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44-478: ChemCam has the ability to record up to 6,144 different wavelengths of ultraviolet, visible, and infrared light. Detection of the ball of luminous plasma is done in the visible, near-UV and near-infrared ranges, between 240 nm and 800 nm. The first initial laser testing of the ChemCam by Curiosity on Mars was performed on a rock, N165 ("Coronation" rock) , near Bradbury Landing on August 19, 2012. Using

88-528: A habitat for microbes. Gale contains a number of fans and deltas that provide information about lake levels in the past, including: Pancake Delta, Western Delta, Farah Vallis delta and the Peace Vallis Fan. Orbital THEMIS and topography data, plus visible and near-infrared images, were used to make a geologic map of the crater. CRISM data indicated the lower bench unit was composed of interstratified clay and sulfates . Curiosity explored

132-480: A higher spatial resolution than the mastcam M100 camera, which is a color camera also capable of imaging nearby objects or distant geologic features. The RMI has been used by the mission for reconnaissance of up-coming terrain as well as imaging distant features such as the rim of Gale Crater . ChemCam has been used, in conjunction with other instruments of the Curiosity rover, to make advancements in understanding

176-412: A humor themed mix of social interaction and Mars content such as " Did you know I was born in a volcano? Basalts like me come from lava. That's why we call it Olympus Mom ". The goal of this initial use of the laser on Mars was to serve as target practice for characterizing the instrument. The rock was primarily selected for its proximity to the rover, rather than any intrinsic scientific value. The rock

220-526: Is a laminated mudstone overlain by a cross-bedded or clinoform sandstone, though in places the base is a conglomerate. Thus, the formation is interpreted to have been deposited in a lacustrine environment adjacent to a fluvial-deltaic one. The Murray Formation is overlain by clay and sulfate-bearing strata. An unusual feature of Gale is an enormous mound of "sedimentary debris" around its central peak, officially named Aeolis Mons (popularly known as "Mount Sharp" ) rising 5.5 km (18,000 ft) above

264-425: Is based on multivariate PLS and PCA models classified using SIMCA with calibration models made using " The Unscramble r " software. ChemCam has also quantified soil chemistry. ChemCam has seen two distinct soil types at Gale crater: a fine-grained mafic material that is more representative of global Martian soils or dust and a coarse-grained felsic material that originates from local Gale crater bedrock. ChemCam has

308-402: Is common for there to be 9 or 10 points of analysis on any given target, but this is not always the case. Some targets have as few as 4 points while some targets have 20 points.  The Remote Micro-Imager is primarily used to capture high-resolution, black and white images of ChemCam targets for context and documentation. Usually, an image of the target of interest is captured before and after

352-436: Is housed in the rover's body. Typically, the laser fires 30 shots at a single point, gathering spectroscopic readings from the vaporized rock for each laser shot, and samples multiple points on a chosen target. For bedrock observations, the first 5 shots of a point are discarded as they are considered to be contaminated by Martian dust. The remaining shots of one point are averaged together for chemical composition calculations. It

396-617: Is not the case–water stayed for some time. Also, with water coming and going on a regular pace, there is a better chance of more complex organic compounds being produced. As water evaporates chemicals are concentrated and have a better chance of combining. For example when amino acids are concentrated they are more likely to link up to form proteins. Curiosity found features that computer simulations show could be caused by past streams. They have been called benches and noses. The "noses" stick out like noses. Computer simulations show that these shapes can be produced by rivers. In July 2024

440-732: Is the plain between the northern wall of Gale and the northern foothills of Aeolis Mons. Peace Vallis , a nearby outflow channel , 'flows' down from the hills to the Aeolis Palus below and seems to have been carved by flowing water . Several lines of evidence suggest that a lake existed inside Gale shortly after the formation of the crater. The NASA Mars rover Curiosity , of the Mars Science Laboratory (MSL) mission, landed in "Yellowknife" Quad 51 of Aeolis Palus in Gale at 05:32 UTC August 6, 2012. NASA named

484-692: Is the surviving remnant of an extensive sequence of deposits. Some scientists believe the crater filled in with sediments and, over time, the relentless Martian winds carved Aeolis Mons, which today rises about 5.5 km (3.4 mi) above the floor of Gale—three times higher than the Grand Canyon is deep. At 10:32 p.m. PDT on August 5, 2012 (1:32 a.m. EDT on August 6, 2012), the Mars Science Laboratory rover Curiosity landed on Mars at 4°30′S 137°24′E  /  4.5°S 137.4°E  / -4.5; 137.4 , at

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528-507: The Curiosity rover . The "approximate" site coordinates are: 4°35′S 137°26′E  /  4.59°S 137.44°E  / -4.59; 137.44 . On August 19, 2012, the rock was the first target of the rover's laser instrument, ChemCam , which can analyze targets at a distance using a laser and spectrometer. A Twitter feed for the rock was created, featuring an anthropomorphized account of its experiences. Its posts include

572-725: The Curiosity rover will continue to explore higher and younger layers of Mount Sharp in order to determine how the lake environment in ancient times on Mars became the drier environment in more modern times. On August 5, 2017, NASA celebrated the fifth anniversary of the Curiosity rover mission landing, and related exploratory accomplishments, on the planet Mars . (Videos: Curiosity 's First Five Years (02:07) ; Curiosity 's POV: Five Years Driving (05:49) ; Curiosity 's Discoveries About Gale Crater (02:54) ) On June 7, 2018, NASA 's Curiosity made two significant discoveries in Gale. Organic molecules preserved in 3.5 billion-year-old bedrock and seasonal variations in

616-550: The Curiosity rover, that there was plenty of water on early Mars . In January 2020, researchers have found certain minerals, made of carbon and oxygen, in rocks at Gale, which may have formed in an ice-covered lake during a cold stage between warmer periods, or after Mars lost most of its atmosphere and became permanently cold. On November 5, 2020, researchers concluded based on data observed by Curiosity rover that Gale experienced megafloods which occurred around 4 billion years ago, taking into consideration antidunes reaching

660-660: The Mars Science Laboratory spacecraft, which was launched November 26, 2011 and landed on Mars inside the crater Gale on the plains of Aeolis Palus on August 6, 2012. Gale was previously a candidate landing site for the 2003 Mars Exploration Rover mission, and has been one of four prospective sites for ESA 's ExoMars . In December 2012, scientists working on the Mars Science Laboratory mission announced that an extensive soil analysis of Martian soil performed by Curiosity showed evidence of water molecules , sulphur and chlorine , as well as hints of organic compounds . However, terrestrial contamination, as

704-430: The density of Mount Sharp in Gale, thereby establishing a clearer understanding of how the mountain was formed. Gale is located at about 5°24′S 137°48′E  /  5.4°S 137.8°E  / -5.4; 137.8 on Mars. Numerous channels eroded into the flanks of the crater's central mound could give access to the layers for study. Gale is the landing site of the Curiosity rover, delivered by

748-520: The French CESR laboratory. The flight model of the mast unit was delivered from the French CNES to Los Alamos National Laboratory . ChemCam marks the first use of Laser Induced Breakdown Spectroscopy ( LIBS ) as part of a planetary science mission. The laser is positioned on the mast of the Curiosity rover and focused by the telescope that also resides on the mast, while the spectrometer

792-707: The Stimson formation is the only stratigraphic unit within the Siccar Point group which has been investigated in-detail by Curiosity . The Stimson formation represents the preserved expression of a dry aeolian dune field , where sediment was transported towards the north, or northeast by palaeowinds within the crater. In the Emerson plateau area (from Marias Pass, to East Glacier), the outcrops are characterised predominantly by simple cross-sets, deposited by simple sinuous-crested dunes, with heights up to ~10 m. To

836-531: The amounts of methane in the atmosphere of the planet Mars ; in addition, organic chemicals were detected in powder drilled from a rock . Also, based on deuterium to hydrogen ratio studies, much of the water at Gale on Mars was found to have been lost during ancient times, before the lakebed in the crater was formed; afterwards, large amounts of water continued to be lost. On October 8, 2015, NASA confirmed that lakes and streams existed in Gale 3.3 to 3.8 billion years ago delivering sediments to build up

880-467: The capability to measure minor or trace elements such as lithium, manganese, strontium, and rubidium. ChemCam has measured MnO up to 25 wt% in fracture fills that suggests Mars was once a more oxygenating environment.    N165 N165 ( "Coronation" rock ) is a rock on the surface of Aeolis Palus in Gale Crater on the planet Mars near the landing site ("Bradbury Landing") of

924-430: The chemical composition of rocks and soils on Mars . LIBS makes it possible to detect and quantify the major oxides: SiO 2 , Al 2 O 3 , FeO T , MgO, TiO 2 , CaO, Na 2 O, and K 2 O of bedrock targets. There are distinguishable geologic units determined from orbital analyses that have been confirmed by averaged bedrock compositions determined from ChemCam and other instruments aboard Curiosity. The identification

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968-630: The crater completely, possibly originally deposited on a lakebed. Evidence of fluvial activity was observed early on in the mission at the Shaler outcrop (first observed on Sol 120, investigated extensively between Sols 309-324). Observations made by the rover Curiosity at the Pahrump Hills strongly support the lake hypothesis: sedimentary facies including sub mm-scale horizontally-laminated mudstones, with interbedded fluvial crossbeds are representative of sediments which accumulate in lakes, or on

1012-426: The crater floor, higher than Mount Rainier rises above Seattle. Gale is roughly the size of Connecticut and Rhode Island. The crater formed when an asteroid or comet hit Mars in its early history, about 3.5 to 3.8 billion years ago. The impactor punched a hole in the terrain, and the subsequent explosion ejected rocks and soil that landed around the crater. Layering in the central mound (Aeolis Mons) suggests it

1056-519: The foot of the layered mountain inside Gale. Curiosity landed within a landing ellipse approximately 7 km (4.3 mi) by 20 km (12 mi). The landing ellipse is about 4,400 m (14,400 ft) below Martian "sea level" (defined as the average elevation around the equator). The expected near-surface atmospheric temperatures at the landing site during Curiosity ' s primary mission (1 Martian year or 687 Earth days) are from −90 to 0 °C (−130 to 32 °F). Scientists chose Gale as

1100-615: The height of 10 meters (33 ft), which were formed by flood waters at least 24 meters (79 ft) deep with a velocity of 10 meters per second (22 mph). Research published in August, 2023 found evidence that liquid water may have existed for a long time and not just when an impact or volcano erupted. Shapes in a field of hexagonal ridges revealed that water appeared and then went away many times. The water did not just result from ground ice melting from something like an asteroid impact. To make these ridges many cycles of water saturating

1144-405: The landing location Bradbury Landing on August 22, 2012. Curiosity is exploring Aeolis Mons and surrounding areas. Gale, named for Walter F. Gale (1865–1945), an amateur astronomer from Australia, spans 154 km (96 mi) in diameter and holds a mountain, Aeolis Mons (informally named "Mount Sharp" to pay tribute to geologist Robert P. Sharp ) rising 18,000 ft (5,500 m) from

1188-422: The landing site for Curiosity because it has many signs that water was present over its history. The crater's geology is notable for containing both clays and sulfate minerals, which form in water under different conditions and may also preserve signs of past life. The history of water at Gale, as recorded in its rocks, is giving Curiosity many clues to study as it pieces together whether Mars ever could have been

1232-521: The laser is fired. Often, the laser makes "LIBS pits" that can be visible in the RMI to show where the laser sampled specifically on a particular target. The resolution of the RMI is higher than the black and white navigational camera (navcam) and the color mast cameras (mastcam). The RMI is primarily used to obtain close-up images of targets sampled by ChemCam, but it can also be used to gather high-resolution images of distant outcrops and landscapes. The RMI has

1276-536: The level of methane in the atmosphere further support the theory that past conditions may have been conducive to life. It is possible that a form of water-rock chemistry might have generated the methane, but scientists cannot rule out the possibility of biological origins. Methane previously had been detected in Mars' atmosphere in large, unpredictable plumes. This new result shows that low levels of methane within Gale repeatedly peak in warm, summer months and drop in

1320-431: The lower layers of Mount Sharp . On June 1, 2017, NASA reported that the Curiosity rover provided evidence of an ancient lake in Gale on Mars that could have been favorable for microbial life ; the ancient lake was stratified , with shallows rich in oxidants and depths poor in oxidants; and, the ancient lake provided many different types of microbe-friendly environments at the same time. NASA further reported that

1364-587: The margins of lakes which grow and contract in response to lake-level. These lake-bed mudstones are referred to as the Murray Formation , and form a significant amount of the Mount Sharp group. The Siccar Point group (named after the famous unconformity at Siccar Point ) overlies the Mount Sharp group, and the two units are separated by a major unconformity which dips toward the North. At present,

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1408-402: The northern crater floor and 4.5 km (15,000 ft) above the southern crater floor—slightly taller than the southern rim of the crater itself. The mound is composed of layered material and may have been laid down over a period of around 2 billion years. The origin of this mound is not known with certainty, but research suggests it is the eroded remnant of sedimentary layers that once filled

1452-468: The northwestern part of the Aeolis quadrangle on Mars . It is 154 km (96 mi) in diameter and estimated to be about 3.5–3.8 billion years old. The crater was named after Walter Frederick Gale , an amateur astronomer from Sydney , Australia, who observed Mars in the late 19th century. Mount Sharp is a mountain in the center of Gale and rises 5.5 km (18,000 ft) high. Aeolis Palus

1496-603: The pediment capping unit. Observations made during the ascent of the Greenheugh pediment between Sols 2665-2734 demonstrated that the pediment capping unit has sedimentary textures, facies and architecture that are consistent with the rest of the Stimson formation. Furthermore, analysis of sedimentary facies and architecture provided evidence which indicates fluctuating wind directions, from a seasonal temporal scale - recorded by interstratified windripple and avalanche strata, through to millennial time scales recorded by reversal of

1540-561: The same collection optics, the RMI provides context images of the LIBS analysis spots. The RMI resolves 1 mm (0.039 in) objects at 10 m (33 ft) distance, and has a field of view covering 20 cm (7.9 in) at that distance. The RMI has also been used to take images of distant geologic features and landscapes. The ChemCam instrument suite was developed by the Los Alamos National Laboratory and

1584-465: The sediment transport direction. These wind reversals suggest variable and changeable atmospheric circulation during this time. Observations of possible cross-bedded strata on the upper mound suggest aeolian processes , but the origin of the lower mound layers remains ambiguous. In February 2019, NASA scientists reported that the Mars Curiosity rover had determined, for the first time,

1628-539: The source of the organic compounds, could not be ruled out. On September 26, 2013, NASA scientists reported that Curiosity detected "abundant, easily accessible" water (1.5 to 3 weight percent) in soil samples at the Rocknest region of Aeolis Palus in Gale. In addition, the rover found two principal soil types: a fine-grained mafic type and a locally derived, coarse-grained felsic type . The mafic type, similar to other martian soils and martian dust ,

1672-565: The south, at the Murray buttes, the outcrop are characterised by compound cross-sets, with a hierarchy of bounding surfaces migration of small dunes superimposed on the lee-slope of a large dune known as a " draa ". These draas have estimates heights of ~40 m, and migrated toward the north, while superimposed dunes migrated toward the east-northeast. Further to the south, at the Greenheugh pediment, compound and simple cross-sets consistent with aeolian depositional processes have been observed in

1716-787: The stratigraphy of the crater consisting of the Bradbury Group and the overlying Mount Sharp Group. Formations within the Bradbury Group include the Yellowknife and Kimberley, while the Murray Formation is at the base of the Mount Sharp Group. The Bradbury Group consists of fluvial conglomerates , cross-bedded sandstones , and mudstones reflecting a basaltic provenance . Sandstone clinoforms indicate deltaic deposits . The Murray Formation

1760-473: The surface and then drying were required. Chemicals were deposited by mineral-rich fluids in cracks. The minerals hardened such that they were harder than the rock around them. Later, when erosion took place, ridges were exposed. This discovery is significant. Much evidence exists to show that impacts and volcanic activity could melt ground ice to make liquid water. However, that water may not last long enough for life to develop. This new finding shows here it

1804-427: The way to Glenelg , was a mugearite and very similar to terrestrial mugearite rocks. On December 9, 2013, NASA reported that, based on evidence from Curiosity studying Aeolis Palus, Gale contained an ancient freshwater lake which could have been a hospitable environment for microbial life . On December 16, 2014, NASA reported detecting, by the Curiosity rover at Gale, an unusual increase, then decrease, in

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1848-518: The winter every year. Organic carbon concentrations were discovered on the order of 10 parts per million or more. This is close to the amount observed in Martian meteorites and about 100 times greater than prior analysis of organic carbon on Mars' surface. Some of the molecules identified include thiophenes, benzene, toluene, and small carbon chains, such as propane or butene. On November 4, 2018, geologists presented evidence, based on studies in Gale by

1892-463: Was associated with hydration of the amorphous phases of the soil. Also, perchlorates , the presence of which may make detection of life-related organic molecules difficult, were found at the Curiosity landing site (and earlier at the more polar site of the Phoenix lander ) suggesting a "global distribution of these salts". NASA also reported that Jake M rock , a rock encountered by Curiosity on

1936-464: Was lasered thirty times over ten seconds. The mission's investigators thought the rock was a basalt prior to lasing, which was confirmed by preliminary results. The ChemCam team reported positive results; they worked on the instrument for eight years before getting to use it on Mars. Gale (crater) Gale is a crater , and probable dry lake , at 5°24′S 137°48′E  /  5.4°S 137.8°E  / -5.4; 137.8 in

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