Statements (55)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:nebula
|
| gptkbp:apparent_magnitude |
maximum magnitude of about -17.5
|
| gptkbp:archaeological_findings |
important for understanding supernova remnants
|
| gptkbp:associated_with |
the galaxy M51
|
| gptkbp:bomb_load |
core-collapse supernova
|
| gptkbp:collaborations |
gptkb:NASA_and_ESA
multiple international observatories enhanced understanding of stellar evolution |
| gptkbp:community_engagement |
captured public interest in astronomy
|
| gptkbp:conference |
presented findings at multiple conferences
|
| gptkbp:conservation_efforts |
gptkb:SN_1994_I_remnant
gptkb:nebula |
| gptkbp:discovered_by |
gptkb:Robert_Kirshner
|
| gptkbp:distance |
approximately 20 million light-years
Tying to Cepheid variables |
| gptkbp:education |
used in educational materials about supernovae
|
| gptkbp:events |
continued for several years after discovery
ongoing analysis of remnants |
| gptkbp:features |
strong hydrogen lines
|
| gptkbp:future_plans |
continues to be a subject of future research.
|
| gptkbp:has_spectral_type |
hydrogen-rich spectrum
provided insights into nucleosynthesis |
| gptkbp:historical_significance |
important for Type II supernova studies
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1994 I
|
| gptkbp:impact |
contributed to understanding of supernova mechanisms
contributed to distance measurement techniques |
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
visible and infrared wavelengths data collected from various telescopes |
| gptkbp:length |
1994-03-26
|
| gptkbp:lighting |
exhibited a plateau phase
occurred about 20 days after explosion used to estimate distance and energy showed variability in brightness over time plateau followed by a decline used to infer explosion parameters |
| gptkbp:located_in |
gptkb:galaxy_NGC_5194
|
| gptkbp:location |
in the spiral arms of NGC 5194
|
| gptkbp:notable_for |
one of the best-studied supernovae
|
| gptkbp:partnerships |
collaborated with universities and research centers
|
| gptkbp:power_output |
released energy equivalent to about 10^51 ergs
|
| gptkbp:produced_by |
elements like iron and nickel
|
| gptkbp:provides_information_on |
data shared among research institutions
|
| gptkbp:publishes |
numerous papers published on findings
|
| gptkbp:research |
photometry and spectroscopy
extensive photometric and spectroscopic data 1994 to 1996 difficulties in early observations due to brightness |
| gptkbp:research_interest |
high interest from astronomers worldwide
|
| gptkbp:scientific_classification |
classified as a Type II-P supernova
|
| gptkbp:species |
studied for years post-explosion
|
| gptkbp:type |
gptkb:Type_II_supernova
|
| gptkbp:year_created |
1994-03-26
|
| gptkbp:bfsParent |
gptkb:M83
|
| gptkbp:bfsLayer |
4
|