Statements (68)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:medical_imaging
gptkb:star |
| gptkbp:advances |
influence on future space missions
|
| gptkbp:analysis |
involves complex modeling
important for analysis |
| gptkbp:archaeological_findings |
documented in scientific literature
|
| gptkbp:associated_with |
black hole candidates
|
| gptkbp:collaboration |
international astronomical community
various space agencies |
| gptkbp:collaborations |
enhance research capabilities
involves multiple institutions |
| gptkbp:collaborative_projects |
involving global research teams
|
| gptkbp:collection |
ongoing research efforts
|
| gptkbp:community |
actively studies its properties.
|
| gptkbp:community_engagement |
featured in science outreach programs
|
| gptkbp:conference |
discussed in astrophysics meetings
|
| gptkbp:contains_star |
a normal star
|
| gptkbp:cross_disciplinary_research |
involves physics and astronomy
|
| gptkbp:discovered_by |
gptkb:NASA
|
| gptkbp:discovery_year |
gptkb:1971
|
| gptkbp:distance_from_earth |
approximately 10,000 light years
|
| gptkbp:economic_impact |
advances in detection methods
|
| gptkbp:educational_value |
used in academic studies
|
| gptkbp:file_system |
present
|
| gptkbp:first_appearance |
gptkb:1971
|
| gptkbp:first_xray_source |
identified in the 1970s
|
| gptkbp:funding |
supported by various grants
allocated for ongoing studies |
| gptkbp:future_prospects |
planned for deeper observations
|
| gptkbp:has_implications_for |
for stellar dynamics and evolution
|
| gptkbp:has_luminosity |
varies with time
about 1000 times that of the Sun |
| gptkbp:has_spectral_type |
varies with observations
|
| https://www.w3.org/2000/01/rdf-schema#label |
Centaurus X-20
|
| gptkbp:impact |
contributes to understanding of cosmic phenomena
provides insights into extreme physics |
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
|
| gptkbp:lighting |
strong
monitored over time high-energy X-rays |
| gptkbp:located_in |
gptkb:Centaurus_constellation
|
| gptkbp:mass |
greater than 10 solar masses
|
| gptkbp:migration |
occurs from secondary to primary
|
| gptkbp:model |
developed to explain its behavior
|
| gptkbp:next_event |
aim to improve understanding of its properties
|
| gptkbp:orbital_period |
approximately 5.5 hours
|
| gptkbp:origin |
derived from its location in Centaurus constellation
|
| gptkbp:power_source |
high during outbursts
|
| gptkbp:primary_star_type |
gptkb:Supernova
|
| gptkbp:provides_information_on |
facilitated by international agreements
from multiple observatories |
| gptkbp:public_interest |
featured in documentaries
|
| gptkbp:publications |
numerous papers published about it
|
| gptkbp:research |
collected in various wavelengths
due to its distance and brightness variations evolving with technology advancements extensive records kept since discovery includes spectroscopy and photometry |
| gptkbp:research_focus |
stellar evolution and compact objects
|
| gptkbp:research_importance |
helps understand black hole formation
|
| gptkbp:secondary_star_type |
gptkb:main-sequence_star
|
| gptkbp:significance |
important for studying neutron stars
|
| gptkbp:system |
other X-ray binaries
|
| gptkbp:type |
gptkb:supermassive_black_hole
gptkb:star |
| gptkbp:variable_star |
yes
|
| gptkbp:xray_binaries |
part of the class of X-ray binaries
|
| gptkbp:xray_flare_events |
recorded during observations
|