Vicinity of (7) Iris in the a_p vs. sin I_p space of proper orbital elements. The eccentricity range is e_p ∈ (0.162;0.262). Asteroids with albedo within ± 0.1 of the Iris value (p_V = 0.252), are plotted in yellow, with symbol size proportional to the body diameter. Asteroids with unknown albedo are plotted as gray dots. The family visible at sin I_p ≐ 0.09 is related to the dark C-type asteroid (163) Erigone. The dashed ellipse corresponds to the escape velocity from Iris, v_esc ≐ 130 m s⁻¹, converted to orbital elements using the Gauss equations. This velocity was computed for true anomaly f = 180° and argument of perihelion ω = 0°.