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The population of Near Earth Asteroids in coorbital motion with Venus

Authors: M.H.M. Morais; Morbidelli, A.

Ref.: Icarus 185, 29-38 (2006)

Abstract: We estimate the size and orbital distributions of Near Earth Asteroids (NEAs) that are expected to be in the 1:1 mean motion resonance with Venus in a steady state scenario. We predict that the number of such objects with absolute magnitudes H<18 and H<22 is 0.14±0.03 and 3.5±0.7, respectively. We also map the distribution in the sky of these Venus coorbital NEAs and we see that these objects, as the Earth coorbital NEAs studied in a previous paper, are more likely to be found by NEAs search programs that do not simply observe around opposition and that scan large areas of the sky.

DOI: 10.1016/j.icarus.2006.06.009

URL: cdsads.u-strasbg.fr