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811 results on '"Arvidson, R"'

1. Plasmonic Nature of the Terahertz Conductivity Peak in Single-Wall Carbon Nanotubes

Author

Zhang, Q., Haroz, E. H., Jin, Z., Ren, L., Wang, X., Arvidson, R. S., Luttge, A., and Kono, J.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

Plasmon resonance is expected to occur in metallic and doped semiconducting carbon nanotubes in the terahertz frequency range, but its convincing identification has so far been elusive. The origin of the terahertz conductivity peak commonly observed for carbon nanotube ensembles remains controversial. Here we present results of optical, terahertz, and DC transport measurements on highly enriched metallic and semiconducting nanotube films. A broad and strong terahertz conductivity peak appears in both types of films, whose behaviors are consistent with the plasmon resonance explanation, firmly ruling out other alternative explanations such as absorption due to curvature-induced gaps., Comment: 8 pages, 4 figure

Published
2013
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2. Midinfrared Third Harmonic Generation from Macroscopically Aligned Ultralong Single-Wall Carbon Nanotubes

Author

Morris, D. T., Pint, C. L., Arvidson, R. S., Luttge, A., Hauge, R. H., Belyanin, A. A., Woods, G. L., and Kono, J.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

We report the observation of strong third harmonic generation from a macroscopic array of aligned ultralong single-wall carbon nanotubes (SWCNTs) with intense midinfrared radiation. Through power-dependent experiments, we determined the absolute value of the third-order nonlinear optical susceptibility, $\chi^{(3)}$, of our SWCNT film to be 5.53 $\times$ 10$^{-12}$ esu, three orders of magnitude larger than that of the fused silica reference we used. Taking account of the filling factor of 8.75% for our SWCNT film, we estimate a $\chi^{(3)}$ of 6.32 $\times$ 10$^{-11}$ esu for a fully dense film. Furthermore, through polarization-dependent experiments, we extracted all the nonzero elements of the $\chi^{(3)}$ tensor, determining the magnitude of the weaker tensor elements to be $\sim$1/6 of that of the dominant $\chi^{(3)}_{zzzz}$ component., Comment: 5 pages, 3 figures

Published
2013
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3. MRO/CRISM Retrieval of Surface Lambert Albedos for Multispectral Mapping of Mars with DISORT-based Rad. Transfer Modeling: Phase 1 - Using Historical Climatology for Temperatures, Aerosol Opacities, & Atmo. Pressures

Author

McGuire, P. C., Wolff, M. J., Smith, M. D., Arvidson, R. E., Murchie, S. L., Clancy, R. T., Roush, T. L., Cull, S. C., Lichtenberg, K. A., Wiseman, S. M., Green, R. O., Martin, T. Z., Milliken, R. E., Cavender, P. J., Humm, D. C., Seelos, F. P., Seelos, K. D., Taylor, H. W., Ehlmann, B. L., Mustard, J. F., Pelkey, S. M., Titus, T. N., Hash, C. D., Malaret, E. R., and Team, the CRISM

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We discuss the DISORT-based radiative transfer pipeline ('CRISM_LambertAlb') for atmospheric and thermal correction of MRO/CRISM data acquired in multispectral mapping mode (~200 m/pixel, 72 spectral channels). Currently, in this phase-one version of the system, we use aerosol optical depths, surface temperatures, and lower-atmospheric temperatures, all from climatology derived from Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) data, and surface altimetry derived from MGS Mars Orbiter Laser Altimeter (MOLA). The DISORT-based model takes as input the dust and ice aerosol optical depths (scaled to the CRISM wavelength range), the surface pressures (computed from MOLA altimetry, MGS-TES lower-atmospheric thermometry, and Viking-based pressure climatology), the surface temperatures, the reconstructed instrumental photometric angles, and the measured I/F spectrum, and then outputs a Lambertian albedo spectrum. The Lambertian albedo spectrum is valuable geologically since it allows the mineralogical composition to be estimated. Here, I/F is defined as the ratio of the radiance measured by CRISM to the solar irradiance at Mars divided by $\pi$. After discussing the capabilities and limitations of the pipeline software system, we demonstrate its application on several multispectral data cubes: the outer northern ice cap of Mars, Tyrrhena Terra, and near the landing site for the Phoenix mission. For the icy spectra near the northern polar cap, aerosols need to be included in order to properly correct for the CO_2 absorption in the H_{2}O ice bands at wavelengths near 2.0 $\mu$m. In future phases of software development, we intend to use CRISM data directly in order to retrieve the spatiotemporal maps of aerosol optical depths, surface pressure and surface temperature.

Published
2009

4. A Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, Mars

Author

Grotzinger, JP, Sumner, DY, Kah, LC, Stack, K, Gupta, S, Edgar, L, Rubin, D, Lewis, K, Schieber, J, Mangold, N, Milliken, R, Conrad, PG, DesMarais, D, Farmer, J, Siebach, K, Calef, F, Hurowitz, J, McLennan, SM, Ming, D, Vaniman, D, Crisp, J, Vasavada, A, Edgett, KS, Malin, M, Blake, D, Gellert, R, Mahaffy, P, Wiens, RC, Maurice, S, Grant, JA, Wilson, S, Anderson, RC, Beegle, L, Arvidson, R, Hallet, B, Sletten, RS, Rice, M, Bell, J, Griffes, J, Ehlmann, B, Anderson, RB, Bristow, TF, Dietrich, WE, Dromart, G, Eigenbrode, J, Fraeman, A, Hardgrove, C, Herkenhoff, K, Jandura, L, Kocurek, G, Lee, S, Leshin, LA, Leveille, R, Limonadi, D, Maki, J, McCloskey, S, Meyer, M, Minitti, M, Newsom, H, Oehler, D, Okon, A, Palucis, M, Parker, T, Rowland, S, Schmidt, M, Squyres, S, Steele, A, Stolper, E, Summons, R, Treiman, A, Williams, R, Yingst, A, Team, MSL Science, Kemppinen, Osku, Bridges, Nathan, Johnson, Jeffrey R, Cremers, David, Godber, Austin, Wadhwa, Meenakshi, Wellington, Danika, McEwan, Ian, Newman, Claire, Richardson, Mark, Charpentier, Antoine, Peret, Laurent, King, Penelope, Blank, Jennifer, Weigle, Gerald, Li, Shuai, Robertson, Kevin, Sun, Vivian, Baker, Michael, Edwards, Christopher, Farley, Kenneth, Miller, Hayden, Newcombe, Megan, Pilorget, Cedric, Brunet, Claude, Hipkin, Victoria, and Léveillé, Richard

Subjects
Bays, Carbon, Exobiology, Extraterrestrial Environment, Geologic Sediments, Hydrogen, Hydrogen-Ion Concentration, Iron, Mars, Nitrogen, Oxidation-Reduction, Oxygen, Phosphorus, Salinity, Sulfur, Water, MSL Science Team, General Science & Technology
Abstract

The Curiosity rover discovered fine-grained sedimentary rocks, which are inferred to represent an ancient lake and preserve evidence of an environment that would have been suited to support a martian biosphere founded on chemolithoautotrophy. This aqueous environment was characterized by neutral pH, low salinity, and variable redox states of both iron and sulfur species. Carbon, hydrogen, oxygen, sulfur, nitrogen, and phosphorus were measured directly as key biogenic elements; by inference, phosphorus is assumed to have been available. The environment probably had a minimum duration of hundreds to tens of thousands of years. These results highlight the biological viability of fluvial-lacustrine environments in the post-Noachian history of Mars.

Published
2014

5. Two Years at Meridiani Planum: Results from the Opportunity Rover

Author

Squyres, S. W., Knoll, A. H., Arvidson, R. E., Clark, B. C., Grotzinger, J. P., Jolliff, B. L., McLennan, S. M., Tosca, N., Bell, J. F., Calvin, W. M., Farrand, W. H., Glotch, T. D., Golombek, M. P., Herkenhoff, K. E., Johnson, J. R., Klingelhöfer, G., McSween, H. Y., and Yen, A. S.

Published
2006

7. Localization and Physical Property Experiments Conducted by Opportunity at Meridiani Planum

Author

Arvidson, R. E., Anderson, R. C., Bartlett, P., Bell, J. F., Christensen, P. R., Chu, P., Davis, K., Ehlmann, B. L., Golombek, M. P., Gorevan, S., Guinness, E. A., Haldemann, A. F. C., Herkenhoff, K. E., Landis, G., Li, R., Lindemann, R., Ming, D. W., Myrick, T., Parker, T., Richter, L., Seelos, F. P., Soderblom, L. A., Squyres, S. W., Sullivan, R. J., and Wilson, J.

Published
2004

8. Mineralogy at Meridiani Planum from the Mini-TES Experiment on the Opportunity Rover

Author

Christensen, P. R., Wyatt, M. B., Glotch, T. D., Rogers, A. D., Anwar, S., Arvidson, R. E., Bandfield, J. L., Blaney, D. L., Budney, C., Calvin, W. M., Fallacaro, A., Fergason, R. L., Gorelick, N., Graff, T. G., Hamilton, V. E., Hayes, A. G., Johnson, J. R., Knudson, A. T., McSween, H. Y., Mehall, G. L., Mehall, L. K., Moersch, J. E., Morris, R. V., Smith, M. D., Squyres, S. W., Ruff, S. W., and Wolff, M. J.

Published
2004

9. Soils of Eagle Crater and Meridiani Planum at the Opportunity Rover Landing Site

Author

Soderblom, L. A., Anderson, R. C., Arvidson, R. E., Bell, J. F., Cabrol, N. A., Calvin, W., Christensen, P. R., Clark, B. C., Economou, T., Ehlmann, B. L., Farrand, W. H., Fike, D., Gellert, R., Glotch, T. D., Golombek, M. P., Greeley, R., Grotzinger, J. P., Herkenhoff, K. E., Jerolmack, D. J., Johnson, J. R., Jolliff, B., Klingelhöfer, G., Knoll, A. H., Learner, Z. A., Li, R., Malin, M. C., McLennan, S. M., McSween, H. Y., Ming, D. W., Morris, R. V., Rice, J. W., Richter, L., Rieder, R., Rodionov, D., Schröder, C., Seelos, F. P., Soderblom, J. M., Squyres, S. W., Sullivan, R., Watters, W. A., Weitz, C. M., Wyatt, M. B., Yen, A., and Zipfel, J.

Published
2004

11. The Opportunity Rover's Athena Science Investigation at Meridiani Planum, Mars

Author

Squyres, S. W., Arvidson, R. E., Bell, J. F., Brückner, J., Cabrol, N. A., Calvin, W., Carr, M. H., Christensen, P. R., Clark, B. C., Crumpler, L., d'Uston, C., Economou, T., Farmer, J., Farrand, W., Folkner, W., Golombek, M., Gorevan, S., Grant, J. A., Greeley, R., Grotzinger, J., Haskin, L., Herkenhoff, K. E., Hviid, S., Johnson, J., Klingelhöfer, G., Knoll, A. H., Landis, G., Lemmon, M., Li, R., Madsen, M. B., Malin, M. C., McLennan, S. M., McSween, H. Y., Ming, D. W., Moersch, J., Morris, R. V., Parker, T., Rice, J. W., Richter, L., Rieder, R., Sims, M., Smith, M., Smith, P., Soderblom, L. A., Sullivan, R., Wänke, H., Wdowiak, T., Wolff, M., and Yen, A.

Published
2004

12. In Situ Evidence for an Ancient Aqueous Environment at Meridiani Planum, Mars

Author

Squyres, S. W., Grotzinger, J. P., Arvidson, R. E., Bell, J. F., Calvin, W., Christensen, P. R., Clark, B. C., Crisp, J. A., Farrand, W. H., Herkenhoff, K. E., Johnson, J. R., Klingelhöfer, G., Knoll, A. H., McLennan, S. M., McSween, H. Y., Morris, R. V., Rice, J. W., Rieder, R., and Soderblom, L. A.

Published
2004

13. Evidence from Opportunity's Microscopic Imager for Water on Meridiani Planum

Author

Herkenhoff, K. E., Squyres, S. W., Arvidson, R., Bass, D. S., Bell, J. F., Bertelsen, P., Ehlmann, B. L., Farrand, W., Gaddis, L., Greeley, R., Grotzinger, J., Hayes, A. G., Hviid, S. F., Johnson, J. R., Jolliff, B., Kinch, K. M., Knoll, A. H., Madsen, M. B., Maki, J. N., McLennan, S. M., McSween, H. Y., Ming, D. W., Rice, J. W., Richter, L., Sims, M., Smith, P. H., Soderblom, L. A., Spanovich, N., Sullivan, R., Thompson, S., Wdowiak, T., Weitz, C., and Whelley, P.

Published
2004

14. Pancam Multispectral Imaging Results from the Opportunity Rover at Meridiani Planum

Author

Bell, J. F., Squyres, S. W., Arvidson, R. E., Arneson, H. M., Bass, D., Calvin, W., Farrand, W. H., Goetz, W., Golombek, M., Greeley, R., Grotzinger, J., Guinness, E., Hayes, A. G., Hubbard, M. Y. H., Herkenhoff, K. E., Johnson, M. J., Johnson, J. R., Joseph, J., Kinch, K. M., Lemmon, M. T., Li, R., Madsen, M. B., Maki, J. N., Malin, M., McCartney, E., McLennan, S., McSween, H. Y., Ming, D. W., Morris, R. V., Parker, T. J., Proton, J., Rice, J. W., Seelos, F., Soderblom, J. M., Soderblom, L. A., Sohl-Dickstein, J. N., Sullivan, R. J., Weitz, C. M., and Wolff, M. J.

Published
2004

15. Basaltic Rocks Analyzed by the Spirit Rover in Gusev Crater

Author

McSween, H. Y., Arvidson, R. E., Bell, J. F., Blaney, D., Cabrol, N. A., Christensen, P. R., Clark, B. C., Crisp, J. A., Crumpler, L. S., Farmer, J. D., Gellert, R., Ghosh, A., Gorevan, S., Graff, T., Grant, J., Haskin, L. A., Herkenhoff, K. E., Johnson, J. R., Jolliff, B. L., Klingelhoefer, G., Knudson, A. T., McLennan, S., Milam, K. A., Moersch, J. E., Morris, R. V., Rieder, R., Ruff, S. W., de Souza, P. A., Squyres, S. W., Wänke, H., Wang, A., Wyatt, M. B., Yen, A., and Zipfel, J.

Published
2004

16. Wind-Related Processes Detected by the Spirit Rover at Gusev Crater, Mars

Author

Greeley, R., Squyres, S. W., Arvidson, R. E., Bartlett, P., Bell, J. F., Blaney, D., Cabrol, N. A., Farmer, J., Farrand, B., Golombek, M. P., Gorevan, S. P., Grant, J. A., Haldemann, A. F. C., Herkenhoff, K. E., Johnson, J., Landis, G., Madsen, M. B., McLennan, S. M., Moersch, J., Rice, J. W., Richter, L., Ruff, S., Sullivan, R. J., Thompson, S. D., Wang, A., Weitz, C. M., and Whelley, P.

Published
2004

17. The Spirit Rover's Athena Science Investigation at Gusev Crater, Mars

Author

Squyres, S. W., Arvidson, R. E., Bell, J. F., Brückner, J., Cabrol, N. A., Calvin, W., Carr, M. H., Christensen, P. R., Clark, B. C., Crumpler, L., d'Uston, C., Economou, T., Farmer, J., Farrand, W., Folkner, W., Golombek, M., Gorevan, S., Grant, J. A., Greeley, R., Grotzinger, J., Haskin, L., Herkenhoff, K. E., Hviid, S., Johnson, J., Klingelhöfer, G., Knoll, A., Landis, G., Lemmon, M., Li, R., Madsen, M. B., Malin, M. C., McLennan, S. M., McSween, H. Y., Ming, D. W., Moersch, J., Morris, R. V., Parker, T., Rice, J. W., Richter, L., Rieder, R., Sims, M., Smith, M., Smith, P., Soderblom, L. A., Sullivan, R., Wänke, H., Wdowiak, T., Wolff, M., and Yen, A.

Published
2004

19. Localization and Physical Properties Experiments Conducted by Spirit at Gusev Crater

Author

Arvidson, R. E., Anderson, R. C., Bartlett, P., Bell, J. F., Blaney, D., Christensen, P. R., Chu, P., Crumpler, L., Davis, K., Ehlmann, B. L., Fergason, R., Golombek, M. P., Gorevan, S., Grant, J. A., Greeley, R., Guinness, E. A., Haldemann, A. F. C., Herkenhoff, K., Johnson, J., Landis, G., Li, R., Lindemann, R., McSween, H., Ming, D. W., Myrick, T., Richter, L., Seelos, F. P., Squyres, S. W., Sullivan, R. J., Wang, A., and Wilson, J.

Published
2004

20. Surficial Deposits at Gusev Crater along Spirit Rover Traverses

Author

Grant, J. A., Arvidson, R., Bell, J. F., Cabrol, N. A., Carr, M. H., Christensen, P., Crumpler, L., Ehlmann, B. L., Farmer, J., Golombek, M., Grant, F. D., Greeley, R., Herkenhoff, K., Li, R., McSween, H. Y., Ming, D. W., Moersch, J., Rice, J. W., Ruff, S., Richter, L., Squyres, S., Sullivan, R., and Weitz, C.

Published
2004

21. Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover

Author

Christensen, P. R., Ruff, S. W., Fergason, R. L., Knudson, A. T., Anwar, S., Arvidson, R. E., Bandfield, J. L., Blaney, D. L., Budney, C., Calvin, W. M., Glotch, T. D., Golombek, M. P., Gorelick, N., Graff, T. G., Hamilton, V. E., Hayes, A., Johnson, J. R., McSween, H. Y., Mehall, G. L., Mehall, L. K., Moersch, J. E., Morris, R. V., Rogers, A. D., Smith, M. D., Squyres, S. W., Wolff, M. J., and Wyatt, M. B.

Published
2004

22. Pancam Multispectral Imaging Results from the Spirit Rover at Gusev Crater

Author

Bell, J. F., Squyres, S. W., Arvidson, R. E., Arneson, H. M., Bass, D., Blaney, D., Cabrol, N., Calvin, W., Farmer, J., Farrand, W. H., Goetz, W., Golombek, M., Grant, J. A., Greeley, R., Guinness, E., Hayes, A. G., Hubbard, M. Y. H., Herkenhoff, K. E., Johnson, M. J., Johnson, J. R., Joseph, J., Kinch, K. M., Lemmon, M. T., Li, R., Madsen, M. B., Maki, J. N., Malin, M., McCartney, E., McLennan, S., McSween, H. Y., Ming, D. W., Moersch, J. E., Morris, R. V., Parker, T. J., Proton, J., Rice, J. W., Seelos, F., Soderblom, J., Soderblom, L. A., Sohl-Dickstein, J. N., Sullivan, R. J., Wolff, M. J., and Wang, A.

Published
2004

23. The Stratigraphy of Central and Western Butte and the Greenheugh Pediment Contact

Author

Bryk, A. B, Dietrich, W. E, Fox, V. K, Bennett, K. A, Banham, S. G, Lamb, M. P, Grotzinger, J. P, Vasavada, A. R, Stack, K. M, Arvidson, R, Fedo, C. M, Gupta, S, Wiens, R. C, Williams, R. M. E, Kronyak, R.E, Turner, M. L, Lewis, K. W, Rubin, D. M, Rapin, W. N, Deit, L. Le, Mouélic, S. Le, Edgett, K. S, Fraeman, A. A, Hughes, M. N, Kah, L. C, and Bedford, C. C

Subjects
Space Sciences (General)
Abstract

The Greenheugh pediment at the base of Aeolis Mons (Mt. Sharp), which may truncate units in the Murray formation and is capped by a thin sandstone unit, appears to represent a major shift in climate history within Gale crater. The pediment appears to be an erosional remnant of potentially a much more extensive feature. Curiosity’s traverse through the southern extent of Glen Torridon (south of Vera Rubin ridge) has brought the rover in contact with several new stratigraphic units that lie beneath the pediment. These strata were visited at two outcrop-forming buttes (Central and Western butte- both remnants of the retreating pediment) south of an orbitally defined boundary marking the transition from the Fractured Clay-bearing Unit (fCU) and the fractured Intermediate Unit (fIU). Here we present preliminary interpretations of the stratigraphy within Central and Western buttes and propose the Western butte cap rocks do not match the pediment capping unit.

Published
2020

24. THE GEDIZ VALLIS SYSTEM IN GALE CRATER ON MARS: HIRISE VIEWS OF THE INVERTED

Author

Wilson, S.A., Thompson, L., Hughes, M., Fedo, C., Arvidson, R., Bryk, A., Davis, J., Dietrich, W.E., Gasnault, O., Grant, J.A., Gupta, S., House, C., Kite, E., Kubacki, T., Larter, S., Newsom, H.E., Paar, G., Rivera-Hernández, F., Roberts, A., Williams, R., Center for Earth and Planetary Studies [Washington] (CEPS), Smithsonian National Air and Space Museum, Smithsonian Institution-Smithsonian Institution, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Imperial College London, Institute of Meteoritics [Albuquerque] (IOM), The University of New Mexico [Albuquerque], and Lunar and Planetary Institute

Subjects
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, [SDU]Sciences of the Universe [physics], [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
Abstract

International audience

Published
2023

27. The Sedimentary History of Mars as Observed by Rovers

Author

Rampe, E. B, Arvidson, R. E, Edgar, L. A, Edgett, K. S, Fedo, C. M, Fraeman, A. A, Grotzinger, J. P, McLennan, S. M, Ming, D. W, Morris, R. V, Siebach, K. L, and Sullivan, R. J

Subjects
Lunar And Planetary Science And Exploration
Abstract

Mars has a sedimentary history that spans billions of years. Orbital images have allowed for the identification of vast regional sedimentary deposits that can be traced over 100s of kilometers and are 100s of meters thick including localized alluvial, deltaic, and lacustrine deposits. Detections of secondary minerals in these deposits from orbital spectroscopy suggest the aqueous history of early Mars varied as a function of space and time. Orbital observations, however, provide a simplified and incomplete picture of Mars’ sedimentary history because measurements for inferring sediment transport and deposition, such as lithology, grain size, and internal structures, and measurements for inferring sediment source and aqueous alteration, such as outcrop-scale mineralogic and geochemical composition and diagenetic features, cannot be identified from orbit. Rover observations have significantly enhanced our view of ancient and modern sedimentary environments on Mars, resulting in detailed reconstructions of paleo-environments and habitability.

Published
2019

28. Deposition, exhumation, and paleoclimate of an ancient lake deposit, Gale crater, Mars

Author

Grotzinger, J. P., Gupta, S., Malin, M. C., Rubin, D. M., Schieber, J., Siebach, K., Sumner, D. Y., Stack, K. M., Vasavada, A. R., Arvidson, R. E., Calef, F., Edgar, L., Fischer, W. F., Grant, J. A., Griffes, J., Kah, L. C., Lamb, M. P., Lewis, K. W., Mangold, N., Minitti, M. E., Palucis, M., Rice, M., Williams, R. M. E., Yingst, R. A., Blake, D., Blaney, D., Conrad, P., Crisp, J., Dietrich, W. E., Dromart, G., Edgett, K. S., Ewing, R. C., Gellert, R., Hurowitz, J. A., Kocurek, G., Mahaffy, P., McBride, M. J., McLennan, S. M., Mischna, M., Ming, D., Milliken, R., Newsom, H., Oehler, D., Parker, T. J., Vaniman, D., Wiens, R. C., and Wilson, S. A.

Published
2015

29. Using Mineralogy of the Bagnold Dune Field in Gale Crater to Interpret Eolian Sediment Sorting on the Martian Surface

Author

Rampe, E. B, Lapotre, M, Bristow, T. F, Arvidson, R. E, Morris, R. V, Achilles, C. N, Weitz, C, Blake, D. F, Ming, D. W, Morrison, S. M, Vaniman, D. T, Chipera, S. J, Downs, R. T, Edgett, K, Grotzinger, J. P, Hazen, R. M, Peretyazhko, T. S, Sutter, B, Tu, V, Yen, A. S, Horgan, B, Castle, N, Craig, P. I, S. Czarnecki, Marais, D. J. Des, Farmer, J, Gabriel, T, Gellert, R, Hardgrove, C, McAdam, A. C, Morookian, J. M, Sarrazin, P. C, and Treiman, A. H

Subjects
Lunar And Planetary Science And Exploration
Abstract

The Mars Science Laboratory Curiosity rover landed in Gale crater in August 2012 to characterize modern and ancient surface environments. Curiosity executed a two-phase campaign to study the morphology, activity, physical properties, and chemical and mineralogical composition of the Bagnold Dune Field, an active eolian dune field on the lower slopes of Aeolis Mons (Mount Sharp). Detectable aspects of dune sand mineralogy have been examined from orbit with the visible/short-wave infrared spectrometer CRISMand the thermal-infrared spectrometers THEMIS and TES. CRISM data demonstrate variations in plagioclase, pyroxene, and olivine abundances across the dune field. Curiosity analyzed sediments from two locations in the dune field to evaluate the causes of the mineralogical differences observed from orbit. The Gobabeb sample was collected from Namib Dune, a barchanoidal dune on the upwind margin of the dune field, and the Ogunquit Beach sample was collected from the Mount Desert Island sand patch located downwind from Namib. These samples were sieved to <150 μm and delivered to the CheMin X-ray diffraction instrument for quantitative mineralogical analysis. CRISM-derived mineralogy of the Namib Dune and Mount Desert Island and CheMin-derived mineralogy of the Gobabeb and Ogunquit Beach samples can be used in a value-added manner to interpret grain segregation at the bedform to dune-field scale and evaluate contributions from local sediment sources. Models of CRISM data demonstrate that Mount Desert Island is more enriched in olivine and less enriched in plagioclase than Namib dune, suggesting that fine-grained mafic sediments are preferentially mobilized downwind. Curiosity data indicate olivine also forms a coarse lag on the lee sides of barchanoidal dunes. Minor abundances of hematite, quartz, and anhydrite and small differences in the crystal chemistry of plagioclase and pyroxene derived from CheMin data suggest that sediments from the underlying lacustrine rocks also contribute to the Bagnold sands.

Published
2018

30. Textures of the Soils and Rocks at Gusev Crater from Spirit's Microscopic Imager

Author

Herkenhoff, K. E., Squyres, S. W., Arvidson, R., Bass, D. S., Bell, J. F., Bertelsen, P., Cabrol, N. A., Gaddis, L., Hayes, A. G., Hviid, S. F., Johnson, J. R., Kinch, K. M., Madsen, M. B., Maki, J. N., McLennan, S. M., McSween, H. Y., Rice, J. W., Sims, M., Smith, P. H., Soderblom, L. A., Spanovich, N., Sullivan, R., and Wang, A.

Published
2004

31. Geology and Stratigraphic Correlation of the Murray and Carolyn Shoemaker Formations Across the Glen Torridon Region, Gale Crater, Mars

Author

Fedo, C. M., primary, Bryk, A. B., additional, Edgar, L. A., additional, Bennett, K. A., additional, Fox, V. K., additional, Dietrich, W. E., additional, Banham, S. G., additional, Gupta, S., additional, Stack, K. M., additional, Williams, R. M. E., additional, Grotzinger, J. P., additional, Stein, N. T., additional, Rubin, D. M., additional, Caravaca, G., additional, Arvidson, R. E., additional, Hughes, M. N., additional, Fraeman, A. A., additional, Vasavada, A. R., additional, Schieber, J., additional, and Sutter, B., additional

Published
2022
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34. Ancient Aqueous Environments at Endeavour Crater, Mars

Author

Arvidson, R. E., Squyres, S. W., Bell, J. F., Catalano, J. G., Clark, B. C., Crumpler, L. S., de Souza, P. A., Fairén, A. G., Farrand, W. H., Fox, V. K., Gellert, R., Ghosh, A., Golombek, M. P., Grotzinger, J. P., Guinness, E. A., Herkenhoff, K. E., Jolliff, B. L., Knoll, A. H., Li, R., McLennan, S. M., Ming, D. W., Mittlefehldt, D. W., Moore, J. M., Morris, R. V., Murchie, S. L., Parker, T. J., Paulsen, G., Rice, J. W., Ruff, S. W., Smith, M. D., and Wolff, M. J.

Published
2014

35. In Situ Radiometric and Exposure Age Dating of the Martian Surface

Author

MSL Science Team, Farley, K. A., Malespin, C., Mahaffy, P., Grotzinger, J. P., Vasconcelos, P. M., Milliken, R. E., Malin, M., Edgett, K. S., Pavlov, A. A., Hurowitz, J. A., Grant, J. A., Miller, H. B., Arvidson, R., Beegle, L., Calef, F., Conrad, P. G., Dietrich, W. E., Eigenbrode, J., Gellert, R., Gupta, S., Hamilton, V., Hassler, D. M., Lewis, K. W., McLennan, S. M., Ming, D., Navarro-González, R., Schwenzer, S. P., Steele, A., Stolper, E. M., Sumner, D. Y., Vaniman, D., Vasavada, A., Williford, K., and Wimmer-Schweingruber, R. F.

Published
2014

36. A Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, Mars

Author

MSL Science Team, Grotzinger, J. P., Sumner, D. Y., Kah, L. C., Stack, K., Gupta, S., Edgar, L., Rubin, D., Lewis, K., Schieber, J., Mangold, N., Milliken, R., Conrad, P. G., DesMarais, D., Farmer, J., Siebach, K., Calef, F., Hurowitz, J., McLennan, S. M., Ming, D., Vaniman, D., Crisp, J., Vasavada, A., Edgett, K. S., Malin, M., Blake, D., Gellert, R., Mahaffy, P., Wiens, R. C., Maurice, S., Grant, J. A., Wilson, S., Anderson, R. C., Beegle, L., Arvidson, R., Hallet, B., Sletten, R. S., Rice, M., Bell, J., Griffes, J., Ehlmann, B., Anderson, R. B., Bristow, T. F., Dietrich, W. E., Dromart, G., Eigenbrode, J., Fraeman, A., Hardgrove, C., Herkenhoff, K., Jandura, L., Kocurek, G., Lee, S., Leshin, L. A., Leveille, R., Limonadi, D., Maki, J., McCloskey, S., Meyer, M., Minitti, M., Newsom, H., Oehler, D., Okon, A., Palucis, M., Parker, T., Rowland, S., Schmidt, M., Squyres, S., Steele, A., Stolper, E., Summons, R., Treiman, A., Williams, R., and Yingst, A.

Published
2014

38. 2001 Mars Odyssey Mission Summary

Author

Saunders, R. S., Arvidson, R. E., Badhwar, G. D., Boynton, W. V., Christensen, P. R., Cucinotta, F. A., Feldman, W. C., Gibbs, R. G., Kloss, C., Jr., Landano, M. R., Mase, R. A., Mcsmith, G. W., Meyer, M. A., Mitrofanov, I. G., Pace, G. D., Plaut, J. J., Sidney, W. P., Spencer, D. A., Thompson, T. W., Zeitlin, C. J., and Russell, Christopher T., editor

Published
2004
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39. Ancient Impact and Aqueous Processes at Endeavour Crater, Mars

Author

Squyres, S. W., Arvidson, R. E., Bell, J. F., Calef, F., Clark, B. C., Cohen, B. A., Crumpler, L. A., de Souza, P. A., Farrand, W. H., Gellert, R., Grant, J., Herkenhoff, K. E., Hurowitz, J. A., Johnson, J. R., Jolliff, B. L., Knoll, A. H., Li, R., McLennan, S. M., Ming, D. W., Mittlefehldt, D. W., Parker, T. J., Paulsen, G., Rice, M. S., Ruff, S. W., Schröder, C., Yen, A. S., and Zacny, K.

Published
2012
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40. Pancam Multispectral and APXS Chemical Examination of Rocks and Soils in Marathon Valley and Points South Along the Rim of Endeavour Crater

Author

Farrand, W. H, Johnson, J. R, Bell, J. F., III, Mittlefehldt, D. W, Gellert, R, VanBommel, S, Arvidson, R. E, and Schroder, C

Subjects
Lunar And Planetary Science And Exploration
Abstract

The Mars Exploration Rover Opportunity has concluded its exploration of Marathon Valley, a 100-meter-wide valley in the western rim of the 22-kilometer-diameter Endeavour crater. Orbital observations from CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) indicated the presence of Fe smectites in Marathon Valley. Since leaving the valley, Opportunity has been traversing along the inner rim of the crater, and currently towards the outer rim. This presentation describes the Pancam 430 to 1009 nanometer (VNIR - Visible and Near Infared) multispectral reflectance and APXS (Alpha Particle X-ray Spectrometer) chemical compositions of rock and soil units observed during the latter portions of the Marathon Valley campaign on the Knudson Ridge area and observations of those materi-als along the traverse to the south. Full Pancam spectral coverage of rock targets consists of 13 filter (13f) data collections with 11 spectrally unique channels with data processing. Data were examined using spectral parameters, decorrelation stretch composites, and spectral mixture analysis. Note that color terms used here refer to colors in various false-color renditions, not true colors. The APXS determines major and select trace element compositions of targets.

Published
2017

41. Rim Structure, Stratigraphy, and Aqueous Alteration Exposures Along Opportunity Rover's Traverse of the Noachian Endeavour Crater

Author

Crumpler, L.S, Arvidson, R. E, Golombek, M, Grant, J. A, Jolliff, B. L, and Mittlefehldt, D. W

Subjects
Lunar And Planetary Science And Exploration
Abstract

The Mars Exploration Rover Opportunity has traversed 10.2 kilometers along segments of the west rim of the 22-kilometer-diameter Noachian Endeavour impact crater as of sol 4608 (01/09/17). The stratigraphy, attitude of units, lithology, and degradation state of bedrock outcrops exposed on the crater rim have been examined in situ and placed in geologic context. Structures within the rim and differences in physical properties of the identified lithologies have played important roles in localizing outcrops bearing evidence of aqueous alteration.

Published
2017

42. Acid-Sulfate Alteration at Gusev Crater and Across Mars: High-SiO2 Residues and Ferric Sulfate Precipitates

Author

Morris, R. V, Catalano, J. G, Klingelhoefer, G, Schroeder, C, Gellert, R, Clark, B. C, Ming, D. W, Yen, A. S, Arvidson, R. E, Cohen, B. A, Fleischer, I, McCoy, T. J, Mittlefehldt, D. W, and Squyres, S. W

Subjects
Lunar And Planetary Science And Exploration
Abstract

The Mars Exploration Rover Spirit ended its mission in Gusev crater on sol 2210 after it had become stuck in a deposit of fined-grained and sulfate rich soil with dust covered solar panels unfavorably pointed toward the sun. Final analysis of remaining data from Spirit's Moessbauer spectrometer (Fe redox and mineralogy) for sols 1529 through 2071 is now complete. We focus here on chemical (APXS) and MB data for targets having high-SiO2 or high-SO3 and process link the targets through mixing and geochemical modelling to an acid-sulfate system centered at Home Plate, which is considered to be a hydrovolcanic complex.

Published
2017

43. H₂O at the Phoenix Landing Site

Author

Smith, P. H., Tamppari, L. K., Arvidson, R. E., Bass, D., Blaney, D., Boynton, W. V., Carswell, A., Catling, D. C., Clark, B. C., Duck, T., DeJong, E., Fisher, D., Goetz, W., Gunnlaugsson, H. P., Hecht, M. H., Hipkin, V., Hoffman, J., Hviid, S. F., Keller, H. U., Kounaves, S. P., Lange, C. F., Lemmon, M. T., Madsen, M. B., Markiewicz, W. J., Marshall, J., McKay, C. P., Mellon, M. T., Ming, D. W., Morris, R. V., Pike, W. T., Renno, N., Staufer, U., Stoker, C., Taylor, P., Whiteway, J. A., and Zent, A. P.

Published
2009
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45. Exploration of Victoria Crater by the Mars Rover Opportunity

Author

Squyres, S. W., Knoll, A. H., Arvidson, R. E., Ashley, J. W., Bell, J. F., Calvin, W. M., Christensen, P. R., Clark, B. C., Cohen, B. A., de Souza, P. A., Edgar, L., Farrand, W. H., Fleischer, I., Gellert, R., Golombek, M. P., Grant, J., Grotzinger, J., Hayes, A., Herkenhoff, K. E., Johnson, J. R., Jolliff, B., Klingelhöfer, G., Knudson, A., Li, R., McCoy, T. J., McLennan, S. M., Ming, D. W., Mittlefehldt, D. W., Morris, R. V., Rice, J. W., Schröder, C., Sullivan, R. J., Yen, A., and Yingst, R. A.

Published
2009
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46. Detection of Silica-Rich Deposits on Mars

Author

Squyres, S. W., Arvidson, R. E., Ruff, S., Gellert, R., Morris, R. V., Ming, D. W., Crumpler, L., Farmer, J. D., Des Marais, D. J., Yen, A., McLennan, S. M., Calvin, W., Bell, J. F., Clark, B. C., Wang, A., McCoy, T. J., Schmidt, M. E., and de Souza, P. A.

Published
2008
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49. Igneous and Sedimentary Compositions from Four Landing Sites on Mars from the Alpha Particle X-Ray Spectrometer (APXS)

Author

Gellert, R, Arvidson, R. E, Clark, B. C, Ming, D. W, Mittlefehldt, D. W, Morris, R. W, Squyres, S. W, VanBommel, S, and Yen, A. S

Subjects
Lunar And Planetary Science And Exploration
Abstract

The APXS - supported and promoted strongly by Heinrich Waenke - on all four Mars Rovers has returned compositional data from about 1000 rocks and soil targets along the combined traverses of over 60 kilometers. Providing precise and accurate bulk chemistry with typically 16 quantified elements, the APXS is a powerful and versatile tool that when combined with the ability to traverse to key rocks and soils has provided critical information needed to understand the geologic evolution of Mars. APXS data allow comparisons among landing sites, provide ground truth for orbiters and connections back to SNC meteorites. The soils and dust are basaltic in character and represent the average Mars composition similar to Adirondack basalts from Gusev crater but with unambiguous elevated and correlated S, Cl and Zn contents. At all four landing sites the APXS found several rocks with a felsic composition. The similarity is best assessed in a logarithmic ratio plot of rock normalized to the average soil composition (Fig.1). High alkaline, Al, and low Mg, Fe, low S, Cl and Ni, Zn as well as an Fe/Mn ratio of approximately 50 indicate a likely unaltered and igneous origin. Sediments, e.g. the Burns formation, with approximately 25 wt% SO3 at Meridiani Planum have been documented over 10s of kilometers (Fig. 2). This formation is compositionally homogeneous, but showing the removal of MgSO4 and a threefold increase in Cl downhill in 2 craters. The degraded rim of the Noachian crater Endeavour resembles average Mars crust, with local Ca, Mg and Fe sulfate alteration and elevated Mn, some felsic rocks, and high Al, Si and low Fe rocks, possibly indicating clays. Unusual soils at Gusev crater in the area surrounding Home Plate include some very rich in ferric sulfate salts (up to 35 wt% SO3) and some with 90% wt% SiO2, possibly indicating fumerolic activities. Rocks in the Columbia Hills show significant signs of alteration including elevated S, Cl and Br in the abraded interior. At Gale Crater, mudstones with approximately 20% clay, less than 1% SO3 and overall average Mars composition indicate a former habitable environment with low acidity. A remarkable diversity of compositions was found during Curiosity's traverses, which likely stems from material influx from the northern Gale rim. At Pahrump, the base of Mount Sharp, a homogeneous mudstone with lower Mg and Ca was encountered. The composition of this Murray unit can be traced over several kilometers with smooth trends of higher Fe/Mn and lower soluble trace elements Ni and Zn at higher elevation. The likely aeolian Stimson formation with average Mars crustal composition intersects in several places in sharp contact with the Murray formation. Both units show local alteration halos with highly elevated SiO2 of up to 75%, usually correlated with increase in Ti and often P.

Published
2016

50. Opportunity, Geologic and Structural Context of Aqueous Alteration in Noachian Outcrops, Marathon Valley and Rim and Endeavour Crater

Author

Crumpler, L. S, Arvidson, R. E, Mittlefehldt, D. W, Jolliff, B. L, Farrand, W. H, Fox, V, and Golombek, M. P

Subjects
Lunar And Planetary Science And Exploration
Abstract

In its 12th year of exploration and 1600 sols since arrival at the rim of the 22 km-diameter Noachian Endeavour impact crater, Mars Exploration Rover Opportunity traversed from the summit of the western rim segment "Cape Tribulation" to "Marathon Valley", a shallow trough dissecting the rim and the site of strong orbital detection of smectites. In situ analysis of the exposures within Marathon Valley is establishing some of the geologic and geochemical controls on the aqueous alteration responsible for smectite detection known to occur in crater rims throughout Noachian terrains of Mars.

Published
2016

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