Properties (48)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:analyzes |
involves complex statistical methods
|
| gptkbp:classification |
standard candle in cosmology
|
| gptkbp:collaboratedWith |
various astronomical institutions
|
| gptkbp:collaborations |
involved international research teams
involved in multi-wavelength observations |
| gptkbp:colors |
0.014
|
| gptkbp:communityEngagement |
engaged with the public through outreach programs
|
| gptkbp:conservationEfforts |
remains of the explosion are still being studied
|
| gptkbp:dataUsage |
results published in scientific journals
data shared with the global astronomical community |
| gptkbp:education |
used in teaching about stellar evolution
|
| gptkbp:established |
gptkb:H._A._Kobayashi
|
| gptkbp:financialPerformance |
discussed in various astrophysics conferences
|
| gptkbp:fuelType |
thermonuclear runaway
|
| gptkbp:hasRecognition |
approximately 15.5
|
| gptkbp:historicalContext |
part of a long history of supernova observations
|
| gptkbp:historicalResearch |
expected to yield more insights into supernova mechanics
|
| gptkbp:hosts |
elliptical galaxy
NGC 1316 |
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1014
|
| gptkbp:impact |
helped refine models of the universe's expansion
|
| gptkbp:internationalClassification |
used to analyze chemical composition
|
| gptkbp:is_essential_for |
used to measure cosmic distances
|
| gptkbp:legacy |
remains a significant case study in supernova research.
|
| gptkbp:length |
about 60 million light-years
|
| gptkbp:lighting |
similar to other Type Ia supernovae
exhibits a typical light curve for Type Ia supernovae reached peak brightness within a few weeks used to determine distance and brightness |
| gptkbp:locatedIn |
the_constellation_Centaurus
|
| gptkbp:officialResidence |
difficult to observe due to distance
data collected from various telescopes observed for several months after discovery utilized advanced imaging techniques |
| gptkbp:publicAccess |
attracted attention from amateur astronomers
|
| gptkbp:relatedEvent |
conducted by multiple observatories
ongoing studies to understand its properties part of a series of supernova discoveries in the early 2000s |
| gptkbp:releaseYear |
November 2001
photographic plates |
| gptkbp:resolution |
approximately 5 billion times that of the Sun
|
| gptkbp:scientificName |
contributes to understanding of dark energy
|
| gptkbp:takeoffDistance |
based on redshift measurements
|
| gptkbp:theory |
challenges existing theories of supernovae
|
| gptkbp:type |
gptkb:Type_Ia_supernova
shows features of iron and silicon |
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|