Asteroid Spectroscopy

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Absorption of these photons produces a feature in the spectrum of the interacting light at the wavelength corresponding to the energy ∆ O 0.3 1 micron region of pyroxene spectrum Reflectance 0.2 0.1 ∆ O 0 0.3 0.5 0.7 0.9 1.1 1.3 Wavelength (um) Absorption feature is characterized by: central wavelength, width and depth
Most cation sites in transition metalbearing minerals are not perfectly symmetric Distortions of an Octahedral Site
Page 1 and 2: Lecture #2 Asteroid Spectroscopy Pr
Page 3 and 4: HAYABUSA Sample Return Mission A la
Page 5 and 6: Remote Sensing Techniques for Chara
Page 7 and 8: Why Mineralogy rather than Composit
Page 9 and 10: Mineralogical Characterizations Min
Page 11 and 12: VNIR Spectra Detection and composit
Page 13 and 14: Transition metal elements commonly
Page 15 and 16: Shell #3 Shell #2 Shell #1 Nucleus
Page 17 and 18: First Series Transition metals Peri
Page 19 and 20: In minerals, the metal cations (e.g
Page 21 and 22: Consider Fe 2+ in an octahedral sit
Page 23: ∆ O is the energy difference betw
Page 27 and 28: The result is multiple absorption f
Page 29 and 30: Spectra of different HED meteorite
Page 31 and 32: The broad 1 µm olivine feature is
Page 33 and 34: Olivine-Pyroxene Mixture Spectra Wi
Page 35 and 36: In Olivine-Pyroxene mixtures, the r
Page 37 and 38: Molecular Vibrations Also Produce S
Page 39 and 40: Some potentially important asteroid
Page 41 and 42: Mineralogical Analysis of Vesta Gaf
Page 43 and 44: Is a Thin Surface Layer Representat
Page 45 and 46: Observational Methodologies Standar
Page 47 and 48: Typical instrumental flux measureme
Page 49 and 50: Correction for extinction using a S
Page 51 and 52: Extinction correction with channel
Page 53 and 54: Implications for Analysis Irrespect
Page 55 and 56: Correction Process - II Offsets sho
Page 57: The Upside -- Asteroid spectra obta

Asteroid Spectroscopy

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