Statements (70)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:age |
approximately 12 billion years
most open clusters |
| gptkbp:apparent_magnitude |
10.4
|
| gptkbp:associated_with |
Milky Way halo
|
| gptkbp:conducts_research_on |
galactic formation
|
| gptkbp:contains |
hundreds of thousands of stars
|
| gptkbp:contains_star |
yes
hundreds of thousands low star formation rate type II globular cluster contains several variable stars |
| gptkbp:coordinates |
l = 200.0°, b = -30.0°
|
| gptkbp:declination |
+38° 52′ 30″
+09° 05′ 00″ |
| gptkbp:discovered_by |
gptkb:William_Herschel
|
| gptkbp:discovery_year |
1788
|
| gptkbp:distance_from_earth |
approximately 300,000 light-years
300,000 light years |
| gptkbp:exhibition |
gptkb:New_General_Catalogue
|
| gptkbp:has_color |
B-V = 0.9
B-V = 0.95 |
| gptkbp:has_globular_cluster_characteristics |
yes
|
| gptkbp:has_high_density |
of stars in the core
|
| gptkbp:has_radius |
approximately 150 light years
|
| gptkbp:has_spectral_type |
various types
|
| https://www.w3.org/2000/01/rdf-schema#label |
NGC 2419
|
| gptkbp:is_associated_with |
the Milky Way's outer halo
|
| gptkbp:is_considered |
a distant globular cluster
one of the most distant globular clusters |
| gptkbp:is_known_for |
its large size and distance
|
| gptkbp:is_located_near |
the celestial equator
the Galactic halo |
| gptkbp:is_notable_for |
its unusual orbit
its distance from the Milky Way |
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
various astronomers |
| gptkbp:is_part_of |
gptkb:Local_Group
gptkb:the_Milky_Way_galaxy gptkb:Milky_Way_galaxy the Local Group of galaxies the Hercules constellation group |
| gptkbp:is_studied_for |
its chemical composition
|
| gptkbp:is_studied_in |
stellar dynamics
stellar evolution |
| gptkbp:is_used_in |
stellar population studies
studies of galaxy formation |
| gptkbp:is_visible_from |
northern hemisphere
the northern hemisphere with binoculars Earth with binoculars |
| gptkbp:located_in |
constellation Lynx
|
| gptkbp:mass |
old stars
|
| gptkbp:metallicity |
[ Fe/ H] = -2.1
|
| gptkbp:notable_features |
high concentration of stars
|
| gptkbp:photography |
by amateur astronomers
|
| gptkbp:population_density |
high density of stars
|
| gptkbp:previous_name |
gptkb:C_0735+090
|
| gptkbp:research |
Hubble Space Telescope images
|
| gptkbp:right_ascension |
07h 38m 12.0s
07h 38m 00s |
| gptkbp:scientific_classification |
a distant globular cluster
|
| gptkbp:size |
approximately 150 light-years in diameter
|
| gptkbp:speed |
-200 km/s
|
| gptkbp:storage |
available in databases
|
| gptkbp:type |
gptkb:Population_II_star_cluster
gptkb:star |
| gptkbp:bfsParent |
gptkb:Perseus
gptkb:Globular_Clusters |
| gptkbp:bfsLayer |
5
|