Properties (51)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:analyzes |
telescopes
|
| gptkbp:associatedWith |
gptkb:the_Crab_Nebula
the Milky Way galaxy |
| gptkbp:conservationEfforts |
gptkb:SN_1006_remnant
over 1000 years hydrogen and helium observed in X-ray wavelengths observed in infrared wavelengths observed in optical wavelengths observed in radio wavelengths |
| gptkbp:culturalImpact |
inspired various historical records
|
| gptkbp:established |
Chinese_astronomers
|
| gptkbp:exhibits |
gptkb:New_General_Catalogue
Messier catalog |
| gptkbp:expansion |
approximately 5,000 km/s
|
| gptkbp:firstAppearance |
visible during daytime
|
| gptkbp:fuelType |
shell-type
|
| gptkbp:hasLocation |
near_the_Galactic_plane
|
| gptkbp:hasRecognition |
-5.5
|
| gptkbp:historical_analysis |
studied for its chemical composition
studied for its expansion dynamics studied for its historical observations studied for its light curve properties studied for its remnant structure |
| gptkbp:historicalRecords |
documented_in_Arabic_texts
documented_in_Chinese_texts documented_in_European_texts |
| gptkbp:historicalResearch |
ongoing studies of remnants
|
| gptkbp:historicalSignificance |
brightest recorded supernova in history
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1006
|
| gptkbp:impact |
influenced studies of stellar evolution
|
| gptkbp:influence |
influenced folklore and mythology
|
| gptkbp:length |
approximately 7,200 light-years
|
| gptkbp:lighting |
May 1006
|
| gptkbp:lightRange |
fast decline
|
| gptkbp:location |
constellation Lupus
|
| gptkbp:notableEvent |
one of the most significant astronomical events of the millennium
|
| gptkbp:notableFeature |
April 30, 1006
July 1006 extremely bright appearance recorded by multiple civilizations |
| gptkbp:officialResidence |
several months
|
| gptkbp:relatedTo |
other historical supernovae
|
| gptkbp:releaseYear |
1006
|
| gptkbp:rotorDiameter |
approximately 60 light-years
|
| gptkbp:scientificName |
important for cosmology
|
| gptkbp:type |
gptkb:Type_Ia_supernova
Type_Ia_spectrum |
| gptkbp:visitedBy |
gptkb:Arab_astronomers
European_astronomers |