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Showing 1 to 20 of 155 for “"Martian"”.

  1. The role of C-O-H volatiles in the martian mantle and the production of the martian atmosphere.

    … suggests that liquid water was once eroding the martian surface at rates comparable to many climates on present-day Earth. However, the thin modern martian atmosphere does not support liquid water. The fundamental variable in the evolution of the martian atmosphere is the storage of C-O-H …

    umn Repository record for The role of C-O-H volatiles in the martian mantle and the production of the martian atmosphere. (opens in a new tab)

  2. Impact Melt-Bearing Deposits Around Martian Craters

    … we investigate impact melt emplacement around Martian craters. We compare our results to melt emplacement processes found on Venus, the Moon, and Mercury. We tentatively find Martian melt emplacement more closely resembles Venusian emplacement, rather than lunar emplacement. This suggests …

    uwo Repository record for Impact Melt-Bearing Deposits Around Martian Craters (opens in a new tab)

  3. Vertically Propagating Tides in the Martian Atmosphere

    … of tides on the mean state of the present-day Martian atmosphere is especially large at high altitudes. Certain tides can propagate away from the region of generation in the lower atmosphere and reach the upper atmosphere, where they can achieve significant amplitudes. Such vertically …

    vt Repository record for Vertically Propagating Tides in the Martian Atmosphere (opens in a new tab)

  4. Non-migrating tides in the Martian thermosphere

    Previous studies have identified longitudinal structures associated with non-migrating tides in observations of the upper neutral atmosphere of Mars. MAVEN’s Imaging Ultraviolet Spectrometer (IUVS) observations of the upper atmosphere reveal variations in density with longitude at altitudes of 130 …

    vt Repository record for Non-migrating tides in the Martian thermosphere (opens in a new tab)

  5. Natural and artificial orbits around the Martian moon Phobos

    … human missions to Mars is the exploration of the Martian moons. In particular, Phobos is becoming an appealing destination for future scientific missions of NASA and ESA. Phobos is a tiny celestial body that orbits around Mars at low altitude. The unique combination of these two characteristics …

    strathclyde Repository record for Natural and artificial orbits around the Martian moon Phobos (opens in a new tab)

  6. A motion vision system for a Martian Micro-Rover

    This thesis describes a monocular, motion vision system that was designed to meet the size, power, and processing constraints of a small, robotic, planetary explorer. The computational requirements of the brightness gradient approach, which is commonly used in motion vision systems, were found to …

    mit Repository record for A motion vision system for a Martian Micro-Rover (opens in a new tab)

  7. Radiative Transfer in the Martian Environment: In-Situ Results from the MSL Curiosity Rover and Laboratory Experimentation on Martian Regolith and Crystalline Rock Analogs

    … Gale Crater. Radiative transfer modeling of the martian atmosphere benefits from this quantification of low-lying dust. This dissertation aims to expand our knowledge of the radiation environment of Mars into its surface and subsurface. The scattering of radiation through analog martian materials …

    york Repository record for Radiative Transfer in the Martian Environment: In-Situ Results from the MSL Curiosity Rover and Laboratory Experimentation on Martian Regolith and Crystalline Rock Analogs (opens in a new tab)

  8. Lithospheric dynamics of Earth’s subduction zones and Martian tectonic provinces

    … dynamics of Earth’s subduction zones and Martian tectonic provinces on multiple time scales. In Chapter 2, I use geodetic observations to constrain the post-seismic viscoelastic deformation following the 1960 M9.5 Valdivia, Chile earthquake and quantify its stressing onto the 2010 M8.8 …

    woods-hole Repository record for Lithospheric dynamics of Earth’s subduction zones and Martian tectonic provinces (opens in a new tab)

  9. Effect of Chemistry on Electrodynamics in the Martian Dynamo Region

    … approach focuses on numerical studies using the Martian Multifluid Magnetohy drodynamic (MF-MHD) Model (M4). The dynamo is a region which varies in time and space due to the lack of a global planetary intrinsic magnetic field, the location of the remnant crustal fields, and the planetary rotation …

    embry-riddle Repository record for Effect of Chemistry on Electrodynamics in the Martian Dynamo Region (opens in a new tab)

  10. Temporal and Geographical Variation in Martian Surface Dust Lifting Processes

    … examining the variability of key aspects of the Martian dust cycle and investigating their importance in predicting conditions for spacecraft atmospheric descent and landing. The dust cycle – lifting, transportation and deposition – is a significant Martian climate cycle. The geographical and …

    the-open-u Repository record for Temporal and Geographical Variation in Martian Surface Dust Lifting Processes (opens in a new tab)

  11. Growth and Survivability of Microorganisms at Martian Temperatures and Pressures

    <p>The discovery of methane in the martian atmosphere via numerous ground- and space-based sources has prompted the study of methanogens as models for life on Mars. Methanogens are microorganisms within the domain Archaea, many of which utilize carbon dioxide (CO2) and hydrogen to produce methane. …

    arkansas Repository record for Growth and Survivability of Microorganisms at Martian Temperatures and Pressures (opens in a new tab)

  12. Investigations of the Martian Mid-Latitudes: Implications for Ground Ice

    This dissertation examines several questions in Martian surface processes relating to water or ice using a combination of geomorphology and modeling. I first examine sublimation of ice from new small mid-latitude craters with freshly exposed ice imaged by the High Resolution Imaging Science …

    arizona-thes Repository record for Investigations of the Martian Mid-Latitudes: Implications for Ground Ice (opens in a new tab)

  13. Lithospheric dynamics of Earth's subduction zones and Martian tectonic provinces

    … dynamics of Earth's subduction zones and Martian tectonic provinces on multiple time scales ranging from short-term earthquake deformation to long-term tectonic loading. In Chapter 2, I use geodetic observations to constrain the postseismic viscoelastic deformation following the 1960 M9.5 …

    mit Repository record for Lithospheric dynamics of Earth's subduction zones and Martian tectonic provinces (opens in a new tab)

  14. The composition of the Martian dark regions : observations and analysis

    Thesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Sciences, 1980.

    mit Repository record for The composition of the Martian dark regions : observations and analysis (opens in a new tab)

  15. Study of the Martian upper atmosphere using radio tracking data

    Since the first in situ observations of the Martian atmosphere were made by the twin Viking landers, we have learned considerably more about its composition, dynamics and variability. Not only did the new data on global atmospheric densities generate opportunities to understand the atmospheric …

    mit Repository record for Study of the Martian upper atmosphere using radio tracking data (opens in a new tab)

  16. A zonally and annually averaged study of potential early Martian atmospheres

    Observations of the surface of Mars suggest a high probability of surface water activity in that planet's past. Consequently, many studies of Mars' early atmosphere have attempted to estimate the carbon dioxide level by requiring that surface temperatures be high enough to support surface liquid …

    rice Repository record for A zonally and annually averaged study of potential early Martian atmospheres (opens in a new tab)

  17. Automatic Classification and Segmentation of Patterned Martian Ground Using Deep Learning Techniques

    … by prioritizing downlink of meaningful data. Martian polygonally cracked ground is actively studied by planetary geologists and may be indicative of subsurface water. Filtering images containing these polygonal features can be used as a case study for science autonomy and to reduce the …

    uwo Repository record for Automatic Classification and Segmentation of Patterned Martian Ground Using Deep Learning Techniques (opens in a new tab)

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