Table 2: Model calculations to find the minimum speed and maximum deviation of the ejected particle from the solar direction. The parent objects are moving on circular orbits (cf. Wehry & Mann 1999).

e0
$q({\rm AU})$ $\beta $ $\gamma(^{\circ})$ $v({\rm {km}~{s^{-1}}})$
      $2.5~ {\rm AU}$ $2.5~ {\rm AU}$

0
0.3 0.5 14 19
  0.8 0.5 24 19
0.3 0.3 0.4 11 27
  0.8 0.4 21 27
0.6 0.3 0.2 14 24
  0.8 0.2 24 24
0.9 0.3 0.2 9 38
  0.8 0.2 19 38
e0  eccentricity of the parent body;
q  perihelion distance;
$\gamma$  angle between the direction of the Sun and the particle velocity;
v  heliocentric speed.


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