Trans-Neptunian objects (TNOs) are primitive remnants of the
planetesimal disk from which the planets of our solar system formed.
They are analogues to the parent bodies of dust in debris disks
observed around other stars. Since 1992 about 1500 TNOs have been
discovered but their basic physical properties have been challenging
to measure. The richness of dynamical structure and varying physical
properties set constraints to models of solar system formation and
evolution.
Herschel Space Observatory open time key program "TNOs are Cool"
observed a sample of 130 TNOs at far-IR wavelengths around their
thermal peaks. The results of radiometric modeling give albedo
and size distributions as well as thermal properties. For
binary systems we obtain an insight in their densities as a
function of size. Thermal light curves of selected targets observed
by Herschel are used together with the optical ones to solve the
ambiguity between shape effects and albedo variegation. Possible
correlations between physical properties
The Universe Colloquium is followed by a social gathering with wine and cheese.