
Hills cloud
Vast, theoretical circumstellar disc

Vast, theoretical circumstellar disc
In astronomy, the Hills cloud (also called the inner Oort cloud and inner cloud) is a theoretical vast circumstellar disc, interior to the Oort cloud and roughly aligned with the solar ecliptic plane, 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 250–1500 AU, well beyond planetary and Kuiper Belt object orbits—but distances might be much greater. If it exists, the Hills cloud likely contains roughly five times as many comets as the Oort cloud.
Read on Wikipedia · Image NASA/ESA and A. Feild (Space Telescope Science Institute), Public domain
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