Properties (22)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:bombLoad |
approximately 1979
|
| gptkbp:chemicalFormula |
produces iron and nickel in the explosion
|
| gptkbp:classification |
classified as a Type Ia supernova due to its light curve and spectrum.
|
| gptkbp:colors |
0.01
|
| gptkbp:conservationEfforts |
the remnant is still observable
|
| gptkbp:energyEfficiency |
approximately 10^51 ergs
|
| gptkbp:established |
gptkb:Robert_P._Kirshner
|
| gptkbp:hasRecognition |
approximately 12.5
|
| gptkbp:hosts |
NGC 5253
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1002
|
| gptkbp:impact |
contributed to the understanding of dark energy
|
| gptkbp:length |
approximately 100 million light-years
|
| gptkbp:lighting |
reached peak brightness within a few weeks
exhibits a characteristic light curve of Type Ia supernovae |
| gptkbp:locatedIn |
the_constellation_Centaurus
|
| gptkbp:officialResidence |
data collected by various telescopes
|
| gptkbp:releaseYear |
1979
|
| gptkbp:significance |
important for understanding Type Ia supernovae
|
| gptkbp:type |
gptkb:Type_Ia_supernova
shows features of iron and nickel |
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|