Results 121 to 130 of about 35,501 (220)

Glen Torridon Mineralogy and the Sedimentary History of the Clay Mineral Bearing Unit [PDF]

Clay minerals are common in ancient terrains on Mars and their presence at the surface alludes to aqueous processes in the Noachian to Early Hesperian (>3.5 Ga). Gale crater was selected as Curiositys landing site largely because of the identification of
Achilles, C. N., Bennett, K. A., Blake, D. F., Bristow, T. F., Castle, N., Chipera, S. J., Craig, P. I., Downs, G. W., Downs, R. T., Fox, V. K., Grotzinger, J. P., Gupta, S., Hazen, R. M., Mahaffy, P. R., Malespin, C.A., Marais, D. J. Des, McAdam, A. C., Ming, D. W., Morris, R. V., Morrison, S. M., Rampe, E. B., Thorpe, M. T., Treiman, A. H., Tu, V., Vaniman, D. T, Vasavada, A. R., Yen, A. S.   +26 more
core   +1 more source

Clay minerals evidences for coldn-warm fluctuations in the Early Silurian. [PDF]

PLoS One
Zhang Z, Zhang J, Wei H, Li H, Guo Y, Zeng C.   +5 more
europepmc   +1 more source

Soil mineralogy and potassium forms distribution and release in some calcareous soils of the Darab Region, Iran. [PDF]

PLoS One
Javan M, Abtahi A, Zareian G, Haghighatnia H.   +3 more
europepmc   +1 more source

Bioinspired Lignin-Aluminosilicate Composite for CO₂ Storage. [PDF]

ACS Omega
Koo JW, Yeo JB, Jang JH, Jo J, Heo J, Yoon J, Jo YI, Ko C, Lee MY, Hong JS, Kim M, Nam KT.   +11 more
europepmc   +1 more source

MSATT Workshop on Chemical Weathering on Mars [PDF]

The topics covered with respect to chemical weathering on Mars include the following: Mars soil, mineralogy, spectroscopic analysis, clays, silicates, oxidation, iron oxides, water, chemical reactions, geochemistry, minerals, Mars atmosphere, atmospheric
Banin, Amos, Burns, Roger
core   +1 more source

Physico-chemical behaviour and microbiological suitability of residual smectitic soils mixed with two mineralized waters for therapeutic and dermocosmetic applications. [PDF]

Int J Biometeorol
Valente A, Rocha F, Cunha Â, Terroso D, Sequeira C, da Silva EF.   +5 more
europepmc   +1 more source

Oxygen isotopic evidence that Gale crater, Mars, was home to an Early Hesperian water reservoir that underwent significant evaporation. [PDF]

Proc Natl Acad Sci U S A
Hofmann AE, Archer PD, McAdam AC, Sutter B, Bristow TF, Eiler JM, Webster CR, Flesch GJ, Fraeman AA, Franz HB, House CH, Rampe EB, Stern JC, Mahaffy PR, Malespin CA, Grotzinger JP, Vasavada AR.   +16 more
europepmc   +1 more source

The spectroscopic, chemical, and photophysical properties of Martian soils and their analogs (MERC, phase 2) [PDF]

A series of variably proportioned iron/calcium smectite clays and iron loaded smectite clays containing iron up to the level found in the Martian soil were prepared from a typical montomorillonite clay using the Banin method.
Banin, Amos, Orenberg, James
core   +1 more source

Controls of Geological Factors on H₂ Adsorption in the Subsurface. [PDF]

ACS Omega
Li X, Walters CC, Zhang T, Sun X.
europepmc   +1 more source

Origin and Evolution of Clay Mineral and Its Impact on Shale Oil Enrichment: Insight from Qingshankou Formation, Songliao Basin, NE China. [PDF]

ACS Omega
Kang Y, Liu K, Zhu R, Zhang S, Wu S, Zhang J, Liu C.   +6 more
europepmc   +1 more source