Difference between revisions of "Jezero Crater"

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[[File:Jezerocraterclose.jpg|Close view of features in and around Jezero Crater]]
 
[[File:Jezerocraterclose.jpg|Close view of features in and around Jezero Crater]]
 
                     Close view of features in and around Jezero Crater
 
                     Close view of features in and around Jezero Crater
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[[File:NASA-Mars-JezeroCrater-20181116.jpg|600pxr|Rivers on the left side of Jezero carried water into the crater, while the overflow went out at the upper right.]]
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Rivers on the left side of Jezero carried water into the crater, while the overflow went out at the upper right.
  
  
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The Mars 2020 rover mission will be able to examine at least 5 types of rock, including clays and carbonates.<ref>https://www.jpl.nasa.gov/news/news.php?feature=7539&utm_source=iContact&utm_medium=email&utm_campaign=nasajpl&utm_content=daily-20191112-1</ref>  These can preserve signs of ancient life.  Additional materials probably washed in from the surroundings; therefore, we will be able to determine mineral information about the area around the crater.
 
The Mars 2020 rover mission will be able to examine at least 5 types of rock, including clays and carbonates.<ref>https://www.jpl.nasa.gov/news/news.php?feature=7539&utm_source=iContact&utm_medium=email&utm_campaign=nasajpl&utm_content=daily-20191112-1</ref>  These can preserve signs of ancient life.  Additional materials probably washed in from the surroundings; therefore, we will be able to determine mineral information about the area around the crater.
  
On September 6, 2021 NASA announced that Perseverance rover collected its first sample of a Martian rock.  Perseverance’s  rotary-percussive drill on its robotic arm cored into a flat, briefcase-size  rock.  It has been called  “Rochette.”  The sample was slightly thicker than a pencil.  It is now enclosed in an airtight titanium sample tube, making it available for retrieval in the future.  NASA and ESA (European Space Agency) are planning future missions to return the rover’s sample tubes to Earth.  This first sample was placed in sample tube serial number 266.<ref>https://mars.nasa.gov/news/9029/nasas-perseverance-rover-collects-first-mars-rock-sample/</ref>
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==Activities and discoveries by Perseverance==
 +
 
 +
On September 6, 2021 NASA announced that Perseverance rover collected its first sample of a Martian rock.  Perseverance’s  rotary-percussive drill on its robotic arm cored into a flat, briefcase-size  rock.  It has been called  “Rochette.”  The sample was slightly thicker than a pencil.  It is now enclosed in an airtight titanium sample tube, making it available for retrieval in the future.  NASA and ESA (European Space Agency) are planning future missions to return the rover’s sample tubes to Earth.  This first sample was placed in sample tube serial number 266.<ref>https://mars.nasa.gov/news/9029/nasas-perseverance-rover-collects-first-mars-rock-sample/</ref>
 +
 
 +
The collection from Rochette came a month after the rover tried and failed to collect a sample from another rock, called “Roubion.”  The first sample attempt failed because the rock was softer; hence  it crumbled.<ref> https://spacenews.com/perseverance-collects-first-mars-samples/</ref>
 +
 
 +
Before drilling to get the core sample from the rock, scientists used instruments on the rover to learn more about its composition.  They determined that the rock was basaltic and contained salt crystals.  The salts may have formed from groundwater  or more likely from  liquid water that had evaporated into the thin Martian atmosphere.  It is hoped that the crystals may also have trapped tiny bubbles of  water.<ref> https://mars.nasa.gov/news/9036/nasas-perseverance-rover-collects-puzzle-pieces-of-mars-history/</ref>
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<gallery class="center"  widths="380px" heights="360px">
 
<gallery class="center"  widths="380px" heights="360px">
  
 
File:Sampletube26218 PIA24808.jpg|Sample tube like the one that contains the first sample of Mars that will be sent back to Earth.
 
File:Sampletube26218 PIA24808.jpg|Sample tube like the one that contains the first sample of Mars that will be sent back to Earth.
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</gallery>
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In October 2021, an article was published online by the journal Science about some initial results from photos from Perseverance.  It was confirmed that there is an actual delta in Jezero Crater because the typical layers in a delta were seen.  Scientists called them bottomsets, foresets and topsets.  They were found in a  steeply fronted Gilbert-type delta.  Since meter-scale boulders were found that may have traveled tens of km, the researchers believe that much rapidly moving water was present at times.<ref>https://www.science.org/doi/10.1126/science.abl4051</ref> <ref> Mangold, N., al al.  2021.  Perseverance rover reveals an ancient delta-lake system and flood deposits at Jezero crater, Mars. Science.  DOI: 10.1126/science.abl4051</ref>
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 +
In December 2021, it was announced that some of the rocks in Jezero were igneous.<ref> https://www.hou.usra.edu/meetings/lpsc2022/pdf/1530.pdf</ref> <ref>Schmidt, M., et al.  2022.  HIGHLY DIFFERENTIATED BASALTIC LAVAS EXAMINED BY PIXL IN JEZERO CRATER.  53rd Lunar and Planetary Science Conference.  1530.pdf</ref>  They had once been molten and then slowly cooled.  At first ,it looked like many of the rocks photographed by Jezero's camera were sedimentary due to the presence of layering.  But, when examined closely, the rocks revealed the mineral olivine surrounded by the mineral pyroxene.  That arrangement happens in thick magma bodies and geologists call this type of texture "Cumulate."<ref> https://www.bbc.com/news/science-environment-59677383</ref>  Carbonate and sulfate minerals were also detected which means that the rocks had been altered by water.  The rocks studied were in location nicknamed "South Séítah."  "Séítah" (means "amidst the sand" in the Navajo language.<ref>https://www.bbc.com/news/science-environment-59677383</ref>  The instrument used for this analysis was the Planetary Instrument for X-ray Lithochemistry (PIXL).  It uses X-ray fluorescence to determine the elemental composition of rocks.<ref>https://www.jpl.nasa.gov/news/nasas-perseverance-mars-rover-makes-surprising-discoveries</ref>
 +
 +
Two formations, called Maaz and Seitah, are both igneous.  Seitah is classified as an olivine-rich cumulate  which means it cooled slowly in a thick mass.  Maaz is rich in the minerals pyroxene and plagioclase.  It cooled quicker on the top of a mass of magma or lava.  Water as altered the chemistry of the rock because
 +
carbonate, iron oxides, amorphous silicates, sulfates,
 +
halite, perchlorates, phosphates, and possible
 +
phyllosilicates were found<ref> https://www.hou.usra.edu/meetings/lpsc2022/pdf/1798.pdf</ref> <ref>Sun, V., et al.  2022.  EXPLORING THE JEZERO CRATER FLOOR: OVERVIEW OF RESULTS FROM THE MARS 2020
 +
PERSEVERANCE ROVER’S FIRST SCIENCE CAMPAIGN.  53rd Lunar and Planetary Science Conference (2022.  1798.pdf</ref> 
 +
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<gallery class="center"  widths="380px" heights="360px">
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File:Perseveranceseith 122237583 map-nc.png|Map showing features and mineral distribution in Jezero Crater delta.  Red shading indicates olivine and green/blue shading pyroxene.  These are common minerals in igneous rocks.  The blue box is where Perseverance is in Seitah.
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</gallery>
 
</gallery>
  
  
[[File:NASA-Mars-JezeroCrater-20181116.jpg|600pxr|Rivers on the left side of Jezero carried water into the crater, while the overflow went out at the upper right.]]
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At the same time, NASA said that organic compounds were found by the SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) instrument. These organics are not only inside  of abraded rocks SHERLOC analyzed, but in the dust on non-abraded rock.
  
Rivers on the left side of Jezero carried water into the crater, while the overflow went out at the upper right.
+
Perseverance uses ground-penetrating radar to look under the surface of Mars. RIMFAX (Radar Imager for Mars' Subsurface Experiment) produces a “radargram” of subsurface features up to about 33 feet (10 meters) deep.
 +
Scientists found that rock formations with a downward tilt continue  into the subsurface.<ref> https://www.jpl.nasa.gov/news/nasas-perseverance-mars-rover-makes-surprising-discoveries</ref>
  
 +
Many dust devils were detected by Perseverance.  In the first 216 Martian days (Sols), the Perseverance Rover in Jezero Crater found that at least four dust devils passed Perseverance on a typical Martian day and that more than one per hour passes by during a peak hourlong period just after noon.  Perseverance made these observations mostly with the its cameras and a group of sensors in the Mars Environmental Dynamics Analyzer (MEDA). MEDA includes wind sensors and light sensors.<ref>https://www.jpl.nasa.gov/news/nasas-perseverance-studies-the-wild-winds-of-jezero-crater?utm_source=iContact&utm_medium=email&utm_campaign=nasajpl&utm_content=Day%20in%20Review%20-%206-1-22</ref>
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<ref>https://www.science.org/doi/10.1126/sciadv.abn3783</ref> <ref> Newman, C., et al.  2022.  The dynamic atmospheric and aeolian environment of Jezero crater, Mars.  Science Advances.  Vol. 8.  Number 21</ref>
  
 
==References==
 
==References==
Line 93: Line 124:
  
 
==External links==
 
==External links==
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* [https://www.youtube.com/watch?v=D-SCOHj8u-A  Water on Mars - James Secosky - 2021 Mars Society Virtual Convention -- Tells where water was and where ice is today on Mars (34 minutes)]
  
 
* https://www.youtube.com/watch?v=uzeQ1aha5D4 NASA's Mars 2020 Crater Will Land in Jezero Crater  https://www.youtube.com/watch?v=uzeQ1aha5D4 NASA's Mars 2020 Crater Will Land in Jezero Crater
 
* https://www.youtube.com/watch?v=uzeQ1aha5D4 NASA's Mars 2020 Crater Will Land in Jezero Crater  https://www.youtube.com/watch?v=uzeQ1aha5D4 NASA's Mars 2020 Crater Will Land in Jezero Crater

Revision as of 05:36, 6 June 2022

Mars topography (MOLA dataset) HiRes (1).jpg

Jezero crater was chosen as the landing site for the Mars 2020 rover mission.[1] [2] [3] Perseverance was the name picked for the rover; it landed right on target near the delta on February 18, 2021.[4]

Jezero is an impact crater located at 18.855 N and 77.519 E (282.481 W) in the Syrtis Major quadrangle.[5] [6] It is 47.52 Km in diameter.[7] The crater was named after one of the towns with this name in Bosnia and Herzegovina.[8]

Features near Jezero Crater

                             Features near Jezero Crater

Close view of features in and around Jezero Crater

                    Close view of features in and around Jezero Crater

Rivers on the left side of Jezero carried water into the crater, while the overflow went out at the upper right.

Rivers on the left side of Jezero carried water into the crater, while the overflow went out at the upper right.


Jezero Crater Delta

Drawing and actual pictures of Perseverance actual landing on Mars

                  Drawing and actual pictures of Perseverance actual landing on Mars

This is the first 360-degree panorama taken by Mastcam-Z, a zoomable pair of cameras aboard NASA’s Perseverance Mars rover


This is the first 360-degree panorama taken by Mastcam-Z, a zoomable pair of cameras aboard NASA’s Perseverance Mars rover.

Rocket Scour and Wheel Prints https://photojournal.jpl.nasa.gov/catalog/PIA24488 Taken on March 5, 2021, this color-calibrated image from a Navigation Camera aboard NASA's Mars 2020 Perseverance rover shows tracks from the rover's first drive (darker marks in the foreground) and an area scoured by the Mars 2020 mission's descent stage rockets (lighter-colored area in the middle ground).

Rocket Scour and Wheel Prints https://photojournal.jpl.nasa.gov/catalog/PIA24488 Taken on March 5, 2021, this color-calibrated image from a Navigation Camera aboard NASA's Mars 2020 Perseverance rover shows tracks from the rover's first drive (darker marks in the foreground) and an area scoured by the Mars 2020 mission's descent stage rockets (lighter-colored area in the middle ground).


Features near Jezero Crater

                             Features in Jezero Crater near delta

Distances from landing site to various features in Jezero Crater

                       Distances from landing site to various features in Jezero Crater

Possible paths for Perseverance in Jezero Crater Possible paths for Perseverance in Jezero Crater Mesa is shown from the ground and from orbit.

Thought to have once been flooded with water, the crater contains a fan-delta deposit rich in clays.[9] The lake in the crater was present when valley networks were forming on Mars.[10] [11] Besides having a delta, the crater shows point bars and inverted channels. From a study of the delta and channels, it was concluded that water stayed in the lake for a time; it did not experience times when the water went down. It probably formed when there was continual surface runoff.[12] Jezero Crater is found on the western edge of Isidis Planitia, which is a giant impact basin just north of the Martian equator. This location contains some of the oldest and most scientifically interesting landscapes of Mars. It is thought that Jezero may hold ancient organic molecules and other signs of microbial life because water and sediments collected in the crater billions of years ago when conditions were much more favorable for life.

A team, lead by Briony Horgan used the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM), high resolution imagery, and digital elevation models, to discover places in Jezero Crater that contain carbonates. These minerals they named “Marginal Carbonates” are found along the inside margin of the crater, near the largest valley and in a delta in the west. The authors of the paper believe they were formed in an old lake in Jezero. Evidence of life could be found in these deposits by the 2020 Rover. Even large fossils of strmatolites could be present.[13] [14]

The Mars 2020 rover mission will be able to examine at least 5 types of rock, including clays and carbonates.[15] These can preserve signs of ancient life. Additional materials probably washed in from the surroundings; therefore, we will be able to determine mineral information about the area around the crater.

Activities and discoveries by Perseverance

On September 6, 2021 NASA announced that Perseverance rover collected its first sample of a Martian rock. Perseverance’s rotary-percussive drill on its robotic arm cored into a flat, briefcase-size rock. It has been called “Rochette.” The sample was slightly thicker than a pencil. It is now enclosed in an airtight titanium sample tube, making it available for retrieval in the future. NASA and ESA (European Space Agency) are planning future missions to return the rover’s sample tubes to Earth. This first sample was placed in sample tube serial number 266.[16]

The collection from Rochette came a month after the rover tried and failed to collect a sample from another rock, called “Roubion.” The first sample attempt failed because the rock was softer; hence it crumbled.[17]

Before drilling to get the core sample from the rock, scientists used instruments on the rover to learn more about its composition. They determined that the rock was basaltic and contained salt crystals. The salts may have formed from groundwater or more likely from liquid water that had evaporated into the thin Martian atmosphere. It is hoped that the crystals may also have trapped tiny bubbles of water.[18]


In October 2021, an article was published online by the journal Science about some initial results from photos from Perseverance. It was confirmed that there is an actual delta in Jezero Crater because the typical layers in a delta were seen. Scientists called them bottomsets, foresets and topsets. They were found in a steeply fronted Gilbert-type delta. Since meter-scale boulders were found that may have traveled tens of km, the researchers believe that much rapidly moving water was present at times.[19] [20]

In December 2021, it was announced that some of the rocks in Jezero were igneous.[21] [22] They had once been molten and then slowly cooled. At first ,it looked like many of the rocks photographed by Jezero's camera were sedimentary due to the presence of layering. But, when examined closely, the rocks revealed the mineral olivine surrounded by the mineral pyroxene. That arrangement happens in thick magma bodies and geologists call this type of texture "Cumulate."[23] Carbonate and sulfate minerals were also detected which means that the rocks had been altered by water. The rocks studied were in location nicknamed "South Séítah." "Séítah" (means "amidst the sand" in the Navajo language.[24] The instrument used for this analysis was the Planetary Instrument for X-ray Lithochemistry (PIXL). It uses X-ray fluorescence to determine the elemental composition of rocks.[25]

Two formations, called Maaz and Seitah, are both igneous. Seitah is classified as an olivine-rich cumulate which means it cooled slowly in a thick mass. Maaz is rich in the minerals pyroxene and plagioclase. It cooled quicker on the top of a mass of magma or lava. Water as altered the chemistry of the rock because carbonate, iron oxides, amorphous silicates, sulfates, halite, perchlorates, phosphates, and possible phyllosilicates were found[26] [27]


At the same time, NASA said that organic compounds were found by the SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) instrument. These organics are not only inside of abraded rocks SHERLOC analyzed, but in the dust on non-abraded rock.

Perseverance uses ground-penetrating radar to look under the surface of Mars. RIMFAX (Radar Imager for Mars' Subsurface Experiment) produces a “radargram” of subsurface features up to about 33 feet (10 meters) deep. Scientists found that rock formations with a downward tilt continue into the subsurface.[28]

Many dust devils were detected by Perseverance. In the first 216 Martian days (Sols), the Perseverance Rover in Jezero Crater found that at least four dust devils passed Perseverance on a typical Martian day and that more than one per hour passes by during a peak hourlong period just after noon. Perseverance made these observations mostly with the its cameras and a group of sensors in the Mars Environmental Dynamics Analyzer (MEDA). MEDA includes wind sensors and light sensors.[29] [30] [31]

References

  1. https://www.space.com/42486-mars-2020-rover-jezero-crater-landing-site.html
  2. https://www.jpl.nasa.gov/news/news.php?feature=7286&utm_source=iContact&utm_medium=email&utm_campaign=nasajpl&utm_content=daily20181119-2
  3. https://www.sciencenews.org/article/nasa-mars-2020-rover-landing-site-ancient-alien-life-river-delta?utm_source=email&utm_medium=email&utm_campaign=latest-newsletter-v2
  4. https://mars.nasa.gov/news/8865/touchdown-nasas-mars-perseverance-rover-safely-lands-on-red-planet/
  5. https://hirise.lpl.arizona.edu/PSP_007925_1990
  6. https://www.space.com/mars-2020-alien-life-hunt-microfossils.html?utm_source=Selligent&utm_medium=email&utm_campaign=10118&utm_content=20191116_SDC_Newsletter+-+adhoc+&utm_term=2946561&m_i=LKHS2VBMPdPBKbRsJssJ6HqkTujMa1rGRCQddp5zz8Ss3OSL%2Bdjwc5LY%2BNjlmSR30MzcdNIUCuC1q%2Bfn0ySWT1TcOiknL7DjLx
  7. https://planetarynames.wr.usgs.gov/Feature/14300
  8. https://planetarynames.wr.usgs.gov/Feature/14300
  9. https://hirise.lpl.arizona.edu/PSP_007925_1990
  10. Fassett and Head Iii, 2005 C.I. Fassett, J.W. Head Iii Fluvial sedimentary deposits on Mars: ancient deltas in a crater lake in the Nili Fossae region Geophys. Res. Lett., 32 (14) (2005), 10.1029/2005GL023456 n/a–n/a
  11. Fassett and Head Iii, 2008 C.I. Fassett, J.W. Head Iii. Valley network-fed, open-basin lakes on Mars: distribution and implications for Noachian surface and subsurface hydrology Icarus, 198 (1) (2008), pp. 37-56, 10.1016/j.icarus.2008.06.016
  12. Goudge, T., et al. 2017. STRATIGRAPHY AND EVOLUTION OF DELTA CHANNEL DEPOSITS, JEZERO CRATER, MARS. Lunar and Planetary Science XLVIII (2017). 1195.pdf.
  13. https://www.sciencedirect.com/science/article/pii/S0019103518306067
  14. Horgan, B., et al. 2019. The mineral diversity of Jezero crater: Evidence for possible lacustrine carbonates on Mars. Icarus. In press. https://doi.org/10.1016/j.icarus.2019.113526
  15. https://www.jpl.nasa.gov/news/news.php?feature=7539&utm_source=iContact&utm_medium=email&utm_campaign=nasajpl&utm_content=daily-20191112-1
  16. https://mars.nasa.gov/news/9029/nasas-perseverance-rover-collects-first-mars-rock-sample/
  17. https://spacenews.com/perseverance-collects-first-mars-samples/
  18. https://mars.nasa.gov/news/9036/nasas-perseverance-rover-collects-puzzle-pieces-of-mars-history/
  19. https://www.science.org/doi/10.1126/science.abl4051
  20. Mangold, N., al al. 2021. Perseverance rover reveals an ancient delta-lake system and flood deposits at Jezero crater, Mars. Science. DOI: 10.1126/science.abl4051
  21. https://www.hou.usra.edu/meetings/lpsc2022/pdf/1530.pdf
  22. Schmidt, M., et al. 2022. HIGHLY DIFFERENTIATED BASALTIC LAVAS EXAMINED BY PIXL IN JEZERO CRATER. 53rd Lunar and Planetary Science Conference. 1530.pdf
  23. https://www.bbc.com/news/science-environment-59677383
  24. https://www.bbc.com/news/science-environment-59677383
  25. https://www.jpl.nasa.gov/news/nasas-perseverance-mars-rover-makes-surprising-discoveries
  26. https://www.hou.usra.edu/meetings/lpsc2022/pdf/1798.pdf
  27. Sun, V., et al. 2022. EXPLORING THE JEZERO CRATER FLOOR: OVERVIEW OF RESULTS FROM THE MARS 2020 PERSEVERANCE ROVER’S FIRST SCIENCE CAMPAIGN. 53rd Lunar and Planetary Science Conference (2022. 1798.pdf
  28. https://www.jpl.nasa.gov/news/nasas-perseverance-mars-rover-makes-surprising-discoveries
  29. https://www.jpl.nasa.gov/news/nasas-perseverance-studies-the-wild-winds-of-jezero-crater?utm_source=iContact&utm_medium=email&utm_campaign=nasajpl&utm_content=Day%20in%20Review%20-%206-1-22
  30. https://www.science.org/doi/10.1126/sciadv.abn3783
  31. Newman, C., et al. 2022. The dynamic atmospheric and aeolian environment of Jezero crater, Mars. Science Advances. Vol. 8. Number 21

See Also

External links