Properties (72)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:analyzes |
utilized advanced computational techniques.
|
| gptkbp:associatedWith |
gamma-ray bursts
|
| gptkbp:bombLoad |
approximately 2002
|
| gptkbp:chemicalFormula |
enriched in heavy elements.
|
| gptkbp:classification |
associated_with_Wolf-Rayet_stars.
|
| gptkbp:collaboratedWith |
NASA_and_ESA.
|
| gptkbp:collaborations |
involved multiple international teams.
involved universities and research centers. |
| gptkbp:collection |
ongoing data collection efforts.
|
| gptkbp:colors |
0.0023
|
| gptkbp:communityEngagement |
involved public outreach efforts.
|
| gptkbp:conservationEfforts |
supernova remnant
|
| gptkbp:contribution |
helped refine distance measurements.
|
| gptkbp:culturalImpact |
inspired art and literature.
|
| gptkbp:dataUsage |
archived in astronomical databases.
collaborative efforts in data sharing. results published in scientific journals. |
| gptkbp:education |
used in teaching about stellar phenomena.
|
| gptkbp:energyEfficiency |
approximately 10^51 ergs
|
| gptkbp:established |
gptkb:K._W._Weiler
|
| gptkbp:financialPerformance |
discussed in various astrophysics conferences.
|
| gptkbp:firstClaim |
planned with next-generation telescopes.
|
| gptkbp:follows |
revealed details about progenitor star.
|
| gptkbp:fuelType |
core-collapse
|
| gptkbp:historicalContext |
part of a series of notable supernovae.
|
| gptkbp:historicalEvent |
part of a long history of supernova observations.
|
| gptkbp:historicalResearch |
expected to focus on progenitor stars.
expected to yield more insights. involved astrophysicists worldwide. |
| gptkbp:hosts |
spiral galaxy NGC 3190
|
| https://www.w3.org/2000/01/rdf-schema#label |
supernova SN 2002ap
|
| gptkbp:impact |
challenged existing models.
provided insights into supernova mechanisms. significant for understanding supernovae. |
| gptkbp:is_monitored_by |
remains a benchmark for future studies.
|
| gptkbp:legacy |
remains a subject of ongoing research.
|
| gptkbp:length |
approximately 10 million light-years
|
| gptkbp:lensType |
showed signs of interaction with circumstellar material.
|
| gptkbp:lighting |
fast rise and decline
occurred around 20 days after explosion. similar to other Type Ic supernovae. used to estimate distance. |
| gptkbp:location |
NGC 3190
|
| gptkbp:model |
tested against observations.
|
| gptkbp:narrativeStyle |
one of the closest supernovae observed in recent years.
|
| gptkbp:notableFeature |
high-velocity_ejecta.
|
| gptkbp:officialResidence |
2002 to present.
affected by interstellar dust. included photometry and spectroscopy. photometric and spectroscopic data available. |
| gptkbp:propagationMethod |
Tying_to_Cepheid_variables.
|
| gptkbp:publicAccess |
featured in popular science media.
|
| gptkbp:relatedEvent |
conducted by various observatories.
|
| gptkbp:releaseYear |
January 2002
|
| gptkbp:research |
supported by various grants.
|
| gptkbp:researchInterest |
featured in educational programs.
active interest from the astrophysics community. formed between institutions. influenced subsequent studies. involved multiple research teams. numerous papers published. |
| gptkbp:scientificName |
important for studying stellar evolution.
important for understanding cosmic events. widely studied by astronomers. |
| gptkbp:targetAudience |
available through various databases.
|
| gptkbp:technology |
included spectroscopy and imaging.
|
| gptkbp:theory |
influenced theories of stellar death.
|
| gptkbp:type |
Type Ic supernova
broad absorption lines |
| gptkbp:unitAwards |
maximum magnitude of about 16.5
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|