Orphan stream

E502433

The Orphan stream is a narrow, elongated stream of stars in the Milky Way’s halo, believed to be the remnants of a disrupted dwarf galaxy or globular cluster.

All labels observed (1)

Label Occurrences
Orphan stream canonical 1

How this entity was disambiguated

Statements (32)

Predicate Object
instanceOf Milky Way halo substructure ⓘ
astronomical structure ⓘ
stellar stream ⓘ
associatedWith possible progenitor dwarf galaxy in Ursa Major region ⓘ
composedOf stars ⓘ
discoveredBy N. W. Evans ⓘ
Sloan Digital Sky Survey ⓘ
Vasily Belokurov ⓘ
discoveredIn 2006 ⓘ
extendsAcross northern Galactic hemisphere ⓘ
hasAlternativeName Orphan stellar stream ⓘ
hasApproximateDistanceFromSun 20–50 kiloparsecs ⓘ
hasApproximateLength ~60 degrees on the sky ⓘ
hasKinematics prograde orbit around Milky Way ⓘ
hasMetallicity [Fe/H] ≈ −1.5 to −2.0 ⓘ
metal-poor ⓘ
hasNotableProperty coherent proper motions in Gaia data ⓘ
large spatial extent ⓘ
low surface brightness ⓘ
hasProgenitorStatus progenitor not definitively identified ⓘ
hasShape elongated ⓘ
narrow ⓘ
locatedIn Milky Way galaxy ⓘ
linked to: Milky Way

Milky Way halo ⓘ
observedBy Gaia space observatory ⓘ
linked to: Gaia observatory

Pan-STARRS ⓘ
linked to: Pan-STARRS survey

Sloan Digital Sky Survey ⓘ
partOf Galactic stellar halo ⓘ
possibleOrigin disrupted dwarf galaxy ⓘ
disrupted globular cluster ⓘ
usedFor studying tidal disruption of satellites ⓘ
tracing Milky Way dark matter halo potential ⓘ

How these facts were elicited

Referenced by (1)

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