Globular clusters

GPTKB entity

Statements (51)
Predicate Object
gptkbp:instanceOf Astronomical object
gptkbp:age 10-13 billion years
gptkbp:cataloguedIn gptkb:NGC_catalogue
gptkb:William_Herschel
gptkb:Charles_Messier
gptkbp:composedOf gptkb:Stars
gptkbp:contains gptkb:Population_II_stars
Low metallicity stars
Old stars
gptkbp:coreDensity Very high
gptkbp:discoveredBy gptkb:Abraham_Ihle
1665
gptkbp:distanceFromEarth Several thousand to hundreds of thousands of light-years
gptkbp:distinctFrom Open clusters
gptkbp:distribution Spherically distributed around galactic centers
gptkbp:doNotContain Significant amounts of gas and dust
Young stars
gptkbp:doNotShow Significant star formation
gptkbp:example gptkb:Messier_13
gptkb:Messier_22
gptkb:Omega_Centauri
gptkb:Messier_15
gptkb:47_Tucanae
gptkbp:formationEpoch gptkb:Early_universe
gptkbp:foundIn gptkb:Galaxies
https://www.w3.org/2000/01/rdf-schema#label Globular clusters
gptkbp:locatedIn gptkb:Galactic_bulge
gptkb:Galactic_halo
gptkbp:luminosity Can be visible to naked eye
Up to a million times the Sun
gptkbp:mass 10^4 to 10^6 solar masses
gptkbp:mayInclude gptkb:X-ray_binaries
Pulsars
Blue straggler stars
gptkbp:numberInMilkyWay About 150-180
gptkbp:observedBy Telescopes
gptkbp:orbitType Galactic center
gptkbp:rating Tens of thousands to millions
gptkbp:shape Spherical
gptkbp:stellarPopulation Homogeneous
Multiple populations (in some clusters)
gptkbp:studiedIn Cosmology
Stellar evolution
Galactic formation
gptkbp:subjectOf Astrophysical research
gptkbp:usedFor Measuring age of the universe
Studying stellar dynamics
Tracing galactic history
gptkbp:bfsParent gptkb:Subdwarf
gptkb:Galaxies
gptkbp:bfsLayer 6