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- Q591406 subject Q14756017.
- Q591406 subject Q6214716.
- Q591406 subject Q6791927.
- Q591406 subject Q7191717.
- Q591406 subject Q7217170.
- Q591406 subject Q8529727.
- Q591406 abstract "Template:ForIn astronomy, the Hills cloud (also called the inner Oort cloud and inner cloud) is a vast theoretical circumstellar disc, interior to the Oort cloud, whose outer border would be located at around 20,000 to 30,000 astronomical units (AU) from the Sun, and whose inner border, less well defined, is hypothetically located at 100-3,000 AU, well beyond planet and Kuiper-belt object orbits, but distances might be much greater. If it exists, the Hills cloud contains roughly 5 times as many comets as the Oort cloud.Oort cloud comets are continually perturbed by their environment. A non-negligible fraction leaves the Solar System or goes in the inner system. Hence it should have depleted itself long ago, but it has not. The Hills cloud theory addresses the longevity of the Oort cloud by postulating a densely populated inner Oort region. Objects ejected from the Hills cloud are likely to end up in the classical Oort cloud region, maintaining the Oort cloud. It is likely that the Hills cloud is the largest concentration of comets in the whole Solar System.The existence of the Hills cloud is plausible, since many bodies have been found already. It would be denser than the Oort cloud, but much smaller. Gravitational interaction with the closest stars and tidal effects from the galaxy have given circular orbits to the comets in the Oort cloud, which must not be the case for the comets in the Hills cloud. The Hills cloud's total mass is unknown; some scientists think it would be more massive than the Oort cloud.".
- Q591406 thumbnail Kuiper_oort.jpg?width=300.
- Q591406 wikiPageExternalLink nph-bib_query?bibcode=1986Icar...65...13H&db_key=AST&data_type=HTML&format=&high=44b52c369006969.
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- Q591406 wikiPageWikiLink Q8529727.
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- Q591406 comment "Template:ForIn astronomy, the Hills cloud (also called the inner Oort cloud and inner cloud) is a vast theoretical circumstellar disc, interior to the Oort cloud, whose outer border would be located at around 20,000 to 30,000 astronomical units (AU) from the Sun, and whose inner border, less well defined, is hypothetically located at 100-3,000 AU, well beyond planet and Kuiper-belt object orbits, but distances might be much greater.".
- Q591406 label "Hills cloud".
- Q591406 depiction Kuiper_oort.jpg.