Bell, J F Squyres, S W Arvidson, R E Arneson, H M Bass, D Blaney, D Nathalie Cabrol Calvin, W Farmer, J Farrand, W H
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Published in
Science
Panoramic Camera images at Gusev crater reveal a rock-strewn surface interspersed with high-to moderate-albedo fine-grained deposits occurring in part as drifts or in small circular swales or hollows. Optically thick coatings of fine-grained ferric iron–rich dust dominate most bright soil and rock surfaces. Spectra of some darker rock surfaces and ...
Greeley, R Squyres, S W Arvidson, R E Bartlett, P Bell, J F Blaney, D Nathalie Cabrol Farmer, J Farrand, B Golombek, M P
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Science
Wind-abraded rocks, ripples, drifts, and other deposits of windblown sediments are seen at the Columbia Memorial Station where the Spirit rover landed. Orientations of these features suggest formative winds from the north-northwest, consistent with predictions from atmospheric models of afternoon winds in Gusev Crater. Cuttings from the rover Rock ...
Grant, J A Arvidson, R Bell, J F Iii Nathalie Cabrol Carr, M H Christensen, P Crumpler, L Marais, D J Des Ehlmann, B L Farmer, J
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Science
The Mars Exploration Rover Spirit has traversed a fairly flat, rock-strewn terrain whose surface is shaped primarily by impact events, although some of the landscape has been altered by eolian processes. Impacts ejected basaltic rocks that probably were part of locally formed lava flows from at least 10 meters depth. Some rocks have been textured a...
Squyres, S W Arvidson, R Bass, D S Bell, J F Iii Bertelsen, Pernille Nathalie Cabrol Gaddis, L Hayes, A G Hviid, S F Johnson, J R
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Science
The Microscopic Imager on the Spirit rover analyzed the textures of the soil and rocks at Gusev crater on Mars at a resolution of 100 micrometers. Weakly bound agglomerates of dust are present in the soil near the Columbia Memorial Station. Some of the brushed or abraded rock surfaces show igneous textures and evidence for alteration rinds, coating...
Porco, C C Baker, E Barbara, J Beurle, K Brahic, A Burns, J A Charnoz, S Cooper, N Dawson, D D Del Genio, A D
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Science
The Cassini Imaging Science Subsystem acquired high-resolution imaging data on the outer Saturnian moon, Phoebe, during Cassini s close flyby on 11 June 2004 and on Iapetus during a flyby on 31 December 2004. Phoebe has a heavily cratered and ancient surface, shows evidence of ice near the surface, has distinct layering of different materials, and ...
Porco, C C Baker, E Barbara, J Beurle, K Brahic, A Burns, J A Charnoz, S Cooper, N Dawson, D D Del Genio, A D
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Published in
Science
Images acquired of Saturn s rings and small moons by the Cassini Imaging Science Subsystem (ISS) during the first 9 months of Cassini operations at Saturn have produced many new findings. These include new saturnian moons; refined orbits of new and previously known moons; narrow diffuse rings in the F-ring region and embedded in gaps within the mai...
Lecellier, Charles-Henri Dunoyer, Patrice Arar, Khalil Jacqueline Lehmann-Che Eyquem, Stephanie Himber, Christophe Ali Saib Voinnet, Olivier
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Science
In eukaryotes, 21- to 24-nucleotide-long RNAs engage in sequence-specific interactions that inhibit gene expression by RNA silencing. This process has regulatory roles involving microRNAs and, in plants and insects, it also forms the basis of a defense mechanism directed by small interfering RNAs that derive from replicative or integrated viral gen...
Serge Luquet Perez, Francisco A Hnasko, Thomas S Palmiter, Richard D
Published in
Science
Hypothalamic neurons that express neuropeptide Y (NPY) and agouti-related protein (AgRP) are thought to be critical regulators of feeding behavior and body weight. To determine whether NPY/AgRP neurons are essential in mice, we targeted the human diphtheria toxin receptor to the Agrp locus, which allows temporally controlled ablation of NPY/AgRP ne...
Lee, C.-C.
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Science
Xinchuan Huang Mccoy, Anne B Bowman, Joel M Johnson, Lindsay M Savage, Chandra Dong, Feng Nesbitt, David J
Published in
Science
We present two quantum calculations of the infrared spectrum of protonated methane (CH 5+) using full-dimensional, ab initio–based potential energy and dipole moment surfaces. The calculated spectra compare well with a low-resolution experimental spectrum except below 1000 cm–1, where the experimental spectrum shows no absorption. The present calcu...