Laurence Soderblom, PhD (Former Employee)
Science and Products
Filter Total Items: 137
Dunes on Titan observed by Cassini Radar Dunes on Titan observed by Cassini Radar
Thousands of longitudinal dunes have recently been discovered by the Titan Radar Mapper on the surface of Titan. These are found mainly within ±30° of the equator in optically-, near-infrared-, and radar-dark regions, indicating a strong proportion of organics, and cover well over 5% of Titan's surface. Their longitudinal duneform, interactions with topography, and correlation with other...
Authors
J. Radebaugh, R. Lorenz, J. I. Lunine, S. Wall, G. Boubin, E. Reffet, Randolph Kirk, R.M. Lopes, E. Stofan, Laurence Soderblom, M. Allison, M. Janssen, P. Paillou, P. Callahan, Carl Spencer
Correlations between Cassini VIMS spectra and RADAR SAR images: Implications for Titan's surface composition and the character of the Huygens Probe Landing Site Correlations between Cassini VIMS spectra and RADAR SAR images: Implications for Titan's surface composition and the character of the Huygens Probe Landing Site
Titan's vast equatorial fields of RADAR-dark longitudinal dunes seen in Cassini RADAR synthetic aperture images correlate with one of two dark surface units discriminated as “brown” and “blue” in Visible and Infrared Mapping Spectrometer (VIMS) color composites of short-wavelength infrared spectral cubes (RGB as 2.0, 1.6, 1.3 μm). In such composites bluer materials exhibit higher...
Authors
Laurence Soderblom, Randolph Kirk, Jonathan Lunine, Jeffrey Anderson, Kevin Baines, Jason Barnes, Janet Barrett, Robert Brown, Bonnie Buratti, Roger Clark, Dale Cruikshank, Charles Elachi, Michael Janssen, Ralf Jaumann, Erich Karkoschka, Stéphane Le Mouélic, Rosaly Lopes, Ralph Lorenz, Thomas McCord, Philip Nicholson, Jani Radebaugh, Bashar Rizk, Christophe Sotin, Ellen Stofan, Tracie Sucharski, Martin Tomasko, Stephen Wall
Cryovolcanic features on Titan's surface as revealed by the Cassini Titan Radar Mapper Cryovolcanic features on Titan's surface as revealed by the Cassini Titan Radar Mapper
The Cassini Titan Radar Mapper obtained Synthetic Aperture Radar images of Titan's surface during four fly-bys during the mission's first year. These images show that Titan's surface is very complex geologically, showing evidence of major planetary geologic processes, including cryovolcanism. This paper discusses the variety of cryovolcanic features identified from SAR images, their...
Authors
Rosaly Lopes, K. Mitchell, Ellen Stofan, Jonathan Lunine, Ralf Lorenz, F. Paganelli, Randolph Kirk, C. Wood, Stephen Wall, L.E. Robshaw, A.D. Fortes, Catherine Neish, Jani Radebaugh, E. Reffet, S.J. Ostro, Charles Elachi, M.D. Allison, Y. Anderson, R. Boehmer, G. Boubin, Philip Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, Michael Janssen, W.T.K. Johnson, K. Kelleher, D.O. Muhleman, G. Ori, R. Orosei, G. Picardi, F. Posa, L.E. Roth, R. Seu, S. Shaffer, Laurence Soderblom, B. Stiles, S. Vetrella, R.D. West, L. Wye, H. A. Zebker
Near-infrared spectral mapping of Titan's mountains and channels Near-infrared spectral mapping of Titan's mountains and channels
We investigate the spectral reflectance properties of channels and mountain ranges on Titan using data from Cassini's Visual and Infrared Mapping Spectrometer (VIMS) obtained during the T9 encounter (26 December 2005). We identify the location of channels and mountains using synthetic aperture radar maps obtained from Cassini's RADAR instrument during the T13 (30 April 2006) flyby...
Authors
Jason Barnes, Jani Radebaugh, Robert Brown, Steve Wall, Laurence Soderblom, Jonathan Lunine, Devon Burr, Christophe Sotin, Stephane Le Mouelic, Sebastien Rodriguez, Bonnie Buratti, Roger Clark, Kevin Baines, Ralf Jaumann, Philip Nicholson, Randolph Kirk, Rosaly Lopes, Ralph Lorenz, Ken Mitchell, Charles Wood
Topography and geomorphology of the Huygens landing site on Titan Topography and geomorphology of the Huygens landing site on Titan
The Descent Imager/Spectral Radiometer (DISR) aboard the Huygens Probe took several hundred visible-light images with its three cameras on approach to the surface of Titan. Several sets of stereo image pairs were collected during the descent. The digital terrain models constructed from those images show rugged topography, in places approaching the angle of repose, adjacent to flatter...
Authors
Laurence Soderblom, Martin Tomasko, Brent Archinal, Tammy Becker, Michael Bushroe, Debbie Cook, Lyn Doose, Donna Galuszka, Trent Hare, Elpitha Howington-Kraus, Erich Karkoschka, Randolph Kirk, Jonathan Lunine, Elisabeth McFarlane, Bonnie Redding, Bashar Rizk, Mark Rosiek, Charles See, Peter Smith
The lakes of Titan The lakes of Titan
The surface of Saturn’s haze-shrouded moon Titan has long been proposed to have oceans or lakes, on the basis of the stability of liquid methane at the surface1,2. Initial visible3 and radar4,5 imaging failed to find any evidence of an ocean, although abundant evidence was found that flowing liquids have existed on the surface5,6. Here we provide definitive evidence for the presence of...
Authors
Ellen Stofan, Charles Elachi, Jonathan Lunine, Ralf Lorenz, B. Stiles, K. Mitchell, S. Ostro, Laurence Soderblom, C. Wood, H. Zebker, S. Wall, Michael Janssen, Randolph Kirk, Rosaly Lopes, F. Paganelli, Jani Radebaugh, L. Wye, Y. Anderson, M. Allison, R. Boehmer, P. Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, W.T.K. Johnson, K. Kelleher, D. Muhleman, Philipe Paillou, G. Picardi, F. Posa, L. Roth, R. Seu, S. Shaffer, S. Vetrella, R. West
Advanced technologies demonstrated by the miniature integrated camera and spectrometer (MICAS) aboard deep space 1 Advanced technologies demonstrated by the miniature integrated camera and spectrometer (MICAS) aboard deep space 1
MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80-185 nm), two high-resolution visible imagers (10-20 ??rad/pixel, 400-900 nm), and a short-wavelength infrared imaging spectrometer (1250-2600 nm). The wavelength ranges were chosen to maximize the science data that could be collected using existing semiconductor technologies and avoiding...
Authors
D.H. Rodgers, P.M. Beauchamp, L.A. Soderblom, R. Brown, G.-S. Chen, M. Lee, B.R. Sandel, D.A. Thomas, R.T. Benoit, R.V. Yelle
Pyroclastic activity at home plate in Gusev crater, Mars Pyroclastic activity at home plate in Gusev crater, Mars
Home Plate is a layered plateau in Gusev crater on Mars. It is composed of clastic rocks of moderately altered alkali basalt composition, enriched in some highly volatile elements. A coarse-grained lower unit lies under a finer-grained upper unit. Textural observations indicate that the lower strata were emplaced in an explosive event, and geochemical considerations favor an explosive...
Authors
S. Squyres, O. Aharonson, B.C. Clark, B. Cohen, L. Crumpler, P.A. de Souza, W. Farrand, Ralf Gellert, J. Grant, J.P. Grotzinger, A. Haldemann, J. Johnson, G. Klingelhofer, K.W. Lewis, R. Li, T. McCoy, A. McEwen, H.Y. McSween, D. Ming, Johnnie Moore, R.V. Morris, T. Parker, J. Rice, S. Ruff, M. Schmidt, C. Schroder, L.A. Soderblom, A. Yen
Comparison of the dust distributions in the innermost comae of comets-1P/Halley and 19P/Borrelly spacecraft observations Comparison of the dust distributions in the innermost comae of comets-1P/Halley and 19P/Borrelly spacecraft observations
We present a comparative study of the inner comae of comets 1P/Halley and 19P/Borrelly using data from the Halley Multicolour Camera (HMC) onboard Giotto and the Miniature Integrated Camera and Spectrometer onboard Deep Space 1 (DS1). We show that the dust brightness dependence as a function of radial distance is different for both comets. We suggest that optical depth or fragmentation...
Authors
T.-M. Ho, N. Thomas, D. Boice, M. Combi, L.A. Soderblom, V. Tenishev
Overview of the Opportunity Mars Exploration Rover Mission to Meridiani Planum: Eagle Crater to Purgatory Ripple Overview of the Opportunity Mars Exploration Rover Mission to Meridiani Planum: Eagle Crater to Purgatory Ripple
The Mars Exploration Rover Opportunity touched down at Meridiani Planum in January 2004 and since then has been conducting observations with the Athena science payload. The rover has traversed more than 5 km, carrying out the first outcrop‐scale investigation of sedimentary rocks on Mars. The rocks of Meridiani Planum are sandstones formed by eolian and aqueous reworking of sand grains...
Authors
S. Squyres, R. E. Arvidson, D. Bollen, J.F. Bell, J. Bruckner, N.A. Cabrol, W. Calvin, M. Carr, P. Christensen, B.C. Clark, L. Crumpler, D.J. Des Marais, C. D'Uston, T. Economou, J. Farmer, W.H. Farrand, W. Folkner, R. Gellert, T.D. Glotch, M. Golombek, S. Gorevan, J. Grant, R. Greeley, J. Grotzinger, Kenneth Herkenhoff, S. Hviid, J. Johnson, G. Klingelhoefer, A.H. Knoll, G. Landis, M. Lemmon, Ron Li, M.B. Madsen, M.C. Malin, S. McLennan, H.Y. McSween, D. Ming, J. Moersch, R.V. Morris, T. Parker, J. Rice, L. Richter, R. Rieder, C. Schroeder, M. Sims, M. Smith, P. Smith, Laurence Soderblom, R. Sullivan, N.J. Tosca, H. Wänke, T. Wdowiak, M. Wolff, A. Yen
Overview of the Microscopic Imager Investigation during Spirit's first 450 sols in Gusev crater Overview of the Microscopic Imager Investigation during Spirit's first 450 sols in Gusev crater
The Microscopic Imager (MI) on the Mars Exploration Rover Spirit has returned images of Mars with higher resolution than any previous camera system, allowing detailed petrographic and sedimentological studies of the rocks and soils at the Gusev landing site. Designed to simulate a geologist's hand lens, the MI is mounted on Spirit's instrument arm and can resolve objects 0.1 mm in size...
Authors
Kenneth Herkenhoff, Steve Squyres, Robert Anderson, Brent Archinal, Raymond Arvidson, Janet Barrett, Kris Becker, James F. Bell, Charles Budney, Nathalie Cabrol, Mary Chapman, Debbie Cook, Bethany Ehlmann, Jack Farmer, Brenda Franklin, Lisa Gaddis, Donna Galuszka, Patricia Garcia, Trent Hare, Elpitha Howington-Kraus, Jeffrey Johnson, Sarah Johnson, Kjartan M Kinch, Randolph Kirk, Ella M. Lee, Craig Leff, Mark Lemmon, Madsen B., Justin Maki, Kevin Mullins, Bonnie Redding, Lutz Richter, Mark Rosiek, Michael Sims, Laurence Soderblom, Nicole Spanovich, Richard Springer, Robert Sucharski, Tracie Sucharski, Robert Sullivan, James Torson, Albert Yen
Overview of the Spirit Mars Exploration Rover mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills Overview of the Spirit Mars Exploration Rover mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills
Spirit landed on the floor of Gusev Crater and conducted initial operations on soil‐covered, rock‐strewn cratered plains underlain by olivine‐bearing basalts. Plains surface rocks are covered by wind‐blown dust and show evidence for surface enrichment of soluble species as vein and void‐filling materials and coatings. The surface enrichment is the result of a minor amount of transport...
Authors
R. E. Arvidson, S. Squyres, R. Anderson, J. Bell, D. Blaney, J. Bruckner, N.A. Cabrol, W. Calvin, M. Carr, P. Christensen, B.C. Clark, L. Crumpler, D. Des Marais, P.A. De Souza, C. D'Uston, T. Economou, J. Farmer, W. Farrand, W. Folkner, M. Golombek, S. Gorevan, J. Grant, R. Greeley, J. Grotzinger, E. Guinness, B.C. Hahn, L. Haskin, Kenneth Herkenhoff, J.A. Hurowitz, S. Hviid, J. Johnson, G. Klingelhoefer, A. Knoll, G. Landis, C. Leff, M. Lemmon, R. Li, M.B. Madsen, M.C. Malin, S. McLennan, H.Y. McSween, D. Ming, J. Moersch, R.V. Morris, T. Parker, J. Rice, L. Richter, R. Rieder, D.S. Rodionov, C. Schroder, M. Sims, M. Smith, P. Smith, Laurence Soderblom, R. Sullivan, S.D. Thompson, N.J. Tosca, A. Wang, H. Wänke, J. Ward, T. Wdowiak, M. Wolff, A. Yen
Science and Products
Filter Total Items: 137
Dunes on Titan observed by Cassini Radar Dunes on Titan observed by Cassini Radar
Thousands of longitudinal dunes have recently been discovered by the Titan Radar Mapper on the surface of Titan. These are found mainly within ±30° of the equator in optically-, near-infrared-, and radar-dark regions, indicating a strong proportion of organics, and cover well over 5% of Titan's surface. Their longitudinal duneform, interactions with topography, and correlation with other...
Authors
J. Radebaugh, R. Lorenz, J. I. Lunine, S. Wall, G. Boubin, E. Reffet, Randolph Kirk, R.M. Lopes, E. Stofan, Laurence Soderblom, M. Allison, M. Janssen, P. Paillou, P. Callahan, Carl Spencer
Correlations between Cassini VIMS spectra and RADAR SAR images: Implications for Titan's surface composition and the character of the Huygens Probe Landing Site Correlations between Cassini VIMS spectra and RADAR SAR images: Implications for Titan's surface composition and the character of the Huygens Probe Landing Site
Titan's vast equatorial fields of RADAR-dark longitudinal dunes seen in Cassini RADAR synthetic aperture images correlate with one of two dark surface units discriminated as “brown” and “blue” in Visible and Infrared Mapping Spectrometer (VIMS) color composites of short-wavelength infrared spectral cubes (RGB as 2.0, 1.6, 1.3 μm). In such composites bluer materials exhibit higher...
Authors
Laurence Soderblom, Randolph Kirk, Jonathan Lunine, Jeffrey Anderson, Kevin Baines, Jason Barnes, Janet Barrett, Robert Brown, Bonnie Buratti, Roger Clark, Dale Cruikshank, Charles Elachi, Michael Janssen, Ralf Jaumann, Erich Karkoschka, Stéphane Le Mouélic, Rosaly Lopes, Ralph Lorenz, Thomas McCord, Philip Nicholson, Jani Radebaugh, Bashar Rizk, Christophe Sotin, Ellen Stofan, Tracie Sucharski, Martin Tomasko, Stephen Wall
Cryovolcanic features on Titan's surface as revealed by the Cassini Titan Radar Mapper Cryovolcanic features on Titan's surface as revealed by the Cassini Titan Radar Mapper
The Cassini Titan Radar Mapper obtained Synthetic Aperture Radar images of Titan's surface during four fly-bys during the mission's first year. These images show that Titan's surface is very complex geologically, showing evidence of major planetary geologic processes, including cryovolcanism. This paper discusses the variety of cryovolcanic features identified from SAR images, their...
Authors
Rosaly Lopes, K. Mitchell, Ellen Stofan, Jonathan Lunine, Ralf Lorenz, F. Paganelli, Randolph Kirk, C. Wood, Stephen Wall, L.E. Robshaw, A.D. Fortes, Catherine Neish, Jani Radebaugh, E. Reffet, S.J. Ostro, Charles Elachi, M.D. Allison, Y. Anderson, R. Boehmer, G. Boubin, Philip Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, Michael Janssen, W.T.K. Johnson, K. Kelleher, D.O. Muhleman, G. Ori, R. Orosei, G. Picardi, F. Posa, L.E. Roth, R. Seu, S. Shaffer, Laurence Soderblom, B. Stiles, S. Vetrella, R.D. West, L. Wye, H. A. Zebker
Near-infrared spectral mapping of Titan's mountains and channels Near-infrared spectral mapping of Titan's mountains and channels
We investigate the spectral reflectance properties of channels and mountain ranges on Titan using data from Cassini's Visual and Infrared Mapping Spectrometer (VIMS) obtained during the T9 encounter (26 December 2005). We identify the location of channels and mountains using synthetic aperture radar maps obtained from Cassini's RADAR instrument during the T13 (30 April 2006) flyby...
Authors
Jason Barnes, Jani Radebaugh, Robert Brown, Steve Wall, Laurence Soderblom, Jonathan Lunine, Devon Burr, Christophe Sotin, Stephane Le Mouelic, Sebastien Rodriguez, Bonnie Buratti, Roger Clark, Kevin Baines, Ralf Jaumann, Philip Nicholson, Randolph Kirk, Rosaly Lopes, Ralph Lorenz, Ken Mitchell, Charles Wood
Topography and geomorphology of the Huygens landing site on Titan Topography and geomorphology of the Huygens landing site on Titan
The Descent Imager/Spectral Radiometer (DISR) aboard the Huygens Probe took several hundred visible-light images with its three cameras on approach to the surface of Titan. Several sets of stereo image pairs were collected during the descent. The digital terrain models constructed from those images show rugged topography, in places approaching the angle of repose, adjacent to flatter...
Authors
Laurence Soderblom, Martin Tomasko, Brent Archinal, Tammy Becker, Michael Bushroe, Debbie Cook, Lyn Doose, Donna Galuszka, Trent Hare, Elpitha Howington-Kraus, Erich Karkoschka, Randolph Kirk, Jonathan Lunine, Elisabeth McFarlane, Bonnie Redding, Bashar Rizk, Mark Rosiek, Charles See, Peter Smith
The lakes of Titan The lakes of Titan
The surface of Saturn’s haze-shrouded moon Titan has long been proposed to have oceans or lakes, on the basis of the stability of liquid methane at the surface1,2. Initial visible3 and radar4,5 imaging failed to find any evidence of an ocean, although abundant evidence was found that flowing liquids have existed on the surface5,6. Here we provide definitive evidence for the presence of...
Authors
Ellen Stofan, Charles Elachi, Jonathan Lunine, Ralf Lorenz, B. Stiles, K. Mitchell, S. Ostro, Laurence Soderblom, C. Wood, H. Zebker, S. Wall, Michael Janssen, Randolph Kirk, Rosaly Lopes, F. Paganelli, Jani Radebaugh, L. Wye, Y. Anderson, M. Allison, R. Boehmer, P. Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, W.T.K. Johnson, K. Kelleher, D. Muhleman, Philipe Paillou, G. Picardi, F. Posa, L. Roth, R. Seu, S. Shaffer, S. Vetrella, R. West
Advanced technologies demonstrated by the miniature integrated camera and spectrometer (MICAS) aboard deep space 1 Advanced technologies demonstrated by the miniature integrated camera and spectrometer (MICAS) aboard deep space 1
MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80-185 nm), two high-resolution visible imagers (10-20 ??rad/pixel, 400-900 nm), and a short-wavelength infrared imaging spectrometer (1250-2600 nm). The wavelength ranges were chosen to maximize the science data that could be collected using existing semiconductor technologies and avoiding...
Authors
D.H. Rodgers, P.M. Beauchamp, L.A. Soderblom, R. Brown, G.-S. Chen, M. Lee, B.R. Sandel, D.A. Thomas, R.T. Benoit, R.V. Yelle
Pyroclastic activity at home plate in Gusev crater, Mars Pyroclastic activity at home plate in Gusev crater, Mars
Home Plate is a layered plateau in Gusev crater on Mars. It is composed of clastic rocks of moderately altered alkali basalt composition, enriched in some highly volatile elements. A coarse-grained lower unit lies under a finer-grained upper unit. Textural observations indicate that the lower strata were emplaced in an explosive event, and geochemical considerations favor an explosive...
Authors
S. Squyres, O. Aharonson, B.C. Clark, B. Cohen, L. Crumpler, P.A. de Souza, W. Farrand, Ralf Gellert, J. Grant, J.P. Grotzinger, A. Haldemann, J. Johnson, G. Klingelhofer, K.W. Lewis, R. Li, T. McCoy, A. McEwen, H.Y. McSween, D. Ming, Johnnie Moore, R.V. Morris, T. Parker, J. Rice, S. Ruff, M. Schmidt, C. Schroder, L.A. Soderblom, A. Yen
Comparison of the dust distributions in the innermost comae of comets-1P/Halley and 19P/Borrelly spacecraft observations Comparison of the dust distributions in the innermost comae of comets-1P/Halley and 19P/Borrelly spacecraft observations
We present a comparative study of the inner comae of comets 1P/Halley and 19P/Borrelly using data from the Halley Multicolour Camera (HMC) onboard Giotto and the Miniature Integrated Camera and Spectrometer onboard Deep Space 1 (DS1). We show that the dust brightness dependence as a function of radial distance is different for both comets. We suggest that optical depth or fragmentation...
Authors
T.-M. Ho, N. Thomas, D. Boice, M. Combi, L.A. Soderblom, V. Tenishev
Overview of the Opportunity Mars Exploration Rover Mission to Meridiani Planum: Eagle Crater to Purgatory Ripple Overview of the Opportunity Mars Exploration Rover Mission to Meridiani Planum: Eagle Crater to Purgatory Ripple
The Mars Exploration Rover Opportunity touched down at Meridiani Planum in January 2004 and since then has been conducting observations with the Athena science payload. The rover has traversed more than 5 km, carrying out the first outcrop‐scale investigation of sedimentary rocks on Mars. The rocks of Meridiani Planum are sandstones formed by eolian and aqueous reworking of sand grains...
Authors
S. Squyres, R. E. Arvidson, D. Bollen, J.F. Bell, J. Bruckner, N.A. Cabrol, W. Calvin, M. Carr, P. Christensen, B.C. Clark, L. Crumpler, D.J. Des Marais, C. D'Uston, T. Economou, J. Farmer, W.H. Farrand, W. Folkner, R. Gellert, T.D. Glotch, M. Golombek, S. Gorevan, J. Grant, R. Greeley, J. Grotzinger, Kenneth Herkenhoff, S. Hviid, J. Johnson, G. Klingelhoefer, A.H. Knoll, G. Landis, M. Lemmon, Ron Li, M.B. Madsen, M.C. Malin, S. McLennan, H.Y. McSween, D. Ming, J. Moersch, R.V. Morris, T. Parker, J. Rice, L. Richter, R. Rieder, C. Schroeder, M. Sims, M. Smith, P. Smith, Laurence Soderblom, R. Sullivan, N.J. Tosca, H. Wänke, T. Wdowiak, M. Wolff, A. Yen
Overview of the Microscopic Imager Investigation during Spirit's first 450 sols in Gusev crater Overview of the Microscopic Imager Investigation during Spirit's first 450 sols in Gusev crater
The Microscopic Imager (MI) on the Mars Exploration Rover Spirit has returned images of Mars with higher resolution than any previous camera system, allowing detailed petrographic and sedimentological studies of the rocks and soils at the Gusev landing site. Designed to simulate a geologist's hand lens, the MI is mounted on Spirit's instrument arm and can resolve objects 0.1 mm in size...
Authors
Kenneth Herkenhoff, Steve Squyres, Robert Anderson, Brent Archinal, Raymond Arvidson, Janet Barrett, Kris Becker, James F. Bell, Charles Budney, Nathalie Cabrol, Mary Chapman, Debbie Cook, Bethany Ehlmann, Jack Farmer, Brenda Franklin, Lisa Gaddis, Donna Galuszka, Patricia Garcia, Trent Hare, Elpitha Howington-Kraus, Jeffrey Johnson, Sarah Johnson, Kjartan M Kinch, Randolph Kirk, Ella M. Lee, Craig Leff, Mark Lemmon, Madsen B., Justin Maki, Kevin Mullins, Bonnie Redding, Lutz Richter, Mark Rosiek, Michael Sims, Laurence Soderblom, Nicole Spanovich, Richard Springer, Robert Sucharski, Tracie Sucharski, Robert Sullivan, James Torson, Albert Yen
Overview of the Spirit Mars Exploration Rover mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills Overview of the Spirit Mars Exploration Rover mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills
Spirit landed on the floor of Gusev Crater and conducted initial operations on soil‐covered, rock‐strewn cratered plains underlain by olivine‐bearing basalts. Plains surface rocks are covered by wind‐blown dust and show evidence for surface enrichment of soluble species as vein and void‐filling materials and coatings. The surface enrichment is the result of a minor amount of transport...
Authors
R. E. Arvidson, S. Squyres, R. Anderson, J. Bell, D. Blaney, J. Bruckner, N.A. Cabrol, W. Calvin, M. Carr, P. Christensen, B.C. Clark, L. Crumpler, D. Des Marais, P.A. De Souza, C. D'Uston, T. Economou, J. Farmer, W. Farrand, W. Folkner, M. Golombek, S. Gorevan, J. Grant, R. Greeley, J. Grotzinger, E. Guinness, B.C. Hahn, L. Haskin, Kenneth Herkenhoff, J.A. Hurowitz, S. Hviid, J. Johnson, G. Klingelhoefer, A. Knoll, G. Landis, C. Leff, M. Lemmon, R. Li, M.B. Madsen, M.C. Malin, S. McLennan, H.Y. McSween, D. Ming, J. Moersch, R.V. Morris, T. Parker, J. Rice, L. Richter, R. Rieder, D.S. Rodionov, C. Schroder, M. Sims, M. Smith, P. Smith, Laurence Soderblom, R. Sullivan, S.D. Thompson, N.J. Tosca, A. Wang, H. Wänke, J. Ward, T. Wdowiak, M. Wolff, A. Yen