Properties (50)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:analyzes |
involves complex data analysis techniques
|
| gptkbp:associatedAct |
NGC 3079
|
| gptkbp:bombLoad |
approximately 1979
|
| gptkbp:classification |
classified as a standard candle for distance measurement
|
| gptkbp:collaboratedWith |
various astrophysical research groups
NASA_and_ESA_missions |
| gptkbp:collaborations |
involved in various collaborative research projects
involved multiple international observatories |
| gptkbp:colors |
z = 0.0077
|
| gptkbp:communityEngagement |
engaged amateur astronomers in observations
|
| gptkbp:conservationEfforts |
remnant is not well-defined due to its distance
|
| gptkbp:contributedTo |
contributed to the understanding of dark energy
|
| gptkbp:culturalImpact |
featured in documentaries and popular science discussions
|
| gptkbp:dataUsage |
data published in multiple scientific journals
data shared with the global scientific community |
| gptkbp:education |
used in educational materials about supernovae
|
| gptkbp:established |
gptkb:Robert_Kirshner
|
| gptkbp:financialPerformance |
discussed in numerous astrophysics conferences
|
| gptkbp:historicalEvent |
part of a long history of supernova observations
|
| gptkbp:historicalLegacy |
remains a significant part of astronomical research.
|
| gptkbp:historicalResearch |
continues to be a target for future observational campaigns
|
| gptkbp:historicalSignificance |
one of the first supernovae to be used in cosmology
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1001
|
| gptkbp:image |
extensively studied for light curve analysis
|
| gptkbp:impact |
influenced the study of Type Ia supernovae
|
| gptkbp:internationalClassification |
used to determine its chemical composition
|
| gptkbp:legacy |
remains a key object of study in modern astrophysics
|
| gptkbp:length |
approximately 30 million light-years
|
| gptkbp:lighting |
declines rapidly after peak brightness
occurred approximately 20 days after discovery exhibits a characteristic light curve of Type Ia supernovae |
| gptkbp:locatedIn |
the_constellation_Ursa_Major
|
| gptkbp:model |
used to test theoretical models of supernova explosions
|
| gptkbp:officialResidence |
data collected in various wavelengths
distance made detailed study challenging utilized both ground-based and space-based telescopes |
| gptkbp:prominence |
approximately -19.3
|
| gptkbp:publicAccess |
captured public interest due to its brightness
|
| gptkbp:relatedEvent |
associated with other astronomical phenomena
conducted in the years following its discovery led to further research on supernova progenitors |
| gptkbp:releaseYear |
1979
|
| gptkbp:researchInterest |
has had a lasting impact on the field of cosmology
|
| gptkbp:searchAndRescueMissions |
involves physics, astronomy, and cosmology
|
| gptkbp:significance |
important for measuring cosmic distances
helps in understanding the expansion of the universe |
| gptkbp:type |
gptkb:Type_Ia_supernova
shows strong silicon absorption lines |
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|