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* - orbital type derived from osculating orbital elements
$ - diameter range derived from H and assumed albedo for C and S type' - 0.04 and 0.20 respectively
# - absolute magnitude H derived from astrometric observation via orbit determination - G value assumed to be 0.15
( 1) M.P.E.C. 2002-A53
( 2) Binzel, R.P. et al. (2004) Meteorit. Planet. Sci. 39, 351-366. (Dynamical and compositional assessment of near-Earth object mission targets) (new spectra and taxonomy of 22 NEOs)
( 3) Binzel, R.P. et al. (2004) Meteorit. Planet. Sci. 39, 351-366. (Dynamical and compositional assessment of near-Earth object mission targets) (new spectra and taxonomy of 22 NEOs)
NEODyS Page of 2002 AT4