|
gptkbp:instanceOf
|
star
|
|
gptkbp:contains
|
old stars
|
|
gptkbp:diameter
|
approximately 1,000 light-years
|
|
gptkbp:established
|
Ibata_et_al.
|
|
gptkbp:geographicalFeature
|
RA 18h 55m 01s, Dec -30° 30′ 00″
|
|
gptkbp:hasAwards
|
yes
|
|
gptkbp:hasCharacter
|
no
|
|
gptkbp:hasCitations
|
dynamically relaxed
isotropic velocity dispersion
|
|
gptkbp:hasColor
|
yes
|
|
gptkbp:hasFilm
|
spheroidal
|
|
gptkbp:hasGoals
|
yes
|
|
gptkbp:hasLength
|
70,000 to 80,000 light-years
|
|
gptkbp:hasLocation
|
low heavy element abundance
|
|
gptkbp:hasPersonnel
|
approximately 12 billion years
|
|
gptkbp:hasPopulation
|
mostly old stars
|
|
gptkbp:hasRelatedPatent
|
dwarf spheroidal
|
|
gptkbp:hasResidence
|
[Fe/H] = -1.5
|
|
gptkbp:hasSibling
|
very low
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Sagittarius Dwarf Spheroidal Galaxy
|
|
gptkbp:interactsWith
|
Milky Way Galaxy
|
|
gptkbp:isAccessibleBy
|
yes
|
|
gptkbp:isAssociatedWith
|
Sagittarius_stream
|
|
gptkbp:isConsidered
|
a candidate for tidal disruption
|
|
gptkbp:isFiledIn
|
B-V = 0.8
|
|
gptkbp:isIntegratedWith
|
with_Milky_Way
|
|
gptkbp:isPartOf
|
gptkb:Sagittarius_constellation
gptkb:Sagittarius_II_group
galaxy formation and evolution
|
|
gptkbp:isReferencedIn
|
1994 paper by Ibata et al.
|
|
gptkbp:isRelatedTo
|
gptkb:Milky_Way's_halo
|
|
gptkbp:isServedBy
|
gptkb:Hubble_Space_Telescope
|
|
gptkbp:isStudiedIn
|
astrophysics
|
|
gptkbp:isTrainedIn
|
dark matter studies
|
|
gptkbp:length
|
14.5
approximately 70,000 light-years
|
|
gptkbp:lighting
|
very low
|
|
gptkbp:localAttraction
|
-110_km/s
|
|
gptkbp:locatedIn
|
constellation_Sagittarius
|
|
gptkbp:mission
|
no
|
|
gptkbp:notableFeature
|
low metallicity
|
|
gptkbp:orbitalInclination
|
about 1.5 billion years
|
|
gptkbp:partOf
|
gptkb:Local_Group
|
|
gptkbp:region
|
no
|
|
gptkbp:releaseYear
|
1994
|
|
gptkbp:resolution
|
very low
about 1.5 x 10^5 solar luminosities
|
|
gptkbp:type
|
satellite galaxy of the Milky Way
|
|
gptkbp:weight
|
about 1.5 x 10^7 solar masses
|