Colin Dundas, Ph.D.
Colin Dundas is a Research Geologist with the Astrogeology Science Center. He studies planetary geomorphology and surface processes using spacecraft imagery and topography data as well as numerical modeling, with a particular focus on active processes and change detection. He is a Co-Investigator and Science Theme Lead for Mass Wasting on the HiRISE camera team.
Past and current research areas include:
- Current activity on Martian slopes, including Recurring Slope Lineae and changes in gullies
- Martian ground ice, ice-exposing impact craters and scarps, and sublimation-thermokarst landforms
- Large lava flows and lava-volatile interactions on Mars, Io, and Earth
- Effects of target properties and secondary craters on crater chronology
- Floods in Martian outflow channels
- Volatile-loss landforms in the Solar System
Professional Experience
2009-2011: Postdoctoral researcher at the University of Arizona.
2011 - Present: Research Geologist at the USGS Astrogeology Science Center
Education and Certifications
Ph.D., Planetary Science (Geoscience minor), The University of Arizona, 2009
B.S., Planetary Science, California Institute of Technology, 2004
Science and Products
Filter Total Items: 77
New craters on Mars: An updated catalog
We present a catalog of new impacts on Mars. These craters formed in the last few decades, constrained with repeat orbital imaging. Crater diameters range from 58 m down to <1 m. For each impact, we report whether it formed a single crater or a cluster (58% clusters); albedo features of the blast zone (88% halos; 64% linear rays; 10% arcuate rays; majority dark-toned; 4% light-toned; 14% dual-tone
Authors
Ingrid J. Daubar, Colin M. Dundas, Alfred S. McEwen, Annabelle Gao, D. Wexler, Sylvain Piqueux, Gareth S. Collins, Katarina Miljkovic, T. Neidhart, J. Eschenfelder, Gwen D. Bart, Kiri L. Wagstaff, Gary Doran, Liliya Posiolova, Michael C. Malin, Gunnar Speth, David Susko, A. Werynski
Comparison of Digital Terrain Models from two photoclinometry methods
We evaluate the horizontal resolution and vertical precision for digital topographic models (DTMs) of the Moon derived from image radiance information, a process known as photoclinometry (PC) or shape-from-shading (SfS). We use the implementations in two available planetary image processing software systems, single image PC in the U.S. Geological Survey Integrated Software for Imagers and Spectrom
Authors
Randolph L. Kirk, David Mayer, Colin M. Dundas, Benjamin H Wheeler, Ross A. Beyer, Oleg Alexandrov
Revealing active Mars with HiRISE digital terrain models
Many discoveries of active surface processes on Mars have been made due to the availability of repeat high-resolution images from the High Resolution Imaging Science Experiment (HiRISE) onboard the Mars Reconnaissance Orbiter. HiRISE stereo images are used to make digital terrain models (DTMs) and orthorectified images (orthoimages). HiRISE DTMs and orthoimage time series have been crucial for adv
Authors
Sarah S. Sutton, Matthew Chojnacki, Alfred S. McEwen, Randolph L. Kirk, Colin M. Dundas, Ethan I Schaefer, Susan J. Conway, Serina Diniega, Ganna Portyankina, Margaret E. Landis, Nicole F Baugh, Rodney Heyd, Shane Byrne, Livio L. Tornabene, Lujendra Ojha, Christopher W. Hamilton
A numerical model for the cooling of a lava sill with heat pipe effects
Understanding the cooling process of volcanic intrusions into wet sediments is a difficult but important problem, given the presence of extremely large temperature gradients and potentially complex water-magma interactions. This report presents a numerical model to study such interactions, including the effect of heat pipes on the cooling of volcanic intrusions. Udell (1985) has shown that heat pi
Authors
Kaj E. Williams, Colin M. Dundas, Laszlo P. Kestay
Active Mars: A dynamic world
Mars exhibits diverse surface changes at all latitudes and all seasons. Active processes include impact cratering, aeolian sand and dust transport, a variety of slope processes, changes in polar ices, and diverse effects of seasonal CO2 frost. The extent of surface change has been surprising and indicates that the present climate is capable of reshaping the surface. Activity has important implicat
Authors
Colin M. Dundas, Patricio Becerra, Shane Byrne, Matthew Chojnacki, Ingrid J. Daubar, Serina Diniega, Candice J. Hansen, Kenneth E. Herkenhoff, Margaret E. Landis, Alfred S. McEwen, Ganna Portyankina, Adomas Valantinas
Introduction: Does water flow on Martian slopes?
No abstract available.
Authors
Colin M. Dundas, Susan J. Conway, David E Stillman
Dry formation of recent Martian slope features
Martian surface conditions are cold and dry, unfavorable for liquid water, yet steep slopes display young and currently active features suggestive of wet processes. These include recurring slope lineae and slope streaks, gully landforms, and small lobate features. Wet origins for these features would imply surprising amounts of liquid water at the surface. However, detailed observations of the mor
Authors
Colin M. Dundas
Mars science helicopter: Compelling science enabled by an aerial platform
This whitepaper describes two conceptual vehicle designs, including possible tradeoffs within those designs, which would enable a wide array of innovative science investigations. In addition to describing vehicle capabilities, flight characteristics, and the breadth of enabled science for the two helicopter designs, we also introduce three mission concepts that showcase investigations made possibl
Authors
Jonathan Bapst, Timothy J Parker, J Balaram, T Tzanetos, L. H. Matthies, C D Edwards, Aaron Freeman, S Withrow-Maser, W. Carter Johnson, E Amador-French, Janice L. Bishop, Ingrid J. Daubar, Colin M. Dundas, Abigail A. Fraeman, Christopher W. Hamilton, C. Hardgrove, Briony H. N. Horgan, C. W. Leung, Y. Lin, A Mittelholz, B. P. Weiss
GANGOTRI mission concept on the glacial key to the Amazonian climate of Mars
The GANGOTRI mission concept would investigate in situ the geologic origins of midlatitudinal Martian glaciers, as underlain by Amazonian climate evolution, by riddling the ice with a hybrid thermo-mechanical drill for deep englacial sampling. GANGOTRI would use regolith compositional measurements to characterize ice-regolith interaction, and stable isotope measurements to characterize fundamental
Authors
Suniti Karunatillake, Ali M Bramson, Kris Zacny, Colin M. Dundas, Lujendra Ojha, Oded Aharonson, Eran Vos, Don R Hood, A. Deanne Rogers, Joseph S. Levy, Peter Doran, Kathleen Mandt, Jack Wilson, Emily B Hughes, Heidi Fuqua-Haviland, Jeffrey Moersch, Scott M. Perl, Dewan E. Haque, J. R. Skok, Harish, S. Vijayan, A. Bhardwaj, Brent Christner, Hanna Sizemore, A Kereszturi, Norbert Schorghofer, Kurt Retherford, Paul Niles, Juan Manuel Lorenzo, Katherine Mesick, Heather Franz, Jose Rodriguez-Manfredi, Daniel Coupland, Peter Bertone
Current activity on the Martian surface: A key subject for future exploration
One of the fundamental discoveries in Mars science in the last decade has been the extent and importance of current surface activity. Recent results have shifted our view of Mars from a world where the most interesting geologic events were in the distant past (similar to the Moon) to a world that undergoes active evolution and one where understanding the present is key to deciphering the planet’s
Authors
Colin M. Dundas, Shane Byrne, Matthew Chojnacki, Serina Diniega, Ingrid J. Daubar, Christopher W. Hamilton, Candice J. Hansen, Alfred S. McEwen, Ganna Portyankina, Hanna G Sizemore
Mid-latitude ice on Mars: A science target for planetary climate histories and an exploration target for in situ resources
In the last decade, aided by the high-resolution data and long-term monitoring by NASA’s Mars Reconnaissance Orbiter (MRO) and other spacecraft, extensive evidence has emerged supporting the presence of abundant H2O ground ice throughout much of the mid-latitudes of Mars. Growing evidence indicates that much of this ice is relatively pure, exists within a few meters of the surface, and reaches low
Authors
Ali Bramson, Chimira Andres, Jonathan Bapst, Patricio Becerra, Samuel W Courville, Colin M. Dundas, Shannon M Hibbard, John W Holt, Suniti Karunatillake, Aditya Khuller, Michael T. Mellon, Gareth A Morgan, R. W. Obbard, Matthew R Perry, Eric I Petersen, Nathaniel E. Putzig, Hanna G Sizemore, Isaac B. Smith, David E Stillman, Paul Wooster
Maximizing the science and resource mapping potential of Orbital VSWIR Spectral measurements of Mars
The last 16 years witnessed a rapid growth in understanding the composition and aqueous alteration of Mars’ surface from orbital data from the Observatoire pour la Mineralogie, l’Eau, les Glaces et l’Activité (OMEGA) [1] and Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) [2]. Both are sensitive to water-, hydroxyl-, sulfate-, and carbonate-bearing and ferric phases that record past l
Authors
Scott L. Murchie, Raymond E. Arvidson, Janice L Bishop, Wendy M. Calvin, John Carter, John Christian, Roger N. Clark, Colin M. Dundas, Bethany L. Ehlmann, Valerie K. Fox, Abigail A. Fraeman, Timothy A Goudge, Briony H. N. Horgan, Madison N Hughes, Ellen K Leask, Alfred S. McEwen, John F Mustard, Mario Parente, Kathryn E Powell, Frank P. Seelos, Kimberly D. Seelos, Jesse D Tarnas, Christina E Viviano, James J. Wray
Science and Products
Filter Total Items: 77
New craters on Mars: An updated catalog
We present a catalog of new impacts on Mars. These craters formed in the last few decades, constrained with repeat orbital imaging. Crater diameters range from 58 m down to <1 m. For each impact, we report whether it formed a single crater or a cluster (58% clusters); albedo features of the blast zone (88% halos; 64% linear rays; 10% arcuate rays; majority dark-toned; 4% light-toned; 14% dual-tone
Authors
Ingrid J. Daubar, Colin M. Dundas, Alfred S. McEwen, Annabelle Gao, D. Wexler, Sylvain Piqueux, Gareth S. Collins, Katarina Miljkovic, T. Neidhart, J. Eschenfelder, Gwen D. Bart, Kiri L. Wagstaff, Gary Doran, Liliya Posiolova, Michael C. Malin, Gunnar Speth, David Susko, A. Werynski
Comparison of Digital Terrain Models from two photoclinometry methods
We evaluate the horizontal resolution and vertical precision for digital topographic models (DTMs) of the Moon derived from image radiance information, a process known as photoclinometry (PC) or shape-from-shading (SfS). We use the implementations in two available planetary image processing software systems, single image PC in the U.S. Geological Survey Integrated Software for Imagers and Spectrom
Authors
Randolph L. Kirk, David Mayer, Colin M. Dundas, Benjamin H Wheeler, Ross A. Beyer, Oleg Alexandrov
Revealing active Mars with HiRISE digital terrain models
Many discoveries of active surface processes on Mars have been made due to the availability of repeat high-resolution images from the High Resolution Imaging Science Experiment (HiRISE) onboard the Mars Reconnaissance Orbiter. HiRISE stereo images are used to make digital terrain models (DTMs) and orthorectified images (orthoimages). HiRISE DTMs and orthoimage time series have been crucial for adv
Authors
Sarah S. Sutton, Matthew Chojnacki, Alfred S. McEwen, Randolph L. Kirk, Colin M. Dundas, Ethan I Schaefer, Susan J. Conway, Serina Diniega, Ganna Portyankina, Margaret E. Landis, Nicole F Baugh, Rodney Heyd, Shane Byrne, Livio L. Tornabene, Lujendra Ojha, Christopher W. Hamilton
A numerical model for the cooling of a lava sill with heat pipe effects
Understanding the cooling process of volcanic intrusions into wet sediments is a difficult but important problem, given the presence of extremely large temperature gradients and potentially complex water-magma interactions. This report presents a numerical model to study such interactions, including the effect of heat pipes on the cooling of volcanic intrusions. Udell (1985) has shown that heat pi
Authors
Kaj E. Williams, Colin M. Dundas, Laszlo P. Kestay
Active Mars: A dynamic world
Mars exhibits diverse surface changes at all latitudes and all seasons. Active processes include impact cratering, aeolian sand and dust transport, a variety of slope processes, changes in polar ices, and diverse effects of seasonal CO2 frost. The extent of surface change has been surprising and indicates that the present climate is capable of reshaping the surface. Activity has important implicat
Authors
Colin M. Dundas, Patricio Becerra, Shane Byrne, Matthew Chojnacki, Ingrid J. Daubar, Serina Diniega, Candice J. Hansen, Kenneth E. Herkenhoff, Margaret E. Landis, Alfred S. McEwen, Ganna Portyankina, Adomas Valantinas
Introduction: Does water flow on Martian slopes?
No abstract available.
Authors
Colin M. Dundas, Susan J. Conway, David E Stillman
Dry formation of recent Martian slope features
Martian surface conditions are cold and dry, unfavorable for liquid water, yet steep slopes display young and currently active features suggestive of wet processes. These include recurring slope lineae and slope streaks, gully landforms, and small lobate features. Wet origins for these features would imply surprising amounts of liquid water at the surface. However, detailed observations of the mor
Authors
Colin M. Dundas
Mars science helicopter: Compelling science enabled by an aerial platform
This whitepaper describes two conceptual vehicle designs, including possible tradeoffs within those designs, which would enable a wide array of innovative science investigations. In addition to describing vehicle capabilities, flight characteristics, and the breadth of enabled science for the two helicopter designs, we also introduce three mission concepts that showcase investigations made possibl
Authors
Jonathan Bapst, Timothy J Parker, J Balaram, T Tzanetos, L. H. Matthies, C D Edwards, Aaron Freeman, S Withrow-Maser, W. Carter Johnson, E Amador-French, Janice L. Bishop, Ingrid J. Daubar, Colin M. Dundas, Abigail A. Fraeman, Christopher W. Hamilton, C. Hardgrove, Briony H. N. Horgan, C. W. Leung, Y. Lin, A Mittelholz, B. P. Weiss
GANGOTRI mission concept on the glacial key to the Amazonian climate of Mars
The GANGOTRI mission concept would investigate in situ the geologic origins of midlatitudinal Martian glaciers, as underlain by Amazonian climate evolution, by riddling the ice with a hybrid thermo-mechanical drill for deep englacial sampling. GANGOTRI would use regolith compositional measurements to characterize ice-regolith interaction, and stable isotope measurements to characterize fundamental
Authors
Suniti Karunatillake, Ali M Bramson, Kris Zacny, Colin M. Dundas, Lujendra Ojha, Oded Aharonson, Eran Vos, Don R Hood, A. Deanne Rogers, Joseph S. Levy, Peter Doran, Kathleen Mandt, Jack Wilson, Emily B Hughes, Heidi Fuqua-Haviland, Jeffrey Moersch, Scott M. Perl, Dewan E. Haque, J. R. Skok, Harish, S. Vijayan, A. Bhardwaj, Brent Christner, Hanna Sizemore, A Kereszturi, Norbert Schorghofer, Kurt Retherford, Paul Niles, Juan Manuel Lorenzo, Katherine Mesick, Heather Franz, Jose Rodriguez-Manfredi, Daniel Coupland, Peter Bertone
Current activity on the Martian surface: A key subject for future exploration
One of the fundamental discoveries in Mars science in the last decade has been the extent and importance of current surface activity. Recent results have shifted our view of Mars from a world where the most interesting geologic events were in the distant past (similar to the Moon) to a world that undergoes active evolution and one where understanding the present is key to deciphering the planet’s
Authors
Colin M. Dundas, Shane Byrne, Matthew Chojnacki, Serina Diniega, Ingrid J. Daubar, Christopher W. Hamilton, Candice J. Hansen, Alfred S. McEwen, Ganna Portyankina, Hanna G Sizemore
Mid-latitude ice on Mars: A science target for planetary climate histories and an exploration target for in situ resources
In the last decade, aided by the high-resolution data and long-term monitoring by NASA’s Mars Reconnaissance Orbiter (MRO) and other spacecraft, extensive evidence has emerged supporting the presence of abundant H2O ground ice throughout much of the mid-latitudes of Mars. Growing evidence indicates that much of this ice is relatively pure, exists within a few meters of the surface, and reaches low
Authors
Ali Bramson, Chimira Andres, Jonathan Bapst, Patricio Becerra, Samuel W Courville, Colin M. Dundas, Shannon M Hibbard, John W Holt, Suniti Karunatillake, Aditya Khuller, Michael T. Mellon, Gareth A Morgan, R. W. Obbard, Matthew R Perry, Eric I Petersen, Nathaniel E. Putzig, Hanna G Sizemore, Isaac B. Smith, David E Stillman, Paul Wooster
Maximizing the science and resource mapping potential of Orbital VSWIR Spectral measurements of Mars
The last 16 years witnessed a rapid growth in understanding the composition and aqueous alteration of Mars’ surface from orbital data from the Observatoire pour la Mineralogie, l’Eau, les Glaces et l’Activité (OMEGA) [1] and Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) [2]. Both are sensitive to water-, hydroxyl-, sulfate-, and carbonate-bearing and ferric phases that record past l
Authors
Scott L. Murchie, Raymond E. Arvidson, Janice L Bishop, Wendy M. Calvin, John Carter, John Christian, Roger N. Clark, Colin M. Dundas, Bethany L. Ehlmann, Valerie K. Fox, Abigail A. Fraeman, Timothy A Goudge, Briony H. N. Horgan, Madison N Hughes, Ellen K Leask, Alfred S. McEwen, John F Mustard, Mario Parente, Kathryn E Powell, Frank P. Seelos, Kimberly D. Seelos, Jesse D Tarnas, Christina E Viviano, James J. Wray