M. Patzold et al., Mass and density determinations of 140 Siwa and 4979 Otawara as expected from the Rosetta flybys, ASTRON ASTR, 370(3), 2001, pp. 1122-1127
During its interplanetary cruise to comet P/Wirtanen, the Rosetta spacecraf
t will encounter the asteroids 4979 Otawara and 140 Siwa on 11 July 2006 an
d 24 July 2008, respectively. The objective of the Rosetta Radio Science in
vestigations (RSI) experiment at these flybys is a determination of the ast
eroid's mass and bulk density by analyzing the radio tracking data (Doppler
and range) received from Rosetta before, during and after closet approach.
The spacecraft's flyby trajectory will be gravitationally deflected by an
amount proportional to the mass of the asteroid for a given flyby distance
and velocity. An analysis of the Doppler noise sources indicates that the m
ass can be determined to an accuracy of 1% for 140 Siwa. The corresponding
bulk density show be accurate to 20%. Unfortunately, a detectable trajector
y perturbation seems to be hopeless for Otawara because of its small size a
nd the large nominal flyby distance.