Properties (48)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:chemicalFormula |
produced heavy elements like nickel and cobalt
|
| gptkbp:collaboratedWith |
NASA_and_ESA
|
| gptkbp:collaborations |
involved multiple international observatories
part of collaborative projects in astrophysics |
| gptkbp:colors |
0.0014
exhibited light echoes observed in subsequent years |
| gptkbp:conservationEfforts |
produced a remnant that is still observable
|
| gptkbp:contributedTo |
enhanced knowledge of supernova mechanisms
|
| gptkbp:dataUsage |
data shared among international research teams
|
| gptkbp:education |
used in educational materials about supernovae
|
| gptkbp:established |
gptkb:Robert_P._Kirshner
|
| gptkbp:financialPerformance |
discussed in numerous scientific conferences
|
| gptkbp:fuelType |
thermonuclear explosion of a white dwarf
|
| gptkbp:historicalResearch |
involved astronomers from various fields
continues to be a focus for future research in astronomy. |
| gptkbp:historicalSignificance |
important for understanding stellar evolution
|
| gptkbp:hosts |
NGC 5128
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1016
|
| gptkbp:image |
collected data on brightness over time
|
| gptkbp:impact |
provided insights into the expansion of the universe
influenced the understanding of cosmic acceleration |
| gptkbp:internationalClassification |
analyzed for elemental composition
|
| gptkbp:legacy |
remains a key subject in supernova research
|
| gptkbp:length |
approximately 10 million light-years
|
| gptkbp:lighting |
declines rapidly after peak brightness
exhibits a characteristic light curve of Type Ia supernovae |
| gptkbp:locatedIn |
the_constellation_Centaurus
|
| gptkbp:model |
tested various theoretical models of supernova explosions
|
| gptkbp:nearbyAttractions |
used to measure cosmic distances
|
| gptkbp:notableFeature |
one of the closest supernovae observed in the last century
|
| gptkbp:officialResidence |
contributed to the study of dark energy
faced challenges due to its brightness and distance observed over several months after explosion utilized photometry and spectroscopy |
| gptkbp:prominence |
approximately -19.3
|
| gptkbp:publicAccess |
captured public interest due to its proximity
|
| gptkbp:publications |
featured in many astronomy journals
|
| gptkbp:reignEnd |
remains are still expanding
|
| gptkbp:relatedEvent |
led to further studies of Type Ia supernovae
continued to be monitored for years after discovery |
| gptkbp:releaseYear |
1987
|
| gptkbp:researchInterest |
numerous papers published regarding its observations
|
| gptkbp:technology |
included both ground-based and space-based observations
|
| gptkbp:timePeriod |
approximately 10 million years
|
| gptkbp:type |
gptkb:Type_Ia_supernova
shows features of iron and silicon |
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|