Book contents
- Frontmatter
- Contents
- List of contributors
- Foreword
- Acknowledgments
- Part I Introduction and historical perspective
- Part II Elemental Composition: Orbital and in situ Surface Measurements
- Part III Mineralogy and Remote Sensing of Rocks, Soil, Dust, and Ices
- 7 Mineralogy of the Martian surface from Mars Express OMEGA observations
- 8 Visible to near-IR multispectral orbital observations of Mars
- 9 Global mineralogy mapped from the Mars Global Surveyor Thermal Emission Spectrometer
- 10 The compositional diversity and physical properties mapped from the Mars Odyssey Thermal Emission Imaging System
- 11 Mars' crustal magnetization: a window into the past
- 12 Multispectral imaging from Mars Pathfinder
- 13 Mars Exploration Rover Pancam multispectral imaging of rocks, soils, and dust at Gusev crater and Meridiani Planum
- 14 The mineralogy of Gusev crater and Meridiani Planum derived from the Miniature Thermal Emission Spectrometers on the Spirit and Opportunity rovers
- 15 Iron mineralogy and aqueous alteration on Mars from the MER Mössbauer spectrometers
- 16 Magnetic properties of Martian surface materials
- 17 Martian meteorites as crustal samples
- Part IV Physical Properties of Surface Materials
- Part V Synthesis
- Part VI Summary, Upcoming Missions, and New Measurement Needs
- Index
- Plate section
- References
14 - The mineralogy of Gusev crater and Meridiani Planum derived from the Miniature Thermal Emission Spectrometers on the Spirit and Opportunity rovers
from Part III - Mineralogy and Remote Sensing of Rocks, Soil, Dust, and Ices
Published online by Cambridge University Press: 10 December 2009
- Frontmatter
- Contents
- List of contributors
- Foreword
- Acknowledgments
- Part I Introduction and historical perspective
- Part II Elemental Composition: Orbital and in situ Surface Measurements
- Part III Mineralogy and Remote Sensing of Rocks, Soil, Dust, and Ices
- 7 Mineralogy of the Martian surface from Mars Express OMEGA observations
- 8 Visible to near-IR multispectral orbital observations of Mars
- 9 Global mineralogy mapped from the Mars Global Surveyor Thermal Emission Spectrometer
- 10 The compositional diversity and physical properties mapped from the Mars Odyssey Thermal Emission Imaging System
- 11 Mars' crustal magnetization: a window into the past
- 12 Multispectral imaging from Mars Pathfinder
- 13 Mars Exploration Rover Pancam multispectral imaging of rocks, soils, and dust at Gusev crater and Meridiani Planum
- 14 The mineralogy of Gusev crater and Meridiani Planum derived from the Miniature Thermal Emission Spectrometers on the Spirit and Opportunity rovers
- 15 Iron mineralogy and aqueous alteration on Mars from the MER Mössbauer spectrometers
- 16 Magnetic properties of Martian surface materials
- 17 Martian meteorites as crustal samples
- Part IV Physical Properties of Surface Materials
- Part V Synthesis
- Part VI Summary, Upcoming Missions, and New Measurement Needs
- Index
- Plate section
- References
Summary
ABSTRACT
Two Miniature Thermal Emission Spectrometers (Mini-TES) operated successfully onboard the two Mars Exploration Rovers (MER) on the Martian surface, one at Gusev crater and the other at Meridiani Planum. Designed to provide remotely sensed information on the bulk mineralogy of surface materials, the Mini-TES instruments served to guide the rovers to targets of interest and extrapolate the observations made by the rovers' mechanical-arm-mounted instruments. The Mini-TES on the Spirit rover in Gusev crater observed a flat plain covered by rocks with an olivine-rich ((Mg,Fe)2SiO4) mineralogy and a soil-like unit mantled by airfall dust occurring between the rocks. The dust is a spectral match to dust observed at Meridiani Planum and across the globe. The soil is basaltic in composition, dominated by plagioclase (NaAlSi3O8–CaAl2Si2O8), pyroxene (Ca(Mg,Fe)Si2O6–(Mg,Fe)SiO3), and olivine that probably was produced in part from the breakdown of local rocks. Approximately 2.5 km from the Spirit lander, the Columbia Hills contain a remarkably diverse set of rocks distinct from the plains. Basaltic glass appears to dominate the mineralogy of various outcropping rocks while plagioclase dominates the float rocks that cover most of the north side of Husband Hill, the tallest of the Columbia Hills. Numerous exotic (out of place) rocks dot the hillside that likely were emplaced as impact ejecta in some cases and perhaps as volcanic intrusions in other cases. Onboard the Opportunity rover in Meridiani Planum, the Mini-TES observed a nearly rock-free plain covered in hematite (Fe2O3) spherules and basaltic sand.
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- Chapter
- Information
- The Martian SurfaceComposition, Mineralogy and Physical Properties, pp. 315 - 338Publisher: Cambridge University PressPrint publication year: 2008
References
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