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gptkbp:instance_of
|
gptkb:Agave
gptkb:supermassive_black_hole
|
|
gptkbp:affects
|
movimiento de estrellas
|
|
gptkbp:associated_with
|
the radio source Sgr A*
emisión de rayos X
|
|
gptkbp:conducts_research_on
|
gptkb:cosmology
gptkb:general_relativity
|
|
gptkbp:coordinates
|
Right Ascension 17h 45m 40.040s, Declination -29° 0' 28.118"
|
|
gptkbp:discovered_by
|
gptkb:Andrea_Ghez
gptkb:Reinhard_Genzel
gptkb:Karl_Jansky
|
|
gptkbp:distance_from_earth
|
26,000 años luz
approximately 26,000 light years
|
|
gptkbp:event_horizon
|
sí
|
|
gptkbp:file_system
|
yes
sí
|
|
gptkbp:has
|
un entorno dinámico
|
|
gptkbp:has_a_focus_on
|
theoretical astrophysics
observational campaigns
scientific inquiry.
many astronomical studies
black hole imaging projects
stellar orbit studies
|
|
gptkbp:has_gravitational_effects_on
|
surrounding stars
|
|
gptkbp:has_nearby_stars
|
yes
|
|
gptkbp:has_supernova
|
yes
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Sagitario A*
|
|
gptkbp:image
|
gptkb:2019
|
|
gptkbp:influence
|
estrellas cercanas
|
|
gptkbp:influences
|
the orbits of nearby stars
|
|
gptkbp:is_a
|
gptkb:supermassive_black_hole
|
|
gptkbp:is_a_center_for
|
gptkb:Milky_Way_Galaxy
the Milky Way's dynamics
|
|
gptkbp:is_a_source_of
|
high-energy astrophysical phenomena
gravitational lensing effects
various astrophysical jets
|
|
gptkbp:is_a_subject_of
|
gptkb:documentaries
public interest
numerous scientific papers
public fascination
|
|
gptkbp:is_akey_focus_in
|
modern astrophysics
|
|
gptkbp:is_aresearch_topic_in
|
quantum gravity
|
|
gptkbp:is_associated_with
|
stellar dynamics
|
|
gptkbp:is_atype_of
|
gptkb:active_galactic_nucleus
|
|
gptkbp:is_considered
|
a key to understanding dark matter
|
|
gptkbp:is_involved_in
|
gravitational wave research
|
|
gptkbp:is_linked_to
|
the formation of stars
|
|
gptkbp:is_located_at
|
gptkb:star
|
|
gptkbp:is_observed_in
|
gptkb:Event_Horizon_Telescope
telescopios de radio
|
|
gptkbp:is_part_of
|
gptkb:Sagittarius_constellation
|
|
gptkbp:is_significant_for
|
understanding galaxy formation
|
|
gptkbp:is_studied_for
|
its accretion processes
|
|
gptkbp:is_studied_in
|
astrophysics
radio telescopes
|
|
gptkbp:is_surrounded_by
|
nubes de gas y polvo
|
|
gptkbp:is_the_center_of_mass_for
|
the Milky Way's gravitational field
|
|
gptkbp:is_the_most_massive_object_in
|
gptkb:the_Milky_Way_Galaxy
|
|
gptkbp:is_theoretical_model_for
|
black hole physics
|
|
gptkbp:is_visible_from
|
infrared spectrum
|
|
gptkbp:lighting
|
yes
|
|
gptkbp:located_in
|
gptkb:Vía_Láctea
gptkb:Milky_Way_Galaxy
|
|
gptkbp:mass
|
4.1 million solar masses
4.1 millones de masas solares
|
|
gptkbp:part_of
|
núcleo galáctico
|
|
gptkbp:targets
|
gptkb:space_mission
|
|
gptkbp:type
|
gptkb:radio_station
|
|
gptkbp:was_akey_figure_in
|
the Milky Way's structure
|