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Showing results for martian crust
Your search for Martina Zrust retrieved no results
Constraints on the martian crust away from the InSight landing site.
Li J, Beghein C, McLennan SM, Horleston AC, Charalambous C, Huang Q, Zenhäusern G, Bozdağ E, Pike WT, Golombek M, Lekić V, Lognonné P, Bruce Banerdt W. Li J, et al. Nat Commun. 2022 Dec 26;13(1):7950. doi: 10.1038/s41467-022-35662-y. Nat Commun. 2022. PMID: 36572693 Free PMC article.
., underside reflections off a subsurface discontinuity halfway between the marsquake and the instrument, which directly constrain the crustal structure away (about 4100-4500 km) from the InSight landing site. Here we show that the Martian crust at the bounce point …
., underside reflections off a subsurface discontinuity halfway between the marsquake and the instrument, which directly constrain the crust …
Thickness and structure of the martian crust from InSight seismic data.
Knapmeyer-Endrun B, Panning MP, Bissig F, Joshi R, Khan A, Kim D, Lekić V, Tauzin B, Tharimena S, Plasman M, Compaire N, Garcia RF, Margerin L, Schimmel M, Stutzmann É, Schmerr N, Bozdağ E, Plesa AC, Wieczorek MA, Broquet A, Antonangeli D, McLennan SM, Samuel H, Michaut C, Pan L, Smrekar SE, Johnson CL, Brinkman N, Mittelholz A, Rivoldini A, Davis PM, Lognonné P, Pinot B, Scholz JR, Stähler S, Knapmeyer M, van Driel M, Giardini D, Banerdt WB. Knapmeyer-Endrun B, et al. Science. 2021 Jul 23;373(6553):438-443. doi: 10.1126/science.abf8966. Science. 2021. PMID: 34437117
A planet's crust bears witness to the history of planetary formation and evolution, but for Mars, no absolute measurement of crustal thickness has been available. Here, we determine the structure of the crust beneath the InSight landing site on Mars using both marsq …
A planet's crust bears witness to the history of planetary formation and evolution, but for Mars, no absolute measurement of crustal …
Elemental composition of the Martian crust.
McSween HY Jr, Taylor GJ, Wyatt MB. McSween HY Jr, et al. Science. 2009 May 8;324(5928):736-9. doi: 10.1126/science.1165871. Science. 2009. PMID: 19423810
The composition of Mars' crust records the planet's integrated geologic history and provides clues to its differentiation. ...Siliceous or calc-alkaline rocks produced by melting and/or fractional crystallization of hydrated, recycled mantle sources, and silica-poor rocks …
The composition of Mars' crust records the planet's integrated geologic history and provides clues to its differentiation. ...Siliceo …
A Review of the "Black Beauty" Martian Regolith Breccia and Its Martian Habitability Record.
Goodwin A, Garwood RJ, Tartèse R. Goodwin A, et al. Astrobiology. 2022 Jun;22(6):755-767. doi: 10.1089/ast.2021.0069. Epub 2022 Feb 25. Astrobiology. 2022. PMID: 35230137 Review.
The regolith breccia Northwest Africa (NWA) 7034 and paired samples are unique meteorite representatives of the martian crust. They are water rich, lithologically varied, and preserve the oldest martian zircon grains yet discovered that formed ca. 4500-4300 M …
The regolith breccia Northwest Africa (NWA) 7034 and paired samples are unique meteorite representatives of the martian crust. …
Origin and age of the earliest Martian crust from meteorite NWA 7533.
Humayun M, Nemchin A, Zanda B, Hewins RH, Grange M, Kennedy A, Lorand JP, Göpel C, Fieni C, Pont S, Deldicque D. Humayun M, et al. Nature. 2013 Nov 28;503(7477):513-6. doi: 10.1038/nature12764. Epub 2013 Nov 20. Nature. 2013. PMID: 24256724
This evidence for early crustal differentiation implies that the Martian crust, and its volatile inventory, formed in about the first 100 million years of Martian history, coeval with earliest crust formation on the Moon and the Earth. In addition, inc …
This evidence for early crustal differentiation implies that the Martian crust, and its volatile inventory, formed in about th …
Martian stable isotopes: volatile evolution, climate change and exobiological implications.
Jakosky BM. Jakosky BM. Orig Life Evol Biosph. 1999 Jan;29(1):47-57. doi: 10.1023/a:1006586319129. Orig Life Evol Biosph. 1999. PMID: 10077868 Review.
Measurements of the ratios of stable isotopes in the martian atmosphere and crust provide fundamental information about the evolution of the martian volatile and climate system. ...Processes of volatile evolution and exchange will fractionate the isotopes in …
Measurements of the ratios of stable isotopes in the martian atmosphere and crust provide fundamental information about the ev …
Observational constraints on the process and products of Martian serpentinization.
Tutolo BM, Tosca NJ. Tutolo BM, et al. Sci Adv. 2023 Feb 3;9(5):eadd8472. doi: 10.1126/sciadv.add8472. Epub 2023 Feb 3. Sci Adv. 2023. PMID: 36735795 Free PMC article.
To constrain the process and products of Martian serpentinization, we studied serpentinized iron-rich olivines from the 1.1-billion-year Duluth Complex. ...The widespread occurrence of oxidized iron-bearing phyllosilicates in highly magnetized regions of the Martian
To constrain the process and products of Martian serpentinization, we studied serpentinized iron-rich olivines from the 1.1-billion-y …
Early oxidation of the martian crust triggered by impacts.
Deng Z, Moynier F, Villeneuve J, Jensen NK, Liu D, Cartigny P, Mikouchi T, Siebert J, Agranier A, Chaussidon M, Bizzarro M. Deng Z, et al. Sci Adv. 2020 Oct 30;6(44):eabc4941. doi: 10.1126/sciadv.abc4941. Print 2020 Oct. Sci Adv. 2020. PMID: 33127679 Free PMC article.
This implies early, impact-induced, oxidation events that increased by five to six orders of magnitude the oxygen fugacity of impact melts from remelting of the crust. Oxygen isotopic compositions of sequentially crystallized phases from the clasts show that progressive ox …
This implies early, impact-induced, oxidation events that increased by five to six orders of magnitude the oxygen fugacity of impact melts f …
The martian surface.
Opik EJ. Opik EJ. Science. 1966 Jul 15;153(3733):255-65. doi: 10.1126/science.153.3733.255. Science. 1966. PMID: 17779983
This, and the low eroded rims of the Martian craters suggest that many of the craters have survived almost since the formation of the crust. ...If not vegetation, it must be something thing specifically Martian; no other hypothesis hitherto proposed is able t …
This, and the low eroded rims of the Martian craters suggest that many of the craters have survived almost since the formation of the …
Surface waves and crustal structure on Mars.
Kim D, Banerdt WB, Ceylan S, Giardini D, Lekić V, Lognonné P, Beghein C, Beucler É, Carrasco S, Charalambous C, Clinton J, Drilleau M, Durán C, Golombek M, Joshi R, Khan A, Knapmeyer-Endrun B, Li J, Maguire R, Pike WT, Samuel H, Schimmel M, Schmerr NC, Stähler SC, Stutzmann E, Wieczorek M, Xu Z, Batov A, Bozdag E, Dahmen N, Davis P, Gudkova T, Horleston A, Huang Q, Kawamura T, King SD, McLennan SM, Nimmo F, Plasman M, Plesa AC, Stepanova IE, Weidner E, Zenhäusern G, Daubar IJ, Fernando B, Garcia RF, Posiolova LV, Panning MP. Kim D, et al. Science. 2022 Oct 28;378(6618):417-421. doi: 10.1126/science.abq7157. Epub 2022 Oct 27. Science. 2022. PMID: 36302020
By measuring group velocity dispersion along the impact-lander path, we obtained a direct constraint on crustal structure away from the InSight lander. The crust north of the equatorial dichotomy had a shear wave velocity of approximately 3.2 kilometers per second in the 5 …
By measuring group velocity dispersion along the impact-lander path, we obtained a direct constraint on crustal structure away from the InSi …
107 results