gptkbp:instance_of
|
gptkb:star
|
gptkbp:bfsLayer
|
3
|
gptkbp:bfsParent
|
gptkb:Columba
gptkb:Globular_Clusters
|
gptkbp:age
|
approximately 13 billion years
|
gptkbp:apparent_magnitude
|
+7.2
|
gptkbp:contains
|
millions of stars
including RR Lyrae stars
|
gptkbp:declination
|
-40° 02′ 00″
|
gptkbp:depicted_in
|
with binoculars
|
gptkbp:diameter
|
approximately 150 light years
|
gptkbp:discovered_by
|
gptkb:John_Herschel
|
gptkbp:distance
|
approximately 42,000 light years
|
gptkbp:has
|
multiple stellar populations
|
gptkbp:has_color
|
B-V = 0.85
|
https://www.w3.org/2000/01/rdf-schema#label
|
NGC 1851
|
gptkbp:is_located_near
|
gptkb:NGC_1850
|
gptkbp:is_observed_in
|
gptkb:Hubble_Space_Telescope
|
gptkbp:is_part_of
|
gptkb:Milky_Way_galaxy
Herschel 400 catalog
|
gptkbp:is_studied_in
|
stellar evolution research
|
gptkbp:located_in
|
constellation Columba
|
gptkbp:metallicity
|
[ Fe/ H] = -1.25
|
gptkbp:notable_for
|
its bright core
|
gptkbp:right_ascension
|
05h 14m 00s
|
gptkbp:subspecies
|
G Cl 12
|
gptkbp:type
|
gptkb:Population_II_star_cluster
|
gptkbp:year_created
|
1837
|