Statements (56)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:analysis |
data analysis techniques improved through its study
|
| gptkbp:apparent_magnitude |
maximum magnitude of about -19.5
|
| gptkbp:archives |
data archived for future research
|
| gptkbp:bomb_load |
approximately 1.2 x 10^51 ergs
|
| gptkbp:collaboration |
involved collaboration among multiple research teams
|
| gptkbp:collaborations |
involved collaborative research efforts
|
| gptkbp:collaborative_projects |
inspired collaborative projects among institutions
|
| gptkbp:community_engagement |
engaged the public through outreach programs
|
| gptkbp:conference |
discussed in various scientific conferences
|
| gptkbp:contribution_to_cosmology |
contributed to the discovery of dark energy
|
| gptkbp:cosmological_implications |
has cosmological implications for the expansion of the universe
|
| gptkbp:discovered_by |
gptkb:Robert_Kirshner
|
| gptkbp:discovery_year |
1990-01-16
|
| gptkbp:distance |
approximately 15 million light-years from Earth
distance measured using various methods |
| gptkbp:educational_value |
has educational impact on astronomy curricula
|
| gptkbp:events |
follow-up observations continued for several years
|
| gptkbp:future_prospects |
future research planned to study its remnant
|
| gptkbp:has_publications |
numerous research papers published about it
|
| gptkbp:has_spectral_type |
shows strong silicon absorption lines
|
| gptkbp:historical_legacy |
scientific legacy continues to be relevant
|
| gptkbp:historical_significance |
historically significant for Type Ia supernova studies
|
| gptkbp:hosts |
NGC 4526
|
| https://www.w3.org/2000/01/rdf-schema#label |
supernova SN 1990 I
|
| gptkbp:impact |
had a significant impact on the field of astronomy
|
| gptkbp:importance |
important for understanding cosmic distances
|
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:legacy |
legacy continues to influence supernova research
|
| gptkbp:light_curve_model |
light curve modeled using various techniques
|
| gptkbp:light_curve_parameters |
light curve parameters analyzed extensively
|
| gptkbp:lighting |
light curve shows a rapid rise and decline
used for light curve fitting studies decline phase is consistent with a Type Ia supernova reached peak brightness in early 1990 |
| gptkbp:located_in |
galaxy NGC 4526
|
| gptkbp:model |
theoretical models developed based on observations
|
| gptkbp:observational_techniques_advancements |
led to advancements in observational techniques
|
| gptkbp:preserved_by |
remnant size estimated to be several light-years across
supernova remnant is still being studied |
| gptkbp:provides_information_on |
data shared among researchers worldwide
|
| gptkbp:public_interest |
generated significant interest in the astronomical community
|
| gptkbp:publications |
numerous publications in scientific journals
|
| gptkbp:redshift |
0.0053
|
| gptkbp:research |
has a rich observational history
observed using both ground-based and space-based telescopes data collected by various observatories faced observational challenges due to its brightness part of various observational campaigns spectroscopy revealed details about the explosion mechanism |
| gptkbp:scientific_classification |
classified as a Type Ia supernova
|
| gptkbp:spectral_evolution |
spectral evolution studied in detail
|
| gptkbp:storage |
photometric data collected over time
|
| gptkbp:type |
gptkb:Type_Ia_supernova
|
| gptkbp:bfsParent |
gptkb:NGC_5254
|
| gptkbp:bfsLayer |
6
|