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Publications

Filter Total Items: 990

Topographic mapping of Mars: From hectometer to micrometer scales Topographic mapping of Mars: From hectometer to micrometer scales

We describe USGS topomapping of Mars at resolutions from 100 m to 30 µm with data from the latest spacecraft missions. Analysis of NASA 2001 Mars Odyssey Thermal Emission Imaging System (THEMIS) data combining daytime visible reflected, daytime IR emitted, and nighttime IR emitted images allows us to isolate the physical effects of topography, albedo, and thermal inertia. To a good...
Authors
Randolph L. Kirk, Steven W. Squyres, Gerhard Neukum

A new Mars Digital Image Model (MDIM 2.1) control network A new Mars Digital Image Model (MDIM 2.1) control network

The U.S. Geological Survey has recently completed a final revised version of its 231 m/pixel global Viking image mosaic of Mars that has substantially improved geodetic accuracy compared to versions released in 1991 and 2001. This mosaic, known as MDIM 2.1, is currently available in the USGS ISIS file format (see http://astrogeology.usgs.gov/Projects/MDIM21/) and will be formatted and...
Authors
Brent A. Archinal, Ella M. Lee, Randolph L. Kirk, T. C. Duxbury, Robert M. Sucharski, Debbie Cook, Janet M. Barrett

A new Mars Digital Image Model (MDIM 2.1) control network A new Mars Digital Image Model (MDIM 2.1) control network

The U.S. Geological Survey has recently completed a final revised version of its 231 m/pixel global Viking image mosaic of Mars that has substantially improved geodetic accuracy compared to versions released in 1991 and 2001. This mosaic, known as MDIM 2.1, is currently available in the USGS ISIS file format and will be formatted and submitted to the NASA Planetary Data System (PDS) in...
Authors
Brent A. Archinal, Ella M. Lee, Randolph L. Kirk, T. C. Duxbury, Robert M. Sucharski, Debbie Cook, Janet M. Barrett

The emplacement of pahoehoe toes: Field observations and comparison to laboratory simulations The emplacement of pahoehoe toes: Field observations and comparison to laboratory simulations

We observed active pahoehoe lobes erupted on Kilauea during May-June 1996, and found a range of emplacement styles associated with variations in local effusion rate, flow velocity, and strain rate. These emplacement styles were documented and quantified for comparison with earlier laboratory experiments. At the lowest effusion rates, velocities, and strain rates, smooth-surfaced lobes...
Authors
Tracy K. P. Gregg, Laszlo P. Keszthelyi

Io after Galileo Io after Galileo

No abstract available.
Authors
Elizabeth P. Turtle, Laszlo P. Keszthelyi, David A. Williams

Mars: Water, water everywhere Mars: Water, water everywhere

Mars is a very watery planet, but all the water seems to be frozen. Divining the amount and distribution of this water, past and present, is essential for understanding martian climates, and more.
Authors
Timothy N. Titus

Preparing for THEMIS controlled global Mars mosaics Preparing for THEMIS controlled global Mars mosaics

We have begun work to prepare for producing controlled 2001 Mars Odyssey THEMIS infrared (IR) and visible (VIS) global mosaics of Mars. This effort is being coordinated with colleagues from Arizona State University and on the THEMIS team who plan to address radiometric issues in making such mosaics. We are concentrating on geometric issues. Several areas of investigation are now in...
Authors
Brent A. Archinal, Lynn A. Weller, Stuart C. Sides, Glen E. Cushing, Randolph L. Kirk, Laurence A. Soderblom, T. C. Duxbury

Comparison of USGS and DLR topographic models of Comet Borrelly and photometric applications Comparison of USGS and DLR topographic models of Comet Borrelly and photometric applications

Stereo analysis of images obtained during the 2001 flyby of Comet Borrelly by NASA's Deep Space 1 (DS1) probe allows us to quantify the shape and photometric behavior of the nucleus. The shape is complex, with planar facets corresponding to the dark, mottled regions of the surface whereas the bright, smooth regions are convexly curved. The photometric as well as textural differences...
Authors
Randolph L. Kirk, Elpitha Howington-Kraus, Laurence A. Soderblom, Bernd Giese, Jurgen Oberst

The nucleus of Comet Borrelly: A study of morphology and surface brightness The nucleus of Comet Borrelly: A study of morphology and surface brightness

Stereo images obtained during the DS1 flyby were analyzed to derive a topographic model for the nucleus of Comet 19P/Borrelly for morphologic and photometric studies. The elongated nucleus has an overall concave shape, resembling a peanut, with the lower end tilted towards the camera. The bimodal character of surface-slopes and curvatures support the idea that the nucleus is a...
Authors
J. Oberst, Elpitha Howington-Kraus, Randolph L. Kirk, Laurence A. Soderblom, B. Buratti, M. Hicks, R. Nelson, D. Britt

A post-Galileo view of Io's interior A post-Galileo view of Io's interior

We present a self-consistent model for the interior of Io, taking the recent Galileo data into account. In this model, Io has a completely molten core, substantially molten mantle, and a very cold lithosphere. Heat from magmatic activity can mobilize volatile compounds such as SO2 in the lithosphere, and the movement of such cryogenic fluids may be important in the formation of surface...
Authors
Laszlo P. Keszthelyi, Windy L. Jaeger, Elizabeth P. Turtle, Moses P. Milazzo, Jani Radebaugh

Ridges and tidal stress on Io Ridges and tidal stress on Io

Sets of ridges of uncertain origin are seen in twenty-nine high-resolution Galileo images, which sample seven locales on Io. These ridges are on the order of a few kilometers in length with a spacing of about a kilometer. Within each locale, the ridges have a consistent orientation, but the orientations vary from place to place. We investigate whether these ridges could be a result of...
Authors
Gwendolyn D. Bart, Elizabeth P. Turtle, Windy L. Jaeger, Laszlo P. Keszthelyi, Richard Greenberg

The Rock Elm meteorite impact structure, Wisconsin: Geology and shock-metamorphic effects in quartz The Rock Elm meteorite impact structure, Wisconsin: Geology and shock-metamorphic effects in quartz

The Rock Elm structure in southwest Wisconsin is an anomalous circular area of highly deformed rocks, ∼6.5 km in diameter, located in a region of virtually horizontal undeformed sedimentary rocks. Shock-produced planar microstructures (PMs) have been identified in quartz grains in several lithologies associated with the structure: sandstones, quartzite pebbles, and breccia. Two distinct...
Authors
B.M. French, W.S. Cordua, J. B. Plescia
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