Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes

By R. Binzel, A. Rivkin, J. S. Stuart, Alan W. Harris, S. Bus, T. Burbine. 2004

339 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/68322b481ee52cb846c6f6c790f9326e39fdbf5a

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Citations in the corpus

PRELIMINARY RESULTS FROM NEOWISE: AN ENHANCEMENT TO THE WIDE-FIELD INFRARED SURVEY EXPLORER FOR SOLAR SYSTEM SCIENCE (2011, background): “…(NEOs), hundreds of thousands of Main Belt asteroids (MBAs) and ∼3000 comets have been discovered to date, detailed physical characterizations have been made for only a small fraction of these objects (e.g., Binzel et al. 2004; Wolters et al. 2008; Harris et al. 2009; Bhattacharya et al. 2010).”
An extension of the Bus asteroid taxonomy into the near-infrared (2009, background): “All these observations were taken on telescope KPNO 4m except 944 on Magellan 6.5m. f Visible data: Binzel et al. (2004b). g Visible data: Binzel et al. (2001). h Near-IR data: Binzel et al. (2004a). i Near-IR data: Rivkin et al. (2005).”
Phase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classification (2012, methodology): “The spectra of the NEAs at visible wavelengths used in the present work were taken from Binzel et al. (2001, 2004) and DeMeo et al. (2009).”
THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics (2006, background): “These bodies have a wide range of taxonomic types (e.g., Binzel et al. 2004).”
SDSS-based taxonomic classification and orbital distribution of main belt asteroids (2010, background): “Both classes are rare among asteroids, with Q-class asteroids observed mostly among the NEO population (Binzel et al. 2004; Mothé-Diniz & Nesvorný 2008).”
Mineralogies and source regions of near-Earth asteroids (2013, background): “Q-type spectra that experience space weathering processes redden and darken to match S-type spectra (Binzel et al., 2004, 1996; Chapman 1996; Sunshine et al., 1993).”
The Compositional Structure of the Asteroid Belt (2015, background): “…and asteroid records lack a substantial population of olivine-dominated or pyroxenedominated bodies (Burbine et al., 1996, Bus & Binzel 2002a, Binzel et al., 2004, Lazzaro et al., 2004, Carvano et al., 2010, DeMeo & Carry 2013), aside from HEDs and Vestoids linked to Vesta (Consolmagno &…”
Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS) (2019, methodology): “55 μm using an average for the visible spectrum (dashed line; Bus and Binzel 2002a; Binzel et al., 2004).”
Evidence for asteroid space weathering from the Sloan Digital Sky Survey (2005, methodology): “, 2002; Morbidelli an Vokrouhlický, 2003; Binzel et al., 2004 ). Whiteley (2001) andBinzel et al.”
Bias-corrected population, size distribution, and impact hazard for the near-Earth objects (2004, methodology): “This correlation is better explaine a dependence of albedo on the jovian Tisserand par ter (Fernández et al., 2001; Binzel et al., 2004).”