At the Kennedy Space Center's (KSC's) Spacecraft and Assembly Encapsulation Facility 2 (SAEF-2), the planetary spacecraft checkout facility, clean-suited technicians work on the Galileo spacecraft prior to moving it to the Vehicle Processing Facility (VPF) for mating with the inertial upper stage (IUS). Galileo is scheduled for launch aboard Atlantis, Orbiter Vehicle (OV) 104, on Space Shuttle Mission STS-34 in October 1989. It will be sent to the planet Jupiter, a journey which will taken more than six years to complete. In December 1995 as the two and one half ton spacecraft orbits Jupiter with its ten scientific instruments, a probe will be released to parachute into the Jovian atmosphere. NASA's Jet Propulsion Laboratory (JPL) manages the Galileo project. View provided by KSC.
STS-34 Galileo processing at KSC's SAEF-2 planetary spacecraft facility
Galileo spacecraft image of the Moon recorded at 9:35 am Pacific Standard Time (PST), 12-09-90, after completing its first Earth Gravity Assist. Western hemisphere of the Moon was taken through a green filter at a range of about 350,000 miles. In the center is Orientale Basin, 600 miles in diameter, formed about 3.8 billion years ago by the impact of an asteroid-size body. Orientale's dark center is a small mare. To the right is the lunar near side with the great, dark Oceanus Procellarum above the small, circular, dark Mare Humorum below. Maria are broad plains formed mostly over 3 billion years ago as vast basaltic lava flows. To the left is the lunar far side with fewer maria, but, at lower left South-Pole-Aitken basin, about 1200 miles in diameter, which resembles Orientale but is much older and more weathered and battered by cratering. The intervening cratered highlands of both sides, as well as the maria, are dotted with bright young craters. This image was "reprojected" so as to center the Orientale Basin, and was filtered to enhance the visibility of small features. The digital image processing was done by DLR, the German Aerospace Research Establishment near Munich, an international collaborator in the Galileo mission. Photo was provided by Jet Propulsion Laboratory (JPL) with alternate number P-37327, 12-19-90.
Western hemisphere of the Moon taken by Galileo spacecraft
(P-37375) Moon craters as seen by Galileo spacecraft
ARC-1990-A91-2012
Line drawing charts the Galileo spacecraft's launch from low Earth orbit and its three planetary and two asteroid encounters in the course of its gravity-assisted flight to Jupiter. These encounters include Venus (February 1990), two Earth passes (December 1990 and December 1992), and the asteroids Gaspra and Ida in the asteroid belt. Galileo will release a probe and will arrive at Jupiter, 12-07-95.
Line drawing of the Galileo spacecraft's encounters on its way to Jupiter
S89-48714 (18 Oct 1989) --- This photograph was taken by the STS-34 crew aboard the Space Shuttle Atlantis and shows the Galileo spacecraft being deployed on Oct.  18, 1989 from the payload bay. Galileo is a scientific craft that will go into orbit around the planet Jupiter and drop a probe into its atmosphere in search of primordial solar system material believed to be present there.  The 70mm motion picture film will be used in the forthcoming "Blue Planet," which will address Earth's environmental problems from the perspective of space-based observation and solar system exploration.  The film is being produced by IMAX Space Technology Inc. for the sponsor, the Smithsonian Institution, with funding provided by the Lockheed Corporation.  PHOTO CREDIT:  NASA/Smithsonian Institution
STS-34 Galileo spacecraft / IUS deployment taken by the IMAX camera
During STS-34 mission, the Galileo spacecraft mounted atop the inertial upper stage (IUS) is tilted to a 58-degree deployment position by the airborne support equipment (ASE) aft frame tilt actuator (AFTA) table in Atlantis', Orbiter Vehicle (OV) 104's, payload bay (PLB). Visible in the foreground is the ASE forward cradle and the umbilical boom which has fallen away from the IUS. OV-104's orbital maneuvering system (OMS) pods and the Earth's limb appear in the background.
STS-34 Galileo spacecraft / IUS deployment sequence in OV-104's payload bay
Artist concept shows Galileo spacecraft while still approaching Jupiter having a satellite encounter. Galileo is flying about 600 miles above Io's volcano-torn surface, twenty times closer than the closest flyby altitude of Voyager in 1979.
Artist concept of Galileo encountering Io during its Jupiter approach
Labeled line drawing entitled GALILEO PROBE identifies the deceleration module aft cover, descent module, and deceleration module aeroshell configurations and dimensions prior to and during entry into Jupiter's atmosphere.
Labeled line drawing of Galileo spacecraft's atmospheric probe
S90-55753 (9 Dec. 1990) --- This color image of the Moon was taken by the Galileo spacecraft at 9:25 a.m. (PST) December 9, 1990, at a range of about 350,000 miles. The color composite uses monochrome images taken through violet, red, and near infrared filters. The concentric, circular Orientale Basin, 600 miles across, is near the center; the near side is to the right, the far side to the left. At the upper right is the large, dark Oceanus Procellarum; below it is the smaller Mare Humorum. These, like the small dark Mare Orientale in the center of the basin, formed over 3 billion years ago as basaltic lava flows. At the lower left, among the southern cratered highlands of the far side, is the South-Pole-Aitken Basin, similar to Orientale but twice as great in diameter and much older and more degraded by crating and weathering. The cratered highlights of the near and far sides and the Maria are covered with scattered bright, young ray-craters.
Moon taken by Galileo after completing its first Earth Gravity Assist
This image of the crescent moon was obtained by the Galileo Solid State imaging system on December 8 at 5 a.m. PST as NASA Galileo spacecraft neared the Earth.  http://photojournal.jpl.nasa.gov/catalog/PIA00224
Moon - Western Near Side
These four images of the Moon are from data acquired by NASA Galileo spacecraft Near-Earth Mapping Spectrometer during Galileo December 1992 Earth/Moon flyby.  http://photojournal.jpl.nasa.gov/catalog/PIA00231
Moon As Seen By NIMS
STS034-72-070 (18 Oct 1989) --- Backdropped against the blackness of space, the Galileo spacecraft and its inertial upper stage (IUS) begin relative separation from the Earth-orbiting Space Shuttle Atlantis. The five-member STS-34 crew deployed the Jupiter-bound satellite within six hours of achieving Earth orbit on Oct. 18, 1989. The scene was exposed with a 70mm handheld Hasselblad camera.
STS-34 Galileo spacecraft / inertial upper stage (IUS) deployment
S89-42940 (April 1989) --- In this artist's rendition, the Galileo spacecraft is being boosted into its inter-planetary trajectory by the Inertial Upper Stage (IUS) rocket.  The Space Shuttle Atlantis, which is scheduled to take Galileo and the IUS from Earth's surface into space, is depicted against the curve of Earth.  Galileo will be placed on a trajectory to Venus, from which it will return to Earth at higher velocity and then gain still more energy in two gravity-assist passes, until it has enough velocity to reach Jupiter.  Passing Venus, it will take scientific data using instruments designed for observing Jupiter; later, it will make measurements at Earth and the moon, crossing above the moon's north pole in the second pass.  Between the two Earth passes, it will edge into the asteroid belt, beyond Mars' orbit; there, the first close-up observation of an asteroid is planned.  Crossing the belt later, another asteroid flyby is possible.
Artist concept of Galileo with inertial upper stage (IUS) in low Earth orbit
This montage of 11 images taken by NASA Galileo spacecraft as it flew by the asteroid Gaspra on Oct. 1991, shows Gaspra growing progressively larger in the field of view of Galileo solid-state imaging camera as the spacecraft approached the asteroid.  http://photojournal.jpl.nasa.gov/catalog/PIA00079
Gaspra Approach Sequence
During the G7 encounter, NASA Galileo spacecraft observed the shadow of Europa on the clouds of Jupiter during Galileo fourth orbit. The bright spot in the clouds is an atmospheric hot spot.
NIMS Observes Europa Shadow
NASA Galileo spacecraft acquired this global mosaic right during Galileo third orbit on Nov. 4, 1996. The lighter bluish area in the upper latitudes is the Asgard multi-ring structure with crater Burr to the north and Tornasuk to the east.
NIMS Callisto Global Mosaic
Artist rendering of NASA Galileo spacecraft flying past Jupiter moon Io. Galileo made multiple close approaches to the volcanically active moon during its time at Jupiter.  http://photojournal.jpl.nasa.gov/catalog/PIA18176
Galileo Over Io Artist Concept
This picture contains two images of Jupiter moon Io and its surrounding sky. This image was taken by NASA Galileo spacecraft in 1996.
Io Sodium Cloud Clear Filter and Green-Yellow Filter with Intensity Contours
The mottled face of Jupiter volcanically active moon Io as viewed by NASA Galileo spacecraft.  http://photojournal.jpl.nasa.gov/catalog/PIA00282
Io - Full Disk Centered on Media Regio
This image from NASA Galileo spacecraft is of Prometheus sunlit plume and Io illuminated crescent.
Io Sodium Cloud Clear and Green-Yellow Filters
This observation of a small section of the Asgard terrain reveals compositional variations over the surface of Callisto was captured by NASA Galileo spacecraft in 1996.
Compositional Variations in Callisto Asgard Impact Structure
Roughly true color image of the Great Red Spot of Jupiter as taken by NASA Galileo spacecraft on June 26, 1996.
True Color of Jupiter Great Red Spot
NASA Galileo spacecraft imaged Io at high spectral resolution during the G2 encounter on Sept. 6, 1996.
Hotspots on Io During the Ganymede 2 Encounter
This image from NASA Galileo spacecraft is of Jupiter moon Io and its surrounding sky is shown in false color.
Io Sodium Cloud On-Chip Format Clear and Green-Yellow Filters Superimposed
The three LEGO figurines flying aboard the Juno spacecraft are the Roman god Jupiter, his wife Juno and Galileo Galilei.
Riding Along with Juno
A very active volcano on Jupiter moon Io, probably composed of erupting lava fountains, was seen by NASA Galileo spacecraft.
Eruption from High Latitude Caldera Viewed by the Near-Infrared Mapping Spectrometer NIMS
This image of the moon was obtained by the Galileo Solid State imaging system on Dec. 8 at 7 p.m. PST as NASA Galileo spacecraft passed the Earth and was able to view the lunar surface from a vantage point not possible from the Earth.  http://photojournal.jpl.nasa.gov/catalog/PIA00225
Far Side of the Moon
On June 27, 1996, during Galileo first orbit around Jupiter, a newly discovered impact crater could be seen just right of the center of this image of Jupiter moon Europa returned by NASA Galileo spacecraft camera.  http://photojournal.jpl.nasa.gov/catalog/PIA00294
Europa Active Surface
Eight days after its encounter with the Earth, the Galileo spacecraft was able to look back and capture this remarkable view of the Moon in orbit about the Earth, taken from a distance of about 6.2 million kilometers (3.9 million miles). The picture was constructed from images taken through the violet, red, and 1.0-micron infrared filters. The Moon is in the foreground, moving from left to right. The brightly-colored Earth contrasts strongly with the Moon, which reflects only about one-third as much sunlight as the Earth. Contrast and color have been computer-enhanced for both objects to improve visibility. Antarctica is visible through clouds (bottom). The Moon's far side is seen; the shadowy indentation in the dawn terminator is the south-Pole/Aitken Basin, one of the largest and oldest lunar impact features. Alternate Jet Propulsion Laboratory (JPL) number is P-41508. View appears in the Space News Roundup v32 n1 p1, 01-11-93.
Galileo view of Moon orbiting the Earth taken from 3.9 million miles
These images demonstrate the dramatic improvement in the resolution of pictures that NASA Galileo spacecraft returned compared to previous images of the Jupiter system.  http://photojournal.jpl.nasa.gov/catalog/PIA00277
Ganymede - Comparison of Voyager and Galileo Resolution
This color image of the Earth was obtained by NASA’s Galileo spacecraft on Dec. 11, 1990, when the spacecraft was about 1.5 million miles from the Earth.  http://photojournal.jpl.nasa.gov/catalog/PIA00122
Earth - India and Australia
This color image of the Earth was obtained by NASA’s Galileo spacecraft early Dec. 12, 1990, when the spacecraft was about 1.6 million miles from the Earth.  http://photojournal.jpl.nasa.gov/catalog/PIA00123
Earth - Pacific Ocean
This image was acquired on May 6, 1997 while Io was in eclipse in Jupiter shadow during NASA Galileo spacecraft eighth orbit, and reveals several dynamic processes.
Io Eclipse/Volcanic Eruption
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in a Methane Band Time Set 1
This image shows the region around the Prometheus volcano on Jupiter moon Io. It was observed by NASA Galileo spacecraft in 1996 as it was flying away from a close approach to Io.
Io Prometheus Regions as Viewed by Galileo NIMS
Volcanic hot spots are seen in this color temperature map of the Prometheus volcano on Jupiter moon Io created with data obtained by NASA Galileo and Voyager spacecraft.
Prometheus/NIMS
This mosaic of Jupiter’s moon Ganymede consists of more than 100 images acquired with NASA’s Voyager and Galileo spacecrafts, showing irregular lumps beneath the icy surface.
Lumps Within Ganymede
This is an image of Io, taken by NASA Galileo spacecraft during the G2 encounter in September 1996. This is a dayside image of Io on the right against the clouds of Jupiter the blue background.
NIMS: hotspots on Io during G2 continued
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in a Methane Band Time Set 2
Topographic detail is seen in a stereoscopic view of this part of Jupiter moon Ganymede. This image is a computer reconstruction from two images taken by NASA Galileo spacecraft in 1996.
Stereo View of Ganymede Galileo Regio
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in Violet Light Time Set 1
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in a Methane Band Time Set 3
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in the Near-Infrared Time Set 4
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in a Methane Band Time Set 1
This mosaic shows the features of Jupiter main visible cloud deck and the hazy cloud layer above it as seen by NASA Galileo spacecraft on April 3, 1997.
Jupiter Northern Hemisphere in Violet Light Time Set 2
NASA Galileo spacecraft imaged most of Europa, including the north polar regions, at high spectral resolution during the G1 encounter on June 28, 1996.
NIMS G1 Observation of Europa
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in a Methane Band Time Set 2
Bright scars on a darker surface testify to a long history of impacts on Jupiter moon Callisto in this image of Callisto from NASA Galileo spacecraft.
Global Callisto in Color
Repeated flybys of Io by NASA Galileo spacecraft have allowed scientists to develop an understanding of Io Tohil-Culann region of interconnected volcanoes and mountains.
Io Culann-Tohil Region in Color
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in the Near-Infrared Time Set 2
New and older lava flows clustered in the Tvashtar region of Jupiter moon Io appeared as hot spots in a temperature map from NASA Galileo spacecraft in 1999.
Io Tvashtar Area in Infrared: Multiple Lava Flows
Three LEGO figurines representing the Roman god Jupiter, his wife Juno and Galileo Galilei are shown here aboard the Juno spacecraft.
LEGO Figurines Aboard Juno
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in Violet Light Time Set 3
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in the Near-Infrared Time Set 1
Jupiter atmospheric circulation is dominated by alternating eastward and westward jets from equatorial to polar latitudes. This image was taken on April 3, 1997, by NASA Galileo spacecraft.
Jupiter Northern Hemisphere in the Near-Infrared Time Set 3
Pele, one of Io best-known volcanoes, was observed by NASA Galileo spacecraft, during the flyby of Jupiter moon Io on February 22, 2000.
Temperature Map of Pele, Io
This enhanced color image shows cracks and ridges on Europa surface that reveal a detailed geologic history. The view was captured by NASA Galileo spacecraft on February 2, 1999.
Cracks and Ridges on Europa
STS034-71-000AK (18 Oct 1989) --- Backdropped against the blackness of space, the Galileo spacecraft and its inertial upper stage (IUS) have just detached from a cradle-like device aboard the Earth-orbiting Space Shuttle Atlantis to begin a six-year journey to Jupiter.  The five-member STS-34 crew deployed the satellite within six hours of achieving Earth orbit on Oct. 18, 1989.  The scene was exposed with a 70mm handheld Hasselblad camera.  Earth's horizon and a thin line representing its airglow and atmosphere are visible on the left side of the frame.
STS-34 Galileo spacecraft / IUS deployment sequence in OV-104's payload bay
This global view of Europa shows the location of a four-frame mosaic of images taken by NASA Galileo spacecraft in 1996, set into low-resolution data obtained by NASA Voyager spacecraft in 1979.
Context of Europa images from Galileo
To present the best information in a single view of Jupiter moon Ganymede, a global image mosaic was assembled, incorporating the best available imagery from NASA Voyager 1 and 2 spacecraft and NASA Galileo spacecraft.
Ganymede Global Geologic Map and Global Image Mosaic
This is a frame from an animation of a rotating globe of Jupiter moon Ganymede, with a geologic map superimposed over a global color mosaic, incorporating the best available imagery from NASA Voyager 1 and 2 spacecraft, and Galileo spacecraft.
Rotating Globe of Ganymede Geology
These images compare surface features observed by NASA Cassini spacecraft at the Xanadu region on Saturn moon Titan left, and features observed by NASA Galileo spacecraft on Jupiter cratered moon Callisto right.
Titan and Callisto
Three full-disk color views of Jupiter volcanic moon Io as seen by NASA Galileo spacecraft are shown in enhanced color to highlight details of the surface.  http://photojournal.jpl.nasa.gov/catalog/PIA00292
Three Views of Io
This view of the north polar region of the Moon was obtained by NASA's Galileo camera during the spacecraft flyby of the Earth-Moon system on December 7 and 8, 1992.  http://photojournal.jpl.nasa.gov/catalog/PIA00126
Moon - North Pole
During its flight, NASA’s Galileo spacecraft returned images of the Earth and Moon. Separate images of the Earth and Moon were combined to generate this view.  http://photojournal.jpl.nasa.gov/catalog/PIA00342
The Earth & Moon
These two images of Venus from NASA Galileo spacecraft show the global structure of cloud patterns at two different depths in the upper cloud layers.  http://photojournal.jpl.nasa.gov/catalog/PIA00073
Venus as Viewed Through Violet and Near Infrared Filters
This composite image shows the asteroid 243 Ida as seen from NASA's Galileo spacecraft during its approach on August 28, 1993.  http://photojournal.jpl.nasa.gov/catalog/PIA00137
Asteroid Ida - 6 Views Showing Rotation
This picture of Venus was taken by the NASA Galileo spacecraft Solid State Imaging System on February 14, 1990, at a range of almost 1.7 million miles from the planet.  http://photojournal.jpl.nasa.gov/catalog/PIA00072
Venus Cloud Patterns colorized and filtered
NASA Galileo spacecraft, now in orbit around Jupiter, returned this optical navigation image June 3, 1996, showing that the spacecraft is accurately targeted for its first flyby of the giant moon Ganymede on June 27.  http://photojournal.jpl.nasa.gov/catalog/PIA00273
Optical Navigation Image of Ganymede
Two sets of laser pulses transmitted from Earth to a spacecraft over a distance of 1.4 million kilometers 870,000 miles in a communications experiment are shown in this long-exposure image made by NASA’s Galileo spacecraft imaging system.  http://photojournal.jpl.nasa.gov/catalog/PIA00230
Galileo Optical Experiment GOPEX
This color image of the Earth was obtained by NASA Galileo spacecraft in Dec. 1990, when the spacecraft was about 1.5 million miles from the Earth. Africa stretches from the center to the top of the picture with the Arabian Peninsula off to its right.  http://photojournal.jpl.nasa.gov/catalog/PIA00076
Earth - Full Disk View of Africa
These images of the surface of the Jovian moon Europa, taken by NASA's Galileo spacecraft, focus on a "region of interest" on the icy moon.      The image at left traces the location of the erupting plumes of material, observed by NASA's Hubble Space Telescope in 2014 and again in 2016. The plumes are located inside the area surrounded by the green oval.      The green oval also corresponds to a warm region on Europa's surface, as identified by the temperature map at right. The map is based on observations by the Galileo spacecraft. The warmest area is colored bright red.      Researchers speculate these data offer circumstantial evidence for unusual activity that may be related to a subsurface ocean on Europa. The dark circle just below center in both images is a crater and is not thought to be related to the warm spot or the plume activity.  https://photojournal.jpl.nasa.gov/catalog/PIA21444
Europa Plumes Located near Warm Spot on Europa
Changes in the volcanoes on Jupiter moon Io can be seen in these three views, taken by NASA Galileo spacecraft during its three flybys of Io in October 1999, November 1999 and February 2000.
Myriad of Hot Spots on Io
This false-color mosaic of part of the Moon was constructed from 54 images taken by the imaging system aboard NASA's Galileo as the spacecraft flew past the Moon on December 7, 1992.  http://photojournal.jpl.nasa.gov/catalog/PIA00129
Moon - False Color Mosaic
This image of Jupiter moon Io and its surrounding sky is shown in false color. This image was taken on Nov. 9, 1996 through the green-yellow filter of the solid state imaging CCD system aboard NASA Galileo spacecraft.
Io Sodium Cloud Green-yellow Filter
Sulfur dioxide, normally a gas at room temperatures, is known to exist on Io surface as a frost, condensing there from the hot gases emanating from the Io volcanoes. This image was taken in 1996 by NASA Galileo spacecraft.
Distribution of Sulfur Dioxide Frost on Io
These two images of Jupiter atmosphere were taken by NASA Galileo spacecraft on June 26, 1996. The bright white spot in the center of each image is to the northwest of Jupiter Great Red Spot GRS.
Time changes in Storm Clouds in Jupiter Atmosphere
The Culann Patera volcano on Jupiter moon Io was observed by the near-infrared mapping spectrometer instrument onboard NASA Galileo spacecraft during its Io flyby on Nov. 25, 1999.
Culann Patera/NIMS
This view of the Moon north pole is a mosaic assembled from 18 images taken by NASA's Galileo imaging system through a green filter as the spacecraft flew by on December 7, 1992.  http://photojournal.jpl.nasa.gov/catalog/PIA00130
Moon - North Pole Mosaic
In August 2001, NASA Galileo spacecraft has returned imagery of a hot spot on Jupiter moon Io that was the source of a towering plume indicating a sulfur-dioxide concentration that may have been fallout from the plume.
A New Hot Spot on Northern Io
This image shows Loki, the most powerful volcano in the solar system, which has been constantly active on Jupiter moon Io. NASA Galileo spacecraft took these images during its approach to Io on October 10, 1999.
Loki as viewed by Galileo NIMS
Reddish spots and shallow pits pepper the enigmatic ridged surface of Europa in this view combining information from images taken by NASA Galileo spacecraft during two different orbits around Jupiter.
Ruddy Freckles on Europa
Jupiter moon Europa, as seen in this image taken June 27, 1996 by NASA Galileo spacecraft, displays features in some areas resembling ice floes seen in Earth polar seas.  http://photojournal.jpl.nasa.gov/catalog/PIA00291
Europa Broken Ice
This near-infrared photograph of the Earth was taken by the Galileo spacecraft at 6:07 a.m. PST on Dec. 11, 1990, at a range of about 1.32 million miles. South America is prominent near the center.  http://photojournal.jpl.nasa.gov/catalog/PIA00226
Global View of Earth in the Near-Infrared
Wonderful colors in a volcanic crater named Tupan Patera on Jupiter moon Io, as seen in this image from NASA Galileo spacecraft, show varied results of lava interacting with sulfur-rich materials.
Colorful Tupan Patera, Io
These images of Jupiter moon Amalthea were taken with NASA Galileo and Voyager spacecraft. Amalthea is almost pure water ice, hinting that it may not have formed where it now orbits.
Amalthea, A Rubble-Pile Moon
These views of Callisto southern hemisphere were taken by NASA Galileo spacecraft on May 6, 1997. The upper left view contains Buri, a crater with a diameter of about 60 km.
Callisto Southern Hemisphere
This artist concept, a cutaway view of Jupiter moon Callisto, is based on recent data from NASA Galileo spacecraft which indicates a salty ocean may lie beneath Callisto icy crust.
Callisto Cutaway with Ocean Artist Concept
This enhanced-color view obtained on September 25, 1998 from NASA Galileo spacecraft shows an intricate pattern of linear fractures on the icy surface of Jupiter moon Europa.
Europa Varied Surface Features
These mosaics 6 frames each show the appearance of the Great Red Spot in infrared light obtained on June 26, 1996 by the Solid State Imaging system on board NASA Galileo spacecraft.
The Great Red Spot at Four Different Wavelengths
Hot eruption sites scattered across Jupiter moon Io stand out dramatically in an infrared image taken Oct. 13, 2001, by NASA Galileo spacecraft as it sped past this most volcanically active of all known worlds.
Io in Infrared, Night and Day
This image, taken by NASA Galileo spacecraft, shows the darkside of Jupiter, the part not illuminated by sunlight. The curved line crossing from the lower left to the upper right is the auroral arc on the horizon.
Aurora Borealis on Jupiter
The active volcano Prometheus on Jupiter moon Io was imaged by NASA Galileo spacecraft during the close flyby of Io on Oct.10, 1999. The spectrometer can detect active volcanoes on Io by measuring their heat in the near-infrared wavelengths.
Galileo Near-Infrared Mapping Spectrometer Detects Active Lava Flows at Prometheus Volcano, Io
This color image of the Simpson Desert in Australia was obtained by NASA’s Galileo spacecraft at about 2:30 p.m. PST, Dec. 8, 1990, at a range of more than 35,000 miles.   http://photojournal.jpl.nasa.gov/catalog/PIA00115
Earth - Simpson Desert, Central Australia
This colorized image of Europa is a product of clear-filter grayscale data from one orbit of NASA Galileo spacecraft, combined with lower-resolution color data taken on a different orbit.
Reddish Bands on Europa
This view of Cilix impact crater on Europa was created in 2013 using 3-D stereo images taken by NASA Galileo spacecraft, combined with advanced image processing techniques.
3-D Cilix Crater on Europa
This false color image of the Eastern Coast of Australia was obtained by NASA’s Galileo spacecraft at about 3:00 p.m. PST, Dec. 8, 1990, at a range of more than 35,000 miles.  http://photojournal.jpl.nasa.gov/catalog/PIA00121
Earth - Eastern Australia Coast
This color picture is made from images taken by the imaging system on NASA Galileo spacecraft about 14 minutes before its closest approach to asteroid 243 Ida on August 28, 1993.  http://photojournal.jpl.nasa.gov/catalog/PIA00069
Ida and Dactyl in Enhanced Color
This image of the western hemisphere of the Moon was taken through a green filter by NASA's Galileo spacecraft at 9:35 a.m. PST Dec. 9 at a range of about 350,000 miles. In the center is the Orientale Basin.  http://photojournal.jpl.nasa.gov/catalog/PIA00120
Moon - Western Hemisphere
This first image of asteroid 951 Gaspra was taken by NASA Galileo spacecraft on October 29, 1991, from a distance of 16,200 kilometers 10,000 miles. The Sun is shining from the right.  http://photojournal.jpl.nasa.gov/catalog/PIA00228
Gaspra - First Image