Statements (62)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:associated_with |
mythology and folklore
various astronomical phenomena neutron star formation cosmic rays production theoretical models of supernova explosions |
| gptkbp:bomb_load |
10^44 joules
|
| gptkbp:contribution |
contributed to the field of cosmology.
|
| gptkbp:cultural_impact |
influenced literature and art
inspired various artworks |
| gptkbp:cultural_references |
referenced in various cultural contexts
|
| gptkbp:discovered_by |
Chinese astronomers
|
| gptkbp:discovery_year |
1054 AD
|
| gptkbp:distance_from_earth |
about 6500 light-years
|
| gptkbp:emissions_standard |
emitted light across various wavelengths
|
| gptkbp:has_spectral_type |
Type II-P
|
| gptkbp:has_supernova |
gptkb:Crab_Nebula
|
| gptkbp:historical_documentation |
documented in Chinese and Arab texts
|
| gptkbp:historical_impact |
significant in the history of astronomy
|
| gptkbp:historical_legacy |
remains a key case study in astrophysics
|
| gptkbp:historical_records |
noted in multiple cultures' records
|
| gptkbp:historical_significance |
first recorded supernova
important for ancient astronomy |
| https://www.w3.org/2000/01/rdf-schema#label |
supernova SN 1054
|
| gptkbp:impact |
contributed to understanding of supernova mechanisms
led to advancements in observational techniques provides insights into the universe's expansion |
| gptkbp:influence_on_star_formation |
affects surrounding star formation processes
|
| gptkbp:is_observed_in |
gptkb:Arab_astronomers
European astronomers |
| gptkbp:issues |
subject of ongoing astrophysical studies
|
| gptkbp:lighting |
analyzed for understanding supernova behavior
characteristic light curve observed light echo observed from the explosion magnitude -6 |
| gptkbp:location |
gptkb:Taurus_constellation
|
| gptkbp:narrative |
documented in historical texts
|
| gptkbp:notable_feature |
brightest supernova recorded in history
|
| gptkbp:observational_evidence |
visible during daytime
|
| gptkbp:power_source |
massive energy output during explosion
|
| gptkbp:preserved_by |
gptkb:Crab_Nebula
approximately 970 years old complex structure observed in the Crab Nebula consists of gas and dust |
| gptkbp:publications |
numerous publications dedicated to its study
|
| gptkbp:pulsar |
gptkb:PSR_B0531+21
|
| gptkbp:remnant_diameter |
approximately 11 light-years
|
| gptkbp:remnant_dynamics |
dynamics studied in astrophysical simulations
|
| gptkbp:remnant_evolution |
evolution studied over time
|
| gptkbp:remnant_observation |
observed in radio wavelengths
continuously studied by astronomers |
| gptkbp:research |
important for understanding stellar evolution
extensive data collected over centuries improved due to its study visible for several weeks |
| gptkbp:research_importance |
key example of supernova phenomena
|
| gptkbp:travel_time |
approximately 6500 years
|
| gptkbp:type |
gptkb:Type_II_supernova
|
| gptkbp:bfsParent |
gptkb:Messier_1
gptkb:the_Crab_Pulsar_system gptkb:the_Crab_Pulsar |
| gptkbp:bfsLayer |
6
|