Two-color polarimetric observations of C-type asteroid 2100 Ra-Shalom were
conducted when its phase angle was 59.7 degrees. No other C-type asteroid h
as so far been observed at such a large phase angle. We relate the new data
point to the available data on C-type asteroids and on Phobos and Deimos a
nd compare the phase curve of these objects with the phase curve of dusty c
omets. The observed polarization of Ra-Shalom is slightly lower than expect
ed from a common curve of the other C-type asteroids and the martian moons.
We conclude that this may be caused by the immature regolith on the surfac
e of this small asteroid. (C) 1999 Academic Press.