Results 11 to 20 of about 109,917 (327)
Seismic detection of the martian core [PDF]
Science, 2021 Single seismometer structure Because of the lack of direct seismic observations, the interior structure of Mars has been a mystery. Khan et al. , Knapmeyer-Endrun et al. , and Stähler et al.Attilio Rivoldini, Constantinos Charalambous, Martin Schimmel, Matthieu Plasman, Suzanne E. Smrekar, Quancheng Huang, Mark P. Panning, Eric Beucler, Raphaël F. Garcia, John Clinton, Vedran Lekic, Daniele Antonangeli, Clément Perrin, Domenico Giardini, W. Bruce Banerdt, A. Cecilia Duran, Eléonore Stutzmann, Savas Ceylan, Anna Horleston, Martin Knapmeyer, Henri Samuel, Ana-Catalina Plesa, Nicholas Schmerr, Paul M. Davis, Zongbo Xu, Jessica C. E. Irving, Angela G. Marusiak, Amir Khan, Amir Khan, W. Thomas Pike, Mélanie Drilleau, Nikolaj Dahmen, Simon Stähler, Taichi Kawamura, Do-Yeon Kim, Ross Maguire, David Sollberger, Martin van Driel, Philippe Lognonné, Cedric Schmelzbach, Tamara Gudkova, Géraldine Zenhäusern +41 moreopenaire +10 more sourcesDirect Formation of Structural Components Using a Martian Soil Simulant. [PDF]
Scientific Reports, 2017 Martian habitats are ideally constructed using only locally available soils; extant attempts to process structural materials on Mars, however, generally require additives or calcination.Chen, Tzehan, Chow, Brian J, Qiao, Yu, Zhong, Ying +3 morecore +2 more sourcesField Measurements of Terrestrial and Martian Dust Devils [PDF]
, 2016 Surface-based measurements of terrestrial and martian dust devils/convective vortices provided from mobile and stationary platforms are discussed. Imaging of terrestrial dust devils has quantified their rotational and vertical wind speeds, translation ...A. Powell, A. Seiff, A.-M. Harri, A.M.C. Oke, A.V. Pathare, B. Jackson, B. Lenoir, C. Bettanini, C. Holstein-Rathlou, C.G. Grant, C.L. Wilson, D. Banfield, D. Reiss, D.A. Gillette, D.A. Gillette, D.E. Fitzjarrald, D.J. Lacks, D.M. Tratt, D.S. Schmidt, D.T. Tyler, D.T. Tyler, E. Leonard-Pugh, E.W.B. Gill, F. Esposito, F. Ferri, Francesca Esposito, G.A. Landis, G.D. Freier, G.D. Hess, G.G. Sorrells, G.G. Sorrells, Gregoire Deprez, H.B. Bluestein, H.P. Gunnlaugsson, Henrik Kahanpää, I.I. Inculet, J. Grotzinger, J. Gómez-Elvira, J. Gómez-Elvira, J. Hallett, J. Ito, J. Latham, J. Latham, J. Lowell, J. Murphy, J. Whiteway, J.-J. Berthelier, J.A. Rodriguez-Manfredi, J.A. Ryan, J.A. Ryan, J.B. Pollack, J.C. Kaimal, J.E. Moores, J.E. Tillman, J.F. Kok, J.F. Kok, J.J. Carroll, J.P. Mason, J.P. Mason, J.P. Merrison, J.P. Williams, J.T. Schofield, J.T. Snow, Jim Murphy, K. Steakley, K.M. Forward, Kathryn Steakley, L. Fenton, L.D.V. Neakrase, L.K. Fenton, L.M. Zelenyi, Lynn Neakrase, M-P. Zorzano, M. Balme, M. Balme, M. Domínguez, M. Golombek, M. Kahre, M. Klose, M.C. Towner, M.D. Ellehoj, M.D. Smith, M.R. Balme, M.S. Howe, M.T. Lemmon, M.T. Lemmon, M.V. Kurgansky, M.V. Kurgansky, M.V. Kurgansky, Manish Patel, Mark Lemmon, Matt Balme, N. Duff, N.O. Renno, N.O. Renno, N.O. Renno, N.R. Williams, Naomi Murdoch, P. Lognonné, P. Lognonné, P. Sinclair, P. Sinclair, P.A. Taylor, P.A. Taylor, P.C. Sinclair, P.H. Smith, P.H. Smith, P.H. Smith, Patrick Whelley, R. Davy, R. Greeley, R. Greeley, R. Lorenz, R. Lorenz, R. Lorenz, R. Sullivan, R.A. Bagnold, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.D. Lorenz, R.G. Harrison, R.G. Horn, R.I. Lambeth, R.L. Ives, R.L. Schwiesow, R.M. Haberle, Ralph Lorenz, S. Maurice, S. Metzger, S. Rafkin, S.D. Fuerstenau, S.J. Desch, S.L. Hess, S.M. Metzger, S.W. Squyres, T.J. Ringrose, T.J. Ringrose, T.L. Jackson, W.D. Crozier, W.D. Flower, W.R. Harper, Y. Shao, Y.P. Shao +153 morecore +6 more sourcesGeologic history of Martian regolith breccia Northwest Africa 7034: Evidence for hydrothermal activity and lithologic diversity in the Martian crust [PDF]
, 2016 The timing and mode of deposition for Martian regolith breccia Northwest Africa (NWA) 7034 were determined by combining petrography, shape analysis, and thermochronology.Adcock, Agee, Andersen, Aström, Bacon, Bagnold, Beck, Bellucci, Bibring, Bibring, Bish, Blake, Blott, Borg, Bradley, Brandon, Cannon, Carr, Cartwright, Chipera, Christensen, Claoué-Long, Collinet, Cooney, Dahl, Day, Domokos, Domokos, Downs, Dreibus, Dyar, Ehlmann, Ehlmann, Farley, Filiberto, Filiberto, Filiberto, Filiberto, Foland, Friedman, Gattacceca, Gellert, Gellert, Goderis, Golden, Greeley, Greenwood, Grimes, Grotzinger, Hartmann, Haskin, Heaman, Herd, Hiess, Hiess, Humayun, Hurowitz, Jerolmack, Jutzeler, Kaminski, Kekäläinen, Keller, Klingelhofer, Lee, Leroux, Liu, Lorand, Ludwig, Ludwig, Malin, Manga, Mattinson, McCanta, McCubbin, McCubbin, McCubbin, McCubbin, McCubbin, McEwen, McKay, McLennan, McLennan, McLennan, McLennan, McSween, McSween, McSween, McSween, McSween, McSween, Medard, Meldrum, Mezger, Monders, Monkawa, Morris, Morris, Moser, Murchie, Musselwhite, Muttik, Nekvasil, Nekvasil, Nemchin, Nyquist, Nyquist, Papike, Papike, Poulet, Santos, Sarbadhikari, Sautter, Sautter, Schmidt, Schmidt, Schoene, Schon, Sha, Sharp, Shearer, Shearer, Squyres, Squyres, Squyres, Stacey, Steele, Stolper, Szabó, Tartèse, Taylor, Taylor, Taylor, Terada, Terada, Thomson, Tosca, Treiman, Tuff, Udry, Usui, Vaniman, Vaniman, Wadhwa, Walker, Wang, Wang, Wiedenbeck, Wiedenbeck, Williams, Wingate, Wittmann, Yen +151 morecore +3 more sourcesA review of volatiles in the Martian interior [PDF]
, 2016 Multiple observations from missions to Mars have revealed compelling evidence for a volatile-rich Martian crust. A leading theory contends that eruption of basaltic magmas was the ultimate mechanism of transfer of volatiles from the mantle toward the ...Baratoux, David, Beaty, David, Breuer, Doris, Farcy, Benjamin J., Filiberto, Justin, Grott, Matthias, Jones, John H., Kiefer, Walter S., Mane, Prajkta, McCubbin, Francis M., Schwenzer, Susanne P. +10 morecore +2 more sourcesThickness and structure of the martian crust from InSight seismic data
Science, 2021 Single seismometer structure Because of the lack of direct seismic observations, the interior structure of Mars has been a mystery. Khan et al., Knapmeyer-Endrun et al., and Stähler et al.B. Knapmeyer‐Endrun, M. Panning, F. Bissig, R. Joshi, Amir Khan, Doyeon Kim, V. Lekić, B. Tauzin, S. Tharimena, M. Plasman, N. Compaire, R. Garcia, L. Margerin, M. Schimmel, É. Stutzmann, N. Schmerr, E. Bozdağ, A. Plesa, M. Wieczorek, A. Broquet, D. Antonangeli, S. McLennan, H. Samuel, C. Michaut, L. Pan, S. Smrekar, C. Johnson, N. Brinkman, A. Mittelholz, A. Rivoldini, P. Davis, P. Lognonné, B. Pinot, John‐Robert Scholz, S. Stähler, M. Knapmeyer, M. van Driel, D. Giardini, W. Banerdt +38 moresemanticscholar +1 more sourceMartian moons exploration MMX: sample return mission to Phobos elucidating formation processes of habitable planets
Earth, Planets and Space, 2021 Martian moons exploration, MMX, is the new sample return mission planned by the Japan Aerospace Exploration Agency (JAXA) targeting the two Martian moons with the scheduled launch in 2024 and return to the Earth in 2029.K. Kuramoto, Y. Kawakatsu, M. Fujimoto, A. Araya, M. Barucci, H. Genda, N. Hirata, H. Ikeda, T. Imamura, J. Helbert, S. Kameda, Masanori Kobayashi, H. Kusano, D. Lawrence, Koji Matsumoto, P. Michel, H. Miyamoto, T. Morota, H. Nakagawa, Tomoki Nakamura, K. Ogawa, H. Otake, M. Ozaki, S. Russell, S. Sasaki, H. Sawada, H. Senshu, S. Tachibana, N. Terada, S. Ulamec, T. Usui, K. Wada, Sei‐ichiro Watanabe, S. Yokota +33 moresemanticscholar +1 more sourceProperties and models of the Martian bow shock
地球与行星物理论评, 2021 Mars does not have a global magnetic field of the internal origin, thus, the solar wind plasma can interact directly with the upper atmosphere and the ionosphere and be shocked with the mass-loading and magnetic pileup processes.Yifan Li, Jiding Wen, Yuan Pan, Haibo Lin, Jianpeng Guo +4 moredoaj +1 more sourceIs the Martian crust also the Martian elastic lithosphere? [PDF]
Journal of Geophysical Research: Planets, 2002 Correlations between topography, gravity, and areoid on Mars are used to constrain the crustal and lithospheric thicknesses on the planet. Assuming that the Hellas basin is in isostatic equilibrium with Airy compensation, point correlations between areoid anomalies and topography are used to obtain the mean crustal density and the crustal thickness. We Turcotte, D L, Shcherbakov, R, Malamud, B D, Kucinskas, A B +3 moreopenaire +2 more sources
