Search Results - "ZUBER, M. T"

A partially differentiated interior for (1) Ceres deduced from its gravity field and shape by Park, R. S., Konopliv, A. S., Bills, B. G., Rambaux, N., Castillo-Rogez, J. C., Raymond, C. A., Vaughan, A. T., Ermakov, A. I., Zuber, M. T., Fu, R. R., Toplis, M. J., Russell, C. T., Nathues, A., Preusker, F.

“…Gravity and shape measurements for Ceres obtained from the Dawn spacecraft mission show that it is in hydrostatic equilibrium with its inferred normalized mean…”
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Dawn arrives at Ceres: Exploration of a small, volatile-rich world by Russell, C. T., Raymond, C. A., Ammannito, E., Buczkowski, D. L., De Santis, M. C., Hiesinger, H., Jaumann, R., Konopliv, A. S., McSween, H. Y., Nathues, A., Park, R. S., Pieters, C. M., Prettyman, T. H., McCord, T. B., McFadden, L. A., Mottola, S., Zuber, M. T., Joy, S. P., Polanskey, C., Rayman, M. D., Castillo-Rogez, J. C., Chi, P. J., Combe, J. P., Ermakov, A., Fu, R. R., Hoffmann, M., Jia, Y. D., King, S. D., Lawrence, D. J., Li, J.-Y., Marchi, S., Preusker, F., Roatsch, T., Ruesch, O., Schenk, P., Villarreal, M. N., Yamashita, N.

“…On 6 March 2015, Dawn arrived at Ceres to find a dark, desiccated surface punctuated by small, bright areas. Parts of Ceres' surface are heavily cratered, but…”
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Dawn at Vesta: Testing the Protoplanetary Paradigm by Russell, C. T., Raymond, C. A., Coradini, A., McSween, H. Y., Zuber, M. T., Nathues, A., De Sanctis, M. C., Jaumann, R., Konopliv, A. S., Preusker, F., Asmar, S. W., Park, R. S., Gaskell, R., Keller, H. U., Mottola, S., Roatsch, T., Scully, J. E. C., Smith, D. E., Tricarico, P., Toplis, M. J., Christensen, U. R., Feldman, W. C., Lawrence, D. J., McCoy, T. J., Prettyman, T. H., Reedy, R. C., Sykes, M. E., Titus, T. N.

“…The Dawn spacecraft targeted 4 Vesta, believed to be a remnant intact protoplanet from the earliest epoch of solar system formation, based on analyses of…”
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Large impact cratering during lunar magma ocean solidification by Miljković, K., Wieczorek, M. A., Laneuville, M., Nemchin, A., Bland, P. A., Zuber, M. T.

“…The lunar cratering record is used to constrain the bombardment history of both the Earth and the Moon. However, it is suggested from different perspectives,…”
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The South Pole‐Aitken Basin: Constraints on Impact Excavation, Melt, and Ejecta by Citron, R. I., Smith, D. E., Stewart, S. T., Hood, L. L., Zuber, M. T.

“…The formation and evolution of the South Pole‐Aitken (SPA) basin is critical to relating large impact basin formation and modification to lunar geophysical…”
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Illumination conditions of the lunar polar regions using LOLA topography by Mazarico, E., Neumann, G.A., Smith, D.E., Zuber, M.T., Torrence, M.H.

“…► We model the illumination conditions in the polar regions with LOLA topography. ► Long simulations (several decades) are used to obtain average illumination…”
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Vesta's Shape and Morphology by Jaumann, R., Williams, D. A., Buczkowski, D. L., Yingst, R. A., Preusker, F., Hiesinger, H., Schmedemann, N., Kneissl, T., Vincent, J. B., Blewett, D. T., Buratti, B. J., Carsenty, U., Denevi, B. W., De Sanctis, M. C., Garry, W. B., Keller, H. U., Kersten, E., Krohn, K., Li, J.-Y., Marchi, S., Matz, K. D., McCord, T. B., McSween, H. Y., Mest, S. C., Mittlefehldt, D. W., Mottola, S., Nathues, A., Neukum, G., O'Brien, D. P., Pieters, C. M., Prettyman, T. H., Raymond, C. A., Roatsch, T., Russell, C. T., Schenk, P., Schmidt, B. E., Scholten, F., Stephan, K., Sykes, M. V., Tricarico, P., Wagner, R., Zuber, M. T., Sierks, H.

“…Vesta's surface is characterized by abundant impact craters, some with preserved ejecta blankets, large troughs extending around the equatorial region,…”
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The global albedo of the Moon at 1064 nm from LOLA by Lucey, P. G., Neumann, G. A., Riner, M. A., Mazarico, E., Smith, D. E., Zuber, M. T., Paige, D. A., Bussey, D. B., Cahill, J. T., McGovern, A., Isaacson, P., Corley, L. M., Torrence, M. H., Melosh, H. J., Head, J. W., Song, E.

“…The Lunar Orbiter Laser Altimeter (LOLA) measures the backscattered energy of the returning altimetric laser pulse at its wavelength of 1064 nm, and these data…”
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Hydrogen Mapping of the Lunar South Pole Using the LRO Neutron Detector Experiment LEND by Mitrofanov, I.G, Sanin, A.B, Boynton, W.V, Chin, G, Garvin, J.B, Golovin, D, Evans, L.G, Harshman, K, Kozyrev, A.S, Litvak, M.L, Malakhov, A, Mazarico, E, McClanahan, T, Milikh, G, Mokrousov, M, Nandikotkur, G, Neumann, G.A, Nuzhdin, I, Sagdeev, R, Shevchenko, V, Shvetsov, V, Smith, D.E, Starr, R, Tretyakov, V.I, Trombka, J, Usikov, D, Varenikov, A, Vostrukhin, A, Zuber, M.T

“…Hydrogen has been inferred to occur in enhanced concentrations within permanently shadowed regions and, hence, the coldest areas of the lunar poles. The Lunar…”
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Constraints on Ceres' Internal Structure and Evolution From Its Shape and Gravity Measured by the Dawn Spacecraft by Ermakov, A. I., Fu, R. R., Castillo‐Rogez, J. C., Raymond, C. A., Park, R. S., Preusker, F., Russell, C. T., Smith, D. E., Zuber, M. T.

“…Ceres is the largest body in the asteroid belt with a radius of approximately 470 km. In part due to its large mass, Ceres more closely approaches hydrostatic…”
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Thermal perturbations caused by large impacts and consequences for mantle convection by Watters, W. A., Zuber, M. T., Hager, B. H.

“…We examine the effects of thermal perturbations on a convecting layer of incompressible fluid with uniform viscosity in the limit of infinite Prandtl number,…”
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Orbit determination of the Lunar Reconnaissance Orbiter by Mazarico, Erwan, Rowlands, D. D., Neumann, G. A., Smith, D. E., Torrence, M. H., Lemoine, F. G., Zuber, M. T.

“…We present the results on precision orbit determination from the radio science investigation of the Lunar Reconnaissance Orbiter (LRO) spacecraft. We describe…”
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Crustal structure of Mars from gravity and topography by Neumann, G. A., Zuber, M. T., Wieczorek, M. A., McGovern, P. J., Lemoine, F. G., Smith, D. E.

“…Mars Orbiter Laser Altimeter (MOLA) topography and gravity models from 5 years of Mars Global Surveyor (MGS) spacecraft tracking provide a window into the…”
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Observations, Meteorites, and Models: A Preflight Assessment of the Composition and Formation of (16) Psyche by Elkins‐Tanton, L. T., Asphaug, E., Bell, J. F., Bercovici, H., Bills, B., Binzel, R., Bottke, W. F., Dibb, S., Lawrence, D. J., Marchi, S., McCoy, T. J., Oran, R., Park, R. S., Peplowski, P. N., Polanskey, C. A., Prettyman, T. H., Russell, C. T., Schaefer, L., Weiss, B. P., Wieczorek, M. A., Williams, D. A., Zuber, M. T.

“…Some years ago, the consensus was that asteroid (16) Psyche was almost entirely metal. New data on density, radar properties, and spectral signatures indicate…”
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Tides on Europa, and the thickness of Europa's icy shell by Wahr, J. M., Zuber, M. T., Smith, D. E., Lunine, J. I.

“…It has been shown previously that measurements of tides on Jupiter's moon Europa can be used to determine whether there is a liquid ocean beneath this moon's…”
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The crust and mantle of Mars by Zuber, Maria T

“…Clues to the history of Mars are recorded in the chemistry and structure of the planet's crust and mantle. The mantle is the rocky, interior region of the…”
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Early evolution of Mars with mantle compositional stratification or hydrothermal crustal cooling by Parmentier, E. M., Zuber, M. T.

“…Analysis of Martian gravity and topography implies that crustal thickness variations created in the earliest evolution of planet have persisted to the present…”
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An improved solution of the gravity field of Mars (GMM-2B) from Mars Global Surveyor by Lemoine, F. G., Smith, D. E., Rowlands, D. D., Zuber, M. T., Neumann, G. A., Chinn, D. S., Pavlis, D. E.

“…A spherical harmonic solution of the Mars gravity field to degree and order 80, Goddard Mars Model 2B (GMM‐2B), has been developed using X band tracking data…”
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A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera by Barker, M K, Mazarico, E, Neumann, G A, Zuber, M T, Haruyama, J, Smith, DE

“…We present an improved lunar digital elevation model (DEM) covering latitudes within plus or minus 60 degree , at a horizontal resolution of 512pixels per…”
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Subsurface Morphology and Scaling of Lunar Impact Basins by Miljkovic, K., Collins, G. S., Wieczorek, M. A., Johnson, B. C., Soderblom, J. M., Neumann, G. A., Zuber, M. T.

“…Impact bombardment during the first billion years after the formation of the Moon produced at least several tens of basins. The Gravity Recovery and Interior…”
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