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: 80
Temperature profile around a basaltic sill intruded into wet sediments Temperature profile around a basaltic sill intruded into wet sediments
The transfer of heat into wet sediments from magmatic intrusions or lava flows is not well constrained from field data. Such field constraints on numerical models of heat transfer could significantly improve our understanding of water–lava interactions. We use experimentally calibrated pollen darkening to measure the temperature profile around a basaltic sill emplaced into wet lakebed...
Authors
Leslie Baker, Andrew Bernard, William C. Rember, Moses P. Milazzo, Colin M. Dundas, Oleg Abramov, Laszlo P. Keszthelyi
Expanded secondary craters in the Arcadia Planitia region, Mars: evidence for tens of Myr-old shallow subsurface ice Expanded secondary craters in the Arcadia Planitia region, Mars: evidence for tens of Myr-old shallow subsurface ice
A range of observations indicates widespread subsurface ice throughout the mid and high latitudes of Mars in the form of both pore-filling and excess ice. It is generally thought that this ice was recently emplaced and is not older than a hundred thousand to a few millions of years old based on ice stability and orbital-induced climate change. We analyze the distribution of subsurface...
Authors
Donna Viola, Alfred S. McEwen, Colin M. Dundas, Shane Byrne
Emplacement and erosive effects of the south Kasei Valles lava on Mars Emplacement and erosive effects of the south Kasei Valles lava on Mars
Although it has generally been accepted that the Martian outflow channels were carved by floods of water, observations of large channels on Venus and Mercury demonstrate that lava flows can cause substantial erosion. Recent observations of large lava flows within outflow channels on Mars have revived discussion of the hypothesis that the Martian channels are also produced by lava. An...
Authors
Colin M. Dundas, Laszlo P. Keszthelyi
HiRISE observations of Recurring Slope Lineae (RSL) during southern summer on Mars HiRISE observations of Recurring Slope Lineae (RSL) during southern summer on Mars
Recurring Slope Lineae (RSL) are active features on Mars that might require flowing water. Most examples observed through 2011 formed on steep, equator-facing slopes in the southern mid-latitudes. They form and grow during warm seasons and fade and often completely disappear during colder seasons, but recur over multiple Mars years. They are recognizable by their incremental growth...
Authors
Lujendra Ojha, Alfred McEwen, Colin M. Dundas, Shane Byrne, Sarah Mattson, James Wray, Marion Masse, Ethan Schaefer
Recurring slope lineae in equatorial regions of Mars Recurring slope lineae in equatorial regions of Mars
The presence of liquid water is a requirement of habitability on a planet. Possible indicators of liquid surface water on Mars include intermittent flow-like features observed on sloping terrains. These recurring slope lineae are narrow, dark markings on steep slopes that appear and incrementally lengthen during warm seasons on low-albedo surfaces. The lineae fade in cooler seasons and...
Authors
Alfred S. McEwen, Colin M. Dundas, Sarah S. Mattson, Anthony D. Toigo, Lujendra Ojha, James J. Wray, Matthew Chojnacki, Shane Byrne, Scott L. Murchie, Nicolas Thomas
HiRISE observations of new impact craters exposing Martian ground ice HiRISE observations of new impact craters exposing Martian ground ice
Twenty small new impact craters or clusters have been observed to excavate bright material inferred to be ice at mid and high latitudes on Mars. In the northern hemisphere, the craters are widely distributed geographically and occur at latitudes as low as 39°N. Stability modeling suggests that this ice distribution requires a long-term average atmospheric water vapor content around 25...
Authors
Colin M. Dundas, Shane Byrne, Alfred S. McEwen, Michael T. Mellon, Megan R. Kennedy, Ingrid J. Daubar, Lee Saper
Science and Products
Filter Total Items: 80
Temperature profile around a basaltic sill intruded into wet sediments Temperature profile around a basaltic sill intruded into wet sediments
The transfer of heat into wet sediments from magmatic intrusions or lava flows is not well constrained from field data. Such field constraints on numerical models of heat transfer could significantly improve our understanding of water–lava interactions. We use experimentally calibrated pollen darkening to measure the temperature profile around a basaltic sill emplaced into wet lakebed...
Authors
Leslie Baker, Andrew Bernard, William C. Rember, Moses P. Milazzo, Colin M. Dundas, Oleg Abramov, Laszlo P. Keszthelyi
Expanded secondary craters in the Arcadia Planitia region, Mars: evidence for tens of Myr-old shallow subsurface ice Expanded secondary craters in the Arcadia Planitia region, Mars: evidence for tens of Myr-old shallow subsurface ice
A range of observations indicates widespread subsurface ice throughout the mid and high latitudes of Mars in the form of both pore-filling and excess ice. It is generally thought that this ice was recently emplaced and is not older than a hundred thousand to a few millions of years old based on ice stability and orbital-induced climate change. We analyze the distribution of subsurface...
Authors
Donna Viola, Alfred S. McEwen, Colin M. Dundas, Shane Byrne
Emplacement and erosive effects of the south Kasei Valles lava on Mars Emplacement and erosive effects of the south Kasei Valles lava on Mars
Although it has generally been accepted that the Martian outflow channels were carved by floods of water, observations of large channels on Venus and Mercury demonstrate that lava flows can cause substantial erosion. Recent observations of large lava flows within outflow channels on Mars have revived discussion of the hypothesis that the Martian channels are also produced by lava. An...
Authors
Colin M. Dundas, Laszlo P. Keszthelyi
HiRISE observations of Recurring Slope Lineae (RSL) during southern summer on Mars HiRISE observations of Recurring Slope Lineae (RSL) during southern summer on Mars
Recurring Slope Lineae (RSL) are active features on Mars that might require flowing water. Most examples observed through 2011 formed on steep, equator-facing slopes in the southern mid-latitudes. They form and grow during warm seasons and fade and often completely disappear during colder seasons, but recur over multiple Mars years. They are recognizable by their incremental growth...
Authors
Lujendra Ojha, Alfred McEwen, Colin M. Dundas, Shane Byrne, Sarah Mattson, James Wray, Marion Masse, Ethan Schaefer
Recurring slope lineae in equatorial regions of Mars Recurring slope lineae in equatorial regions of Mars
The presence of liquid water is a requirement of habitability on a planet. Possible indicators of liquid surface water on Mars include intermittent flow-like features observed on sloping terrains. These recurring slope lineae are narrow, dark markings on steep slopes that appear and incrementally lengthen during warm seasons on low-albedo surfaces. The lineae fade in cooler seasons and...
Authors
Alfred S. McEwen, Colin M. Dundas, Sarah S. Mattson, Anthony D. Toigo, Lujendra Ojha, James J. Wray, Matthew Chojnacki, Shane Byrne, Scott L. Murchie, Nicolas Thomas
HiRISE observations of new impact craters exposing Martian ground ice HiRISE observations of new impact craters exposing Martian ground ice
Twenty small new impact craters or clusters have been observed to excavate bright material inferred to be ice at mid and high latitudes on Mars. In the northern hemisphere, the craters are widely distributed geographically and occur at latitudes as low as 39°N. Stability modeling suggests that this ice distribution requires a long-term average atmospheric water vapor content around 25...
Authors
Colin M. Dundas, Shane Byrne, Alfred S. McEwen, Michael T. Mellon, Megan R. Kennedy, Ingrid J. Daubar, Lee Saper