Properties (38)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:aftermath |
approximately 10 light-years across
|
| gptkbp:associatedWith |
gptkb:the_Crab_Nebula
|
| gptkbp:chemicalFormula |
iron, nickel, cobalt
|
| gptkbp:colors |
observed in subsequent years
|
| gptkbp:conservationEfforts |
Centaurus A
mostly hydrogen and helium over 1000 years old |
| gptkbp:culturalImpact |
mentioned in various historical accounts
|
| gptkbp:duration |
several months
|
| gptkbp:energyEfficiency |
equivalent to billions of suns
|
| gptkbp:established |
Chinese_astronomers
|
| gptkbp:growthRate |
estimated at 1 per century in the Milky Way
|
| gptkbp:hasInternationalClassification |
thermonuclear explosion
|
| gptkbp:hasRecognition |
-5.5
|
| gptkbp:historical_analysis |
analyzed by astronomers using modern telescopes
|
| gptkbp:historicalEvent |
noted by multiple civilizations
|
| gptkbp:historicalRecords |
documented_in_Chinese_historical_texts
|
| gptkbp:historicalSignificance |
one of the brightest supernovae recorded in history
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1008
|
| gptkbp:impact |
contributed to understanding of dark energy
influenced studies of stellar evolution |
| gptkbp:legacy |
remains a subject of study in astrophysics.
|
| gptkbp:length |
approximately 7,000 light-years
|
| gptkbp:lighting |
around 1006 AD
|
| gptkbp:lightRange |
fast decline
|
| gptkbp:location |
constellation_Centaurus
|
| gptkbp:notableFeature |
visible during the day
|
| gptkbp:officialResidence |
difficult to observe due to distance
naked eye observation |
| gptkbp:releaseYear |
1006
|
| gptkbp:takeoffDistance |
parallax measurements
|
| gptkbp:type |
gptkb:Type_Ia_supernova
supernova remnant elliptical galaxy Type_Ia_spectrum |
| gptkbp:visitedBy |
gptkb:Arab_astronomers
European_astronomers |