Aims. Here we continue to discuss the principle of the local measurement of dark energy using the normalized Hubble diagram describing the environment of a system of galaxies. Methods. We calculate the present locus of test particles injected a fixed time ago (∼the age of the universe), in the standard Λ cosmology and for different values of the system parameters (the model includes a central point mass M and a local dark energy density ρ loc ) and discuss the position of the zero-gravity distance R v in the Hubble diagram. Results. Our main conclusion are: 1) when the local DE density ρ loc is equal to the global DE density ρ v , the outflow reaches the global Hubble rate at the distance R 2 = (1 + z v )R v , where z v is the global zero-acceleration redshift (≈0.7 for the standard model). This is also the radius of the ideal Einstein-Straus vacuole, 2) for a wide range of the local-to-global dark energy ratio ρ loc /ρ v , the local flow reaches the known global rate (the Hubble constant) at a distance R 2 > ∼ 1.5 × R v . Hence, R v will be between R 2 /2 and R 2 , giving upper and lower limits to ρ loc /M. For the Local Group, this supports the view that the local density is near the global one.