Publications
Filter Total Items: 337
Discovery of jarosite within the Mawrth Vallis region of Mars: Implications for the geologic history of the region Discovery of jarosite within the Mawrth Vallis region of Mars: Implications for the geologic history of the region
Analysis of visible to near infrared reflectance data from the MRO CRISM hyperspectral imager has revealed the presence of an ovoid-shaped landform, approximately 3 by 5 km in size, within the layered terrains surrounding the Mawrth Vallis outflow channel. This feature has spectral absorption features consistent with the presence of the ferric sulfate mineral jarosite, specifically a K...
Authors
W. H. Farrand, T.D. Glotch, J. W. Rice, J.A. Hurowitz, G.A. Swayze
Storm clouds on Saturn: Lightning-induced chemistry and associated materials consistent with Cassini/VIMS spectra Storm clouds on Saturn: Lightning-induced chemistry and associated materials consistent with Cassini/VIMS spectra
Thunderstorm activity on Saturn is associated with optically detectable clouds that are atypically dark throughout the near-infrared. As observed by Cassini/VIMS, these clouds are ~20% less reflective than typical neighboring clouds throughout the spectral range from 0.8 ??m to at least 4.1 ??m. We propose that active thunderstorms originating in the 10-20 bar water-condensation region...
Authors
K. H. Baines, M.L. Delitsky, T.W. Momary, R. H. Brown, B. J. Buratti, R. N. Clark, P. D. Nicholson
Fast forward modeling of Titan's infrared spectra to invert VIMS/Cassini hyperspectral images Fast forward modeling of Titan's infrared spectra to invert VIMS/Cassini hyperspectral images
The surface of Titan, the largest icy moon of Saturn, is veiled by a very thick and hazy atmosphere. The Visual and Infrared Mapping Spectrometer onboard the Cassini spacecraft, in orbit around Saturn since July 2004, conduct an intensive survey of Titan with the objective to understand the complex nature of the atmosphere and surface of the mysterious moon and the way they interact...
Authors
S. Rodriguez, Stéphane Le Mouélic, P. Rannou, J. #NAME? Combe, L.L. Corre, G. Tobie, J. W. Barnes, Christophe Sotin, R. H. Brown, K. H. Baines, B. J. Buratti, R. N. Clark, P. D. Nicholson
Characterization of clouds in Titan's tropical atmosphere Characterization of clouds in Titan's tropical atmosphere
Images of Titan's clouds, possible over the past 10 years, indicate primarily discrete convective methane clouds near the south and north poles and an immense stratiform cloud, likely composed of ethane, around the north pole. Here we present spectral images from Cassini's Visual Mapping Infrared Spectrometer that reveal the increasing presence of clouds in Titan's tropical atmosphere...
Authors
C.A. Griffith, P. Penteado, S. Rodriguez, Stéphane Le Mouélic, K. H. Baines, B. Buratti, R. Clark, P. Nicholson, R. Jaumann, Christophe Sotin
Mapping potentialy asbestos-bearing rocks using imaging spectroscopy Mapping potentialy asbestos-bearing rocks using imaging spectroscopy
Rock and soil that may contain naturally occurring asbestos (NOA), a known human carcinogen, were mapped in the Sierra Nevada, California, using the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) to determine if these materials could be uniquely identified with spectroscopy. Such information can be used to prepare or refine maps of areas that may contain minerals that can be...
Authors
G.A. Swayze, R.F. Kokaly, C.T. Higgins, J.P. Clinkenbeard, R. N. Clark, H.A. Lowers, S. J. Sutley
Discovery of lake-effect clouds on Titan Discovery of lake-effect clouds on Titan
Images from instruments on Cassini as well as from telescopes on the ground reveal the presence of sporadic small-scale cloud activity in the cold late-winter north polar region of Saturn's large moon Titan. These clouds lie underneath the previously discovered uniform polar cloud attributed to a quiescent ethane cloud at ???40 km and appear confined to the same latitudes as those of the...
Authors
M.E. Brown, E.L. Schaller, H.G. Roe, C. Chen, J. Roberts, R. H. Brown, K. H. Baines, R. N. Clark
Saturn's north polar cyclone and hexagon at depth revealed by Cassini/VIMS Saturn's north polar cyclone and hexagon at depth revealed by Cassini/VIMS
A high-speed cyclonic vortex centered on the north pole of Saturn has been revealed by the visual-infrared mapping spectrometer (VIMS) onboard the Cassini-Huygens Orbiter, thus showing that the tropospheres of both poles of Saturn are occupied by cyclonic vortices with winds exceeding 135 m/s. High-spatial-resolution (~200 km per pixel) images acquired predominantly under night-time...
Authors
K. H. Baines, T.W. Momary, L.N. Fletcher, A.P. Showman, M. Roos-Serote, R. H. Brown, B. J. Buratti, R. N. Clark, P. D. Nicholson
Character and spatial distribution of OH/H2O on the surface of the moon seen by M3 on chandrayaan-1 Character and spatial distribution of OH/H2O on the surface of the moon seen by M3 on chandrayaan-1
The search for water on the surface of the anhydrous Moon had remained an unfulfilled quest for 40 years. However, the Moon Mineralogy Mapper (M 3) on Chandrayaan-1 has recently detected absorption features near 2.8 to 3.0 micrometers on the surface of the Moon. For silicate bodies, such features are typically attributed to hydroxyl- and/or water-bearing materials. On the Moon, the...
Authors
C.M. Pieters, J.N. Goswami, R. N. Clark, M. Annadurai, J. Boardman, B. Buratti, J. #NAME? Combe, M.D. Dyar, R. Green, J.W. Head, C. Hibbitts, M. Hicks, P. Isaacson, R. Klima, G. Kramer, S. Kumar, E. Livo, S. Lundeen, E. Malaret, T. McCord, J. Mustard, J. Nettles, N. Petro, C. Runyon, M. Staid, J. Sunshine, L.A. Taylor, S. Tompkins, P. Varanasi
Detection of adsorbed water and hydroxyl on the moon Detection of adsorbed water and hydroxyl on the moon
Data from the Visual and Infrared Mapping Spectrometer (VIAAS) on Cassini during its flyby of the AAoon in 1999 show a broad absorption at 3 micrometers due to adsorbed water and near 2.8 micrometers attributed to hydroxyl in the sunlit surface on the AAoon. The amounts of water indicated in the spectra depend on the type of mixing and the grain sizes in the rocks and soils but could be...
Authors
R. N. Clark
Reflectance spectroscopy of organic compounds: 1. Alkanes Reflectance spectroscopy of organic compounds: 1. Alkanes
Reflectance spectra of the organic compounds comprising the alkane series are presented from the ultraviolet to midinfrared, 0.35 to 15.5 /??m. Alkanes are hydrocarbon molecules containing only single carbon-carbon bonds, and are found naturally on the Earth and in the atmospheres of the giant planets and Saturn's moon, Titan. This paper presents the spectral properties of the alkanes as...
Authors
R. N. Clark, J. M. Curchin, T.M. Hoefen, G.A. Swayze
Photometric changes on Saturn's Titan: Evidence for active cryovolcanism Photometric changes on Saturn's Titan: Evidence for active cryovolcanism
We report infrared spectrophotometric variability on the surface of Saturn's moon Titan detected in images returned by the Visual and Infrared Mapping Spectrometer (VIMS) onboard the Cassini Saturn Orbiter. The changes were observed at 7°S, 138°W and occurred between October 27, 2005 and January 15, 2006. After that date the surface was unchanged until the most recent observation, March...
Authors
Robert M. Nelson, Lucas W. Kamp, Rosaly Lopes, Dennis L. Matson, Randolph L. Kirk, Bruce W. Hapke, Stephen D. Wall, Mark D. Boryta, Frank E. Leader, William D. Smythe, Karl L. Mitchell, Kevin H. Baines, Ralf Jaumann, Christophe Sotin, Roger N. Clark, Dale P. Cruikshank, Pierre Drossart, Jonathan I. Lunine, Michel Combes, Giancarlo Bellucci, Jean-Pierre Bibring, Fabrizio Capaccioni, Pricilla Cerroni, Angioletta Coradini, Vittorio Formisano, Gianrico Filacchione, Yves Langevin, Thomas B. McCord, Vito Mennella, Philip D. Nicholson, Bruno Sicardy, Patrick G.J. Irwin, John C. Pearl
The geology of Hotei Regio, Titan: Correlation of Cassini VIMS and RADAR The geology of Hotei Regio, Titan: Correlation of Cassini VIMS and RADAR
Joint Cassini VIMS and RADAR SAR data of ∼700-km-wide Hotei Regio reveal a rich collection of geological features that correlate between the two sets of images. The degree of correlation is greater than anywhere else seen on Titan. Central to Hotei Regio is a basin filled with cryovolcanic flows that are anomalously bright in VIMS data (in particular at 5 μm) and quite variable in...
Authors
L.A. Soderblom, R. H. Brown, J.M. Soderblom, J. W. Barnes, R. L. Kirk, Christophe Sotin, R. Jaumann, D. J. MacKinnon, D.W. Mackowski, K. H. Baines, B. J. Buratti, R. N. Clark, P. D. Nicholson