The arrival of the roveron Mars, which complemented instruments already on site, such as or the allowed to explore a new Martian environment: the Jezero crater.
The first observations quickly established that this crater was once occupied by a large lake,
Geology is a scientific discipline that focuses on the outer layers of the Earth, in particular its structure…” data-image=”https://cdn.futura-sciences.com/buildsv6/images/midioriginal/3 / d /7/3d738ba741_45745_def-geologie-bonacherajf-flickr.jpg” data-url=”https://news.google.com/planete/definitions/structure-terre-geologie-13943/” data-more=”Read more “> of the place: nature of the rocks, mineralogy, sedimentary architecture attesting to the episodes and conditions Volcano: what is the difference between lava and magma?
The morphologies created…” data-image=”https://cdn.futura-sciences.com/buildsv6/images/midioriginal/9/e/0/9e09305935_113602_volcanisme.jpg” data-url=”https://news .google.com/planete/definitions/volcanologie-volcanisme-972/” data-more=”Read more”> …
While waiting for the samples to return to Earth,However, the analyzes are going well from the data transmitted by the rover. Four new studies detailing the nature of the floor and subsurface of Jezero Crater have just been published together.
The Jezero Crater floor is composed of magmatic rocks of deep origin
During its journey into the heart of the ancient lake, the Perseverance rover has carried out various analyzes of the rocks that form the bottom of the crater. When everyone expected to find
Volcanic rocks are subject to classification based on various…” data-image=”https://cdn.futura-sciences.com/buildsv6/images/midioriginal/5/6/5/565eaa89c9_50034262_meteorites-mars-zagami- pierre-thomas-ens-lyon.jpg” data-url=”https://news.google.com/planete/definitions/structure-terre-roche-volcanique-1102/” data-more=”Read more”> like old streams the data revealed that the crater floor is actually . Find this type of rock surprising, because these are rocks called that is to say that they usually form in depth, generally within magma chambers and volcanoes
Coming from the Earth’s mantle through one or more conduits, the accumulated molten rock can…” data-image=”https://cdn.futura-sciences.com/buildsv6/images/midioriginal/d/d/9/ dd921d8236_45733_def -magma-chamber-semhur-volcano-wikimediacommons.jpg” data-url=”https://news.google.com/planet/definitions/earth-structure-magma-chamber-451/” data-more=”Read next “> or at the bottom of lava lakes. They are the result in fact of a slow cooling of the magma formation
It forms at high temperature and under high pressure…” data-image=”https://cdn.futura-sciences.com/buildsv6/images/midioriginal/6/1/2/612232a1f7_50034213_gabbro-piotr-sosnowski-wikipedia . jpg” data-url=”https://news.google.com/planete/definitions/structure-terre-magma-461/” data-more=”Read more”> . The crystals that form as the temperature decreases will gradually settle to the bottom of the magma reservoir and accumulate to form a layered rock.
In both cases, the presence of this type of rock in the outcrop at the bottom of the crater can only mean one thing: all the material that covered it has been removed by the slow process of erosion over billions of years. We are still talking about a thickness of rock several hundred meters thick! These results were published in the journal Sciences under the titleMarch as well as in the article appeared in Progress of science.
Eastfrom the basement of Jezero Crater was confirmed by radar images made by Perseverance. In fact, the instrument carried by the rover has made it possible to obtain images of the subsoil at a depth of about 15 meters, revealing a highly stratified architecture, which can be explained by the magmatic origin of the rocks, but also by the presence of lacustrine sedimentary deposits. . These results are presented in the article published in the magazine Progress of science.
One thing is certain, the rocks analyzed by the rover testify to a magmatic episode prior to the formation of the Jezero delta. Therefore, they could allow a lower age limit to be established for this sedimentary formation.
Different traces of weathering by water.
Their discovery is doubly interesting as these rocks also show traces of weathering by water. theBeing particularly easy to date, the samples taken by Perseverance could make it possible to establish a precise chronology of the various hydrological events at the site and, in particular, to date the formation of the lake. These data are one of the key elements that allow a better understanding of the evolution of the Martian. Therefore, the study of these rocks could allow us to know precisely when the planet’s climate allowed the establishment of a water system on the surface and when the situation changed drastically towards the cold and arid conditions that we observe today.
Perseverance is not, however, in a position to carry out such dates. Therefore, we will have to wait patiently for the samples to return to Earth. However, thanks to the instruments on board the rover, a detailed study of the cumulus clouds present at the bottom of the crater is possible. Their mineralogical analysis shows that they are composed of small intricate crystals ofand pyroxene, indicating slow crystallization. But what most interests specialists are the traces of weathering by water. In fact, the different samples taken by Perseverance at different points in the crater appear to have been altered in different ways.
The rocks of the Máaz site contain in their pores
Brackish water may appear as a result of…” data-image=”https://cdn.futura-sciences.com/buildsv6/images/midioriginal/9/2/f/92fa4767c3_50035363_marycesyl-flikr-cc-02.jpg ” data-url=”https://news.google.com/planete/definitions/oceanographie-eau-saumatre-6598/” data-more=”Read more”> , Very salty. In contrast, rocks from the Seitah site show traces of reaction with carbonate-rich water. The two samples testify to a change in the conditions of the lake over time, which may be related to . Once again, we will have to wait for the samples to return to Earth in order to accurately date these different stages and establish their chronology. The detail of the analysis is available in the article. published in Sciences.
However, the low abundance of minerals resulting from the weathering of igneous rocks suggests that the lake’s period of existence was relatively short.
Apart from the very local case of Jezero, further study of olivine-rich accumulates could help to better understand Mars’ magmatic activity. Combined with satellite imagery, the data reported by Perseverance could help paint a larger-scale picture of the planet’s magmatic history.
We better understand the value of the samples taken by Perseverance and the precautions taken by the scientists in charge of the mission to ensure theirand his arrival on Earth in 11 years. In each of the four sites studied, the samples taken were duplicated. These duplicates will be stored at a backup site near the delta in case the samples held by Perseverance cannot be retrieved, due to mechanical failure, for example. Sedimentary rock samples recently collected by the rover at the delta level will also be stored at this site. New samples that should also provide us with valuable information about the past of Mars.
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