Spectral Properties of Near-Earth Objects: Palomar and IRTF Results for 48 Objects Including Spacecraft Targets (9969) Braille and (10302) 1989 ML

By R. Binzel, Alan W. Harris, S. Bus, T. Burbine. 2001

175 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/df0aa895b5ddf42ca4a8645c732674b6f3596227

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In Astronomy and Astrophysics

1. F. DeMeo
2. R. Binzel
3. S. Bus
4. S. Slivan
5. J. Carvano
6. D. Lazzaro
7. T. Mothé-Diniz
8. P. Hasselmann

Citations in the corpus

• 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).”
• 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).”
• An experimental approach to understanding the optical effects of space weathering (2007, methodology): “12 are shown reflectance spectra of two near-Earth S-type asteroids (Binzel et al., 2001) compared to samples from the SG2, SG6 and SG25 suites.”
• The rate of small impacts on Earth (2006, background): “Although NEOs appear to show a greater spectral diversity than Main Belt asteroids (Binzel et al. 2001), they are also a closer match to the meteorite population.”