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
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
Evaluating planetary digital terrain models-The HRSC DTM test Evaluating planetary digital terrain models-The HRSC DTM test
The High Resolution Stereo Camera (HRSC) has been orbiting the planet Mars since January 2004 onboard the European Space Agency (ESA) Mars Express mission and delivers imagery which is being used for topographic mapping of the planet. The HRSC team has conducted a systematic inter-comparison of different alternatives for the production of high resolution digital terrain models (DTMs)...
Authors
C. Heipke, J. Oberst, J. Albertz, M. Attwenger, P. Dorninger, E. Dorrer, M. Ewe, S. Gehrke, K. Gwinner, H. Hirschmuller, J.R. Kim, Randolph Kirk, H. Mayer, Jan-Peter Muller, R. Rengarajan, M. Rentsch, R. Schmidt, F. Scholten, J. Shan, M. Spiegel, M. Wahlisch, G. Neukum
Titan's surface from Cassini RADAR SAR and high resolution radiometry data of the first five flybys Titan's surface from Cassini RADAR SAR and high resolution radiometry data of the first five flybys
The first five Titan flybys with Cassini's Synthetic Aperture RADAR (SAR) and radiometer are examined with emphasis on the calibration and interpretation of the high-resolution radiometry data acquired during the SAR mode (SAR-radiometry). Maps of the 2-cm wavelength brightness temperature are obtained coincident with the SAR swath imaging, with spatial resolution approaching 6 km. A...
Authors
F. Paganelli, Michael Janssen, B. Stiles, R. West, Ralf Lorenz, Jonathan Lunine, Stephen Wall, Philip Callahan, Rosaly Lopes, Ellen Stofan, Randolph Kirk, W.T.K. Johnson, L. Roth, Charles Elachi
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 and seas of Titan The lakes and seas of Titan
No abstract available.
Authors
Rosaly Lopes, Karl Mitchell, Stephen Wall, Giuseppe Mitri, Michael Janssen, Steven Ostro, Randolph Kirk, Alexander Hayes, Ellen Stofan, Jonathan Lunine, Ralph Lorenz, Charles Wood, Jani Radebaugh, Philipe Paillou, H. Zebker, Flora Paganelli
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
A closer look at water-related geologic activity on Mars A closer look at water-related geologic activity on Mars
Water has supposedly marked the surface of Mars and produced characteristic landforms. To understand the history of water on Mars, we take a close look at key locations with the High-Resolution Imaging Science Experiment on board the Mars Reconnaissance Orbiter, reaching fine spatial scales of 25 to 32 centimeters per pixel. Boulders ranging up to ∼2 meters in diameter are ubiquitous in...
Authors
Alfred McEwen, C.J. Hansen, W.A. Delamere, E. Eliason, Kenneth Herkenhoff, Laszlo P. Keszthelyi, V. Gulick, Randolph Kirk, M. Mellon, J. Grant, N. Thomas, C.M. Weitz, S. Squyres, N.T. Bridges, S.L. Murchie, F. Seelos, K. Seelos, C.H. Okubo, M.P. Milazzo, L.L. Tornabene, W.L. Jaeger, S. Byrne, P.S. Russell, J.L. Griffes, S. Martinez-Alonso, A. Davatzes, F. Chuang, B.J. Thomson, K.E. Fishbaugh, C. Dundas, K.J. Kolb, M. Banks, J.J. Wray
Mars reconnaissance orbiter's high resolution imaging science experiment (HiRISE) Mars reconnaissance orbiter's high resolution imaging science experiment (HiRISE)
The HiRISE camera features a 0.5 m diameter primary mirror, 12 m effective focal length, and a focal plane system that can acquire images containing up to 28 Gb (gigabits) of data in as little as 6 seconds. HiRISE will provide detailed images (0.25 to 1.3 m/pixel) covering ∼1% of the Martian surface during the 2‐year Primary Science Phase (PSP) beginning November 2006. Most images will...
Authors
Alfred McEwen, Eric Eliason, James Bergstrom, Nathan Bridges, Candice Hansen, W. Delamere, John Grant, Virginia Gulick, Kenneth Herkenhoff, Laszlo P. Keszthelyi, Randolph Kirk, Michael Mellon, Steven Squyres, Nicolas Thomas, Catherine Weitz
The Unified Lunar Control Network 2005 The Unified Lunar Control Network 2005
This report documents a new general unified lunar control network and lunar topographic model based on a combination of Clementine images and a previous network derived from Earth-based & Apollo photographs, and Mariner 10, & Galileo images. This photogrammetric network solution is the largest planetary control network ever completed. It includes the determination of the 3-D positions of...
Authors
Brent Archinal, Mark Rosiek, Randolph Kirk, Bonnie Redding
Topomapping of Mars with HRSC Images, ISIS, and a commercial stereo workstation Topomapping of Mars with HRSC Images, ISIS, and a commercial stereo workstation
We demonstrate that the freely available USGS planetary cartography software package ISIS and the commercial photogrammetric software SOCET SET jointly provide a complete environment for the processing of Mars Express High Resolution Stereo Camera (HRSC) images. Capabilities include bundle adjustment, automated production and interactive editing of stereo digital terrain models (DTMs)...
Authors
Randolph Kirk, Elpitha Howington-Kraus, Donna Galuszka, Bonnie Redding, Trent Hare
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
Titan Radar Mapper observations from Cassini's T3 fly-by Titan Radar Mapper observations from Cassini's T3 fly-by
Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of impact craters on the surface of Titan, networks of fluvial channels and surficial dark streaks that may be...
Authors
C. Elachi, S. Wall, M. Janssen, E. Stofan, R. Lopes, Randolph Kirk, R. Lorenz, J. Lunine, F. Paganelli, Laurence Soderblom, C. Wood, L. Wye, H. Zebker, Y. Anderson, S. Ostro, M. Allison, R. Boehmer, P. Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, W. Johnson, K. Kelleher, D. Muhleman, G. Picardi, F. Posa, L. Roth, R. Seu, S. Shaffer, B. Stiles, S. Vetrella, R. West
Science and Products
Filter Total Items: 165
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
Evaluating planetary digital terrain models-The HRSC DTM test Evaluating planetary digital terrain models-The HRSC DTM test
The High Resolution Stereo Camera (HRSC) has been orbiting the planet Mars since January 2004 onboard the European Space Agency (ESA) Mars Express mission and delivers imagery which is being used for topographic mapping of the planet. The HRSC team has conducted a systematic inter-comparison of different alternatives for the production of high resolution digital terrain models (DTMs)...
Authors
C. Heipke, J. Oberst, J. Albertz, M. Attwenger, P. Dorninger, E. Dorrer, M. Ewe, S. Gehrke, K. Gwinner, H. Hirschmuller, J.R. Kim, Randolph Kirk, H. Mayer, Jan-Peter Muller, R. Rengarajan, M. Rentsch, R. Schmidt, F. Scholten, J. Shan, M. Spiegel, M. Wahlisch, G. Neukum
Titan's surface from Cassini RADAR SAR and high resolution radiometry data of the first five flybys Titan's surface from Cassini RADAR SAR and high resolution radiometry data of the first five flybys
The first five Titan flybys with Cassini's Synthetic Aperture RADAR (SAR) and radiometer are examined with emphasis on the calibration and interpretation of the high-resolution radiometry data acquired during the SAR mode (SAR-radiometry). Maps of the 2-cm wavelength brightness temperature are obtained coincident with the SAR swath imaging, with spatial resolution approaching 6 km. A...
Authors
F. Paganelli, Michael Janssen, B. Stiles, R. West, Ralf Lorenz, Jonathan Lunine, Stephen Wall, Philip Callahan, Rosaly Lopes, Ellen Stofan, Randolph Kirk, W.T.K. Johnson, L. Roth, Charles Elachi
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 and seas of Titan The lakes and seas of Titan
No abstract available.
Authors
Rosaly Lopes, Karl Mitchell, Stephen Wall, Giuseppe Mitri, Michael Janssen, Steven Ostro, Randolph Kirk, Alexander Hayes, Ellen Stofan, Jonathan Lunine, Ralph Lorenz, Charles Wood, Jani Radebaugh, Philipe Paillou, H. Zebker, Flora Paganelli
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
A closer look at water-related geologic activity on Mars A closer look at water-related geologic activity on Mars
Water has supposedly marked the surface of Mars and produced characteristic landforms. To understand the history of water on Mars, we take a close look at key locations with the High-Resolution Imaging Science Experiment on board the Mars Reconnaissance Orbiter, reaching fine spatial scales of 25 to 32 centimeters per pixel. Boulders ranging up to ∼2 meters in diameter are ubiquitous in...
Authors
Alfred McEwen, C.J. Hansen, W.A. Delamere, E. Eliason, Kenneth Herkenhoff, Laszlo P. Keszthelyi, V. Gulick, Randolph Kirk, M. Mellon, J. Grant, N. Thomas, C.M. Weitz, S. Squyres, N.T. Bridges, S.L. Murchie, F. Seelos, K. Seelos, C.H. Okubo, M.P. Milazzo, L.L. Tornabene, W.L. Jaeger, S. Byrne, P.S. Russell, J.L. Griffes, S. Martinez-Alonso, A. Davatzes, F. Chuang, B.J. Thomson, K.E. Fishbaugh, C. Dundas, K.J. Kolb, M. Banks, J.J. Wray
Mars reconnaissance orbiter's high resolution imaging science experiment (HiRISE) Mars reconnaissance orbiter's high resolution imaging science experiment (HiRISE)
The HiRISE camera features a 0.5 m diameter primary mirror, 12 m effective focal length, and a focal plane system that can acquire images containing up to 28 Gb (gigabits) of data in as little as 6 seconds. HiRISE will provide detailed images (0.25 to 1.3 m/pixel) covering ∼1% of the Martian surface during the 2‐year Primary Science Phase (PSP) beginning November 2006. Most images will...
Authors
Alfred McEwen, Eric Eliason, James Bergstrom, Nathan Bridges, Candice Hansen, W. Delamere, John Grant, Virginia Gulick, Kenneth Herkenhoff, Laszlo P. Keszthelyi, Randolph Kirk, Michael Mellon, Steven Squyres, Nicolas Thomas, Catherine Weitz
The Unified Lunar Control Network 2005 The Unified Lunar Control Network 2005
This report documents a new general unified lunar control network and lunar topographic model based on a combination of Clementine images and a previous network derived from Earth-based & Apollo photographs, and Mariner 10, & Galileo images. This photogrammetric network solution is the largest planetary control network ever completed. It includes the determination of the 3-D positions of...
Authors
Brent Archinal, Mark Rosiek, Randolph Kirk, Bonnie Redding
Topomapping of Mars with HRSC Images, ISIS, and a commercial stereo workstation Topomapping of Mars with HRSC Images, ISIS, and a commercial stereo workstation
We demonstrate that the freely available USGS planetary cartography software package ISIS and the commercial photogrammetric software SOCET SET jointly provide a complete environment for the processing of Mars Express High Resolution Stereo Camera (HRSC) images. Capabilities include bundle adjustment, automated production and interactive editing of stereo digital terrain models (DTMs)...
Authors
Randolph Kirk, Elpitha Howington-Kraus, Donna Galuszka, Bonnie Redding, Trent Hare
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
Titan Radar Mapper observations from Cassini's T3 fly-by Titan Radar Mapper observations from Cassini's T3 fly-by
Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of impact craters on the surface of Titan, networks of fluvial channels and surficial dark streaks that may be...
Authors
C. Elachi, S. Wall, M. Janssen, E. Stofan, R. Lopes, Randolph Kirk, R. Lorenz, J. Lunine, F. Paganelli, Laurence Soderblom, C. Wood, L. Wye, H. Zebker, Y. Anderson, S. Ostro, M. Allison, R. Boehmer, P. Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, W. Johnson, K. Kelleher, D. Muhleman, G. Picardi, F. Posa, L. Roth, R. Seu, S. Shaffer, B. Stiles, S. Vetrella, R. West