Asteroid Vesta Imagery

Diverse images from NASA's Dawn spacecraft showcasing the terrain and surface details of asteroid Vesta, including color variations and geological features.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Sextilia quadrangle, in Vesta's southern hemisphere.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Urbinia quadrangle, in Vesta's southern hemisphere.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Urbinia quadrangle, in asteroid Vesta's southern hemisphere.

These composite images from NASA's Dawn spacecraft show three views of a terrain with ridges and grooves near Aquilia crater in the southern hemisphere of the giant asteroid Vesta.

These images from NASA's Dawn spacecraft show the brightness/darkness of asteroid Vesta's surface. These images are located in Vesta's Marcia quadrangle.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Sextilia quadrangle, in Vesta's southern hemisphere.

NASA's Dawn spacecraft of asteroid Vesta shows the apparent brightness of asteroid Vesta's surface. Aquilia crater, located in Vesta's Pinaria quadrangle, is the large crater that dominates the top part of both images.

These apparent brightness and topography images from NASA's Dawn spacecraft are located in asteroid Vesta's Gegania quadrangle, in Vesta's southern hemisphere.

Located in the Marcia quadrangle, the left-hand image from NASA's Dawn spacecraft shows the apparent brightness of asteroid Vesta's surface. The right-hand image is based on this apparent brightness image.

These images from NASA's Dawn spacecraft show Urbinia crater on asteroid Vesta. Urbinia crater is distinctive because is has an irregularly shaped rim due to the formation of other impact craters along its rim and then subsequent erosion.

These composite images from NASA's Dawn spacecraft show three views of a terrain with ridges and grooves near Aquilia crater in the southern hemisphere of the giant asteroid Vesta.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Tuccia quadrangle, in Vesta's southern hemisphere.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Tuccia quadrangle, in Vesta's southern hemisphere.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Numisia quadrangle, a few degrees below Vesta's equator.

The color coding on this CRISM composite image of an area on Mars is based on infrared spectral information interpreted as evidence of various minerals present. Carbonate, which is indicative of a wet and non-acidic history, occurs in very small patches.

A Martian target rock called 'Nova,' shown here, displayed an increasing concentration of aluminum as a series of laser shots from NASA's Curiosity Mars rover penetrated through dust on the rock's surface.

CRISM's First 'Targeted' Observation of Mars

Livonia, New York, Students Study Past Martian Water

NASA's Dawn spacecraft shows the area surrounding the 'snowman craters' in asteroid Vesta's northern hemisphere.

These apparent brightness and topography images from NASA's Dawn spacecraft are located in asteroid Vesta's Floronia quadrangle, in Vesta's northern hemisphere.

Depth-to-Ice Map of an Arctic Site on Mars

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Numisia quadrangle, in Vesta's northern hemisphere.

Two different instruments on NASA's Cassini spacecraft combined their observations to create a more detailed portrait of the Hotei Regio area on Saturn's moon Titan. Blue lines on top show the location of channels that stand out in the bottom of image.

NASA Mars Odyssey observations are used in this global view of Mars in intermediate-energy, or epithermal, neutrons. Soil enriched by hydrogen is indicated by the deep blue colors on the map, which show a low intensity of epithermal neutrons.

This 3-D stereo view from NASA's Mars rover Opportunity shows contrasting textures and colors of 'Hinners Point,' at the northern edge of 'Marathon Valley,' and swirling reddish zones on the valley floor to the left.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Sextilia quadrangle, in Vesta's southern hemisphere.

This image montage features a two-dimensional radar cross section of Mars' north polar cap collected by SHARAD instrument on NASA's Mars Reconnaissance Orbiter spacecraft (top), and a color image mosaic of the polar cap from NASA's Viking project (bottom)

Titan's Surface

NASA's Dawn spacecraft obtained these images with its framing camera on Aug.17 and Sept.17, 2011. The left hand image shows scarps, mostly near the bottom. The right hand image is a close up, higher resolution view of a large part of the raised mound.

Topographic data provided by NASA's Shuttle Radar Topography Mission can provide many clues to geologic history and processes.

Vigorous vegetation growth in the Southern United States after heavy rains fell during April and early May, 2004, is quantified in these images and data products from NASA's Terra spacecraft.

This image from NASA's Dawn mission shows the varied minerals on the surface of the giant asteroid Vesta in false color.

NASA's Dawn spacecraft shows the central area of the south polar basin. The mountain-central complex is the roughly circular feature in the center of the image.

This topographic image acquired in February 2000 by NASA's Shuttle Radar Topography Mission (SRTM) shows an area south of the Sao Francisco River in Brazil.

The San Andreas Fault and a Strike-slip Fault on Europa

This is a three-dimensional perspective view of Saline Valley, about 30 km (19 miles) east of the town of Independence, California created by combining two spaceborne radar images using a technique known as interferometry.

This perspective view of Venus, generated by computer from Magellan data and color-coded with emissivity, shows the impact crater Markham, named after the English aviator Beryl Markham (the crater was briefly known unofficially as Franklin; the earlier name was not approved by the Nomenclature Committee of the International Astronomical Union). Markham, with a diameter of 71 km, is one of more than 400 Venusian craters whose formation triggered the outflow of highly fluid materials. .

The view from NASA's Magellan spacecraft shows most of Galindo (V-40) quadrangle looking east; Atete Corona, in the foreground, is a 600-km-long and about 450-km-wide, circular volcano-tectonic feature.

South Polar Terrains of Enceladus - Highest Resolution View

This image is a shortened version of a 360-degree panorama taken by the Opportunity rover's Panoramic Camera (Pancam) from May 13 through June 10, 2018, or sols (Martian days) 5,084 through 5,111. This is the last panorama Opportunity acquired before the solar-powered rover succumbed to a global Martian dust storm on the same June 10. The panorama appears in 3D when seen through blue-red glasses with the red lens on the left. To the right of center and near the top of the frame, the rim of Endeavour Crater rises in the distance. Just to the left of that, rover tracks begin their descent from over the horizon towards the location that would become Opportunity's final resting spot in Perseverance Valley, where the panorama was taken. At the bottom, just left of center, is the rocky outcrop Opportunity was investigating with the instruments on its robotic arm. To the right of center and halfway down the of the frame is another rocky outcrop about 23 feet (7 meters) distant from the camera

Data from NASA's Cassini spacecraft have enabled scientists to make the highest-resolution heat intensity maps yet for the hottest part of a 'tiger stripe' fissure on Saturn's moon Enceladus.

This map shows footprints of images taken from Mars orbit by the HiRISE camera onbard NASA's Mars Reconnaissance Orbiter as part of advance analysis of the area where NASA's InSight mission will land in 2018.

First HiRISE Image of Mars: Topographic Model from Photoclinometry

The area where NASA's Curiosity rover will land on Aug. 5 PDT (Aug. 6 EDT) has a geological diversity that scientists are eager to investigate, as seen in this false-color map based on data from NASA's Mars Odyssey orbiter.

Six Landing Sites on Mars

This image shows the landing site of NASA's Curiosity rover and destinations scientists want to investigate. Curiosity landed inside Gale Crater on Mars on Aug. 5 PDT (Aug. 6 EDT) at the green dot, within the Yellowknife quadrangle.

A global map of Jupiter's moon Io derived from eight images taken by the Long Range Reconnaissance Imager (LORRI) on the New Horizons spacecraft, as it passed Jupiter on its way to Pluto in late February 2007.

This perspective view acquired by NASA's Shuttle Radar Topography Mission (SRTM) from data collected in the year 2000 shows Patagonia, Argentina, a spectacular landscape formed by volcanoes, rivers, and wind.

ECOSTRESS acquired this image the night of July 9, 2018, over Egypt. Yellow and red indicate generally higher temperatures. The River Nile is visible as a thin blue line on the main image. The black-and-white inset shows the level of detail available from ECOSTRESS, with the relatively cool Nile River and surrounding vegetation appearing darker.

Potassium Concentrations on Mars

Researchers estimating the amount of carbon held in the ground at the largest known carbonate-containing deposit on Mars utilized data including physical properties from THEMIS (left) and mineral information from CRISM (right).

Mars Through Infrared Eyes of Spirit-3

Four Types of Deposits From Wet Conditions on Early Mars

Bouncing Down to Mars

These L-band images of the Manaus region of Brazil were acquired by NASA's Spaceborne Imaging Radar-C and X-band Synthetic Aperture Radar (SIR-C/X-SAR) aboard the space shuttle Endeavour.

This map shows the topography of the south polar region of Mars, including topography buried by thick deposits of icy material

3-D View of Mars Particle

Volcanism and erosion are prominently seen in this view of the eastern flank of the Andes Mountains taken by NASA's Shuttle Radar Topography Mission (SRTM).

Map of Iapetus - May 2008

Liquid Lakes on Titan

Curiosity's Quadrant Themes. This map shows all the quadrant themes for NASA's Curiosity Mars rover, which is currently in the Roraima quadrant seen at the bottom. The red oval indicates the landing ellipse where the rover was targeted to touch down in 2012. The yellow-tinted quadrants are areas the rover has driven through since then. Themes are chosen in advance of the rover's arrival in a new quadrant; the rover's path couldn't be planned until after the team knew where it landed. Martian latitude and longitude is provided around the outside of the map. With the Curiosity mission, scientists began using quadrant themes to organize the long lists of unofficial nicknames needed to catalog its observations, whether hills, craters, boulders, rocks, and even tiny features on rock surfaces. Scientist deplete these lists of names quickly - especially with Curiosity, which has used more than 10,000 names over nearly 11 years of exploring Mars. Different science targets all require names - i

The lower portion of a mountain inside Gale crater on Mars contains layers that may be examined by NASA's Mars Science Laboratory. A landing site in Gale, close to the foot of the mountain, has been selected for the mission.

Northern Topography

Active Cryovolcanic Features on Titan

New QuickMap Feature: 3-D!

Images from NASA's New Horizons mission suggest that Pluto's largest moon, Charon, once had a subsurface ocean that has long since frozen and expanded, pushing out on the moon's surface.

This annotated image, taken in 2014, shows where features seen in an observation by NASA's Mars Reconnaissance Orbiter have been interpreted as hardware from the Dec. 25, 2003, arrival at Mars of the United Kingdom's Beagle 2 Lander.

NASA's Lunar Reconnaissance Orbiter captures high noon at Tranquility Base.

Polar Stereographic Projection

A depression called 'Scamander Crater,' dominates the terrain near NASA's Mars Exploration Rover Spirit in this map that emphasizes local topography by removing the regional tilt to the northwest.

This area was designated 'Region D' in the process of evaluating potential landing sites for NASA's Phoenix Mars Lander. The topographical information is from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor orbiter.

NASA's Mars Exploration Rover Spirit drove a total of 4,143 meters (2.57 miles) between its landing in January 2004 and its 404th martian day, or sol (Feb. 20, 2005). This map on an image taken by the Mars Orbiter Camera on NASA's Mars Global Surveyor shows the course the rover drove during that time. The rover has recently been approaching a ridge overlooking Tennessee Valley on the north flank of Husband Hill. http //photojournal.jpl.nasa.gov/catalog/PIA07393

Elevations Within the Floor of the Valles Marineris

Images from Phoenix's MECA Instruments

Opportunity Traverse Map, 'Eagle' to 'Victoria'

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.

This image is a shaded relief mosaic of Umnak Island in Alaska's Aleutian Islands acquired by NASA's Airborne Synthetic Aperture Radar (AIRSAR) in 2001.

Mars Orbiter Camera High Resolution Images: Some Results From The First 6 Weeks In Orbit

A 300-mile-long linear gravity anomaly on the far side of the moon has been revealed by gravity gradients measured by NASA's GRAIL mission. GRAIL data are shown on the left, with red and blue corresponding to stronger gravity gradients.

a Category 5 storm.

These images were obtained by the Dawn spacecraft on July 23, 2011. The bottom two images are false-color, where different colors represent visible and infrared light wavelengths.

Three-Dimensional Perspective View of Eistla Regio on Venus by Magellan (Digitally Generated)

NASA's Terra spacecraft captured these views of the dust and sand that swept over northeast China on March 10, 2004.

An Olivine-Rich Crater in Tyrrhena Terra

MLA Montage

MGS MOC Release No. MOC2-319, 8 August 2002. Inca City is the informal name given by Mariner 9 scientists in 1972 to a set of intersecting, rectilinear ridges that are located among the layered materials of the south polar region of Mars. Their origin has never been understood; most investigators thought they might be sand dunes, either modern dunes or, more likely, dunes that were buried, hardened, then exhumed. Others considered them to be dikes formed by injection of molten rock (magma) or soft sediment into subsurface cracks that subsequently hardened and then were exposed at the surface by wind erosion. The Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) has provided new information about the Inca City ridges, though the camera's images still do not solve the mystery. The new information comes in the form of a MOC red wide angle context frame taken in mid-southern spring, shown above left and above right. The original Mariner 9 view of the ridges is seen at the center. The MO

A major dust storm moved across the eastern and northeastern regions of Australia on Sept. 23, 2009, out towards the Pacific as seen by NASA's Aqua satellite.

This image illustrates how spacecraft landings on Mars have become more and more precise over the years. Since NASA's first Mars landing of Viking in 1976, the targeted landing regions, or ellipses, have shrunk.

This map of Ceres, constructed from data collected by NASA's Dawn spacecraft, shows the dwarf planet's surface with features that have been named as of August 14, 2015.

On this polar stereographic map of Enceladus' south polar terrain, all 100 geysers have been plotted whose source locations have been determined in NASA's Cassini's imaging survey of the moon's geyser basin.

NASA's Dawn spacecraft obtained these images with its visible and infrared instrument of asteroid Vesta. The top image is a simulated true-color picture of the asteroid's surface.

Magnetic Strips Preserve Record of Ancient Mars

This perspective view acquired by NASA's Shuttle Radar Topography Mission (SRTM) from data collected on February 18, 2000 shows three Hawaiian islands: Molokai (lower left), Lanai (right), and the northwest tip of Maui (upper left).

This map shows the route driven by NASA's Curiosity Mars rover from the 'Bradbury Landing' location where it landed in August 2012 (the start of the line in upper right) to a major waypoint called 'the Kimberley'.

MPL LANDING SITE - DEM

A look at smoke from the Chisholm forest fire, which ignited on May 23, 2001 about 160 kilometers north of Edmonton in Alberta, Canada, as seen by NASA's Terra spacecraft.

The Prometheus region of Jupiter's moon Io was imaged by NASA's Galileo spacecraft in 1999. The maps made from spectrometer data show the interplay between hot silicates on the surface and sulfur dioxide frost.

Air and oil bubbles inside water base form patterns

Topographic Profiles from the NEAR Laser Rangefinder

On Sept. 16, 2015, a magnitude 8.3 earthquake struck near the coast of central Chile along the boundary of the Nazca and South American tectonic plates. Maps known as interferograms show how the quake moved the ground, as observed by Sentinel-1A

wissenschaftlicher Bodenquerschnitt zur Erklärung von Subduktion und Plattentektonik - 3d-Illustration scientific ground cross-section to explain subduction and plate tectonics - 3d illustration Copyright: xZoonar.com/ChristophxBurgstedtx 22561209

of 2