SN 1006 remnant

GPTKB entity

Statements (45)
Predicate Object
gptkbp:instanceOf supernova remnant
gptkbp:aftermath irregular
featured in documentaries and articles
expanding shell of gas
contributed to understanding of supernovae
approximately 60 light-years across
based on expansion rate
complex and filamentary
studied over centuries
with surrounding interstellar medium
gptkbp:analyzes reveals chemical composition
gptkbp:associatedWith cosmic rays
theories of stellar evolution
historical records of a bright star
gptkbp:communityImpact inspired further supernova studies
gptkbp:conservationEfforts over 1,000 years
hydrogen, helium, and heavier elements
important for cosmology
gptkbp:culturalImpact influenced art and literature
gptkbp:established Chinese_astronomers
gptkbp:expansion about 5,000 km/s
gptkbp:finalDisposal provides insights into elemental abundances
gptkbp:hasLocation southern hemisphere sky
gptkbp:historicalLegacy remains a key subject in astronomy
gptkbp:historicalResearch ongoing in astrophysics
promises new discoveries in astrophysics
gptkbp:historicalSignificance documented in multiple cultures
https://www.w3.org/2000/01/rdf-schema#label SN 1006 remnant
gptkbp:imageStabilization captured in various wavelengths
gptkbp:isEngagedIn in the year 1006
gptkbp:legacy included in astronomical catalogs
gptkbp:length approximately 7,200 light-years
gptkbp:lighting monitored for brightness changes
magnitude -7.5
gptkbp:locatedIn constellation_Centaurus
gptkbp:notableFeature observed in daylight
gptkbp:occursAnnually one of the brightest supernovae in recorded history
gptkbp:officialResidence optical telescopes
gptkbp:releaseYear 1006
gptkbp:researchFocus detected_by_Chandra_X-ray_Observatory
gptkbp:scientificName helps study supernova explosions
gptkbp:standardFeatures bright optical filaments
gptkbp:stations detected by various radio telescopes
gptkbp:type gptkb:Type_Ia_supernova
gptkbp:visitedBy European_astronomers