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Vaniman, D.
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Forni, O.
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- Creator:
- Anderson, Ryan, Bridges, J. C., Williams, A., Edgar, L., Ollila, A., Williams, J., Nachon, M., Mangold, N., Fisk, M., Schieber, J., Gupta, S., Dromart, G., Wiens, R., Le Mouélic, S., Forni, O., Lanza, N., Mezzacappa, A., Sautter, V., Blaney, D., Clark, B., Clegg, S., Gasnault, O., Lasue, J., Léveillé, R., Lewin, E., Lewis, K. W., Maurice, S., Newsom, H., Schwenzer, S. P., and Vaniman, D.
- Abstract:
- The ChemCam campaign at the fluvial sedimentary outcrop ‘‘Shaler’’ resulted in observations of 28 non-soil targets, 26 of which included active laser induced breakdown spectroscopy (LIBS), and all of which included Remote Micro-Imager (RMI) images. The Shaler outcrop can be divided into seven facies based on grain size, texture, color,...
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- Article
- Full Text:
- ., Williams, A., Edgar, L., Ollila, A., Williams, J., ... & Vaniman, D. (2015). ChemCam results from the
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- Creator:
- Blake, D. F., Morris, R. V., Kocurek, G., Morrison, S. M., Downs, R. T., Bish, D., Ming, D. W., Edgett, K. S., Rubin, D., Goetz, W., Madsen, M. B., Sullivan, R., Gellert, R., Campbell, I., Treiman, A. H., McLennan, S. M., Yen, A. S., Grotzinger, J., Vaniman, D. T., Chipera, S. J., Achilles, C. N., Rampe, E. B., Sumner, D., Meslin, P.-Y., Maurice, S., Forni, O., Gasnault, O., Fisk, M., Schmidt, M., Mahaffy, P., Leshin, L. A., Glavin, D., Steele, A., Freissinet, C., Navarro-González, R., Yingst, R. A., Kah, L. C., Bridges, N., Lewis, K. W., Bristow, T. F., Farmer, J. D., Crisp, J. A., Stolper, E. M., Des Marais, D. J., Sarrazin, P., and MSL Science Team
- Abstract:
- The Rocknest aeolian deposit is similar to aeolian features analyzed by the Mars Exploration Rovers (MERs) Spirit and Opportunity. The fraction of sand <150 micrometers in size contains ~55% crystalline material consistent with a basaltic heritage and ~45% x-ray amorphous material. The amorphous component of Rocknest is iron-rich and silicon-poor...
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- Article
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- I. Campbell,11 A. H. Treiman,12 S. M. McLennan,13 A. S. Yen,14 J. Grotzinger,15 D. T. Vaniman,16 S
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- Creator:
- Meslin, P.-Y., Gasnault, O., Forni, O., Schröder, S., Cousin, A., Berger, G., Clegg, S. M., Lasue, J., Maurice, S., Sautter, V., Le Mouélic, S., Wiens, R. C., Fabre, C., Goetz, W., Bish, D., Mangold, N., Ehlmann, B., Lanza, N., Harri, A.-M., Anderson, R., Rampe, E., McConnochie, T. H., Pinet, P., Blaney, D., Léveillé, R., Archer, D., Barraclough, B., Bender, S., Blake, D., Blank, J. G., Bridges, N., Clark, B. C., DeFlores, L., Delapp, D., Dromart, G., Dyar, M. D., Fisk, M., Gondet, B., Grotzinger, J., Herkenhoff, K., Johnson, J., Lacour, J.-L., Langevin, Y., Leshin, L., Lewin, E., Madsen, M. B., Melikechi, N., Mezzacappa, A., Mischna, M. A., Moores, J. E., Newsom, H., Ollila, A., Perez, R., Renno, N., Sirven, J.-B., Tokar, R., de la Torre, M., d’Uston, L., Vaniman, D., Yingst, A., and MSL Science Team
- Abstract:
- Abstract: The ChemCam instrument, which provides insight into martian soil chemistry at the submillimeter scale, identified two principal soil types along the Curiosity rover traverse: a fine-grained mafic type and a locally derived, coarse-grained felsic type. The mafic soil component is representative of widespread martian soils and is similar in...
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- Article
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- . Ollila,30 R. Perez,31 N. Renno,32 J.-B. Sirven,24 R. Tokar,16 M. de la Torre,9 L. d’Uston,1,2 D. Vaniman
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- Creator:
- Mangold, N., Thompson, L. M., Forni, O., Williams, A. J., Fabre, C., Le Deit, L., Wiens, R. C., Williams, R., Anderson, R. B., Blaney, D. L., Calef, F., Cousin, A., Clegg, S. M., Dromart, G., Dietrich, W. E., Edgett, K. S., Fisk, M. R., Gasnault, O., Gellert, R., Grotzinger, J. P., Kah, L., Le Mouélic, L., McLennan, S. M., Maurice, S., Meslin, P-Y., Newsom, H. E., Palucis, M. C., Rapin, W., Sautter, V., Siebach, K. L., Stack, K., Sumner, D., and Yingst, A.
- Abstract:
- The Curiosity rover has analyzed various detrital sedimentary rocks at Gale Crater, among which fluvial and lacustrine rocks are predominant. Conglomerates correspond both to the coarsest sediments analyzed and the least modified by chemical alteration, enabling us to link their chemistry to that of source rocks on the Gale Crater...
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- Article
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- , R. C. Wiens6, R. Williams7, R. B. Anderson8, D. L. Blaney9, F. Calef9, A. Cousin3, S. M. Clegg6, G