Book contents
- Meteorite Mineralogy
- Cambridge Planetary Science
- Meteorite Mineralogy
- Copyright page
- Dedication
- Contents
- Preface
- 1 Minerals and Meteorites
- 2 Definitions and Explications
- 3 Brief Review of Crystallography and Crystal Chemistry
- 4 Properties of Minerals
- 5 Identification of Meteoritic Minerals in Reflected Light, by Backscattered Electron Imaging, and by Energy Dispersive X-Ray Spectroscopy, Wavelength-Dispersive X-Ray Spectroscopy, and Electron Backscatter Diffraction Analysis
- 6 Meteorite Classification and Taxonomy
- 7 Mineralogy of Major Physical Components of Chondrites
- 8 Petrologic and Mineralogical Characteristics of Meteorite Groups
- 9 Cosmomineralogy
- 10 Formation of Meteoritic Minerals in Gas- and Dust-Rich Environments
- 11 Formation of Meteoritic Minerals on Parent Bodies
- 12 Formation of Meteoritic Minerals in the Terrestrial Environment
- 13 The Strange Case of the Aluminum-Copper Alloys
- Summary
- Epilogue
- References
- Index
- Plate Section (PDF Only)
9 - Cosmomineralogy
Published online by Cambridge University Press: 11 August 2021
- Meteorite Mineralogy
- Cambridge Planetary Science
- Meteorite Mineralogy
- Copyright page
- Dedication
- Contents
- Preface
- 1 Minerals and Meteorites
- 2 Definitions and Explications
- 3 Brief Review of Crystallography and Crystal Chemistry
- 4 Properties of Minerals
- 5 Identification of Meteoritic Minerals in Reflected Light, by Backscattered Electron Imaging, and by Energy Dispersive X-Ray Spectroscopy, Wavelength-Dispersive X-Ray Spectroscopy, and Electron Backscatter Diffraction Analysis
- 6 Meteorite Classification and Taxonomy
- 7 Mineralogy of Major Physical Components of Chondrites
- 8 Petrologic and Mineralogical Characteristics of Meteorite Groups
- 9 Cosmomineralogy
- 10 Formation of Meteoritic Minerals in Gas- and Dust-Rich Environments
- 11 Formation of Meteoritic Minerals on Parent Bodies
- 12 Formation of Meteoritic Minerals in the Terrestrial Environment
- 13 The Strange Case of the Aluminum-Copper Alloys
- Summary
- Epilogue
- References
- Index
- Plate Section (PDF Only)
Summary
Mercury is the smallest and innermost major planet (Figure 9.1); from the perspective of Earth-bound observers, it never appears more than 28° from the Sun. It is locked in a state of spin-orbit coupling: its rotation period (58.646 Earth days) is exactly two-thirds of its year (87.969 Earth days). Mercury is named after the Greco-Roman messenger to the gods, perhaps because of its rapid apparent day-to-day movement with respect to the Sun. Compared to the other major planets, Mercury has the most eccentric orbit (e = 0.2056), the highest inclination relative to the ecliptic (7.007°), and the smallest axial tilt (0.01°). It has a weak magnetic field (~1.1 percent as strong as Earth’s) and no natural satellites.
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- Meteorite Mineralogy , pp. 200 - 238Publisher: Cambridge University PressPrint publication year: 2021