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53. Distribution of Phyllosilicates on Ceres

Author

Ammannito, E., Desanctis, M.C., Ciarniello, M., Frigeri, A., Carrozzo, G., Combe, J. P., Ehlmann, B., Marchi, S., McSween, H.Y., Raponi, A., Castillo-Rogez, J., Toplis, M., Tosi, F., Capaccioni, F., Capria, M. T., Fonte, S., Giardino, M., Jaumann, R., Longobardo, A, Joy, S.P., Magni, G., McCord, T. B., McFadden, L.A., Palomba, E., Pieters, C., Polanskey, C.A., Rayman, M.D., Raymond, C.A., Schenk, P., Zambon, F., and Russell, C. T.

Subjects
Planetengeologie, Ceres, DAWN
Published
2016

54. Detection of H2O-Rich Materials on Ceres by the Dawn Mission

Author

Combe, J. -Ph., McCord, T. B., TOSI, Federico, RAPONI, Andrea, DE SANCTIS, MARIA CRISTINA, Ammannito, E., Raymond, C. A., Russell, C. T., ITA, and USA

Abstract

Exposed H2O ice or H2O-bearing minerals in crater Oxo on Ceres are revealed by near-infrared reflectance spectra acquired by the Dawn mission.

Published
2016

55. VIRTIS-Rosetta Observations of 67P/Churyumov-Gerasimenko Nucleus and Coma During the Mission Pre-Landing Phase

Author

Capaccioni, F., Filacchione, G., Erard, S., Arnold, Gabriele, Capria, M. T., De Sanctis, M.C., Tosi, Nicola, Ciarniello, M., Bockelee-Morvan, D., Leyrat, C., Palomba, E., Piccioni, G., Raponi, A., Longobardo, A, Migliorini, A., Ammannito, E., Combi, M., Fink, U., McCord, T. B., Carlson, R. W., Jaumann, R., Drossart, P., Formisano, M., Schmitt, B., Frigeri, A., Flamini, E., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
comet, Rosetta, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience

Published
2014

56. Vesta Mineralogy in the Light of Dawn

Author

De Sanctis, M.C., Ammannito, E., Combe, J. P., Jaumann, R., McCord, T. B., McFadden, L.A., McSween, H.Y., Pieters, C.M., Raymond, C.A., and Russell, C.T.

Subjects
Vesta, DAWN, Mineralogy
Published
2014

57. A close look at the Vestan Rheasilvia basin

Author

Ammannito, E., De Sanctis, M.C., Capaccioni, F., Capria, M. T., Combe, J. P., Frigeri, A., Hoffmann, M., Jaumann, R., Longobardo, A, Marchi, S., McCord, T. B., McSween, H.Y., Mest, S., Mittlefehldt, David W., Stephan, K., Tosi, F., Yingst, R. Aileen, Raymond, C.A., and Russell, C.T.

Subjects
Planetengeologie, Vesta, Dawn Mission
Published
2014

58. ACETYLENE ON TITAN’S SURFACE

Author

Singh, S., primary, McCord, T. B., additional, Combe, J-Ph., additional, Rodriguez, S., additional, Cornet, T., additional, Mouélic, S. Le, additional, Clark, R. N., additional, Maltagliati, L., additional, and Chevrier, V. F., additional

Published
2016
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59. Dawn Completes its Mission at Vesta

Author

Russell, C. T., Raymond, C.A., Jaumann, R., McSween, H.Y., De Sanctis, M.C., Nathues, A., Prettyman, T.H., Ammannito, E., Reddy, V., Preusker, Frank, O´Brain, D. P., Marchi, S., Denevi, B., Buczkowski, D.L., Pieters, C., McCord, T. B., Li, J. Y., Mittlefelhldt, D.W., Combe, J. P., Williams, D.A., Hiesinger, H., Yingst, R. A., Polanskey, C.A., and Joy, S.P.

Subjects
Vesta, mineralogical, impact basin, Dawn
Published
2013

60. The Geology of Vesta’s Dark Material

Author

Jaumannn, R., Otto, K., Nass, A., Krohn, Katrin, McCord, T. B., Williams, D.A., Yingst, A., Combe, J. P., Palomba, E., Tosi, F., DeSanctis, M.C., Stephan, K., Hiesinger, H., Blewett, D., Reddy, V., LeCorre, L., Raymond, C.A., and Russell, C.T.

Subjects
Vesta Dawn Dark material
Published
2013

61. Dark and Bright Albedo Changes in the Wake of a Titan Rainstorm

Author

Barnes, Jason W., Buratti, B. J., Turtle, E. P., Bow, J., Dalba, P. A., Perry, J., Rodriguez, S., LeMouelic, S., Baines, K. H., Sotin, C., Lorenz, R. D., Malaska, M. J., McCord, T. B., Clark, R. N., Jaumann, R., Hayne, P. O., Nicholson, P. D., Soderblom, J. M., and Soderblom, L. A.

Subjects
Albedo, ISS, VIMS, Cassini, Titan
Published
2012

62. Mineralogical Mapping of the Av-8 Marcia and Av-9 Numisia Quadrangles of Asteroid 4 Vesta

Author

Capaccioni, F., De Sanctis, M.C., Nathues, A., Ammannito, E., Tosi, F., Zambon, F., Palomba, E., Frigeri, A., Le Corre, L., Reddy, V., Jaumann, R., Stephan, K., Preusker, Frank, Denevi, B., and McCord, T. B.

Subjects
Planetengeologie, Vesta, Dawn
Abstract

Asteroid 4 Vesta is currently observed by NASA's Dawn orbiter. The Dawn Team is conducting mineralogical mapping of the surface in the form of 15 quadrangle maps, and here we report results from the mapping of the two adjacent quadrangles Marcia (Av-8) and Numisia (Av-9). The mapping is based on a Framing Camera (FC) color band ratio and Visible and InfraRed (VIR) hyperspectral images. Av-8 Marcia Quadrangle covers 144˚-216˚E longitude while Av-9 Numisia extends from 216˚-288˚E longitude; both quadrangles are located in the equatorial region from ±21˚ latitude. Av-8 Marcia is dominated by a cratered regions, which is a low-albedo ejecta field containing craters Marcia, (68 km by 58 km), Calpurnia (54 km by 52 km), and Minucia (26 km by 23 km). A hill with a dark-rayed crater, named Aricia Tholus, is also nearby (size about 42.5 km and 28 km). Av-9 Numisia is dominated by Vestalia Terra, a distinct region of Vesta. Many of the impact craters in Av-9 have both bright and dark layers in their walls and also distinct ejecta lobes. The largest feature in Av-9 is the 33 km diameter Numisia crater which is centrally located at 7°S, 247°E. The other significant feature is the 15 km diameter Cornelia crater. Cornelia, smaller than Numisia is apparently more interesting has it shows a greater color diversity and an extensive ray system. In particular FC color data show an inner dark albedo region surrounded by an extended light colored ray system, this is also shown in the VIR images. Both FC color ratio images and VIR images show compositional variations within the Marcia quadrangle (De Sanctis et al., LPSC2012). The band depth distribution is uneven in this region and associated with the geological structures present in the quadrangles. On average the dominant terrains are the so called ET ( Equatorial Terrains) characterized by intermediate band depths, but associated with Marcia we see also terrains with very deep band depth similar to the ST (Southern Terrains) and deep band depth as the MLT (Mid Latitude Terrains). The low albedo ejecta field, derived from the Marcia and Calpurnia craters (located in Av-9), mantles underlying older terrains and is associated with the CET (Copious ejecta Terrains): the band depth are very shallow. VIR data show strong 1 µm and 2 µm absorptions exposed within the walls and floor of impact crater Marcia, suggesting excavation of pyroxene-rich material and/or variations in particle sizes. FC color ratio images, as well as VIR color ratio (Red:750/430 nm; Green :750/920 nm; Blue:430/750 nm) show color differences in Marcia and Calpurnia. The color and spectral data show the difference between the eastern side of the Marcia and Calpurnia ejecta field from its western side. Moreover it appears an unusual diffuse deposit surrounding an unnamed crater on the western side of the quadrangle. Further study is underway to investigate the significance of these color variations. The authors gratefully acknowledge the support of the Dawn Instrument, Operations, and Science Teams. This work is supported by an Italian Space Agency (ASI) grant and by NASA through the Dawn project and a Dawn at Vesta Participating Scientist grant.

Published
2012

63. Mineralogical Mapping of the Av-5 Floronia Quadrangle of Asteroid 4 Vesta

Author

Combe, J. P., Fulchinioni, M., McCord, T. B., Ammannito, E., De Sanctis, M.C., Nathues, A., Capaccioni, F., Frigeri, A., Jaumann, R., Le Corre, L., Palomba, E., Preusker, Frank, Reddy, V., Stephan, K., Tosi, F., Zambon, F., Raymond, C.A., and Russell, C.T.

Subjects
Planetengeologie, Vesta, Dawn
Abstract

Asteroid 4 Vesta is currently under investigation by NASA's Dawn orbiter. The Dawn Science Team is conducting mineralogical mapping of Vesta's surface in the form of 15 quadrangle maps, and here we report results from the mapping of Floronia quadrangle Av-5. The maps are based on the data acquired by the Visible and Infrared Mapping Spectrometer (VIR-MS) and the Framing Camera (FC) (De Sanctis et al., this meeting). This abstract is focused on the analysis of band ratios, as well as the depth and position of the 2-µm absorption band of pyroxenes, but additional information will be presented. Absorption band depth is sensitive to abundance, texture and multiple scattering effects. Absorption band position is controlled by composition, shorter wavelength positions indicate less Calcium (and more Magnesium) in pyroxenes. The inferred composition is compared with that of Howardite, Eucite and Diogenite meteorites (HEDs). Diogenites are Mg-rich with large orthopyroxene crystals suggesting formation in depth; Eucrites are Ca-poor pyroxene, with smaller crystals. Av-5 Floronia Quadrangle is located between ~20-66˚N and 270˚-360˚E. It covers a portion of the heavily-cratered northern hemisphere of Vesta, and part of it is in permanent night, until August 2012. Long shadows make the visualization of albedo variations difficult, because of limited effectiveness of photometric corrections. Most of the variations of the band depth at 2 µm are partly affected by illumination geometry in this area. Only regional tendencies are meaningful at this time of the analysis. The 2-µm absorption band depth seems to be deeper towards the south of the quadrangle, in particular to the south of Floronia crater. It is not possible to interpret the value of the band depth in the floor the craters because of the absence of direct sunlight. However, the illuminated rims seem to have a deeper 2-µm absorption band, as does the ejecta from an unnamed crater located further south, within quadrangle Av-10 (Tosi et al., 2010, this meeting). The absorption band seems slightly shifted towards shorter wavelengths in the neighborhood of the same crater, which may indicate a more diogenitic composition, consistent with materials of the deeper crust. Relationships between craters, ejecta and composition will be investigated further. The authors acknowledge the support of the Dawn Science, Instrument and Operations Teams. This work was supported by the NASA Dawn Project under contract from UCLA and by the NASA Dawn at Vesta Participating Scientist program.

Published
2012

64. Mega-Impacts into Planetary Bodies: Global Effects of the Giant Rheasilvia Impact Basin on Vesta

Author

Schenk, P., Marchi, S., O'Brien, D.P., Buczkowski, D.L., Jaumann, R., Yingst, R. Aileen, McCord, T. B., Gaskell, R.W., Roatsch, Thomas, Keller, H. U., Raymond, C.A., and Russell, C.T.

Subjects
Planetengeologie, Vesta, Rheasilvia, Dawn
Abstract

Vesta has been hammered by large impacts, including two large (400-500 km) basins at the South Pole, the largest basins in proportion to target radius so far seen in the solar system. Here we examine the global effects of impacts at planetary scales.

Published
2012

65. Dark Material On Vesta: Synthesis And Interpretations From Dawn Observations

Author

McCord, T. B., Combe, J. P., Jaumann, R., Palomba, E., Reddy, V., Blewett, D., McSween, H.Y., Raymond, C.A., Williams, D.A., and Dawn, Science Team

Subjects
Planetengeologie, Vesta, Asteroids, Dawn
Abstract

Unusual deposits of “Dark Material” (DM) on Vesta’s surface were recently discovered by the Dawn Mission [1,2]. A focused study of these deposits is underway within the Dawn team and the three preceeding presentations in this session [3,4,5] treat different aspects (geological, morphological and compositional) of the Dawn observations analysis. This report is a synthesis of these findings, presents some further analysis and interprets them in terms of origin( s) and processes.

Published
2012

66. Geologic mapping of the AV-3 Caparronia quadrangle of asteroid 4 Vesta

Author

Young, B.L., Blewett, David T., Williams, D.A., O´Brien, D.P, Gaskell, R.W., Yingst, R. Aileen, Garry, W.B., Buczkowski, D.L., Hiesinger, Harald, McCord, T. B., Combe, J.-P., Schenk, P., Jaumann, R., Pieters, Carle M., Nathues, A., Le Corre, L., Hoffmann, M., Reddy, V., Roatsch, Thomas, Preusker, Frank, Marchi, S., Scully, J., Russell, C.T., Raymond, C.A., and Desanctis, M.C.

Subjects
Planetengeologie, Vesta, Dawn
Abstract

NASA’s Dawn spacecraft began orbiting the inner main belt asteroid 4 Vesta on July 16, 2011, and will characterize the geology, elemental and mineralogical composition, topography, and internal structure of Vesta before departing for asteroid 1 Ceres in late 2012. As part of the Dawn data analysis, the science team is constructing geological mapping of the surface, in the form of 15 quadrangle maps. This abstract reports preliminary results from mapping of quadrangle Av-3, named for Caparronia crater.

Published
2012

67. First mineralogical maps of 4 Vesta

Author

De Sanctis, Maria Cristina, Nathues, A., Ammannito, E., Capaccioni, F., Frigen, A., Le Corre, L., Jaumann, Ralf, Palomba, E., Pieters, Carle M., Reddy, V., Stephan, K., Tosi, Nicola, Yingst, A., Zambon, A., Barucci, M. A., Blewett, D., Capria, M. T., Combe, J. P., Denevi, B., Keller, H. U., Marchi, S., McCord, T. B., McFadden, L.A., McSween, H.Y., Raymond, C.A., Russell, C.T., Li, J. Y., Sunshine, J.M., and Toplis, M.

Subjects
Planetengeologie, Vesta, asteroid, mineralogy, Dawn
Abstract

Before Dawn arrived at 4 Vesta only very low spatial resolution (~50 km) albedo and color maps were available from HST data. Also ground-based color and spectroscopic data were utilized as a first attempt to map Vesta’s mineralogical diversity [1-4]. The VIR spectrometer [5] onboard Dawn has ac-quired hyperspectral data while the FC camera [6] ob-tained multi-color data of the Vestan surface at very high spatial resolutions, allowing us to map complex geologic, morphologic units and features. We here re-port about the results obtained from a preliminary global mineralogical map of Vesta, based on data from the Survey orbit. This map is part of an iterative map-ping effort; the map is refined with each improvement in resolution.

Published
2012

68. Geologic mapping of the AV-8 Marcia Quadrangle of Asteroid 4 Vesta

Author

Williams, D., Schenk, P., Jaumann, R., Buczkowski, D.L., McCord, T. B., Yingst, R. Aileen, Hiesinger, H., Garry, W. Brent, Combe, J. P., Pieters, C., Nathues, A., Le Corre, L., Hoffmann, M., Reddy, V., Roatsch, Thomas, Preusker, Frank, Marchi, S., Russell, C.T., Raymond, C.A., Neukum, G., Schmedemann, N., Ammannito, E., De Sanctis, M. C., and Dawn, Science Team

Subjects
Planetengeologie, Vesta, Asteroid, Dawn
Abstract

NASA’s Dawn spacecraft entered orbit of the inner main belt asteroid 4 Vesta on July 16, 2011, and is spending one year in orbit to characterize the geology, chemical and mineralogical composition, topography, shape, and internal structure of Vesta before departing to asteroid 1 Ceres in late 2012. As part of the Dawn data analysis the Science Team is conducting geological mapping of the surface, in the form of 15 quadrangle maps. This abstract reports results from the mapping of quadrangle Av-8, named Marcia. Data: The base for mapping this quadrangle is a monochrome Framing Camera (FC) mosaic produced from the High Altitude Mapping Orbit (HAMO) data with a spatial resolution of ~70 m/pixel. This base is supplemented by a Digital Terrain Model (DTM) derived from Survey orbit stereo image data with a lateral spacing of 450 m/pixel (10 pixels per degree) and a vertical accuracy of ~30 meters. Also used to support the mapping are FC color ratio images from the Survey orbit with a spatial resolution of ~250 m/pixel, slope and contour maps derived from the DTM, and Visible and InfraRed (VIR) hyperspectral images from the Survey and HAMO orbits with spatial resolutions of 700 and 200 m/pixel, respectively.

Published
2012

69. Saturn’s system ices: a comparative spectral study by Cassini-VIMS

Author

Filacchione, G., Capaccioni, F., Clark, R.N., Cuzzi, J. N., Cruikshank, D.P., Coradini, A., Cerroni, P., Tosi, F., Ciarnello, M., Nicholson, P. D., McCord, T. B., Brown, R.H., Buratti, B. J., Jaumann, R., and Stephan, K.

Subjects
Planetengeologie, Saturn, VIMS, Cassini
Published
2010

70. Revised Full-Disk Spectra by Cassini-Vims of the Saturnian Minor Icy Moons

Author

Filacchione, G., Cuzzi, J. N., Clark, R. N., Buratti, B. J., Capaccioni, F., Tosi, F., Coradini, A., Cerroni, P., Adriani, A., Cruikshank, D. P., Jaumann, R., Stephan, K., Brown, R. H., Nicholson, P. D., Baines, K. H., Nelson, R. M., and McCord, T. B.

Subjects
Planetengeologie, Cassini-VIMS, Saturnian Icy Moons
Published
2009

71. VIMS spectral mapping observations of Titan during the Cassini prime mission

Author

Barnes, J. W., Soderblom J. M., Brown R. H., Buratti B. J., Sotin, C., Baines K. H., Clark R. N., Jaumann, R., Mccord T. B., Nelson, R., Stéphane Le Mouélic, Rodriguez, S., Griffith, C., Penteado, P., Tosi, F., Pitmam K. M., Soderblom, L., Stephan, K., Hayne, P., Vixie, G., P, Bibring J., Capaccioni, F., Cerroni, P., Coradini, A., Cruikshank D. P., Drossart, P., Formisano, V., Langevin, Y., Matson D. L., Nicholson P. D., Sicardy, B., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences, ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2009

72. VIMS coverage of Saturn's icy satellite Rhea

Author

Stephan, K., Jaumann, R., Wagner, R., Clark, R.N., Cruikshank, D. P., Hibbitts, C.A., Roatsch, Thomas, Brown, R.H., Buratti, B.J., Filacchione, G., Hansen, G.B., McCord, T. B., Baines, K. H., and Nicholson, P. D.

Subjects
Geologie, Dione, Saturnmond, Spektroskopie
Published
2009

74. The Diversity of Saturn´s Main Rings: A Cassini VIMS Perspective

Author

Filacchione, G., Capaccioni, F., Tosi, F., Coradini, A., Cerroni, P., Nelson, R. M., Clark, R. N., Nicholson, P. D., Cuzzi, J. N., Hedman, M. H., Showalter, M. R., Jaumann, R., Stephan, K., Cruikshank, D. P., Brown, R. H., Baines, K. H., and McCord, T. B.

Subjects
Planetengeologie, Saturn Rings, Cassini-VIMS
Published
2008

75. Analysis of the Saturnian icy satellites full-disk spectra by Cassini-VIMS

Author

Filacchione, G., Capaccioni, F., Tosi, F., Coradini, A., Cerroni, P., McCord, T. B., Baines, K. H., Belluci, G., Brown, R.H., Burratti, B.J., Clark, R. N., Cruikshank, D. P., Cuzzi, J.N., Jaumann, R., Stephan, K., Matson, D. L., Nelson, R.M., and Nicholson, P. D.

Subjects
Saturnmonde
Published
2008

76. The diversity of Saturn’s main rings investigated by Cassini-VIMS

Author

Filacchione, G., Capaccioni, F., Tosi, F., Coradini, A., Cerroni, P., Clark, R. N., Nicholson, P. D., Cuzzi, J.N., Hedman, M.H., Showalter, M., Jaumann, R., Stephan, K., Cruikshank, D. P., Brown, R.H., Baines, K. H., Nelson, R.M., and McCord, T. B.

Subjects
Saturnringe
Published
2008

77. VIS-NIR Spectrophotometric Study of the Saturnian icy Satellites by Cassini-VIMS

Author

Filacchione, G., Capaccioni, F., Tosi, F., Coradini, A., Cerroni, P., Adriani, A., Mccord, T. B., Baines, K. H., Bellucci, G., Brown, R. H., Bibring, J., Buratti, B. J., Clark, R. N., Combes, M., Cruikshank, D. P., Formisano, V., Jaumann, R., Langevin, Y. G., Matson, D. L., Vito Mennella, Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience

Published
2007

78. The high-resolution stereo camera (HRSC) experiment on Mars Express: Instrument aspects and experiment conduct from interplanetary cruise through nominal mission

Author

Jaumann, R., Neukum, G., Behnke, T., Duxbury, T. C., Eichentopf, K., Flohrer, J., van Gasselt, S., Giese, B., Gwinner, K., Hauber, E., Hoffmann, H., Hoffmeister, A., Köhler, U., Matz, K.-D., McCord, T. B., Mertens, V., Oberst, J., Pischel, R., Reiss, D., Ress, E., Roatsch, T., Saiger, P., Scholten, F., Schwarz, Gottfried, Stephan, K., Wählisch, M., and HRSC Co-Investigator Team

Subjects
HRSC, Stereo imaging, Planetary missions, Mars, Mars Express, Imaging instruments
Published
2007

82. Considerations on the Titan Topography Based on the Cassini-VIMS Measurements in the NIR Range

Author

Moriconi, M., Adriani, A., Gardini, A., Coradini, A., Filacchione, G., Orosei, R., D Aversa, E., Capaccioni, F., Cerroni, P., Bellucci, G., Brown, R. H., Baines, K. H., Bibring, J. -P, Buratti, B. J., Clark, R. N., Combes, M., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[SDU]Sciences of the Universe [physics], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2006

83. Determination of the Haze Layer Parameters in the Saturn Atmosphere from Cassini-VIMS Images

Author

Adriani, A., Moriconi, M., Colosimo, F., Coradini, A., Filacchione, G., Orosei, R., D Aversa, E., Capaccioni, F., Cerroni, P., Bellucci, G., Brown, R. H., Baines, K. H., Bibring, J. -P, Buratti, B. J., Clark, R. N., Combes, M., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
Planetengeologie, Saturn, Atmosphere, Haze layers, VIMS, Cassini, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2006

84. VIS-NIR Spectral Properties of Saturn's Minor Icy Moons

Author

Filacchione, G., Coradini, A., Capaccioni, F., Cerroni, P., Bellucci, G., Brown, R. H., Baines, K. H., Bibring, J. -P, Buratti, B. J., Clark, R. N., Combes, M., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C., Adriani, A., Moriconi, M., D Aversa, E., Tosi, F., Colosimo, F., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[SDU]Sciences of the Universe [physics], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2006

85. Cassini/VIMS observations of Titan: geological implications

Author

Sotin, C., Rodriguez, S., Le Mouélic, S., Tobie, G., Buratti, B. J., Brown, R. H., Jaumann, R., Clark, R. N., Baines, K. H., McCord, T. B., Nelson, R. M., and VIMS Science Team

Subjects
Planetengeologie, geology, VIMS, Cassini, Titan
Published
2006

86. Cassini observations of the opposition effect of Saturn's rings 1

Author

Nelson, R. M., Hapke, B. W., Brown, R. H., Spilker, L. J., Smythe, W. D., Kamp, L., Boryta, M., Leader, F., Matson, D. L., Edgington, S., Nicholson, P. D., Filacchione, G., Clark, R. N., Bibring, J.-P., Baines, K. H., Buratti, B., Bellucci, G., Capaccioni, F., Cerroni, P., Combes, M., Coradini, A., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., McCord, T. B., Mennella, V., Sicardy, B., and Sotin, C.

Subjects
Planetengeologie, Saturn, VIMS, Cassini, opposition effect, rings
Published
2006

87. Full-disk observations of the saturnian moons in the VIS-NIR spectral range by Cassini- VIMS

Author

Filacchione, G., Capaccioni, F., Coradini, A., Cerroni, P., Tosi, F., Adriani, A., Mccord, T. B., Baines, K. H., Bellucci, G., Brown, R. H., Bibring, J., Buratti, B. J., Clark, R. N., Combes, M., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Vito Mennella, Robert, N. M., Nicholson, P. D., Sicardy, B., Sotin, C., Moriconi, M., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

During the first two years of the Cassini's nominal mission, VIMS (Visual and Infrared Mapping Spectrometer) has explored the whole system of Saturnian icy satellites. Here we report a comparative analysis of more than 600 full-disk observations obtained from July 2004 to nowadays for 15 regular and minor satellites: Atlas, Prometheus, Pandora, Janus, Epimetheus, Mimas, Enceladus, Tethys, Telesto, Calypso, Dione, Rhea, Hyperion, Iapetus and Phoebe. These observations, done from the equatorial plane, are particularly suitable to highlight the spectral differences between the leading and trailing sides of the regular satellites as function of the illumination angle (Filacchione et al., 2006a, 2006b); a byproduct of this activity is the measurement of the phase curves. The combined use of several VIS and IR spectral quantities (e.g. spectral slopes, water ice bands strengths, continuum levels, etc.) allows to find correlations between classes of satellites orbiting at different distances from Saturn: in this way it is possible to discriminate the almost pure ice surfaces of Enceladus and Calypso from the organic rich Hyperion, Iapetus and Phoebe (Tosi et al., 2006). This research was completed thanks to the support of the Italian Space Agency (ASI), Grant ASI/Cassini I/031/05/0. Filacchione et al., 2006a. Saturn's icy satellites investigated by Cassini-VIMS. I. Full-disk properties: 350-5100 nm reflectance spectra and phase curves, Icarus, in press. Filacchione et al., 2006b. VIS-NIR Spectral Properties of Saturn's Minor Icy Moons. 37th LPSC, abstract no.1271 Tosi et al., 2006. Iapetus, Phoebe and Hyperion: Are They Related? 37th LPSC, abstract no.1582

Published
2006

88. Titan: surface composition from Cassini VIMS

Author

McCord, T. B., Hansen, G. B., Buratti, B. J., Clark, R. N., Cruikshank, D. P., D'Aversa, E., Griffith, C. A., Baines, K. H., Brown, R. H., Dalle Ore, C. M., Filacchione, G., Formisano, V., Hibbitts, C. A., Jaumann, R., Lunine, J. I., Nelson, R. M., Sotin, C., and Cassini VIMS Team

Subjects
Planetengeologie, Saturnian system, surface composition, VIMS, Cassini, Titan
Published
2006

89. Iapetus, Phoebe and Hyperion: are they related?

Author

Tosi, F., Coradini, A., Capaccioni, F., Cerroni, P., Filacchione, G., Bellucci, G., Adriani, A., Moriconi, M., D Aversa, E., Brown, R. H., Baines, K. H., Bibring, J. -P, Buratti, B. J., Clark, R. N., Combes, M., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Planetengeologie, Phoebe, [SDU]Sciences of the Universe [physics], Iapetus, Saturnian moons, VIMS, Cassini, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS, Hyperion
Abstract

International audience

Published
2006

92. An Apparent Increase in Flux from a Surface Feature on Titan: Implications for Surface and Atmosphere

Author

Nelson, R. M., Hapke, B. W., Smythe, W. D., Kamp, L., Boryta, M., Leader, F., Jaumann, R., Clark, R. N., Lunine, J., Cruikshank, D. P., Drossart, P., Soderblom, L., Baines, K. H., Bellucci, G., Birbring, J. P., Buratti, B. J., Capaccioni, F., Cerroni, P., Combes, M., Coradini, A., Formisano, V., Langevin, R. Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2005

93. Cassini VIMS Photometric Investigation of Selected Features on the Surface of Titan: Relevance to Widespread Precipitation

Author

Nelson, R. M., Brown, R. H., Hapke, B. W., Smythe, W. D., Kamp, L., Boryta, M., Baines, K. H., Bellucci, G., Biebring, J., Buratti, B. J., Capaccioni, F., Cerroni, P., Clark, R. N., Coradini, A., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2005

94. Cassini VIMS Preliminary Exploration of Titan's Surface Hemispheric Albedo Dichotomy

Author

Nelson, R. M., Brown, R. H., Hapke, B. W., Smythe, W. D., Kamp, L., Boryta, M., Baines, K. H., Bellucci, G., Biebring, J. P., Buratti, B. J., Capaccioni, F., Cerroni, P., Clark, R. N., Coradini, A., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
Institut für Planetenforschung, albedo dichotomy, VIMS, Cassini, Saturnian satellites, Titan, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2005

95. Cassini VIMS at Saturn: The first 6 months

Author

Brown, R. H., Baines, K. H., Bellucci, G., Buratti, B. J., Capaccioni, F., Cerroni, P., Clark, R. N., Coradini, A., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Matson, D. L., Mccord, T. B., Vito Mennella, Nelson, R. M., Nicolson, P., Sicardy, B., Sotin, C., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
Saturn, Institut für Planetenforschung, VIMS, Saturnian Satellites, Cassini, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience

Published
2005

96. The Surface Properties of Titan as Revealed by Cassini VIMS

Author

Buratti, B. J., Sotin, C., Mccord, T. B., Brown, R. H., Clark, R., Cruikshank, D. P., Jaumann, R., Baines, K., Bellucci, G., Bibring, J., Capaccioni, F., Cerroni, P., Combes, M., Coradini, A., Drossart, P., Formisano, V., Langevin, Y., Matson, D., Vito Mennella, Nelson, R., Nicholson, P., Sicardy, B., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2005

97. Spectral Imaging of Saturn by Cassini/VIMS: Early Science Results

Author

Baines, K. H., Drossart, P., Formisano, V., Brown, R. H., Bellucci, G., Bibring, J., Buratti, B., Capaccioni, F., Cerroni, P., Clark, R. N., Coradini, A., Cruikshank, D. P., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C., Momary, T. W., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2004

98. Iapetus: First data from the Cassini Visual Infrared Mapping Spectrometer

Author

Buratti, B. J., Cruikshank, D. P., Clark, R., Brown, R. H., Bauer, J. M., Simonelli, D. P., Jaumann, R., Hibbitts, K., Mccord, T. B., Soderlund, K., Baines, K. H., Bellucci, G., Bibring, J. P., Capaccioni, F., Cerroni, P., Coradini, A., Drossart, P., Formisano, V., Langevin, Y., Matson, D. L., Vito Mennella, Nelson, R., Nicholson, P. D., Sicardy, B., Sotin, C., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2004

99. Initial Results of the Cassini VIMS Investigation at Saturn

Author

Brown, R. H., Baines, K., Bellucci, G., Buratti, B. J., Capaccioni, F., Cerroni, P., Coradini, R., Cruikshank, D. P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., Mccord, T. B., Vito Mennella, Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C., Baugh, N., Griffith, C. A., Hansen, G. B., Hibbitts, C. A., Showalter, M. R., Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2004

100. The Cassini Visual and Infrared Mapping Spectrometer (VIMS) Investigation

Author

Brown, R. H., primary, Baines, K. H., additional, Bellucci, G., additional, Bibring, J.-P., additional, Buratti, B. J., additional, Capaccioni, F., additional, Cerroni, P., additional, Clark, R. N., additional, Coradini, A., additional, Cruikshank, D. P., additional, Drossart, P., additional, Formisano, V., additional, Jaumann, R., additional, Langevin, Y., additional, Matson, D. L., additional, Mccord, T. B., additional, Mennella, V., additional, Miller, E., additional, Nelson, R. M., additional, Nicholson, P. D., additional, Sicardy, B., additional, and Sotin, C., additional

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