An extension of the Bus asteroid taxonomy into the near-infrared

By F. DeMeo, R. Binzel, S. Slivan, S. Bus. 2009

821 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/78e7f1f15bc17a7891befbbe953fde7655d8cdf2

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Citations in the corpus

Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, background): “Cloutis et al. (2006) interpreted the reflectance spectrum out to ∼1.65 m of O-type (3628) Božněmcová to be consistent with an angrite-like mineralogy, but near-infrared spectra out to 2.5 m of Božněmcová (DeMeo et al., 2009; Burbine et al., 2011) show a 2 m band that is not consistent with an a”
Mineralogies and source regions of near-Earth asteroids (2013, neutral): “Taxonomic classifications (DeMeo et al., 2009) of the NEAs from this study are listed in Appendix A.”
Spectral reflectance properties of carbonaceous chondrites: 1. CI chondrites (2012, background): “This characteristic extends to many possible CC parent bodies, such as cometary nuclei and dark asteroids (e.g., Abell et al., 2005; DeMeo et al., 2009; Clark et al., 2010).”
INITIAL PERFORMANCE OF THE NEOWISE REACTIVATION MISSION (2014, positive): “…diameters can be computed using infrared measurements alone, the combination of visible and thermal measurements allows for determination of albedo, which yields clues as to whether an object is stony or carbonaceous (e.g. Tholen & Barucci 1989; DeMeo et al. 2009; Mainzer et al. 2011e, 2012b).”
Phase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classification (2012, methodology): “For this reason we have decided to combine data from Reddy (2009), DeMeo et al. (2009), Abell et al. (2007), Binzel et al. (2001) and the MIT-UH-IRTF Joint Campaign for NEO Spectral Reconnaissance (NEOSR).”
The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys (2013, methodology): “We base the classification on the 371 spectra used to create the Bus-DeMeo taxonomy (DeMeo et al. 2009), whose classes are very similar those of the Bus taxonomy (Bus and Binzel 2002a), with a few classes removed.”
LSST: From Science Drivers to Reference Design and Anticipated Data Products (2008, methodology): “Spectral energy distributions are assigned using the C and S type asteroids of DeMeo et al. (2009).”
Space weathering and the interpretation of asteroid reflectance spectra (2010, background): “(DeMeo et al. (2009) is an exception to this generalization in that it removes the spectral slope parameter prior to type classification.”
The Compositional Structure of the Asteroid Belt (2015, methodology): “An extension of the Bus taxonomy, the so-called Bus-DeMeo taxonomy, was created to classify both the visible and near-infrared data in such a way as to be as consistent with the Bus taxonomy as possible (DeMeo et al., 2009).”
Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS) (2019, methodology): “Plotted are the first and second principal component scores (PC1′ and PC2′) based on the eigenvectors defined in the BusDeMeo taxonomy (DeMeo et al., 2009), where the input data span visible plus near-infrared wavelengths and the added notation (') indicates spectral slope has been removed prior to ”
Ion irradiation of carbonaceous chondrites: A new view of space weathering on primitive asteroids (2017, background): “Primitive asteroids (C-complex; [Bus & Binzel, 2002; DeMeo et al., 2009]) are especially studied because they are thought to contain organic compounds and some water, key elements for life on Earth.”
SDSS-based taxonomic classification and orbital distribution of main belt asteroids (2010, background): “Direct comparison and mineralogical inferences based on NIR spectra tend to confirm this association for the Q class (Binzel et al. 2001), but the situation is not as clear for the O class (Chapman 1996a; Binzel et al. 2001; Burbine & Binzel 2002; DeMeo et al. 2009).”
Populating the asteroid belt from two parent source regions due to the migration of giant planets—“The Grand Tack” (2012, background): “However, this is not to imply that there are only two specific types of asteroids—rather compositional variations within each group would account for a large variety of asteroid taxonomic classes and meteorite groups (Burbine et al. 2002; Bus et al. 2002; DeMeo et al. 2009).”
Density of asteroids (2012, methodology): “These asteroids have been grouped together in the taxonomy by DeMeo et al. (2009) owing to their spectra similarity.”
Planetary Spectrum Generator: An accurate online radiative transfer suite for atmospheres, comets, small bodies and exoplanets (2018, methodology): “Bus-DeMeo asteroid taxonomy with 25 classes based on PCA of combined visible and near-IR spectral data [68] Number of components: 25 Spectral coverage: 0.”
Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations (2012, neutral): “The taxonomy data were taken from Tholen (1989), Bus and Binzel (2002), DeMeo et al. (2009), Xu et al. (1995), and Lazzaro et al. (2004), as compiled in Neese (2010); they are given in columns Taxon.”
MAIN BELT ASTEROIDS WITH WISE/NEOWISE. I. PRELIMINARY ALBEDOS AND DIAMETERS (2011, background): “IR reflectance The reflectance spectrum for most asteroids (but not all, e.g. B-types) show an increasing value as the wavelength moves from the visible to near-infrared (NIR) region of the spectrum (e.g. DeMeo et al. 2009, etc.).”