This can be a result of accretion driven planetary formation. The number of science projects increase with the number of scientists involved. All AGN projects were tied to interferometry as their study involves the inner sub-parsec regions. Spectra of star clusters to continue study of the age-metallicity degeneracy. Galaxy dynamics of nearby elliptical galaxies.
Main goal is to break the mass-isotropy degeneracy.
Interferometry better than 1 mas to see into the cores of AGNs. Orientation of link for unification pictures. Measure a variety of detailed SF histories using CMD analysis. Measure chemical evolution history. Individual stellar spectroscopy.