  We present the $360^\circ$ catalogue of physical properties of Hi-GAL compact
sources, detected between 70 and 500 $\mu$m. This release not only completes
the analogous catalogue previously produced by the Hi-GAL collaboration for
$-71^\circ \lesssim \ell \lesssim 67^\circ$, but also meaningfully improves it
thanks to a new set of heliocentric distances, 120808 in total. About a third
of the 150223 entries are located in the newly added portion of the Galactic
plane. A first classification based on detection at 70 $\mu$m as a signature of
ongoing star-forming activity distinguishes between protostellar sources
(23~per cent of the total) and starless sources, with the latter further
classified as gravitationally bound (pre-stellar) or unbound. The integral of
the spectral energy distribution, including ancillary photometry from
$\lambda=21$ to 1100 $\mu$m, gives the source luminosity and other bolometric
quantities, while a modified black body fitted to data for $\lambda \geq 160\,
\mu$m yields mass and temperature. All tabulated clump properties are then
derived using photometry and heliocentric distance, where possible. Statistics
of these quantities are discussed with respect to both source Galactic location
and evolutionary stage. No strong differences in the distributions of
evolutionary indicators are found between the inner and outer Galaxy. However,
masses and densities in the inner Galaxy are on average significantly larger,
resulting in a higher number of clumps that are candidates to host massive star
formation. Median behaviour of distance-independent parameters tracing source
evolutionary status is examined as a function of the Galactocentric radius,
showing no clear evidence of correlation with spiral arm positions.
