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Moore JM, McKinnon WB, Spencer JR, Howard AD, Schenk PM, Beyer RA, Nimmo F, Singer KN, Umurhan OM, White OL, Stern SA, Ennico K, Olkin CB, Weaver HA, Young LA, Binzel RP, Buie MW, Buratti BJ, Cheng AF, Cruikshank DP, Grundy WM, Linscott IR, Reitsema HJ, Reuter DC, Showalter MR, Bray VJ, Chavez CL, Howett CJA, Lauer TR, Lisse CM, Parker AH, Porter SB, Robbins SJ, Runyon K, Stryk T, Throop HB, Tsang CCC, Verbiscer AJ, Zangari AM, Chaikin AL, Wilhelms DE. The geology of Pluto and Charon through the eyes of New Horizons. Science 2016; 351:1284-93. [PMID: 26989245 DOI: 10.1126/science.aad7055] [Citation(s) in RCA: 40] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
NASA's New Horizons spacecraft has revealed the complex geology of Pluto and Charon. Pluto's encounter hemisphere shows ongoing surface geological activity centered on a vast basin containing a thick layer of volatile ices that appears to be involved in convection and advection, with a crater retention age no greater than ~10 million years. Surrounding terrains show active glacial flow, apparent transport and rotation of large buoyant water-ice crustal blocks, and pitting, the latter likely caused by sublimation erosion and/or collapse. More enigmatic features include tall mounds with central depressions that are conceivably cryovolcanic and ridges with complex bladed textures. Pluto also has ancient cratered terrains up to ~4 billion years old that are extensionally faulted and extensively mantled and perhaps eroded by glacial or other processes. Charon does not appear to be currently active, but experienced major extensional tectonism and resurfacing (probably cryovolcanic) nearly 4 billion years ago. Impact crater populations on Pluto and Charon are not consistent with the steepest impactor size-frequency distributions proposed for the Kuiper belt.
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Affiliation(s)
- Jeffrey M Moore
- National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA.
| | - William B McKinnon
- Department of Earth and Planetary Sciences, Washington University in St. Louis, St. Louis, MO 63130, USA
| | | | - Alan D Howard
- Department of Environmental Sciences, University of Virginia, Charlottesville, VA 22904, USA
| | - Paul M Schenk
- Lunar and Planetary Institute, Houston, TX 77058, USA
| | - Ross A Beyer
- The SETI Institute, Mountain View, CA 94043, USA. National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA
| | | | | | - Orkan M Umurhan
- National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA
| | - Oliver L White
- National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA
| | - S Alan Stern
- Southwest Research Institute, Boulder, CO 80302, USA
| | - Kimberly Ennico
- National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA
| | - Cathy B Olkin
- Southwest Research Institute, Boulder, CO 80302, USA
| | - Harold A Weaver
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | | | | | - Marc W Buie
- Southwest Research Institute, Boulder, CO 80302, USA
| | | | - Andrew F Cheng
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | - Dale P Cruikshank
- National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA
| | | | | | | | | | | | | | - Carrie L Chavez
- The SETI Institute, Mountain View, CA 94043, USA. National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA
| | | | - Tod R Lauer
- National Optical Astronomy Observatory, Tucson, AZ 85719, USA
| | - Carey M Lisse
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | | | - S B Porter
- Southwest Research Institute, Boulder, CO 80302, USA
| | | | - Kirby Runyon
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | - Ted Stryk
- Roane State Community College, Oak Ridge, TN 37830, USA
| | | | | | - Anne J Verbiscer
- Department of Astronomy, University of Virginia, Charlottesville, VA 22904, USA
| | | | | | - Don E Wilhelms
- U.S. Geological Survey, Retired, Menlo Park, CA 94025, USA
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Claudin P, Jarry H, Vignoles G, Plapp M, Andreotti B. Physical processes causing the formation of penitentes. PHYSICAL REVIEW. E, STATISTICAL, NONLINEAR, AND SOFT MATTER PHYSICS 2015; 92:033015. [PMID: 26465564 DOI: 10.1103/physreve.92.033015] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/01/2015] [Indexed: 05/05/2023]
Abstract
Snow penitentes form in sublimation conditions by differential ablation. Here we investigate the physical processes at the initial stage of penitente growth and perform the linear stability analysis of a flat surface submitted to the solar heat flux. We show that these patterns do not simply result from the self-illumination of the surface-a scale-free process-but are primarily controlled by vapor diffusion and heat conduction. The wavelength at which snow penitentes emerge is derived and discussed. We found that it is controlled by aerodynamic mixing of vapor above the ice surface.
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Affiliation(s)
- P Claudin
- Laboratoire de Physique et Mécanique des Milieux Hétérogènes, PMMH UMR 7636 ESPCI, CNRS, University Paris Diderot, University Pierre et Marie Curie, 10 rue Vauquelin, 75005, Paris, France
| | - H Jarry
- Laboratoire de Physique et Mécanique des Milieux Hétérogènes, PMMH UMR 7636 ESPCI, CNRS, University Paris Diderot, University Pierre et Marie Curie, 10 rue Vauquelin, 75005, Paris, France
| | - G Vignoles
- Laboratoire des Composites ThermoStructuraux, LCTS UMR 5801 CNRS, UB1, CEA-Safran, 3 allée La Boetie, 33600 Pessac, France
| | - M Plapp
- Condensed Matter Physics, Ecole Polytechnique, CNRS, 91128 Palaiseau, France
| | - B Andreotti
- Laboratoire de Physique et Mécanique des Milieux Hétérogènes, PMMH UMR 7636 ESPCI, CNRS, University Paris Diderot, University Pierre et Marie Curie, 10 rue Vauquelin, 75005, Paris, France
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Muñoz-García J, Gago R, Cuerno R, Sánchez-García JA, Redondo-Cubero A, Castro M, Vázquez L. Independence of interrupted coarsening on initial system order: ion-beam nanopatterning of amorphous versus crystalline silicon targets. JOURNAL OF PHYSICS. CONDENSED MATTER : AN INSTITUTE OF PHYSICS JOURNAL 2012; 24:375302. [PMID: 22913935 DOI: 10.1088/0953-8984/24/37/375302] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/01/2023]
Abstract
Interrupted coarsening (IC) has recently been identified as an important feature for the dynamics of the typical length-scale in pattern-forming systems on surfaces. In practice, it can be beneficial to improve pattern ordering since it combines a certain degree of defect suppression with a limited increase in the typical pattern wavelength. However, little is known about its robustness with respect to changes in the preparation of the initial system for cases with potential applications. Working in the context of nano-scale pattern formation by ion-beam sputtering (IBS), we prove that IC properties do not depend on sample preparation. Specifically, interface dynamics under IBS is quantitatively compared on virgin amorphous and crystalline silicon surfaces, using 1 keV Ar(+) ions at normal incidence where nanodot pattern formation is triggered by concurrent co-deposition of Fe atoms during processing. Atomic force microscopy shows that dot patterns with similar spatial order and dynamics are obtained in both cases, underscoring the key dynamical role of the amorphous surface layer produced by irradiation. Both systems have been quantitatively described by an effective interface equation. We employ a new procedure based on the linear growth of the initial surface correlations to accurately estimate the equation coefficients. Such a method improves the predictive power of the interface equation with respect to previous studies and leads to a better description of the experimental pattern and its dynamical features.
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Affiliation(s)
- J Muñoz-García
- Departamento de Matemáticas and Grupo Interdisciplinar de Sistemas Complejos (GISC), Universidad Carlos III de Madrid, Leganés, Spain.
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Muñoz-García J, Cuerno R, Castro M. Coupling of morphology to surface transport in ion-beam-irradiated surfaces: normal incidence and rotating targets. JOURNAL OF PHYSICS. CONDENSED MATTER : AN INSTITUTE OF PHYSICS JOURNAL 2009; 21:224020. [PMID: 21715758 DOI: 10.1088/0953-8984/21/22/224020] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/31/2023]
Abstract
Continuum models have proved their applicability to describe nanopatterns produced by ion-beam sputtering of amorphous or amorphizable targets at low and medium energies. Here we pursue the recently introduced 'hydrodynamic approach' in the cases of bombardment at normal incidence, or of oblique incidence onto rotating targets, known to lead to self-organized arrangements of nanodots. Our approach stresses the dynamical roles of material (defect) transport at the target surface and of local redeposition. By applying results previously derived for arbitrary angles of incidence, we derive effective evolution equations for these geometries of incidence, which are then numerically studied. Moreover, we show that within our model these equations are identical (albeit with different coefficients) in both cases, provided surface tension is isotropic in the target. We thus account for the common dynamics for both types of incidence conditions, namely formation of dots with short-range order and long-wavelength disorder, and an intermediate coarsening of dot features that improves the local order of the patterns. We provide for the first time approximate analytical predictions for the dependence of stationary dot features (amplitude and wavelength) on phenomenological parameters, that improve upon previous linear estimates. Finally, our theoretical results are discussed in terms of experimental data.
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Affiliation(s)
- Javier Muñoz-García
- Grupo Interdisciplinar de Sistemas Complejos (GISC) and School of Mathematical Sciences and Complex and Adaptive Systems Laboratory, University College Dublin, Belfield, Dublin 4, Republic of Ireland
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