Asteroid (101955) 1999 RQ36: Spectroscopy from 0.4 to 2.4μm and meteorite analogs
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Richard P. Binzel | Michael Mueller | Francesca E. DeMeo | Dante S. Lauretta | Carl W. Hergenrother | Edward A. Cloutis | Philip R. Christensen | Alicia M. Soderberg | Ellen Susanna Howell | Harold C. Connolly | Maria Antonietta Barucci | E. Cloutis | A. Soderberg | E. Howell | B. Clark | D. Lauretta | F. DeMeo | M. Barucci | R. Binzel | H. Connolly | L. Lim | M. Ockert-Bell | C. Hergenrother | Maureen E. Ockert-Bell | Beth E. Clark | Lucy F. G. Lim | J. P. Emery | J. Emery | P. Christensen | M. Mueller | M. Ockert-Bell | F. DeMeo
[1] Andrew S. Rivkin,et al. Detection of ice and organics on an asteroidal surface , 2010, Nature.
[2] Julie Ziffer,et al. Spectroscopy of B-type Asteroids: Subgroups and meteorite analogs , 2010 .
[3] T. Gehrels,et al. Physical studies of minor planets , 1971 .
[4] Roger N. Clark,et al. Spectral properties of mixtures of montmorillonite and dark carbon grains: Implications for remote sensing minerals containing chemically and physically adsorbed water , 1983 .
[5] S. Lord. A new software tool for computing Earth's atmospheric transmission of near- and far-infrared radiation , 1992 .
[6] Jennifer L. Piatek,et al. Mineralogical Variations within the S-Type Asteroid Class , 1993 .
[7] Alan W. Harris,et al. A Thermal Model for Near-Earth Asteroids , 1998 .
[8] Sho Sasaki,et al. Developing space weathering on the asteroid 25143 Itokawa , 2006, Nature.
[9] J. Mustard,et al. Effects of Hyperfine Particles on Reflectance Spectra from 0.3 to 25 μm , 1997 .
[10] C. Barbieri,et al. Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites , 1999 .
[11] M. Zolensky,et al. The Kaidun Microbreccia Meteorite: A Harvest from the Inner and Outer Asteroid Belt , 2003 .
[12] Stefano Mottola,et al. Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect , 2007, 0704.1915.
[13] R. Morris,et al. Spectral and other physicochemical properties of submicron powders of hematite (alpha-Fe2O3), maghemite (gamma-Fe2O3), magnetite (Fe3O4), goethite (alpha-FeOOH), and lepidocrocite (gamma-FeOOH). , 1985, Journal of geophysical research.
[14] Thermophysical Characterization of Potential Spacecraft Target (101955) 1999 RQ36 , 2010 .
[15] M. Gaffey. A systematic study of the spectral reflectivity characteristics of the meteorite classes with applications to the interpretation of asteroid spectra for mineralogical and petrological information , 1974 .
[16] Paul Mann,et al. Spectral reflectance properties of carbonaceous chondrites: 1. CI chondrites , 2012 .
[17] R. Binzel,et al. High‐calcium pyroxene as an indicator of igneous differentiation in asteroids and meteorites , 2004 .
[18] A. Dollfus. Physical Studies of Asteroids by Polarization of the Light , 1971 .
[19] Torrence V. Johnson,et al. Optical properties of carbonaceous chondrites and their relationship to asteroids , 1973 .
[20] Richard P. Binzel,et al. Constraining near-Earth object albedos using near-infrared spectroscopy , 2005 .
[21] C. Pieters,et al. Reflectance spectra of some fractions of Migei and Murchison SM chondrites in the range of 0.3-2.6 microns , 1991 .
[22] B. Yang,et al. Water in B-type Asteroids , 2010 .
[23] M. Zolensky,et al. Thermal metamorphism of the C, G, B, and F asteroids seen from the 0.7 μm, 3 μm, and UV absorption strengths in comparison with carbonaceous chondrites , 1996 .
[24] A. Dollfus,et al. 6. The Nature of Asteroid Surfaces, from Optical Polarimetry , 1977 .
[25] Julie Ziffer,et al. Water ice and organics on the surface of the asteroid 24 Themis , 2010, Nature.
[26] R. Binzel,et al. Characterizing the Visible and Near-IR Spectra of Asteroids using Principal Component Analysis , 2003 .
[27] Richard P. Binzel,et al. An extension of the Bus asteroid taxonomy into the near-infrared , 2009 .
[28] Michael Mueller,et al. Surface Properties of Asteroids from Mid-Infrared Observations and Thermophysical Modeling , 2007, 1208.3993.
[29] Faith Vilas,et al. A Cheaper, Faster, Better Way to Detect Water of Hydration on Solar System Bodies , 1994 .
[30] R. S. Hudson,et al. The Shape and Spin of 101955 (1999 RQ36) from Arecibo and Goldstone Radar Imaging , 2007 .
[31] John T. Rayner,et al. SpeX: A Medium‐Resolution 0.8–5.5 Micron Spectrograph and Imager for the NASA Infrared Telescope Facility , 2003 .
[32] Dorian G. W. Smith,et al. Reflectance spectra of mafic silicate-opaque assemblages with applications to meteorite spectra , 1990 .
[33] K. Tsiganis,et al. THE ORIGIN OF ASTEROID 101955 (1999 RQ36) , 2010 .
[34] D. Tholen,et al. Asteroid Taxonomy from Cluster Analysis of Photometry. , 1984 .
[35] C. M. Pieters,et al. Strength of mineral absorption features in the transmitted component of near-infrared reflected light - First results from RELAB. [spectrogoniometer for planetary and lunar surface composition experiments] , 1983 .
[36] M. Gaffey,et al. Composition of 298 Baptistina: Implications for the K/T impactor link , 2009 .
[37] S. N. Milam,et al. The impact and recovery of asteroid 2008 TC3 , 2009, Nature.
[38] J. Mustard,et al. Estimating Absolute H2O Content of Low-Albedo Materials Using Reflectance Spectroscopy , 2006 .