The origin of halley-type comets: Probing the inner Oort cloud

We have integrated the orbits of 27,700 test particles initially entering t he planetary system from the Oort cloud in order to study the origin of Hal ley-type comets (HTCs). We included the gravitational influence of the Sun, giant planets, passing stars, and Galactic tides. We find that an isotropi cally distributed Oort cloud does not reproduce the observed orbital elemen t distribution of the HTCs. In order to match the observations, the initial inclination distribution of the progenitors of the HTCs must be similar to the observed HTC inclination distribution. We can match the observations w ith an Oort cloud that consists of an isotropic outer cloud and a disklike massive inner cloud. These idealized two-component models have inner disks with median inclinations that range from 10 degrees to 50 degrees. This ana lysis represents the first link between observations and the structure of t he inner Oort cloud.