|
gptkbp:instance_of
|
gptkb:galaxy
|
|
gptkbp:angular_size
|
about 30 arcminutes
|
|
gptkbp:apparent_magnitude
|
approximately 10.5
|
|
gptkbp:associated_with
|
gptkb:Leo_constellation
|
|
gptkbp:collaborations
|
collaborative research projects conducted
|
|
gptkbp:contains
|
gptkb:Messier_65
gptkb:NGC_3628
gptkb:NGC_3642
gptkb:NGC_3650
gptkb:Messier_66
|
|
gptkbp:contains_dark_matter
|
dark matter halo
|
|
gptkbp:contains_gas_clouds
|
interstellar gas clouds
|
|
gptkbp:contains_star
|
ongoing star formation
many stars
|
|
gptkbp:declination
|
+13° 00′ 00″
|
|
gptkbp:diameter
|
approximately 100,000 light-years
|
|
gptkbp:discovered_by
|
gptkb:Pierre_Méchain
gptkb:William_Herschel
|
|
gptkbp:discovery_year
|
gptkb:1780
|
|
gptkbp:distance
|
35 million light-years from Earth
|
|
gptkbp:distance_from_earth
|
approximately 35 million light-years
|
|
gptkbp:exhibition
|
gptkb:Messier_Catalog
|
|
gptkbp:has_astrophysical_research
|
subject of astrophysical research
|
|
gptkbp:has_color
|
varied color index
|
|
gptkbp:has_cosmological_importance
|
important for cosmology studies
|
|
gptkbp:has_educational_importance
|
important for educational purposes
|
|
gptkbp:has_features
|
SAB spiral galaxies
|
|
gptkbp:has_galactic_interactions
|
galactic interactions observed
|
|
gptkbp:has_galactic_nucleus
|
gptkb:active_galactic_nucleus
|
|
gptkbp:has_galaxy_clusters
|
associated galaxy clusters
|
|
gptkbp:has_galaxy_dynamics
|
complex galaxy dynamics
|
|
gptkbp:has_gravitational_effects
|
gravitational effects observed
|
|
gptkbp:has_imaging
|
high-resolution imaging available
|
|
gptkbp:has_luminosity
|
high luminosity
|
|
gptkbp:has_observational_data
|
extensive observational data available
|
|
gptkbp:has_photometry
|
photometric measurements taken
|
|
gptkbp:has_publications
|
numerous scientific publications
|
|
gptkbp:has_simulation_studies
|
simulation studies performed
|
|
gptkbp:has_spectral_type
|
various spectral types
|
|
gptkbp:has_spectroscopy
|
spectroscopic studies conducted
|
|
gptkbp:has_supernova
|
gptkb:supernova_remnants
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Leo Triplet
|
|
gptkbp:is_observed_in
|
gptkb:Hubble_Space_Telescope
|
|
gptkbp:lighting
|
low surface brightness
magnitude 12.0
|
|
gptkbp:located_in
|
constellation Leo
|
|
gptkbp:mass
|
estimated mass of 10^12 solar masses
|
|
gptkbp:notable_feature
|
interacting galaxies
|
|
gptkbp:orbital_period
|
tidal interactions present
|
|
gptkbp:part_of
|
gptkb:Virgo_Supercluster
|
|
gptkbp:population_density
|
varied star density
|
|
gptkbp:public_interest
|
of public interest in astronomy.
|
|
gptkbp:redshift
|
0.0023
|
|
gptkbp:research
|
observed since the 18th century
|
|
gptkbp:right_ascension
|
11h 20m 15s
|
|
gptkbp:significance
|
important for studying galaxy interactions
|
|
gptkbp:speed
|
approximately 690 km/s
|
|
gptkbp:type
|
interacting galaxies
spiral galaxy group
|
|
gptkbp:bfsParent
|
gptkb:Messier_65
gptkb:NGC_3628
gptkb:Messier_66
|
|
gptkbp:bfsLayer
|
6
|