Keck observations of near-Earth asteroids in the thermal infrared

By M. Delbo’, Alan W. Harris, R. Binzel, P. Pravec, J. Davies. 2003

152 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/7320efe3abc7ab20cd6210c4f3fe5ae1c6076528

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In Astronomy and Astrophysics

Citations in the corpus

The sizes, shapes, albedos, and colors of cometary nuclei (2004, background): “The beaming parameter η, however, is still largely unconstrained for comets and remains the largest uncertainty; we are only beginning to understand the variety of values possible for near-Earth asteroids comparable in size to the cometary nuclei (e.g., Delbo et al., 2003).”
NEOWISE OBSERVATIONS OF NEAR-EARTH OBJECTS: PRELIMINARY RESULTS (2011, background): “While a rigorous comparison of our results with those of earlier studies (Delbó et al. 2003; Harris 2006, e.g.) would require data for NEOs of the same taxonomic types in the same size range, our result suggests that the apparent correlations between size and albedo reported by others could be…”
Physical Properties of Kuiper Belt and Centaur Objects: Constraints from the Spitzer Space Telescope (2007, methodology): “L., Cruikshank D. P. , Emery J. P.et al. (2006). The Albedo, Size, and Density of Binary Kuiper Belt Object (47171) 1999 TC 36.”
PRELIMINARY RESULTS FROM NEOWISE: AN ENHANCEMENT TO THE WIDE-FIELD INFRARED SURVEY EXPLORER FOR SOLAR SYSTEM SCIENCE (2011, methodology): “As with visible data, shape and rotation state can be derived from WISE observations (c.f. Delbó et al. 2003; Wright et al. 2007).”
Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect (2007, methodology): “…generated through a TPM, using realistic distributions of the input parameters P, θSS, θSE, φSE, and A derived from the literature (see Table 1 with published η-values from Harris, 1998, Harris et al. (1998); Harris and Davies (1999); Delbo’ et al. (2003); Delbo’ (2004); and Wolters et al. (2005).”
Bias-corrected population, size distribution, and impact hazard for the near-Earth objects (2004, methodology): “There are suggestions that the albedos of S-type asteroids increase with decreasing size when main-belt asteroids are combined with NEOs (Binzel et al., 2002b, 2004; Delbo et al., 2003).”
Near Earth Asteroids with measurable Yarkovsky effect (2012, methodology): “The rectangles correspond to reasonable values of q according to the taxonomic type and to a reasonable range of C (Delbó et al., 2007). D. Farnocchia et al. / Icarus 224 (2013) 1–13 11”