|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
* - 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. 1998-O16
( 2) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes.)
( 3) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes.)
NEODyS Page of ( 12538) 1998 OH