Density and Axis-size relationship of five main-belt asterids: 2017 January-March

Despite many decades of minor planet studies focused
on external and dynamical properties, there are still
hundreds of asteroids that have never been measured.
Presented here are the results of photometric analysis
applied to five main-belt asteroids. In addition to
calculating rotation period, axis ratios assuming a simple
ellipsoidal shape and the estimated minimum density of
each asteroid are reported.

2017MPBu___44__276A

Associated tables:

T1
T2