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- GCl_38 abstract "GCl 38 is a globular cluster located in theconstellation Hercules.It was discovered in 1958 by Sidney van den Bergh and Halton Arp during inspection of the photographic plates from the Palomar Sky Survey.This is a round, diffuse cluster located in the outerhalo of the Milky Way galaxy. It is about 3–4 billion years younger than a typical galactic cluster.The metallicity of the cluster is [Fe/H] = −1.50, indicating a lower abundance of elements with mass greater that helium compared to the Sun. The combined mass of the main sequence stars in the cluster is 1340 ± 50 solar masses, and the combined mass of observed stars within the half-light radius is 6020 ± 50 solar masses. (This is the inner radius of the cluster that emits half the total luminosity.) These mass estimates provide lower bounds for determining the total mass of the cluster. The median radial velocity of stars within the cluster is 72.19 ± 0.18 km/s.Because of the cluster's location on the outer fringes of the Milky Way, it was used as a test case for modified newtonian dynamics (MOND). This is an alternative hypothesis to explain the galactic rotation problem.".
- GCl_38 wikiPageID "23538398".
- GCl_38 wikiPageLength "3312".
- GCl_38 wikiPageOutDegree "19".
- GCl_38 wikiPageRevisionID "639769612".
- GCl_38 wikiPageWikiLink Category:Globular_clusters.
- GCl_38 wikiPageWikiLink Constellation.
- GCl_38 wikiPageWikiLink Epoch_(astronomy).
- GCl_38 wikiPageWikiLink Galaxy_rotation_curve.
- GCl_38 wikiPageWikiLink Globular_cluster.
- GCl_38 wikiPageWikiLink Halton_Arp.
- GCl_38 wikiPageWikiLink Helium.
- GCl_38 wikiPageWikiLink Hercules_(constellation).
- GCl_38 wikiPageWikiLink Light-year.
- GCl_38 wikiPageWikiLink Main_sequence.
- GCl_38 wikiPageWikiLink Milky_Way.
- GCl_38 wikiPageWikiLink Modified_Newtonian_dynamics.
- GCl_38 wikiPageWikiLink Parsec.
- GCl_38 wikiPageWikiLink Sidney_van_den_Bergh.
- GCl_38 wikiPageWikiLink Solar_mass.
- GCl_38 wikiPageWikiLink Star.
- GCl_38 wikiPageWikiLink Sun.
- GCl_38 wikiPageWikiLink Year.
- GCl_38 wikiPageWikiLinkText "GCl 38".
- GCl_38 age Year.
- GCl_38 age "10".
- GCl_38 appmagV "14.7".
- GCl_38 constellation Hercules_(constellation).
- GCl_38 distLy Light-year.
- GCl_38 distLy "244000".
- GCl_38 distPc Parsec.
- GCl_38 distPc "74.7".
- GCl_38 epoch Epoch_(astronomy).
- GCl_38 name "GCl 38".
- GCl_38 names "C1608 + 150".
- GCl_38 names "Palomar 14, Arp 1,".
- GCl_38 vHb "20".
- GCl_38 wikiPageUsesTemplate Template:Astronomy-stub.
- GCl_38 wikiPageUsesTemplate Template:DEC.
- GCl_38 wikiPageUsesTemplate Template:Infobox_globular_cluster.
- GCl_38 wikiPageUsesTemplate Template:RA.
- GCl_38 wikiPageUsesTemplate Template:Reflist.
- GCl_38 subject Category:Globular_clusters.
- GCl_38 hypernym Cluster.
- GCl_38 type Language.
- GCl_38 comment "GCl 38 is a globular cluster located in theconstellation Hercules.It was discovered in 1958 by Sidney van den Bergh and Halton Arp during inspection of the photographic plates from the Palomar Sky Survey.This is a round, diffuse cluster located in the outerhalo of the Milky Way galaxy. It is about 3–4 billion years younger than a typical galactic cluster.The metallicity of the cluster is [Fe/H] = −1.50, indicating a lower abundance of elements with mass greater that helium compared to the Sun.".
- GCl_38 label "GCl 38".
- GCl_38 sameAs Q942362.
- GCl_38 sameAs Palomar_14.
- GCl_38 sameAs Palomar_14.
- GCl_38 sameAs Palomar_14.
- GCl_38 sameAs m.06wb3hg.
- GCl_38 sameAs Palomar_14.
- GCl_38 sameAs Q942362.
- GCl_38 sameAs GCl_38.
- GCl_38 wasDerivedFrom GCl_38?oldid=639769612.
- GCl_38 isPrimaryTopicOf GCl_38.