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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
! - quality code according to Lagerkvist et al. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.),' Univ.Ariz.Press, Tucson, USA, pp. 1162-1179.
( 1) M.P.E.C. 1994-P07
( 2) Pravec, P. et al. (2012) Icarus 221, 365-387 (Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations)
( 3) Pravec, P. et al. (2012) Icarus 221, 365-387 (Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations)
( 4) Petr Pravec's Ondrejov NEO Photometric Program Webpage
( 5) R. Behrend Courbes des lumiere, Observatoire de Geneve website
( 6) JPL's NEO Radar Detection Program Webpage
NEODyS Page of ( 37655) Illapa