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The universality of semiclassical gravity is investigated by considering thebehavior of the quantities < \phi^2 > and < {T^a}_b >, along with quantumcorrections to the effective Newtonian potential in the far field limits ofstatic spherically symmetric objects ranging from stars in the weak fieldNewtonian limit to black holes. For scalar fields it is shown that whendifferences occur they all result from the behavior of a single mode with zerofrequency and angular momentum and are thus due to a combination of infraredand s-wave effects. An intriguing combination of similarities and differencesbetween the extreme cases of a Schwarzschild black hole and a star in the weakfield Newtonian limit is explained.Comment: Title change, some details added, minor changes, acknowledgement  added, references added, 7 pages, no figure

Apparent universality of semiclassical gravity in the far field limit