Hills cloud

E106161

The Hills cloud is a hypothesized dense inner region of the Oort Cloud thought to be a major reservoir of long-period comets surrounding the outer Solar System.

All labels observed (1)

Label Occurrences
Hills cloud canonical 1

How this entity was disambiguated

Statements (25)

Predicate Object
instanceOf comet reservoir
component of the Oort Cloud
hypothetical astronomical structure
alsoKnownAs Oort cloud
surface form: inner Oort Cloud
characterizedAs major reservoir of long-period comets
contains long-period comets
describedAs dense inner region of the Oort Cloud
distinguishedFrom Oort cloud
surface form: outer Oort Cloud
hasDensityComparedTo denser than outer Oort Cloud
hasOuterBoundaryRelationTo Oort cloud
surface form: classical Oort Cloud
hasRelationTo Solar System formation theories
dynamical evolution of comets
hasRole source region for some long-period comets
hasStatus hypothetical
hasTheoreticalSupportFrom dynamical simulations of comet orbits
hasUncertainProperty exact population of comets
exact spatial extent
hypothesizedBy Jack G. Hills
locatedIn outer Solar System
namedAfter Jack G. Hills
orbits Sun
partOf Oort cloud
surface form: Oort Cloud
spatiallySurrounds Kuiper Belt
surface form: Kuiper Belt (at much larger distances)
studiedInField astronomy
planetary science

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.