Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Linda M. V. Martel"'
Autor:
G. Jeffrey Taylor, Jeffrey J. Gillis-Davis, Linda M. V. Martel, Paul G. Lucey, Philippe Sarrazin, David F. Blake
Publikováno v:
Geochimica et Cosmochimica Acta. 266:17-28
We used X-Ray Diffraction (XRD) and Rietveld refinement to determine the modal mineralogy of 118 lunar regolith samples (
Publikováno v:
Meteoritics & Planetary Science. 47:861-879
– We have studied 27 KREEP basalt fragments in six thin sections of samples collected from four Apollo 15 stations. Based on local geology and regional remote sensing data, these samples represent KREEP basalt lava flows that lie beneath the younge
Publikováno v:
Geophysical Research Letters. 37
[1] Orbital gamma ray spectrometry shows that the Martian surface has a mean Cl/K ratio of 1.3 ± 0.2, indistinguishable from the ratio in CI chondrites (1.28). Although Cl and K fractionate by magma degassing and aqueous processing, during igneous p
Autor:
Sylvestre Maurice, Kyeong Ja Kim, James M. Dohm, Daniel M. Janes, Linda M. V. Martel, Gerlind Dreibus, Kris Kerry, Robert C. Reedy, D. M. Drake, D. K. Hamara, Steven W. Squyres, William V. Boynton, J. Brückner, Scott M. McLennan, B. C. Hahn, Heinrich Wänke, John Keller, Victor R. Baker, Olivier Gasnault, Julie Stopar, R. D. Starr, Ann L. Sprague, G. Jeffrey Taylor, Claude d’Uston, Larry G. Evans, Suniti Karunatillake, P. A. J. Englert
Publikováno v:
Journal of Geophysical Research. 112
[1] K/Th determined by the Mars Odyssey Gamma Ray Spectrometer varies by a factor of 3 on Mars (3000 to 9000), but over 95% of the surface area has K/Th between 4000 and 7000. K/Th is distinctly lower than average in some areas, including west of Oly
Autor:
Ronald Greeley, Linda M. V. Martel
Publikováno v:
International Journal of Remote Sensing. 9:1071-1085
Radar images of Craters of the Moon, Idaho were used to study the backscatter characteristics of basaltic lava flows of predominantly pahoehoe textures and to determine the ability to detct fissure vents. Four images were obtained: X-band HH, X-band