Randolph L Kirk, Ph.D.
Randolph Kirk’s research interests span both geoscience and mapping of planetary bodies. He has participated in many missions to the Moon, Venus, Mars, asteroids, comets, and icy satellites. He helped direct planetary mapping at the USGS since the early 1990s, and has developed practical methods for topomapping by shape from shading and by adapting commercial stereo workstations to planetary use.
Recent Accomplishments
- In 2020, NASA's Mars 2020 rover Perseverance landed in Jezero crater at a site mapped by the Astrogeology Science Center. Perseverence was the ninth Mars lander or rover to go to a site we mapped, all of which landed successfully. (Starting in 1962, 10 Mars landings attempted without USGS mapping failed for a variety of reasons. Just days before Perseverence the Chinese landerTianwen-1 became the first such mission to succeed.) Perseverance also carried our maps onboard and used them to guide its final descent, a technological first.
- We are helping to design and caibrate the Europa Imaging System (EIS) cameras for NASA's Europa Clipper mission and to develop software and procedures for making controlled image and topographic maps. As part of this task, we invented and demonstrated a new technique for correcting distortions in frame images that are read out line-by-line so that they can be used for precision mapping.
- We have used stereo images of Mars obtained by different cameras with pixel scales differing up to 50x to assess the resolution and precision of digital topographic models obtained under real-world (Mars) conditions. We are currently using similar techniques with images of Earth’s Moon to quantify how topographic models can be improved by photoclinometry (shape from shading) techniques using one or multiple images.
Education
- Ph.D., Planetary Science, Minor in Physics, California Institute of Technology, January 1987
- M.S., Planetary Science, California Institute of Technology, June 1984
- B.S., Physics, Stanford University, June 1981
Space Mission Participation
- Member, Europa Imaging System Science Team, May 2015–Present
- Member, ExoMars Trace Gas Orbiter CaSSIS Science Team, August 2010–Present
- Member, LRO and Chandrayaan-1 Mini-RF Science Teams, July 2006–Present
- Member, Mars Reconnaissance Orbiter HiRISE Science Team, December 2001–Present
- Member, Mars Exploration Rovers Science Team, August 2000–June 2018
- Associate, Deep Space 1 MICAS Science Team, March 2000–December 2002
- Participating Scientist, NEAR MSI/NIS Team, August 1999–July 2001
- Associate, Imager for Mars Pathfinder Science Team, July 1996–August 1998
- Member, Mars Express HRSC Science Team, January 2000–March 2020
- Associate, Mars 96 HRSC/WAOSS Science Team, March 1993–December 1996
- Member, Cassini RADAR Instrument Team, December 1990–September 2018
- Magellan Guest Investigator, October 1990–September 1994
- Associate, Voyager Imaging Science Team, 1989
Working Groups
- Member, IAU Working Group on Cartographic Coords & Rotational Elements, August 2012–present
- Member, NASA Lunar Geodesy/Cartography Working Group, December 2007–present
- Member, NASA Mars Geodesy/Cartography Working Group, June 1998–present
- Member, ISPRS Working Group “Planetary Mapping & Remote Sensing”, November 1996–present
- Chair, November 2000-October 2004, Co-Chair, Nove
Science and Products
Filter Total Items: 165
Digital mapping of the Mars Pathfinder landing site: Design, acquisition, and derivation of cartographic products for science applications Digital mapping of the Mars Pathfinder landing site: Design, acquisition, and derivation of cartographic products for science applications
The Imager for Mars Pathfinder (IMP) acquired more than 16,000 images and provided panoramic views of the surface of Mars at the Mars Pathfinder landing site in Ares Vallis. This paper describes the stereoscopic, multispectral IMP imaging sequences and focuses on their use for digital mapping of the landing site and for deriving cartographic products to support science applications of...
Authors
Lisa R. Gaddis, Randolph L. Kirk, J. R. Johnson, Laurence A. Soderblom, A. W. Ward, J. Barrett, Kris J. Becker, Tammy L. Becker, J. Blue, D. Cook, E. Eliason, Trent M. Hare, Elpitha Howington-Kraus, C. Isbell, E.M. Lee, Bonnie L. Redding, Robert M. Sucharski, Tracie L. Sucharski, P. H. Smith, D.T. Britt
Grooved Terrain on Ganymede: First Results from Galileo High-Resolution Imaging Grooved Terrain on Ganymede: First Results from Galileo High-Resolution Imaging
High-resolution Galileo imaging has provided important insight into the origin and evolution of grooved terrain on Ganymede. The Uruk Sulcus target site was the first imaged at high resolution, and considerations of resolution, viewing geometry, low image compression, and complementary stereo imaging make this region extremely informative. Contrast variations in these low-incidence angle...
Authors
Robert T. Pappalardo, James W. Head, Geoffrey C. Collins, Randolph L. Kirk, Gerhard Neukum, Jurgen Oberst, Bernd Giese, Ronald Greeley, Clark R. Chapman, Paul Helfenstein, Jeffrey M. Moore, Alfred S. McEwen, B. Randy Tufts, David A. Senske, H. Herbert Breneman, Kenneth P. Klaasen
Large impact features on Europa: Results of the Galileo Nominal Mission Large impact features on Europa: Results of the Galileo Nominal Mission
The Galileo Orbiter examined several impact features on Europa at considerably better resolution than was possible from Voyager. The new data allow us to describe the morphology and infer the geology of the largest impact features on Europa, which are probes into the crust. We observe two basic types of large impact features: (1) “classic” impact craters that grossly resemble well...
Authors
Jeffrey M. Moore, Erik Asphaug, Robert J. Sullivan, James E. Klemaszewski, Kelly C. Bender, Ronald Greeley, Paul E. Geissler, Alfred S. McEwen, Elizabeth P. Turtle, Cynthia B. Phillips, B. Randy Tufts, James W. Head, Robert T. Pappalardo, Kevin B. Jones, Clark R. Chapman, Michael J.S. Belton, Randolph L. Kirk, David Morrison
Results from the Mars Pathfinder camera Results from the Mars Pathfinder camera
Images of the martian surface returned by the Imager for Mars Pathfinder (IMP) show a complex surface of ridges and troughs covered by rocks that have been transported and modified by fluvial, aeolian, and impact processes. Analysis of the spectral signatures in the scene (at 440- to 1000-nanometer wavelength) reveal three types of rock and four classes of soil. Upward-looking IMP images...
Authors
P. H. Smith, J. F. Bell, N. T. Bridges, D.T. Britt, Lisa R. Gaddis, R. Greeley, H.U. Keller, Kenneth E. Herkenhoff, R. Jaumann, J. R. Johnson, Randolph L. Kirk, M. Lemmon, J.N. Maki, M.C. Malin, S.L. Murchie, J. Oberst, T. J. Parker, R.J. Reid, R.M. Sablotny, Laurence A. Soderblom, C. Stoker, R. Sullivan, N. Thomas, M.G. Tomasko, W. Ward, E. Wegryn
Radar reflectivities of plausible Titan surfaces Radar reflectivities of plausible Titan surfaces
We consider plausible reflectivity ranges for candidate Titan surfaces, with application to radar altimeter investigations on both the Cassini Orbiter and Huygens Probe. The appropriate measure of surface scattering is the specific backscatter cross-section at normal incidence or, for smooth surfaces, the specific backscatter averaged over the sensitivity of the altimeter beam pattern. A...
Authors
Randolph L. Kirk, J. I. Lunine
The imager for Mars Pathfinder experiment The imager for Mars Pathfinder experiment
The imager for Mars Pathfinder (IMP), a stereoscopic, multispectral camera, is described in terms of its capabilities for studying the Martian environment. The camera's two eyes, separated by 15.0 cm, provide the camera with range‐finding ability. Each eye illuminates half of a single CCD detector with a field of view of 14.4×14.0° and has 12 selectable filters. The ƒ/18 optics have a...
Authors
P. H. Smith, M.G. Tomasko, D. Britt, D.G. Crowe, R. Reid, H.U. Keller, N. Thomas, F. Gliem, P. Rueffer, R. Sullivan, R. Greeley, J. M. Knudsen, M.B. Madsen, H.P. Gunnlaugsson, S.F. Hviid, W. Goetz, Laurence A. Soderblom, L. Gaddis, Randolph L. Kirk
Physiography, Geomorphic/geologic Mapping and Stratigraphy of Venus Physiography, Geomorphic/geologic Mapping and Stratigraphy of Venus
No abstract available.
Authors
K. L. Tanaka, D.A. Senske, M. Price, Randolph L. Kirk
The Topography of Asteroid Ida: A Comparison between Photogrammetric and ShapeForm-Shading Image Analysis The Topography of Asteroid Ida: A Comparison between Photogrammetric and ShapeForm-Shading Image Analysis
We derived high resolution Digital Terrain Models from stereo images of the asteroid Ida that were obtained by the Galileo spacecraft during the flyby in August 1993 and compared these results with terrain models derived from two-dimensional photoclinometry. The comparison shows that there are striking discrepancies between the results from the two models depending on the spatial scale...
Authors
Bernd Giese, Juergen Oberst, Randolph L. Kirk, W. Zeitler
Data base of impact craters on Venus based on analysis of Magellan radar images and altimetry data Data base of impact craters on Venus based on analysis of Magellan radar images and altimetry data
No abstract available.
Authors
Gerald G. Schaber, Randolph L. Kirk, Robert G. Strom
A migratory mantle plume on Venus: Implications for Earth? A migratory mantle plume on Venus: Implications for Earth?
A spatially fixed or at least internally rigid hotspot reference frame has been assumed for determining relative plate motions on Earth. Recent 1:5,000,000 scale mapping of Venus, a planet without terrestrial-style plate tectonics and ocean cover, reveals a systematic age and dimensional progression of corona-like arachnoids occurring in an uncinate chain. The nonrandom associations...
Authors
Mary G. Chapman, Randolph L. Kirk
Geology of 243 Ida Geology of 243 Ida
The surface of 243 Ida is dominated by the effects of impacts. No complex crater morphologies are observed. A complete range of crater degradation states is present, which also reveals optical maturation of the surface (darkening and reddening of materials with increasing exposure age). Regions of bright material associated with the freshest craters might be ballistically emplaced...
Authors
R. Sullivan, R. Greeley, R. Pappalardo, E. Asphaug, Johnnie N. Moore, D. Morrison, M. J. S. Belton, M. Carr, C. R. Chapman, Paul E. Geissler, R. Greenberg, J. Granahan, J. W. Head, Randolph L. Kirk, A. McEwen, P. Lee, P.C. Thomas, J. Veverka
Science and Products
Filter Total Items: 165
Digital mapping of the Mars Pathfinder landing site: Design, acquisition, and derivation of cartographic products for science applications Digital mapping of the Mars Pathfinder landing site: Design, acquisition, and derivation of cartographic products for science applications
The Imager for Mars Pathfinder (IMP) acquired more than 16,000 images and provided panoramic views of the surface of Mars at the Mars Pathfinder landing site in Ares Vallis. This paper describes the stereoscopic, multispectral IMP imaging sequences and focuses on their use for digital mapping of the landing site and for deriving cartographic products to support science applications of...
Authors
Lisa R. Gaddis, Randolph L. Kirk, J. R. Johnson, Laurence A. Soderblom, A. W. Ward, J. Barrett, Kris J. Becker, Tammy L. Becker, J. Blue, D. Cook, E. Eliason, Trent M. Hare, Elpitha Howington-Kraus, C. Isbell, E.M. Lee, Bonnie L. Redding, Robert M. Sucharski, Tracie L. Sucharski, P. H. Smith, D.T. Britt
Grooved Terrain on Ganymede: First Results from Galileo High-Resolution Imaging Grooved Terrain on Ganymede: First Results from Galileo High-Resolution Imaging
High-resolution Galileo imaging has provided important insight into the origin and evolution of grooved terrain on Ganymede. The Uruk Sulcus target site was the first imaged at high resolution, and considerations of resolution, viewing geometry, low image compression, and complementary stereo imaging make this region extremely informative. Contrast variations in these low-incidence angle...
Authors
Robert T. Pappalardo, James W. Head, Geoffrey C. Collins, Randolph L. Kirk, Gerhard Neukum, Jurgen Oberst, Bernd Giese, Ronald Greeley, Clark R. Chapman, Paul Helfenstein, Jeffrey M. Moore, Alfred S. McEwen, B. Randy Tufts, David A. Senske, H. Herbert Breneman, Kenneth P. Klaasen
Large impact features on Europa: Results of the Galileo Nominal Mission Large impact features on Europa: Results of the Galileo Nominal Mission
The Galileo Orbiter examined several impact features on Europa at considerably better resolution than was possible from Voyager. The new data allow us to describe the morphology and infer the geology of the largest impact features on Europa, which are probes into the crust. We observe two basic types of large impact features: (1) “classic” impact craters that grossly resemble well...
Authors
Jeffrey M. Moore, Erik Asphaug, Robert J. Sullivan, James E. Klemaszewski, Kelly C. Bender, Ronald Greeley, Paul E. Geissler, Alfred S. McEwen, Elizabeth P. Turtle, Cynthia B. Phillips, B. Randy Tufts, James W. Head, Robert T. Pappalardo, Kevin B. Jones, Clark R. Chapman, Michael J.S. Belton, Randolph L. Kirk, David Morrison
Results from the Mars Pathfinder camera Results from the Mars Pathfinder camera
Images of the martian surface returned by the Imager for Mars Pathfinder (IMP) show a complex surface of ridges and troughs covered by rocks that have been transported and modified by fluvial, aeolian, and impact processes. Analysis of the spectral signatures in the scene (at 440- to 1000-nanometer wavelength) reveal three types of rock and four classes of soil. Upward-looking IMP images...
Authors
P. H. Smith, J. F. Bell, N. T. Bridges, D.T. Britt, Lisa R. Gaddis, R. Greeley, H.U. Keller, Kenneth E. Herkenhoff, R. Jaumann, J. R. Johnson, Randolph L. Kirk, M. Lemmon, J.N. Maki, M.C. Malin, S.L. Murchie, J. Oberst, T. J. Parker, R.J. Reid, R.M. Sablotny, Laurence A. Soderblom, C. Stoker, R. Sullivan, N. Thomas, M.G. Tomasko, W. Ward, E. Wegryn
Radar reflectivities of plausible Titan surfaces Radar reflectivities of plausible Titan surfaces
We consider plausible reflectivity ranges for candidate Titan surfaces, with application to radar altimeter investigations on both the Cassini Orbiter and Huygens Probe. The appropriate measure of surface scattering is the specific backscatter cross-section at normal incidence or, for smooth surfaces, the specific backscatter averaged over the sensitivity of the altimeter beam pattern. A...
Authors
Randolph L. Kirk, J. I. Lunine
The imager for Mars Pathfinder experiment The imager for Mars Pathfinder experiment
The imager for Mars Pathfinder (IMP), a stereoscopic, multispectral camera, is described in terms of its capabilities for studying the Martian environment. The camera's two eyes, separated by 15.0 cm, provide the camera with range‐finding ability. Each eye illuminates half of a single CCD detector with a field of view of 14.4×14.0° and has 12 selectable filters. The ƒ/18 optics have a...
Authors
P. H. Smith, M.G. Tomasko, D. Britt, D.G. Crowe, R. Reid, H.U. Keller, N. Thomas, F. Gliem, P. Rueffer, R. Sullivan, R. Greeley, J. M. Knudsen, M.B. Madsen, H.P. Gunnlaugsson, S.F. Hviid, W. Goetz, Laurence A. Soderblom, L. Gaddis, Randolph L. Kirk
Physiography, Geomorphic/geologic Mapping and Stratigraphy of Venus Physiography, Geomorphic/geologic Mapping and Stratigraphy of Venus
No abstract available.
Authors
K. L. Tanaka, D.A. Senske, M. Price, Randolph L. Kirk
The Topography of Asteroid Ida: A Comparison between Photogrammetric and ShapeForm-Shading Image Analysis The Topography of Asteroid Ida: A Comparison between Photogrammetric and ShapeForm-Shading Image Analysis
We derived high resolution Digital Terrain Models from stereo images of the asteroid Ida that were obtained by the Galileo spacecraft during the flyby in August 1993 and compared these results with terrain models derived from two-dimensional photoclinometry. The comparison shows that there are striking discrepancies between the results from the two models depending on the spatial scale...
Authors
Bernd Giese, Juergen Oberst, Randolph L. Kirk, W. Zeitler
Data base of impact craters on Venus based on analysis of Magellan radar images and altimetry data Data base of impact craters on Venus based on analysis of Magellan radar images and altimetry data
No abstract available.
Authors
Gerald G. Schaber, Randolph L. Kirk, Robert G. Strom
A migratory mantle plume on Venus: Implications for Earth? A migratory mantle plume on Venus: Implications for Earth?
A spatially fixed or at least internally rigid hotspot reference frame has been assumed for determining relative plate motions on Earth. Recent 1:5,000,000 scale mapping of Venus, a planet without terrestrial-style plate tectonics and ocean cover, reveals a systematic age and dimensional progression of corona-like arachnoids occurring in an uncinate chain. The nonrandom associations...
Authors
Mary G. Chapman, Randolph L. Kirk
Geology of 243 Ida Geology of 243 Ida
The surface of 243 Ida is dominated by the effects of impacts. No complex crater morphologies are observed. A complete range of crater degradation states is present, which also reveals optical maturation of the surface (darkening and reddening of materials with increasing exposure age). Regions of bright material associated with the freshest craters might be ballistically emplaced...
Authors
R. Sullivan, R. Greeley, R. Pappalardo, E. Asphaug, Johnnie N. Moore, D. Morrison, M. J. S. Belton, M. Carr, C. R. Chapman, Paul E. Geissler, R. Greenberg, J. Granahan, J. W. Head, Randolph L. Kirk, A. McEwen, P. Lee, P.C. Thomas, J. Veverka