Statements (103)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:apparent_magnitude |
-6
|
| gptkbp:associated_with |
gptkb:pulsar_PSR_B0531+21
gptkb:pulsar_wind_nebula X-ray emissions infrared emissions gamma-ray emissions Chinese records ultraviolet emissions radio emissions neutron star formation optical emissions Mesoamerican records |
| gptkbp:associated_with_galaxy |
gptkb:Milky_Way
|
| gptkbp:bomb_load |
10^44 joules
about 1 foe approximately 10^44 joules |
| gptkbp:brightness_peak |
lasted for about 23 days
|
| gptkbp:contributed_to |
cosmic ray production
|
| gptkbp:cultural_impact |
inspired various artworks
influenced art recorded in historical texts inspired mythology noted in folklore observed by indigenous peoples |
| gptkbp:discovered_by |
Chinese astronomers
|
| gptkbp:discovery_year |
1054
July 4, 1054 |
| gptkbp:distance_from_earth |
6500 light years
approximately 6,500 light-years about 6500 light-years |
| gptkbp:expansion_plans |
about 1500 km/s
|
| gptkbp:first_appearance |
July 4, 1054
in the year 1054 |
| gptkbp:has_spectral_type |
Type II-P supernova
Type II-P |
| gptkbp:has_supernova |
gptkb:Crab_Nebula
|
| gptkbp:historical_impact |
cultural significance in various civilizations
|
| gptkbp:historical_significance |
first recorded supernova
noted in various historical records one of the brightest supernovae recorded |
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1054
|
| gptkbp:impact |
led to advancements in understanding supernovae
|
| gptkbp:influenced |
local star formation
|
| gptkbp:influenced_by |
surrounding interstellar medium
|
| gptkbp:is_observed_in |
gptkb:Arab_astronomers
European astronomers modern telescopes daytime sky optical and radio wavelengths |
| gptkbp:is_visible_from |
daytime
|
| gptkbp:known_as |
gptkb:Crab_Supernova
|
| gptkbp:lighting |
asymmetric
magnitude -6.0 observed in 2010 |
| gptkbp:location |
gptkb:Taurus_constellation
|
| gptkbp:modern_observation |
gptkb:Chandra_X-ray_Observatory
gptkb:Hubble_Space_Telescope radio telescopes optical telescopes |
| gptkbp:notable_event |
one of the first supernovae recorded in history
|
| gptkbp:notable_feature |
gptkb:pulsar_wind_nebula
X-ray emissions radio emissions remains visible in the night sky remnant nebula visible during the day optical emissions appeared for 23 days has a central pulsar remnant contains complex structures |
| gptkbp:preserved_by |
gptkb:pulsar_wind_nebula
gptkb:Crab_Nebula gptkb:Crab_Pulsar hydrogen and helium approximately 10 light years across hydrogen, helium, and heavier elements approximately 970 years |
| gptkbp:recorded_in |
Chinese historical texts
Islamic historical texts Japanese historical texts |
| gptkbp:remnant_diameter |
approximately 11 light-years
about 11 light-years |
| gptkbp:remnant_discovery |
discovered in 1731
|
| gptkbp:remnant_luminosity |
about 1000 times that of the Sun
|
| gptkbp:remnant_mass |
about 1.4 solar masses
|
| gptkbp:remnant_observation |
observed in multiple wavelengths
|
| gptkbp:remnant_research |
ongoing studies
|
| gptkbp:remnant_significance |
important for understanding supernovae
|
| gptkbp:remnant_temperature |
around 10 million K
|
| gptkbp:research |
gptkb:cosmology
astrophysics stellar evolution 23 days important for understanding stellar evolution documented by multiple cultures extensively studied in astrophysics |
| gptkbp:resulted_in |
gptkb:Crab_Nebula
|
| gptkbp:travel_time |
approximately 6500 years
|
| gptkbp:type |
gptkb:Type_II_supernova
|
| gptkbp:year |
1054
|
| gptkbp:bfsParent |
gptkb:Supernova_in_the_East
|
| gptkbp:bfsLayer |
8
|