absolute zero. SIRTF will carry three versatile instruments to analyze the radiation it collects, the Multiband Imaging Photometer, the Infrared Array Camera, and the Infrared Spectrograph. SIRTF long lifetime - 5 years or more - will permit astronomers of all disciplines to use the facililty to carry out a wide variety of astrophysical programs. It will provide ongoing coverage of variable objects, such as quasars, as well as the capability to study rare and transient events such as comets and supernovae. SIRTF's long lifetime will also allow it to distinguish nearby objects by detecting their gradual motions relative to the more distant background stars.

One of the two pictures of Tempel 1 (see also PIA02101) taken by Deep Impact's medium-resolution camera is shown next to data of the comet taken by the spacecraft's infrared spectrometer. This instrument breaks apart light like a prism to reveal the "fingerprints," or signatures, of chemicals. Even though the spacecraft was over 10 days away from the comet when these data were acquired, it detected some of the molecules making up the comet's gas and dust envelope, or coma. The signatures of these molecules -- including water, hydrocarbons, carbon dioxide and carbon monoxide -- can be seen in the graph, or spectrum. Deep Impact's impactor spacecraft is scheduled to collide with Tempel 1 at 10:52 p.m. Pacific time on July 3 (1:52 a.m. Eastern time, July 4). The mission's flyby spacecraft will use its infrared spectrometer to sample the ejected material, providing the first look at the chemical composition of a comet's nucleus. These data were acquired from June 20 to 21, 2005. The picture of Tempel 1 was taken by the flyby spacecraft's medium-resolution instrument camera. The infrared spectrometer uses the same telescope as the high-resolution instrument camera. http://photojournal.jpl.nasa.gov/catalog/PIA02100

Martian surface frost, made up largely of carbon dioxide, appears blueish-white in these images from the Thermal Emission Imaging System (THEMIS) camera aboard NASA's 2001 Odyssey orbiter. THEMIS takes images in both visible light perceptible to the human eye and heat-sensitive infrared. https://photojournal.jpl.nasa.gov/catalog/PIA25233

STS039-87-012 (28 April-6 May 1991) --- A handheld 70mm camera onboard the Space Shuttle Discovery exposed this infrared frame showing oil fires near the Kuwait coast as well as south-bound oil slicks in the Gulf. Pools of oil on the land are recognized as white objects near the burning wells.

ISS013-E-63453 (3 August 2006) --- Astronaut Thomas Reiter, who represents the European Space Agency on the Expedition 13 crew, handles the infrared camera used to photograph a set of reinforced carbon carbon (RCC) samples for possible detection of damage caused by variations in temperature between sound and damaged RCC test sections.

This image shows two merging galaxies known as Arp 302, also called VV 340. It is composed of images from three Spitzer Infrared Array Camera (IRAC) channels: IRAC channel 1 in blue, IRAC channel 2 in green and IRAC channel 3 in red. https://photojournal.jpl.nasa.gov/catalog/PIA23008

ISS031-E-084464 (25 May 2012) --- A vertical view from the International Space Station shows the relative approach of the orbital outpost and the SpaceX Dragon cargo craft prior to grapple by the Canadarm2 robotic arm, controlled by the Expedition 31 crew members.

ISS031-E-084463 (25 May 2012) --- A vertical view from the International Space Station shows the relative approach of the orbital outpost and the SpaceX Dragon cargo craft prior to grapple by the Canadarm2 robotic arm, controlled by the Expedition 31 crew members.

Apollo 9 This infrared color photograph of the Mississippi Valley area was taken by the four synchronized cameras in the Earth Resources Survey SO65 experiment. Shown in this picture are Vicksburg and Greenville Bend. At 1:08 p.m. EST when this photo was made, the Apollo spacecraft was at an altitude of 105 nautical miles and the Sun elevation was 55 degrees above the horizon. Location of the point on the Earth's surface at which the four-camera combination was aimed was 32 degrees 41 minutes North latitude and 91 degrees 13 minutes West longitude.

STS109-E-5722 (8 March 2002) --- Astronaut John M. Grunsfeld (center), STS-109 payload commander, attired in the extravehicular mobility unit (EMU) space suit, is photographed with astronauts James H. Newman (left) and Michael J. Massimino, both mission specialists, prior to the fifth space walk. Activities for EVA-5 centered around the Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) to install a Cryogenic Cooler and its Cooling System Radiator. The image was recorded with a digital still camera.

The mast-mounted portion of SuperCam awaits integration into the Perseverance rover. Part of SuperCam is contained in the belly of the rover, while this unit, containing the laser, infrared spectrometer, telescope, camera, and electronics, sits at the top of the remote sensing mast. The red "remove before flight" cover protects a clear window in front of the telescope and camera and was removed when SuperCam was installed in the rover. https://photojournal.jpl.nasa.gov/catalog/PIA24207

This Spitzer false-color image is a composite of data from the 24 micron channel of Spitzer's multiband imaging photometer (red), and three channels of its infrared array camera: 8 micron (yellow), 5.6 micron (blue), and 4.8 micron (green). Stars are most prominent in the two shorter wavelengths, causing them to show up as turquoise. The supernova remnant is most prominent at 24 microns, arising from dust that has been heated by the supernova shock wave, and re-radiated in the infrared. The 8 micron data shows infrared emission from regions closely associated with the optically emitting regions. These are the densest regions being encountered by the shock wave, and probably arose from condensations in the surrounding material that was lost by the supernova star before it exploded. The composite above (PIA06908, PIA06909, and PIA06910) represent views of Kepler's supernova remnant taken in X-rays, visible light, and infrared radiation. Each top panel in the composite above shows the entire remnant. Each color in the composite represents a different region of the electromagnetic spectrum, from X-rays to infrared light. The X-ray and infrared data cannot be seen with the human eye. Astronomers have color-coded those data so they can be seen in these images. http://photojournal.jpl.nasa.gov/catalog/PIA06910

KENNEDY SPACE CENTER, FLA. -- In the Vertical Processing Facility, workers watch while an overhead crane lowers the Advanced Camera for Surveys (ACS) toward the Axial Science Instrument Protective Enclosure (ASIPE). The ACS is part of the payload on the Hubble Space Telescope Servicing Mission, STS-109. The goal of the mission is to service the HST, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the ACS, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation. Mission STS-109 is scheduled for launch no earlier than Feb. 21, 2002

KENNEDY SPACE CENTER, Fla. -- In the Vertical Processing Facility a worker removes the protective covering from the equipment to be used on mission STS-109. The mission is to service the Hubble Space Telescope, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the Advanced Camera for Surveys, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation on bays 5 through 8. Mission STS-109 is scheduled for launch Feb. 14, 2002

KENNEDY SPACE CENTER, Fla. -- Part of the equipment to be used on mission STS-109, servicing the Hubble Space Telescope, arrives at a facility at KSC. The primary servicing tasks of the mission are to replace Solar Array 2 with Solar Array 3, replace the Power Control Unit, remove the Faint Object Camera and install the Advanced Camera for Surveys, install the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and install New Outer Blanket Insulation on bays 5 through 8. Mission STS-109 is scheduled for launch in mid-February 2002

KENNEDY SPACE CENTER, Fla. - Members of the STS-109 crew are lowered into the payload bay of orbiter Columbia to check out some of the equipment. The crew is at KSC to take part in Crew Equipment Interface Test activities that include familiarization with the orbiter and equipment. The goal of the mission is to service the HST, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the Advanced Camera for Surveys, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation on bays 5 through 8. Mission STS-109 is scheduled for launch Feb. 14, 2002

KENNEDY SPACE CENTER, FLA. -- In the Vertical Processing Facility, workers watch while an overhead crane lifts the Advanced Camera for Surveys (ACS) off the stand. The ACS is part of the payload on the Hubble Space Telescope Servicing Mission, STS-109. The goal of the mission is to service the HST, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the ACS, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation. Mission STS-109 is scheduled for launch no earlier than Feb. 21, 2002

KENNEDY SPACE CENTER, FLA. -- In the Vertical Processing Facility, workers watch while the Advanced Camera for Surveys (ACS) is lowered into the Axial Science Instrument Protective Enclosure (ASIPE). The ACS is part of the payload on the Hubble Space Telescope Servicing Mission, STS-109. The goal of the mission is to service the HST, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the ACS, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation. Mission STS-109 is scheduled for launch no earlier than Feb. 21, 2002

KENNEDY SPACE CENTER, FLA. -- In the Vertical Processing Facility, workers watch while an overhead crane lowers the Advanced Camera for Surveys (ACS) into the Axial Science Instrument Protective Enclosure (ASIPE). The ACS is part of the payload on the Hubble Space Telescope Servicing Mission, STS-109. The goal of the mission is to service the HST, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the ACS, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation. Mission STS-109 is scheduled for launch no earlier than Feb. 21, 2002

KENNEDY SPACE CENTER, Fla. - STS-109 Mission Specialist Nancy Currie arrives at KSC aboard a T-38 jet aircraft to begin launch preparations. This is Currie's fourth Shuttle flight. The goal of the 11-day mission is repair and maintenance on the Hubble Space Telescope. Five spacewalks are planned to replace Solar Array 2 with Solar Array 3, replace the Power Control Unit, remove the Faint Object Camera and install the Advanced Camera for Surveys (ACS), install the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and install New Outer Blanket Layer insulation. Launch is scheduled for Feb. 28 at 6:48 a.m. EST

KENNEDY SPACE CENTER, Fla. - STS-109 Payload Commander John Grunsfeld arrives at KSC aboard a T-38 jet aircraft to begin launch preparations. This is Grunsfeld's fourth Shuttle flight. The goal of the 11-day mission is repair and maintenance on the Hubble Space Telescope. Five spacewalks are planned to replace Solar Array 2 with Solar Array 3, replace the Power Control Unit, remove the Faint Object Camera and install the Advanced Camera for Surveys (ACS), install the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and install New Outer Blanket Layer insulation. Launch is scheduled for Feb. 28 at 6:48 a.m. EST

KENNEDY SPACE CENTER, FLA. -- In the Vertical Processing Facility, workers watch while an overhead crane lowers the Advanced Camera for Surveys (ACS) toward the Axial Science Instrument Protective Enclosure (ASIPE). The ACS is part of the payload on the Hubble Space Telescope Servicing Mission, STS-109. The goal of the mission is to service the HST, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the ACS, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation. Mission STS-109 is scheduled for launch no earlier than Feb. 21, 2002

KENNEDY SPACE CENTER, FLA. - STS-109 Mission Specialist Richard Linnehan arrives at KSC aboard a T-38 jet aircraft to begin launch preparations. This is Linnehan's third Shuttle flight. The goal of the 11-day mission is repair and maintenance on the Hubble Space Telescope. Five spacewalks are planned to replace Solar Array 2 with Solar Array 3, replace the Power Control Unit, remove the Faint Object Camera and install the Advanced Camera for Surveys (ACS), install the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and install New Outer Blanket Layer insulation. Launch is scheduled for Feb. 28 at 6:48 a.m. EST

KENNEDY SPACE CENTER, FLA. -- In the Vertical Processing Facility, workers watch while the Advanced Camera for Surveys (ACS) is lowered into the Axial Science Instrument Protective Enclosure (ASIPE). The ACS is part of the payload on the Hubble Space Telescope Servicing Mission, STS-109. The goal of the mission is to service the HST, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the ACS, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation. Mission STS-109 is scheduled for launch no earlier than Feb. 21, 2002

KENNEDY SPACE CENTER, Fla. - STS-109 Shuttle Commander Scott Altman arrives at KSC aboard a T-38 jet aircraft to begin launch preparations. This is Altman's third Shuttle flight. The goal of the 11-day mission is repair and maintenance on the Hubble Space Telescope. Five spacewalks are planned to replace Solar Array 2 with Solar Array 3, replace the Power Control Unit, remove the Faint Object Camera and install the Advanced Camera for Surveys (ACS), install the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and install New Outer Blanket Layer insulation. Launch is scheduled for Feb. 28 at 6:48 a.m. EST

KENNEDY SPACE CENTER, Fla. -- In the Vertical Processing Facility, part of the equipment to be used on mission STS-109 is revealed after removal of the protective cover. The mission is to service the Hubble Space Telescope, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the Advanced Camera for Surveys, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation on bays 5 through 8. Mission STS-109 is scheduled for launch Feb. 14, 2002

KENNEDY SPACE CENTER, Fla. -- A large truck arrives at the gate to KSC, delivering part of the equipment to be used on mission STS-109, the Hubble Servicing mission. The primary tasks of the mission are to replace Solar Array 2 with Solar Array 3, replace the Power Control Unit, remove the Faint Object Camera and install the Advanced Camera for Surveys, install the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and install New Outer Blanket Layer insulation on bays 5 through 8. Mission STS-109 is scheduled for launch Feb. 14, 2002

KENNEDY SPACE CENTER, Fla. -- The truck delivering part of the equipment to be used on mission STS-109 moves into the Vertical Processing Facility at KSC. The mission is to service the Hubble Space Telescope, replacing Solar Array 2 with Solar Array 3, replacing the Power Control Unit, removing the Faint Object Camera and installing the Advanced Camera for Surveys, installing the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) Cooling System, and installing New Outer Blanket Layer insulation on bays 5 through 8. Mission STS-109 is scheduled for launch Feb. 14, 2002.