“…Recently, it was used in a somewhat modified form by Bronshten (1 999), who constructed the diagram: (trajectory azimuthHentry velocity) and showed what combinations of these parameters lead to orbits typical of particular classes of bodies (asteroids, short-period comets, and long-period comets) and to hyperbolic orbits. For the most probable trajectory azimuth, 104' (Zotkin, 1972;Bronshten, 1999), cometary orbits correspond to geocentric velocities v , > 27 km/s, whereas for an azimuth of llOo, preferred by Sekanina, the bounding velocity will be 29 k d s . The value a1 = 3 AU is chosen here as a conventional boundary.…”