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The sands of Mars are green as well as red, rover Perseverance discovers

Geological discoveries hint at conditions when life arose on Earth -- and possibly on Mars

Date:
August 25, 2022
Source:
Purdue University
Summary:
The accepted view of Mars is red rocks and craters as far as the eye can see. That's much what scientists expected when they landed the rover Perseverance in the Jezero Crater, a spot chosen partly for the crater's history as a lake and as part of a rich river system, back when Mars had liquid water, air and a magnetic field. What the rover found once on the ground was startling: Rather than the expected sedimentary rocks -- washed in by rivers and accumulated on the lake bottom -- many of the rocks are volcanic in nature. Specifically, they are composed of large grains of olivine, the muddier less-gemlike version of peridot that tints so many of Hawaii's beaches dark green.
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The accepted view of Mars is red rocks and craters as far as the eye can see. That's much what scientists expected when they landed the rover Perseverance in the Jezero Crater, a spot chosen partly for the crater's history as a lake and as part of a rich river system, back when Mars had liquid water, air and a magnetic field.

What the rover found once on the ground was startling: Rather than the expected sedimentary rocks -- washed in by rivers and accumulated on the lake bottom -- many of the rocks are volcanic in nature. Specifically, they are composed of large grains of olivine, the muddier less-gemlike version of peridot that tints so many of Hawaii's beaches dark green.

Planetary scientists Roger Wiens, professor of earth, atmospheric, and planetary sciences, and Briony Horgan, associate professor of earth, atmospheric, and planetary sciences, in Purdue's College of Science, were instrumental in the discovery and analysis of this data, recently published in a suite of papers in the journals Science and Science Advances.

Wiens led the design and construction of Perseverance's SuperCam, which helps analyze the rock samples and determine their type and origin. Horgan helped select Jezero Crater as the rover's landing site and now uses the Mastcam-Z cameras on Perseverance to put its discoveries into geological context.

"We started to realize that these layered igneous rocks we were seeing look different from the igneous rocks we have these days on Earth," Wiens said. "They're very like igneous rocks on Earth early in its existence."

The rocks and lava the rover is examining on Mars are nearly 4 billion years old. Rocks that old exist on Earth but are incredibly weathered and beaten, thanks to Earth's active tectonic plates as well as the weathering effects of billions of years of wind, water and life. On Mars, these rocks are pristine and much easier to analyze and study.

Understanding the rocks on Mars, their evolution and history, and what they reveal about the history of planetary conditions on Mars helps researchers understand how life may have arisen on Mars and how that compares with early life and conditions on ancient Earth.

"One of the reasons we don't have a great understanding of where and when life first evolved on Earth is because those rocks are mostly gone, so it's really hard to reconstruct what ancient environments on Earth were like," Horgan said. "The rocks Perseverance is roving over in Jezero have more or less just been sitting at the surface for billions of years, waiting for us to come look at them. That's one of the reasons that Mars is an important laboratory for understanding the early solar system."

Scientists can use conditions on early Mars to help extrapolate the environment and conditions on Earth at the same time when life was beginning to arise. Understanding how, and under what conditions, life began will help scientists know where to look for it on other planets and moons, as well as lead to a deeper understanding of biological processes here on Earth.

The search for life is one of Perseverance's main goals and one of the reasons it landed in Jezero Crater in the first place. Discovering the potential for habitable environments in something as uninhabitable as Jezero Crater's aged lava flows raises hopes for what lies in the sedimentary rocks the mission is examining now.

"We're excited to see even better results about organics and ancient habitable environments," Horgan said. "I think it's really setting the stage that Mars is this watery, habitable place, and all the samples we're getting back are going to help us understand the history of ancient microbial life on Mars."

The equipment and innovative instruments are helping the rover carry out its mission in a way no other rover yet has, emphasizing the need to land on the planet so scientists can examine and understand what's really going on.

"From orbit, we looked at these rocks and said, 'Oh, they have beautiful layers!' So we thought they were sedimentary rocks," Horgan said. "And it wasn't until we were very close up and looked at them, at the millimeter scale, that we understood that these are not sedimentary rocks. They're actually ancient lava. It was a huge moment when we figured that out on the ground, and it really illustrated why we need this kind of exploration. The tools we have on the rover are vital because it was impossible to understand the origin of these rocks until we got up close and used all our amazing microscopic instruments to look at them."

The search for life is one of Perseverance's main goals and one of the reasons it landed in Jezero Crater in the first place. Discovering the potential for habitable environments in something as uninhabitable as Jezero Crater's aged lava flows raises hopes for what lies in the sedimentary rocks the mission is examining now.

"We're excited to see even better results about organics and ancient habitable environments," Horgan said. "I think it's really setting the stage that Mars is this watery, habitable place, and all the samples we're getting back are going to help us understand the history of ancient microbial life on Mars."

The equipment and innovative instruments are helping the rover carry out its mission in a way no other rover yet has, emphasizing the need to land on the planet so scientists can examine and understand what's really going on.

"From orbit, we looked at these rocks and said, 'Oh, they have beautiful layers!' So we thought they were sedimentary rocks," Horgan said. "And it wasn't until we were very close up and looked at them, at the millimeter scale, that we understood that these are not sedimentary rocks. They're actually ancient lava. It was a huge moment when we figured that out on the ground, and it really illustrated why we need this kind of exploration. The tools we have on the rover are vital because it was impossible to understand the origin of these rocks until we got up close and used all our amazing microscopic instruments to look at them."


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Materials provided by Purdue University. Note: Content may be edited for style and length.


Journal References:

  1. Roger C. Wiens, Arya Udry, Olivier Beyssac, Cathy Quantin-Nataf, Nicolas Mangold, Agnès Cousin, Lucia Mandon, Tanja Bosak, Olivier Forni, Scott M. McLennan, Violaine Sautter, Adrian Brown, Karim Benzerara, Jeffrey R. Johnson, Lisa Mayhew, Sylvestre Maurice, Ryan B. Anderson, Samuel M. Clegg, Larry Crumpler, Travis S. J. Gabriel, Patrick Gasda, James Hall, Briony H. N. Horgan, Linda Kah, Carey Legett, Juan Manuel Madariaga, Pierre-Yves Meslin, Ann M. Ollila, Francois Poulet, Clement Royer, Shiv K. Sharma, Sandra Siljeström, Justin I. Simon, Tayro E. Acosta-Maeda, Cesar Alvarez-Llamas, S. Michael Angel, Gorka Arana, Pierre Beck, Sylvain Bernard, Tanguy Bertrand, Bruno Bousquet, Kepa Castro, Baptiste Chide, Elise Clavé, Ed Cloutis, Stephanie Connell, Erwin Dehouck, Gilles Dromart, Woodward Fischer, Thierry Fouchet, Raymond Francis, Jens Frydenvang, Olivier Gasnault, Erin Gibbons, Sanjeev Gupta, Elisabeth M. Hausrath, Xavier Jacob, Hemani Kalucha, Evan Kelly, Elise Knutsen, Nina Lanza, Javier Laserna, Jeremie Lasue, Stéphane Le Mouélic, Richard Leveille, Guillermo Lopez Reyes, Ralph Lorenz, Jose Antonio Manrique, Jesus Martinez-Frias, Tim McConnochie, Noureddine Melikechi, David Mimoun, Franck Montmessin, Javier Moros, Naomi Murdoch, Paolo Pilleri, Cedric Pilorget, Patrick Pinet, William Rapin, Fernando Rull, Susanne Schröder, David L. Shuster, Rebecca J. Smith, Alexander E. Stott, Jesse Tarnas, Nathalie Turenne, Marco Veneranda, David S. Vogt, Benjamin P. Weiss, Peter Willis, Kathryn M. Stack, Kenneth H. Williford, Kenneth A. Farley. Compositionally and density stratified igneous terrain in Jezero crater, Mars. Science Advances, 2022; 8 (34) DOI: 10.1126/sciadv.abo3399
  2. Y. Liu, M. M. Tice, M. E. Schmidt, A. H. Treiman, T. V. Kizovski, J. A. Hurowitz, A. C. Allwood, J. Henneke, D. A. K. Pedersen, S. J. VanBommel, M. W. M. Jones, A. L. Knight, B. J. Orenstein, B. C. Clark, W. T. Elam, C. M. Heirwegh, T. Barber, L. W. Beegle, K. Benzerara, S. Bernard, O. Beyssac, T. Bosak, A. J. Brown, E. L. Cardarelli, D. C. Catling, J. R. Christian, E. A. Cloutis, B. A. Cohen, S. Davidoff, A. G. Fairén, K. A. Farley, D. T. Flannery, A. Galvin, J. P. Grotzinger, S. Gupta, J. Hall, C. D. K. Herd, K. Hickman-Lewis, R. P. Hodyss, B. H. N. Horgan, J. R. Johnson, J. L. Jørgensen, L. C. Kah, J. N. Maki, L. Mandon, N. Mangold, F. M. McCubbin, S. M. McLennan, K. Moore, M. Nachon, P. Nemere, L. D. Nothdurft, J. I. Núñez, L. O’Neil, C. M. Quantin-Nataf, V. Sautter, D. L Shuster, K. L. Siebach, J. I. Simon, K. P. Sinclair, K. M. Stack, A. Steele, J. D. Tarnas, N. J. Tosca, K. Uckert, A. Udry, L. A. Wade, B. P. Weiss, R. C. Wiens, K. H. Williford, M.-P. Zorzano. An olivine cumulate outcrop on the floor of Jezero crater, Mars. Science, 2022; DOI: 10.1126/science.abo2756
  3. K. A. Farley, K. M. Stack, D. L. Shuster, B. H. N. Horgan, J. A. Hurowitz, J. D. Tarnas, J. I. Simon, V. Z. Sun, E. L. Scheller, K. R. Moore, S. M. McLennan, P. M. Vasconcelos, R. C. Wiens, A. H. Treiman, L. E. Mayhew, O. Beyssac, T. V. Kizovski, N. J. Tosca, K. H. Williford, L. S. Crumpler, L. W. Beegle, J. F. Bell, B. L. Ehlmann, Y. Liu, J. N. Maki, M. E. Schmidt, A. C. Allwood, H. E. F. Amundsen, R. Bhartia, T. Bosak, A. J. Brown, B. C. Clark, A. Cousin, O. Forni, T. S. J. Gabriel, Y. Goreva, S. Gupta, S.-E. Hamran, C. D. K. Herd, K. Hickman-Lewis, J. R. Johnson, L. C. Kah, P. B. Kelemen, K. B. Kinch, L. Mandon, N. Mangold, C. Quantin-Nataf, M. S. Rice, P. S. Russell, S. Sharma, S. Siljeström, A. Steele, R. Sullivan, M. Wadhwa, B. P. Weiss, A. J. Williams, B. V. Wogsland, P. A. Willis, T. A. Acosta-Maeda, P. Beck, K. Benzerara, S. Bernard, A. S. Burton, E. L. Cardarelli, B. Chide, E. Clavé, E. A. Cloutis, B. A. Cohen, A. D. Czaja, V. Debaille, E. Dehouck, A. G. Fairén, D. T. Flannery, S. Z. Fleron, T. Fouchet, J. Frydenvang, B. J. Garczynski, E. F. Gibbons, E. M. Hausrath, A. G. Hayes, J. Henneke, J. L. Jørgensen, E. M. Kelly, J. Lasue, S. Le Mouélic, J. M. Madariaga, S. Maurice, M. Merusi, P.-Y. Meslin, S. M. Milkovich, C. C. Million, R. C. Moeller, J. I. Núñez, A. M. Ollila, G. Paar, D. A. Paige, D. A. K. Pedersen, P. Pilleri, C. Pilorget, P. C. Pinet, J. W. Rice, C. Royer, V. Sautter, M. Schulte, M. A. Sephton, S. K. Sharma, S. F. Sholes, N. Spanovich, M. St. Clair, C. D. Tate, K. Uckert, S. J. VanBommel, A. G. Yanchilina, M.-P. Zorzano. Aqueously altered igneous rocks sampled on the floor of Jezero crater, Mars. Science, 2022; DOI: 10.1126/science.abo2196

Cite This Page:

Purdue University. "The sands of Mars are green as well as red, rover Perseverance discovers." ScienceDaily. ScienceDaily, 25 August 2022. <www.sciencedaily.com/releases/2022/08/220825205856.htm>.
Purdue University. (2022, August 25). The sands of Mars are green as well as red, rover Perseverance discovers. ScienceDaily. Retrieved October 12, 2024 from www.sciencedaily.com/releases/2022/08/220825205856.htm
Purdue University. "The sands of Mars are green as well as red, rover Perseverance discovers." ScienceDaily. www.sciencedaily.com/releases/2022/08/220825205856.htm (accessed October 12, 2024).

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