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Layered, massive and thin sediments on Mars: Possible Late Noachian to Late Amazonian tephra? Layered, massive and thin sediments on Mars: Possible Late Noachian to Late Amazonian tephra?

Data from instruments on the currently orbiting Mars Global Surveyor (MGS) suggest that as an alternative interpretation to lacustrine deposits, widespread sediments on Mars may be tephra deposits of variable age, formed in part by volcano-ice interactions. The materials are often associated with outcrops of mapped geological units that have each been previously interpreted as volcanic...
Authors
M. G. Chapman

Remotely sensed geology from lander-based to orbital perspectives: Results of FIDO rover May 2000 field tests Remotely sensed geology from lander-based to orbital perspectives: Results of FIDO rover May 2000 field tests

Blind field tests of the Field Integration Design and Operations (FIDO) prototype Mars rover were carried out 7-16 May 2000. A Core Operations Team (COT), sequestered at the Jet Propulsion Laboratory without knowledge of test site location, prepared command sequences and interpreted data acquired by the rover. Instrument sensors included a stereo panoramic camera, navigational and hazard...
Authors
B. Jolliff, A. Knoll, R.V. Morris, J. Moersch, H. McSween, M. Gilmore, R. Arvidson, R. Greeley, Kenneth E. Herkenhoff, S. Squyres

Catastrophic erosion of Hellas basin rim on Mars induced by magmatic intrusion into volatile-rich rocks Catastrophic erosion of Hellas basin rim on Mars induced by magmatic intrusion into volatile-rich rocks

Malea and Hesperia Plana form large sectors of the rim of Hellas basin that display partly eroded volcanic shields and plains. These regions have topographic profiles that appear to be several hundred meters lower than those of adjacent rim sectors and lack prominent massifs of remnant basement that would be expected to stand above the lava plains. We interpret that before the volcanic...
Authors
K. L. Tanaka, J.S. Kargel, D. J. MacKinnon, T.M. Hare, N. Hoffman

Topography and geologic characteristics of aeolian grooves in the south polar layered deposits of Mars Topography and geologic characteristics of aeolian grooves in the south polar layered deposits of Mars

The topographic and geologic characteristics of grooves and groove-like features in the south polar layered deposits near the Mars Polar Lander/Deep Space 2 landing sites are evaluated using Mariner 9 images and their derived photoclinometry, normalized using Mars Orbiter Laser Altimeter data. Although both Mariner 9 and Viking images of the south polar layered deposits were available at...
Authors
N.T. Bridges, Kenneth E. Herkenhoff

Observations of comet 19P/Borrelly by the miniature integrated camera and spectrometer aboard deep space 1 Observations of comet 19P/Borrelly by the miniature integrated camera and spectrometer aboard deep space 1

The nucleus of the Jupiter-family comet 19P/Borrelly was closely observed by the Miniature Integrated Camera and Spectrometer aboard the Deep Space 1 spacecraft on 22 September 2001. The 8-kilometer-long body is highly variegated on a scale of 200 meters, exhibiting large albedo variations (0.01 to 0.03) and complex geologic relationships. Short-wavelength infrared spectra (1.3 to 2.6...
Authors
Laurence A. Soderblom, T.L. Becker, G. Bennett, D. C. Boice, D.T. Britt, R. H. Brown, B. J. Buratti, C. Isbell, B. Giese, T. Hare, M.D. Hicks, Elpitha Howington-Kraus, Randolph L. Kirk, M. Lee, R.M. Nelson, J. Oberst, T.C. Owen, M.D. Rayman, B.R. Sandel, S. A. Stern, N. Thomas, R.V. Yelle

Lunar orbiter digitization and cartographic processing Lunar orbiter digitization and cartographic processing

Digitization and cartographic processing of 5 Lunar Orbiter (LO) IV frames (109H, 110H, 114H, 115H, and 114M) are now complete, and these data are available online at http://wwwflag.wr.usgs.gov/USGSFlag/Space/LunarOrbiter/lunorbWebtop.html. Coverage ofthese data extends from Eratosthenes crater on the west to Mare Serenitatis in the east, and from Aristoteles crater in the north to Rima...
Authors
Lisa R. Gaddis, Tammy L. Becker, Tracie L. Sucharski, A. Gitlin, Randolph L. Kirk, Elpitha Howington-Kraus

Validation of the USGS sensor model for topographic mapping of Venus using Magellan radar stereoimagery Validation of the USGS sensor model for topographic mapping of Venus using Magellan radar stereoimagery

The Magellan spacecraft went into Venus orbit in 1990 and by 1992 had made three complete cycles of polar orbits, each cycle covering the full range of longitudes. During this time the spacecraft obtained synthetic aperture radar (SAR) images of >96% of the planet at a resolution of 75 m/pixel. Images taken with a decreased look angle from vertical, primarily during Cycle 3, provide...
Authors
Elpitha Howington-Kraus, Randolph L. Kirk, Donna M. Galuszka, Trent M. Hare, Bonnie L. Redding

High resolution digital elevation models of Mars from MOC Narrow Angle stereoimages High resolution digital elevation models of Mars from MOC Narrow Angle stereoimages

In this abstract we report on our initial experiences performing stereotopographic mapping of Mars with high-resolution images from the Mars Global Surveyor Mars Orbiter Camera Narrow-Angle subsystem (MGS MOC-NA; [1]). Accurate topographic information, and, in particular, high-resolution digital elevation models (DEMs) are of intense interest at all phases of Mars exploration and...
Authors
Randolph L. Kirk, Elpitha Howington-Kraus, Brent A. Archinal

Combining lunar photogrammetric topographic data with Clementine LIDAR data Combining lunar photogrammetric topographic data with Clementine LIDAR data

During the Clementine Mission both oblique and vertical multispectral images were collected. The oblique and vertical images from a single spectral band collected during the same orbit form a stereo pair that can be used to derive the topography. These stereo pairs were used to derive the topography of an area surrounding the lunar South Pole (90°S - 64°S latitude) and North Pole (90°N -...
Authors
Mark R. Rosiek, Randolph L. Kirk, Elpitha Howington-Kraus

Optical designs for the Mars '03 rover cameras Optical designs for the Mars '03 rover cameras

In 2003, NASA is planning to send two robotic rover vehicles to explore the surface of Mars. The spacecraft will land on airbags in different, carefully chosen locations. The search for evidence indicating conditions favorable for past or present life will be a high priority. Each rover will carry a total of ten cameras of five various types. There will be a stereo pair of color...
Authors
Gregory Hallock Smith, E.C. Hagerott, Lawrence M. Scherr, Kenneth E. Herkenhoff, James F. Bell

Planetary Interactive GIS-on-the-Web Analyzable Database (PIGWAD) Planetary Interactive GIS-on-the-Web Analyzable Database (PIGWAD)

The United States Geological Survey (USGS) in Flagstaff, Arizona is producing a Web-based, user-friendly interface that integrates powerful Geographic Information Systems (GIS) statistical and spatial relational tools for analyses of planetary datasets. The interface, known as “Planetary Interactive GIS-on-the-Web Analyzable Database” (PIGWAD), provides database support for the research...
Authors
Trent M. Hare, Kenneth L. Tanaka

Mars exploration Mars exploration

An international flotilla of spacecraft are to be sent to Mars over the next decade in an effort to understand the planet's geology and climate history, and to determine whether some form of life ever started there. At least two spacecraft will be sent at each launch opportunity, and at times up to four spacecraft may be operating simultaneously at the planet.
Authors
M. H. Carr, James B. Garvin
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