|
gptkbp:instance_of
|
gptkb:galaxy
|
|
gptkbp:apparent_magnitude
|
10.5
-12.0
|
|
gptkbp:contains
|
old stars
|
|
gptkbp:contains_star
|
very low star formation rate
|
|
gptkbp:diameter
|
approximately 1.5 kpc
|
|
gptkbp:discovered_by
|
gptkb:Harlow_Shapley
gptkb:Robert_G._Harrington
|
|
gptkbp:discovery_year
|
1950
|
|
gptkbp:distance_from_earth
|
820000 light years
|
|
gptkbp:has_color
|
B-V = 0.9
|
|
gptkbp:has_spectral_type
|
gptkb:spiral_galaxy
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Leo I Galaxy
|
|
gptkbp:is_associated_with
|
gptkb:Leo_constellation
|
|
gptkbp:is_characterized_by
|
high dark matter content
|
|
gptkbp:is_home_to
|
globular clusters
|
|
gptkbp:is_known_for
|
low luminosity
|
|
gptkbp:is_located_at
|
RA 10h 08m 00s, Dec +12° 18′ 00″
|
|
gptkbp:is_located_near
|
gptkb:Virgo_Cluster
|
|
gptkbp:is_observed_in
|
gptkb:Hubble_Space_Telescope
|
|
gptkbp:is_part_of
|
gptkb:Laniakea_Supercluster
gptkb:Local_Group
gptkb:Virgo_Supercluster
|
|
gptkbp:is_studied_for
|
galactic evolution
|
|
gptkbp:is_studied_in
|
astrophysics
|
|
gptkbp:is_visible_from
|
with telescopes
under dark skies
|
|
gptkbp:lighting
|
19.5 mag/arcsec²
|
|
gptkbp:located_in
|
gptkb:Virgo_constellation
constellation Leo
|
|
gptkbp:mass
|
approximately 10 million solar masses
|
|
gptkbp:metallicity
|
low metallicity
|
|
gptkbp:orbit_type
|
gptkb:Leo_II_Galaxy
Leo I II
Leo I III
Leo I IV
|
|
gptkbp:redshift
|
0.0023
|
|
gptkbp:type
|
gptkb:spiral_galaxy
|