Statements (73)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:apparent_magnitude |
-6
|
| gptkbp:artistic_influence |
depicted in various artworks
|
| gptkbp:associated_with |
gptkb:pulsar_PSR_B0531+21
Chinese records neutron star formation Native American oral traditions M1 (Messier 1) |
| gptkbp:barrel_type |
core-collapse supernova
|
| gptkbp:collaborations |
led to international research efforts
|
| gptkbp:cultural_impact |
recorded in historical texts
inspired various myths and legends recorded in folklore |
| gptkbp:cultural_references |
featured in documentaries
|
| gptkbp:date |
July 4, 1054
|
| gptkbp:discovered_by |
Chinese astronomers
|
| gptkbp:discovery |
led to discovery of pulsars.
|
| gptkbp:distance_from_earth |
about 6,500 light-years
approximately 6,500 light-years |
| gptkbp:duration |
several weeks
about 2 years |
| gptkbp:educational_value |
used in teaching stellar phenomena
|
| gptkbp:effect_on_earth |
visible during daytime
|
| gptkbp:exhibition |
Chinese historical texts
|
| gptkbp:expansion_plans |
about 1,500 km/s
|
| gptkbp:first_appearance |
July 4, 1054
|
| gptkbp:has_spectral_type |
Type II-P
|
| gptkbp:historical_records |
noted in Japanese records
|
| gptkbp:historical_significance |
one of the most studied supernovae
one of the brightest supernovae recorded important for cosmology studies |
| https://www.w3.org/2000/01/rdf-schema#label |
1054 supernova event
|
| gptkbp:impact |
led to advancements in supernova research
led to the discovery of neutron stars contributed to understanding of nuclear processes |
| gptkbp:influenced_artists |
mentioned in historical texts
|
| gptkbp:is_a_phenomenon_that |
gptkb:supernova_remnants
gamma-ray bursts |
| gptkbp:is_influenced_by |
advancements in telescopes
|
| gptkbp:is_observed_in |
gptkb:Arab_astronomers
gptkb:Native_American_culture European astronomers the year 1054 |
| gptkbp:last_visible |
about 2 years after explosion
|
| gptkbp:lighting |
asymmetric
magnitude -6 observed in later years |
| gptkbp:location |
gptkb:Taurus_constellation
|
| gptkbp:notable_feature |
bright optical display
|
| gptkbp:notable_for |
visible during the day
appeared as a new star |
| gptkbp:notable_traits |
high luminosity
|
| gptkbp:observational_legacy |
influenced future astronomical observations
|
| gptkbp:observational_records |
important for historical astronomy
|
| gptkbp:observational_technology |
naked eye
|
| gptkbp:power_source |
approximately 10^44 joules
|
| gptkbp:preserved_by |
gptkb:Supernova
gptkb:Crab_Nebula gptkb:Crab_Pulsar approximately 1,000 years complex and asymmetric |
| gptkbp:public_interest |
increased interest in astronomy
|
| gptkbp:related_event |
other historical supernovae
|
| gptkbp:research |
important for understanding stellar evolution
difficult to study due to distance inspired new methods in astronomy |
| gptkbp:research_importance |
provides insights into stellar death
|
| gptkbp:resulted_in |
gptkb:Crab_Nebula
|
| gptkbp:scientific_classification |
core-collapse supernova
|
| gptkbp:significance |
study of stellar evolution
|
| gptkbp:topics |
studies on cosmic rays
|
| gptkbp:travel_time |
6,500 years
|
| gptkbp:type |
gptkb:Type_II_supernova
|