Properties (49)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:aftermath |
studied for years post-explosion
|
| gptkbp:analyzes |
provided insights into nucleosynthesis processes
|
| gptkbp:associatedWith |
the galaxy's spiral arms
|
| gptkbp:bombLoad |
1994-03-26
|
| gptkbp:collaborations |
involved multiple observatories
involved multiple observatories across the globe |
| gptkbp:conservationEfforts |
gptkb:SN_1994I_remnant
primarily hydrogen and helium remains still observable today |
| gptkbp:established |
gptkb:Robert_Kirshner
|
| gptkbp:fuelType |
core-collapse supernova
|
| gptkbp:hasInternationalClassification |
classified as a core-collapse supernova
|
| gptkbp:historicalLegacy |
remains a key subject in supernova research.
|
| gptkbp:historicalResearch |
involved international teams of astronomers
|
| gptkbp:historicalSignificance |
one of the best-studied supernovae in history
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1994I
|
| gptkbp:impact |
contributed to understanding of supernova mechanisms
helped refine distance measurements in the universe |
| gptkbp:length |
approximately 20 million light-years
|
| gptkbp:lensType |
showed strong hydrogen lines
|
| gptkbp:lighting |
exhibited a plateau phase
occurred approximately 20 days after explosion provided data for theoretical models showed variability in brightness over time typical of Type II supernovae used to estimate distance and energy output |
| gptkbp:locatedIn |
galaxy NGC 5194
|
| gptkbp:notableFor |
one of the closest supernovae observed in the 1990s
|
| gptkbp:officialResidence |
extensive photometric and spectroscopic data
1994 to 1998 used both ground-based and space-based telescopes faced challenges due to its brightness and location |
| gptkbp:powerOutput |
released energy equivalent to about 10^51 ergs
|
| gptkbp:propagationMethod |
Tying to Cepheid variables
|
| gptkbp:publicAccess |
captured the attention of both scientists and the public
|
| gptkbp:relatedEvent |
continued for several years after discovery
led to new insights into supernova remnants triggered interest in nearby supernovae |
| gptkbp:releaseYear |
1994-03-26
|
| gptkbp:researchInterest |
important for studying stellar evolution
numerous papers published in scientific journals |
| gptkbp:theory |
influenced theories on supernova explosions
|
| gptkbp:type |
spiral galaxy
Type II supernova hydrogen-rich spectrum |
| gptkbp:unitAwards |
maximum magnitude of about -17.5
|
| gptkbp:universe |
contributed to the study of supernova remnants in general
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|