Rohit Bhartia of NASA's Mars 2020 mission holds a slice of a meteorite scientists have determined came from Mars. This slice will likely be used here on Earth for testing a laser instrument for NASA's Mars 2020 rover; a separate slice will go to Mars on the rover. Martian meteorites are believed to be the result of impacts to the Red Planet's surface, resulting in rock being blasted into the atmosphere. After traveling through space for eons, some of these rocks entered Earth's atmosphere. Scientists determine whether they are true Martian meteorites based on their rock and noble gas chemistry and mineralogy. The gases trapped in these meteorites bear the unique fingerprint of the Martian atmosphere, as recorded by NASA's Viking mission in 1976. The rock types also show clear signs of igneous processing not possible on smaller bodies, such as asteroids. https://photojournal.jpl.nasa.gov/catalog/PIA22245

Close-up of a slice of a meteorite scientists have determined came from Mars. This slice will likely be used here on Earth for testing a laser instrument for NASA's Mars 2020 rover; a separate slice will go to Mars on the rover. Martian meteorites are believed to be the result of impacts to the Red Planet's surface, resulting in rock being heaved into the atmosphere. After traveling through space for eons, some of these rocks entered Earth's atmosphere. Scientists determine whether they are true Martian meteorites based on their rock and noble gas chemistry and mineralogy. The gases trapped in these meteorites bear the unique fingerprint of the Martian atmosphere, as recorded by NASA's Viking mission in 1976. The rock types also show clear signs of igneous processing not possible on smaller bodies, such as asteroids. https://photojournal.jpl.nasa.gov/catalog/PIA22246

Iron Meteorite on Mars

This 4.5 billion-year-old rock, labeled meteorite ALH84001, is one of 10 rocks from Mars in which researchers have found organic carbon compounds that originated on Mars without involvement of life. http://photojournal.jpl.nasa.gov/catalog/PIA00289

Possible Meteorite in Columbia Hills on Mars False Color

This rock encountered by NASA Curiosity Mars rover is an iron meteorite called Lebanon, similar in shape and luster to iron meteorites found on Mars by the previous generation of rovers, Spirit and Opportunity.

A slice of a meteorite scientists have determined came from Mars placed inside an oxygen plasma cleaner, which removes organics from the outside of surfaces. This slice will likely be used here on Earth for testing a laser instrument for NASA's Mars 2020 rover; a separate slice will go to Mars on the rover. Martian meteorites are believed to be the result of impacts to the Red Planet's surface, resulting in rock being blasted into the atmosphere. After traveling through space for eons, some of these rocks entered Earth's atmosphere. Scientists determine whether they are true Martian meteorites based on their rock and noble gas chemistry and mineralogy. The gases trapped in these meteorites bear the unique fingerprint of the Martian atmosphere, as recorded by NASA's Viking mission in 1976. The rock types also show clear signs of igneous processing not possible on smaller bodies, such as asteroids. https://photojournal.jpl.nasa.gov/catalog/PIA22247

This scanning electron microscope image of a polished thin section of a meteorite from Mars shows tunnels and curved microtunnels.

This slice of a Martian meteorite, seen floating inside the International Space Station, is now part of a calibration target for SuperCam, one of the instruments aboard NASA's Perseverance Mars rover. A piece of a different Martian meteorite is part of the calibration target for the instrument known as SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals). Scientists use calibration targets as a kind of default they can use to check and fine-tune the settings of their instruments. A small number of meteorites on Earth have been determined to have originated on Mars based on mineral and chemical analyses by past NASA spacecraft. https://photojournal.jpl.nasa.gov/catalog/PIA24179

This scanning electron microscope image shows speroidal features embedded in a layer of iddingsite, a mineral formed by action of water, in a meteorite that came from Mars.

Composition measurements by NASA Mars Exploration Rover Opportunity confirm that this rock on the Martian surface is an iron-nickel meteorite. 3D glasses are necessary to view this image.

This photograph shows orange-colored carbonate mineral globules found in a meteorite, called ALH84001, believed to have once been a part of Mars. http://photojournal.jpl.nasa.gov/catalog/PIA00290

This view of a rock called Block Island, the largest meteorite yet found on Mars, comes from the panoramic camera Pancam on NASA Mars Exploration Rover Opportunity.

In the center of this electron microscope image of a small chip from a meteorite are several tiny structures that are possible microscopic fossils of primitive, bacteria-like organisms that may have lived on Mars more than 3.6 billion years ago. http://photojournal.jpl.nasa.gov/catalog/PIA00283

The dark, smooth-surfaced object at the center of this Oct. 30, 2016, image from the Mast Camera (Mastcam) on NASA's Curiosity Mars rover was examined with laser pulses and confirmed to be an iron-nickel meteorite. The grid of shiny points visible on the object resulted from that laser zapping by Curiosity's Chemistry and Camera (ChemCam) instrument. The meteorite is about the size of a golf ball. It is informally named "Egg Rock," for a site in Maine. Locations around Bar Harbor, Maine, are the naming theme for an area on Mars' Mount Sharp that Curiosity reached in October. Iron-nickel meteorites are a common class of space rocks found on Earth, and previous examples have been found on Mars, but Egg Rock is the first on Mars to be examined with a laser-firing spectrometer. The scene is presented with a color adjustment that approximates white balancing, to resemble how the rocks and sand would appear under daytime lighting conditions on Earth. Figure 1 includes a scale bar of 5 centimeters (about 2 inches). http://photojournal.jpl.nasa.gov/catalog/PIA21134

The dark, golf-ball-size object in this composite, colorized view from the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity Mars rover shows a grid of shiny dots where ChemCam had fired laser pulses used for determining the chemical elements in the target's composition. The analysis confirmed that this object, informally named "Egg Rock," is an iron-nickel meteorite. Iron-nickel meteorites are a common class of space rocks found on Earth, and previous examples have been found on Mars, but Egg Rock is the first on Mars to be examined with a laser-firing spectrometer. The laser pulses on Oct. 30, 2016, induced bursts of glowing gas at the target, and ChemCam's spectrometer read the wavelengths of light from those bursts to gain information about the target's composition. The laser pulses also burned through the dark outer surface, exposing bright interior material. This view combines two images taken later the same day by ChemCam's remote micro-imager (RMI) camera, with color added from an image taken by Curiosity's Mast Camera (Mastcam). A Mastcam image of Egg Rock is at PIA21134. http://photojournal.jpl.nasa.gov/catalog/PIA21133

This iron-nickel meteorite found near Fort Stockton, Texas, in 1952 shows a surface texture similar to some portions of the surface of an iron-nickel meteorite that NASA Mars Exploration Rover Opportunity found on Mars in July, 2009.

NASA Mars Exploration Rover Opportunity has found a rock that apparently is another meteorite, less than three weeks after driving away from a larger meteorite that the rover examined for six weeks.

Philippe Étienne, French Ambassador to the U.S. touches a Mars meteorite at the NASA exhibit during the 70th International Astronautical Congress, Wednesday, Oct. 23, 2019, at the Walter E. Washington Convention Center in Washington. Photo credit: (NASA/Aubrey Gemignani)

NASA's Curiosity Mars rover captured this image of an iron-nickel meteorite nicknamed "Cacao" on Jan, 28, 2023, the 3,725th Martian day, or sol, of the mission. This meteorite, discovered in the "sulfate-bearing unit," a region on Mars' Mount Sharp, is estimated to be about 1 foot (30 centimeters) across. It's one of several meteorites Curiosity has seen while exploring Mars. Curiosity's Mast Camera, or Mastcam, took the panorama with its 100-millimeter focal length lens. The panorama is made up of 19 individual images that were stitched together after being sent to Earth. The color has been adjusted to match lighting conditions as the human eye would perceive them on Earth. https://photojournal.jpl.nasa.gov/catalog/PIA25737

The image is an excerpt from an observation from NASA Mars Reconnaissance Orbiter showing a meteorite impact that excavated this crater on Mars exposed bright ice that had been hidden just beneath the surface at this location.

This Mars Global Surveyor MGS Mars Orbiter Camera MOC image shows a field of small craters formed by secondary debris thrown from a larger meteoritic impact on the plains south of the Cerberus region

An artist's rendition of Mars, highlighting one of InSight's goals -- to figure out just how tectonically active Mars is today and how often meteorites impact it. Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, or InSight, is scheduled to launch from Vandenberg Air Force Base on the California coast between May 5 through June 8, 2018, and land on Mars six months later. InSight will give the Red Planet its first thorough check up since it formed, 4.5 billion years ago. The InSight lander carries a seismometer, SEIS, that listens to the pulse of Mars. The seismometer records the waves traveling through the interior structure of a planet. Studying seismic waves tells us what might be creating the waves. On Mars, scientists suspect that the waves may be caused by marsquakes, meteorites striking the surface, or hot, molten magma moving at great depths underneath the surface. https://photojournal.jpl.nasa.gov/catalog/PIA22230

Martian Meteorite (ALH84001) Life on Mars? Microscopic Fossils

An iron meteorite is the latest quarry for NASA Mars Exploration Rover Opportunity. Shown here is the left-eye view of a stereo pair of images. 3D glasses are necessary to view this image.

NASA Mars Exploration Rover Opportunity used its panoramic camera to capture this view of a dark rock the size of a toaster that may be an iron meteorite. Part of the rim of Endurance Crater is on the horizon.

If a meteorite breaks in two shortly before hitting the ground, the typical bowl shape of a single impact crater becomes doubled. This image is from NASA Mars Odyssey, one of an All Star set.

NASA Mars Exploration Rover Opportunity found this image of a meteorite. The science team used two tools on Opportunity arm, the microscopic imager and the alpha particle X-ray spectrometer, to inspect the rock texture and composition.

NASA Mars Exploration Rover Opportunity took this picture of a rock informally named Marquette Island as the rover was approaching the rock for investigations that have suggested the rock is a stony meteorite.

NASA Mars Exploration Rover Opportunity found and examined this meteorite. The science team used two tools on Opportunity arm, the microscopic imager and the alpha particle X-ray spectrometer, to inspect the rock texture and composition.

This doublet crater was formed when two meteorites impacted at the same time. The shock waves interact to form the straight central rim and the wings of ejecta on the outside of the rims. This image is from NASA Mars Odyssey.

S85-39565 (For release August 1996) --- According to scientists, this 4.5 billion year old rock, labeled meteorite ALH84001, is believed to have once been a part of Mars and to contain fossil evidence that primitive life may have existed on Mars more than 3.6 billion years ago. The rock is a portion of a meteorite that was dislodged from Mars by a huge impact about 16 million years ago and that fell to Earth in Antarctica 13,000 years ago. The meteorite was found in Allan Hills ice field, Antarctica, by an annual expedition of the National Science Foundation?s Antarctic Meteorite Program in 1984. It is preserved for study at the Johnson Space Center?s (JSC) Meteorite Processing Laboratory in Houston, Texas.

New results from the Sample Analysis at Mars, or SAM, instrument on NASA Curiosity rover detected about 2,000 times as much argon-40 as argon-36, which weighs less, confirming the connection between Mars and Martian meteorites found on Earth.

NASA Mars Exploration Rover Opportunity used its microscopic imager to get this view of the surface of a rock called Block Island during the 1,963rd Martian day, or sol, of the rover mission on Mars Aug. 1, 2009.

By providing a set of base measurements that were taken on Earth, this calibration target will help fine-tune the settings on the Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals (SHERLOC) instrument carried aboard NASA's Perseverance Mars rover. There are 10 kinds of materials on SHERLOC's calibration target, including a fragment of a Martian meteorite and five of the first spacesuit materials sent to Mars. They'll be observed to see how they hold up in the intense radiation on the Martian surface. https://photojournal.jpl.nasa.gov/catalog/PIA23980

An artist's impression of the InSight lander on Mars. InSight, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, is designed to give the Red Planet its first thorough check up since it formed 4.5 billion years ago. It is scheduled to launch from Vandenberg Air Force Base on the California coast between May 5 through June 8, 2018, and land on Mars six months later. InSight will look for tectonic activity and meteorite impacts, study how much heat is still flowing through the planet, and track Mars' wobble as it orbits the sun. While InSight is a Mars mission, it's more than a Mars mission. InSight will help answer key questions about the formation of the rocky planets of the solar system. https://photojournal.jpl.nasa.gov/catalog/PIA22226

Martian Meteorite (ALH84001): This high resolution transmission electron microscope image is of a cast, or replica, from a chip of a Martian meteorite, labeled ALH84001, that shows the outline of what are believed to be possible microscopic fossils of bacteria-like organisms that may have lived on Mars more than 3.6 billion years ago. The tubular features in this image are less than a micrometer in size, or about 1/500th the diameter of a human hair. (JSC ref: S96-12637)

The collision that created Hargraves Crater impacted into diverse bedrock lithologies of ancient Mars; the impact ejecta is a rich mix of rock types with different colors and textures, as seen by NASA Mars Reconnaissance Orbiter. The crater is named after Robert Hargraves who discovered and studied meteorite impacts on the Earth. https://photojournal.jpl.nasa.gov/catalog/PIA21609

This electron microscope image shows extremely tiny tubular structures that are possible microscopic fossils of bacteria-like organisms that may have lived on Mars more than 3.6 billion years ago. http://photojournal.jpl.nasa.gov/catalog/PIA00285

This electron microscope image shows egg-shaped structures, some of which may be possible microscopic fossils of Martian origin as discussed by NASA research published in the Aug. 16, 1996. http://photojournal.jpl.nasa.gov/catalog/PIA00286

This electron microscope image shows tubular structures of likely Martian origin. These structures are very similar in size and shape to extremely tiny microfossils found in some Earth rocks. http://photojournal.jpl.nasa.gov/catalog/PIA00287

This electron microscope image is a close-up of the center part of photo number S96-12301. http://photojournal.jpl.nasa.gov/catalog/PIA00284

This high-resolution scanning electron microscope image shows an unusual tube-like structural form that is less than 1/100th the width of a human hair in size found in meteorite ALH84001, a meteorite believed to be of Martian origin. http://photojournal.jpl.nasa.gov/catalog/PIA00288

Debris in space often impacts planets, and on Mars, we are finding new craters from recent impacts. The meteorite that caused the small crater in this image, just seven meters across, hit Mars sometime between April 2018 and January 2019. Context Camera images are used to identify changes in large areas and then HiRISE images are scheduled to verify that there is, indeed, a new crater on Mars. https://photojournal.jpl.nasa.gov/catalog/PIA23476

The calibration target for SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) an instrument on the end of the Perseverance Mars rover's 7-foot-long (3-meter-long) robotic arm, includes a geocaching target, spacesuit materials, and a slice of a Martian meteorite. Scientists rely on calibration targets to fine-tune instrument settings using materials with known properties. The bottom row of this target features spacesuit materials that scientists will observe to see how they react over time to the irradiated Martian atmosphere. The first sample at left is polycarbonate for use in a helmet visor; inscribed with the address of the fictional detective Sherlock Holmes, it doubles as a geochache for the public. Other materials in the bottom row, from left: Vectran; Ortho-Fabric; Teflon; coated Teflon. Top row, from left: aluminum gallium nitride on sapphire; a quartz diffuser; a slice of Martian meteorite; a maze for testing laser intensity; a separate aluminum gallium nitride on sapphire with different properties. https://photojournal.jpl.nasa.gov/catalog/PIA24261

An artist illustration of the InSight lander on Mars. InSight, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, is designed to give the Red Planet its first thorough check up since it formed 4.5 billion years ago. The mission will look for tectonic activity and meteorite impacts, study how much heat is still flowing through the planet, and track Mars' wobble as it orbits the sun. While InSight is a Mars mission, it's more than a Mars mission. InSight will help answer key questions about the formation of the rocky planets of the solar system. https://photojournal.jpl.nasa.gov/catalog/PIA22745

Meteorites hit Mars and create small craters like the one we've imaged here. Usually we spot these new craters in lower-resolution images from the Context Camera because the impact disturbs dust on the surface and creates a dark mark that's much bigger than the crater. This meteorite hit a dusty area and made a crater, but did something a little more special to the surrounding dust. We can see dozens of dark, dust-free, streaks on slopes surrounding the crater. These slope streaks form when dust slumps downhill and happen naturally on a regular basis. In this case though, the impact and explosion that made the crater seems to have set off many of these downhill slumps of dust simultaneously. This could have happened from the explosion's blast wave passing through the air or the shaking of the ground that it caused. https://photojournal.jpl.nasa.gov/catalog/PIA24382

This image captured by NASA 2001 Mars Odyssey spacecraft is located in Noachis Terra. The unnamed crater at the bottom of the image contains a central pit. Central features such as pits and peaks can provide information about both the impacted surface and the size of the meteorite. Orbit Number: 65680 Latitude: -28.4965 Longitude: 349.805 Instrument: VIS Captured: 2016-10-03 22:49 http://photojournal.jpl.nasa.gov/catalog/PIA21180

NASA scientist Trevor Graff peers at a calibration target, which will help fine-tune settings on the Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals (SHERLOC) instrument carried aboard NASA's Perseverance Mars rover. The calibration target is housed inside a special environmental chamber that was used to ship it from NASA's Johnson Space Center, Houston, to the agency's Jet Propulsion Laboratory in Southern California, where the target was added to the rover. There are 10 kinds of materials on SHERLOC's calibration target, including a fragment of a Martian meteorite and five of the first spacesuit materials sent to Mars. They'll be observed to see how they hold up in the intense radiation on the Martian surface. https://photojournal.jpl.nasa.gov/catalog/PIA23979

NASA's InSight lander placed its seismometer onto Mars on Dec. 19, 2018. This was the first time a seismometer had ever been placed onto the surface of another planet. The seismometer is the copper-colored object in this image, which was taken around Martian dusk. The seismometer, called Seismic Explorations for Interior Structure (SEIS), will measure seismic waves caused by marsquakes, meteorite strikes and other phenomena. Watching how these waves travel through Mars' interior will let scientists study how the planet's crust, mantle and core are layered. It will also reveal more about how all rocky bodies are formed, including Earth and its Moon. https://photojournal.jpl.nasa.gov/catalog/PIA22956

This image from NASA's Mars Reconnaissance Orbiter shows one of millions of small (10s of meters in diameter) craters and their ejecta material that dot the Elysium Planitia region of Mars. The small craters were likely formed when high-speed blocks of rock were thrown out by a much larger impact (about 10-kilometers in diameter) and fell back to the ground. Some of these blocks may actually escape Mars, which is how we get samples in the form of meteorites that fall to Earth. Other ejected blocks have insufficient velocity, or the wrong trajectory, to escape the Red Planet. As such, when one of these high-speed blocks impacts the surface, it makes what is called a "secondary" crater. These secondaries can form dense "chains" or "rays," which are radial to the crater that formed them. https://photojournal.jpl.nasa.gov/catalog/PIA21769

An artist's rendition of the InSight lander operating on the surface of Mars. InSight, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, is a lander designed to give Mars its first thorough check up since it formed 4.5 billion years ago. It is scheduled to launch from Vandenberg Air Force Base on the California coast between May 5 through June 8, 2018, and land on Mars six months later, on Nov. 26, 2018. InSight complements missions orbiting Mars and roving around on the planet's surface. The lander's science instruments look for tectonic activity and meteorite impacts on Mars, study how much heat is still flowing through the planet, and track the planet's wobble as it orbits the sun. This helps answer key questions about how the rocky planets of the solar system formed. So while InSight is a Mars mission, it's also more than a Mars mission. Surface operations begin a minute after landing at Elysium Planitia. The lander's prime mission is one Mars year (approximately two Earth years). https://photojournal.jpl.nasa.gov/catalog/PIA22228

Different kinds of carbon-based molecules called organic compounds were viewed within a rock target called "Garde" by SHERLOC, one of the instruments on the end of the robotic arm aboard NASA's Perseverance Mars rover. The rover used its drill to abrade, or grind away, a patch of rock so that SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) could analyze its interior. This data was taken on Sept. 18, 2021, the 207th Martian day, or sol, of the mission. Nonbiological, geological processes can form organics. The organics found in PIXL's data and their association with the rocks that they're embedded within bear a striking resemblance to nonbiological organics within Martian meteorites, suggesting that these organics were formed by geological processes. Therefore, these organics findings are not biosignatures (compounds that indicate the presence of a biological process). SHERLOC made the first detection of organics on the Martian surface since the Curiosity rover. It is also the first detection of organics on the Martian surface made through ultraviolet fluorescence spectroscopy (whereas the Curiosity rover utilized a different methodology known as mass spectrometry), and it is the first discovery of the spatial distribution of organics on the Martian surface. The organics were found to be simple aromatics present at low concentrations, which is similar to what was found by the Curiosity rover and within Martian meteorites. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA25042

Mars is a dusty place and in some locations thick blankets of its characteristically red dust can slowly settle out of the atmosphere and accumulate on slopes. This dust is also a lot brighter than the dust-free terrain on Mars; so, if you scrape off the dust, you'll see a darker surface underneath. This particular image shows one of these dusty areas. The dark streaks on the slopes are locations where the dust has slumped downhill revealing a less dusty surface underneath. In some cases, these slope streaks might be triggered by Marsquakes or nearby meteorite impacts. Scientists think they form quickly: more like an avalanche than dust slowly creeping downhill. Look more closely and you'll notice that some streaks are darker than others. Dust is settling out of the atmosphere all the time and these dark streaks get slowly buried by fresh dust so that they fade back into their brighter redder surroundings. It's not certain how long this fading takes to happen, but it's probably close to a few decades. Dust is an important player in the weather and climate on Mars. Images like this are used to monitor slow changes in these streaks over time to better understand how much dust is settling on the surface. http://photojournal.jpl.nasa.gov/catalog/PIA19456

At left is NASA's Perseverance Mars rover. The annotation shows where spacesuit materials can be found attached to a calibration target for SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals), one of the rover's instruments. At right is a close-up of the calibration target. Scientists rely on calibration targets to fine-tune instrument settings using materials with known properties. In the case of SHERLOC's calibration target, they are also studying how the five swatches of spacesuit materials arranged along the bottom row degrade in the Martian environment. Those materials, from left to right: a piece of polycarbonate visor used in spacesuit helmets; Vectran, a cut-resistant material used for the palms of astronaut gloves; a commonly used spacesuit material called Ortho-Fabric; and two kinds of Teflon, which has dust-repelling nonstick properties. Top row, left to right: two gallium nitride targets that glow different colors when illuminated with SHERLOC's laser; a slice of Martian meteorite named Sayh al Uhaymir 008 (SaH 008); a maze designed to focus SHERLOC's camera; and a diffuse transmission target that measures how SHERLOC's laser scatters light. This image was taken by the WATSON (Wide Angle Topographic Sensor for Operations and eNgineering) camera, which is part of SHERLOC on the end of Perseverance's robotic arm. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith. NASA's Mars Sample Return Program, in cooperation with ESA (European Space Agency), is designed to send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Mars Exploration Program (MEP) portfolio and the agency's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA26520

jsc2017e011393 (01/30/2017) --- Space exploration will feature prominently at Super Bowl LIVE, a nine-day fan festival running Jan. 28 through Feb. 5 on Discovery Green, Houston Texas where 100,000 visitors are expected each day. NASA is collaborating with the Houston Super Bowl Host Committee, which is the fan festival organizer, to share NASA’s contributions with the Houston community and to the nation. At NASA's Future Flight, the primary attraction at the free fan festival, riders will take a trip to Mars and back using virtual reality goggles on a 90-foot drop tower ride. Visitors also will get a chance to see several NASA assets that have been transported to downtown Houston for the activities. These assets include: the Orion mockup used for water recovery testing, Space Exploration Vehicle (SEV /Rover), the Driven to Explore mobile exhibit, Mars Science Laboratory – Curiosity Rover - replica, Robonaut 1 (Centaur configuration), EMU space suit presentation unit, Arctic meteorite and astromaterials display, and the Mark III advanced space suit photo-op. Several of NASA’s industry partners sponsoring Future Flight will also have assets on display, and a replica of the James Webb Space Telescope will be located near but not inside the activities on Discovery Green. NASA and industry partner volunteers will be staffing the Future Flight area. NASA PHOTOGRAPHER: Bill Stafford

The interior of Mars is simply modeled as a core and mantle with a thin crust, similar to Earth. Mars' size and total mass have been determined by previous missions. Given four parameters, the core size and mass, and mantle size and mass can be determined. The combination of Pathfinder Doppler data with earlier data from the Viking landers has determined a third parameter, the moment of inertia, through measurement of Mars' precession rate. A fourth measurement is needed to complete the interior model. This may be achieved through future Doppler tracking of Pathfinder, since the presence of a fluid core may be detectable through its effect on Mars' nutation. The determination of the moment of inertia is a significant constraint on possible models for Mars' interior. If the core is as dense as possible (i.e. completely iron) and the mantle is similar to Earth's (or similar to the SNC meteorites thought to originate on Mars) then the minimum core radius is about 1300 km. If the core is made of less-dense material (i.e. a mixture of iron and sulfur) then the core radius is probably no more than 2000 km. Sojourner spent 83 days of a planned seven-day mission exploring the Martian terrain, acquiring images, and taking chemical, atmospheric and other measurements. The final data transmission received from Pathfinder was at 10:23 UTC on September 27, 1997. Although mission managers tried to restore full communications during the following five months, the successful mission was terminated on March 10, 1998. http://photojournal.jpl.nasa.gov/catalog/PIA00974

Nothing gets a geologist more excited than layered bedrock, except perhaps finding a fossil or holding a meteorite in your hand. All of these things create a profound feeling of history, the sense of a story that took place ages ago, long before we came appeared. Layered bedrock in particular tells a story that was set out chapter by chapter as each new layer was deposited on top of older, previously deposited layers. Here in Nili Fossae, we see layered bedrock as horizontal striations in the light toned sediments in the floor of a canyon near Syrtis Major. (Note: illumination is from the top of the picture) The ancient layered rocks appear in pale whitish and bluish tones. They are partially covered by much younger ripples made up of dust and other wind blown sediments. The rock of the nearby canyon wall is severely fractured and appears to have shed sand and rocks and boulders onto the floor. This canyon did not form by fluvial erosion: it is part of a system of faults that formed a series of graben like this one, but water probably flowed through Nili Fossae in the distant past. Orbital spectral measurements by the OMEGA instrument on Mars Express and CRISM on MRO detected an abundance of clay minerals of different types in the layered sediments inside Nili Fossae, along with other minerals that are typical of sediments that were deposited by water. The various colors and tones of the layered rocks record changes in the composition of the sediments, details that can tell us about changes in the Martian environment eons ago. Nili Fossae is a candidate site for a future landed robotic mission that could traverse across these layers and make measurements that could be used to unravel a part of the early history of Mars. Nili Fossae is a history book that is waiting to be read. http://photojournal.jpl.nasa.gov/catalog/PIA21206

Impact ejecta is material that is thrown up and out of the surface of a planet as a result of the impact of an meteorite, asteroid or comet. The material that was originally beneath the surface of the planet then rains down onto the environs of the newly formed impact crater. Some of this material is deposited close to the crater, folding over itself to form the crater rim, visible here as a yellowish ring. Other material is ejected faster and falls down further from the crater rim creating two types of ejecta: a "continuous ejecta blanket" and "discontinuous ejecta." Both are shown in this image. The blocky area at the center of the image close to the yellowish crater rim is the "continuous" ejecta. The discontinuous ejecta is further from the crater rim, streaking away from the crater like spokes on a bicycle. (Note: North is to the right.) http://photojournal.jpl.nasa.gov/catalog/PIA11180