Gale (crater)

Gale is a crater, and probable dry lake, at in the northwestern part of the Aeolis quadrangle on Mars. It is 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. Aeolis Mons, also known as Mount Sharp, is a mountain in the center of Gale and rises high. Aeolis Palus 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 the landing location Bradbury Landing on August 22, 2012. ''Curiosity'' is exploring Aeolis Mons and surrounding areas.

Description

Gale, named for Walter F. Gale (1865–1945), an amateur astronomer from Australia, spans in diameter and holds a mountain, Aeolis Mons (informally named "Mount Sharp" to pay tribute to geologist Robert P. Sharp) rising from 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 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 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 , at the foot of the layered mountain inside Gale. ''Curiosity'' landed within a landing ellipse approximately by . The landing ellipse is about 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 .

Scientists chose Gale as 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 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.

Geology

Orbital THEMIS and topography data, plus visible and near-infrared images, were used to make a geological map of the crater. CRISM data indicated the lower bench unit was composed of interstratified clay and sulfates. Curiosity explored 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 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 above the northern crater floor and 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 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 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, 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 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 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 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, the density of Mount Sharp in Gale, thereby establishing a clearer understanding of how the mountain was formed.

Gale is located at about on Mars.

Spacecraft exploration

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 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 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, 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 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 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 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 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'' First Five Years (02:07)''Curiosity'' POV: Five Years Driving (05:49)''Curiosity'' 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 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 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 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 the height of , which were formed by flood waters at least deep with a velocity of .

Research published in August, 2023 found evidence that liquid water may have existed over thousands to millions of years 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 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.

File:Mudcracks on Mars.jpg, Mudcracks as seen by ''Curiosity'' in Gale. Shapes imply that water saturated the area and dried out many times; hence, the existence of water was not just a one-time, short-lived event.

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 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 the Rover cracked open a rock with its wheel and found crystals of sulfur. Minerals containing sulfur were discovered, but never the pure element. It was found in Gediz Vallis.

Research published in February 2025 described wave ripples in Gale that show that liquid water flowed there. The ripples were found in two different time periods. Calculations based on their shape and sizes revealed that they were formed in shallow moving water. The water could have been as deep as 2 meters. Before this study, it was thought that any exposed body of water would quickly develop a sheet of ice at the top.

Images

Image:Daybreak at Gale Crater.jpg, Mars between day and night, with an area containing Gale crater, beginning to catch the morning light
Image:Schiaparelli 1889 versus Mars crop.jpg, Maps of Mars - old and new - Gale is noted in the middle of the image
Image:MSL landing sites topograph.png, Map of actual (and proposed) rover landing sites including Gale
Image:Elysium Planitia topo.jpg, Map of Elysium Planitia - Gale is in the lower left - Aeolis Mons is in the middle of the crater
Image:Aeolis map.JPG, Map of Aeolis quadrangle - Gale is in the upper left - Aeolis Mons is in the middle of the crater
Image:PIA19674-Mars-GaleCrater-SurfaceMaterials-20150619.jpg, Gale crater - surface materials (false colors; THEMIS; 2001 Mars Odyssey)
Image:Mars Science Laboratory landing ellipse reduced.jpg, Gale crater landing site is within Aeolis Palus near Aeolis Mons - north is down.
Image:PIA19080-MarsRoverCuriosity-AncientGaleLake-Simulated-20141208.jpg, Ancient Lake fills Gale Crater on Mars (simulated view).
Image:PIA17596-MarsCuriosityRover-AncientLake-20131209.jpg, Estimated size of ancient lake on Aeolis Palus in Gale
Image:PIA16158-Mars Curiosity Rover-Water-AlluvialFan.jpg, Peace Vallis and alluvial fan near the ''Curiosity'' rover landing ellipse and site (noted by +)
Image:Curiosity landing site (artist's rendition with 2x vertical exaggeration).jpg, Gale crater - landing site is noted - also, alluvial fan (blue) and sediment layers in Aeolis Mons (cutaway)
Image:Topography gravity gale crater.jpg, Gale crater - topographic and gravity field maps - landing site is noted
Mars gravity model 2011
Image:Moundshigh.jpg, Aeolis Mons may have formed from the erosion of sediment layers that once filled Gale.
Image:Gale crater layers.JPG, Gale sediment layers may have formed by lake or windblown particle deposition.
Image:Gale Crater Grand Canyon.JPG, Gale's "Grand Canyon", as seen by HiRISE - scale bar is 500 meters long
Image:PIA16064-Mars Curiosity Rover Treasure Map.jpg, ''Curiosity'' landing site (green dot) - blue dot marks " Glenelg Intrigue" - blue spot marks base of Aeolis Mons - a planned area of study
Image:Curiosity Rover Landing Site - Quadmapping Yellowknife.jpg, ''Curiosity'' landing site - " quad map" includes "Yellowknife" ''Quad 51'' of Aeolis Palus in Gale crater
Image:Mars Curiosity Rover - Yellowknife Landing Site.jpg, ''Curiosity'' landing site - "Yellowknife" ''Quad 51'' (1-mi-by-1-mi) of Aeolis Palus in Gale
Image:PIA15696-HiRISE-MSL-Sol11 2 -br2.jpg, MSL debris field viewed by HiRISE on August 17, 2012 - parachute is from the roverMars Science Laboratory: Multimedia-Images
/ref> (3-D
rover
and
parachute

Image:Curiosity Rover (Exaggerated Color) - HiRISE - 20120814.jpg, ''Curiosity'' landing site (" Bradbury Landing") viewed by HiRISE ( MRO) (August 14, 2012)
Image:PIA17085-MarsCuriosityRover-TraverseMap-Sol351-20130801.jpg, First-year and first-mil
traverse map
of ''Curiosity'' on Mars (August 1, 2013)
3-D

Image:PIA19400-MarsCuriosityRover-GaleCrater-Sunset-20150415.jpg, Sunset - Gale crater (April 15, 2015)
Image:PIA19401-MarsCuriosityRover-GaleCrater-Sunset-Animation-20150415.gif, Sunset (animated) - Gale crater (April 15, 2015)

Surface images

Image:673885main PIA15986-full full.jpg, Aeolis Palus and Aeolis Mons in Gale as viewed by ''Curiosity'' (August 6, 2012)
Image:First two full-resolution images from the Curosity rover.jpg, The rim and floor of Gale as viewed by ''Curiosity'' (August 9, 2012)
Image:676029main pia16052-color-full full.jpg, Gale rim about north of ''Curiosity'' (August 9, 2012)
Image:PIA16105 malin04ano-br2.jpg, Layers at the base of Aeolis Mons - dark rock in inset is same size as ''Curiosity'' ( white balanced image)
Image:PIA16068 - Mars Curiosity Rover - Aeolis Mons - 20120817.jpg, Aeolis Mons in Gale as viewed by ''Curiosity'' (August 9, 2012) ( white balanced image)
Image:PIA16134-Mars Curiosity Rover Wheels.jpg, Wheels on ''Curiosity'' - Aeolis Mons is in the background ( MAHLI, September 9, 2012).
Image:PIA16204-MarsCuriosityRover-Rocknest-20120928.jpg, ''" Rocknest"'' sand patch in Gale - between " Bradbury Landing" and Glenelg (September 28, 2012)

See also

References

External links

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Google Mars scrollable map
– centered on Gale Crater

Gale Crater – ''Curiosity'' rover "StreetView" (Sol 2 – 08/08/2012) – NASA/JPL – 360° panorama
from 360pano.eu
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Gale Crater – Central Debris Mound
from lpl.arizona.edu

Gale Crater – Layers
from lpl.arizona.edu


from mars.asu.edu (Zoomable)
small


Gale Crater – Surroundings
from HRSCview.fu-berlin.de

Gale Crater – 3D version by ESA

Video (04:32) – Evidence: Water "Vigorously" Flowed On Mars – September, 2012
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{{Portal bar, Solar System, Astronomy, Biology

Aeolis quadrangle
Impact craters on Mars
Mars Science Laboratory
Water on Mars