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We present the $360^\circ$ catalogue of physical properties of Hi-GAL compactsources, detected between 70 and 500 $\mu$m. This release not only completesthe analogous catalogue previously produced by the Hi-GAL collaboration for$-71^\circ \lesssim \ell \lesssim 67^\circ$, but also meaningfully improves itthanks to a new set of heliocentric distances, 120808 in total. About a thirdof the 150223 entries are located in the newly added portion of the Galacticplane. A first classification based on detection at 70 $\mu$m as a signature ofongoing star-forming activity distinguishes between protostellar sources(23~per cent of the total) and starless sources, with the latter furtherclassified as gravitationally bound (pre-stellar) or unbound. The integral ofthe spectral energy distribution, including ancillary photometry from$\lambda=21$ to 1100 $\mu$m, gives the source luminosity and other bolometricquantities, while a modified black body fitted to data for $\lambda \geq 160\,\mu$m yields mass and temperature. All tabulated clump properties are thenderived using photometry and heliocentric distance, where possible. Statisticsof these quantities are discussed with respect to both source Galactic locationand evolutionary stage. No strong differences in the distributions ofevolutionary 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 starformation. Median behaviour of distance-independent parameters tracing sourceevolutionary status is examined as a function of the Galactocentric radius,showing no clear evidence of correlation with spiral arm positions.

The Hi-GAL compact source catalogue -- II. The 360{\deg} catalogue of clump physical properties