Statements (59)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:advances |
spurred advancements in observational technology
|
| gptkbp:archives |
data archived for future studies
|
| gptkbp:associated_with |
gptkb:SN_1987_A_remnant
|
| gptkbp:brightness_peak |
magnitude 18.5
|
| gptkbp:chemical_elements_produced |
heavy elements like iron and nickel
|
| gptkbp:collaboration |
international collaboration in research
|
| gptkbp:collaborative_projects |
led to collaborative projects in astronomy
|
| gptkbp:conference |
discussed in numerous conferences
|
| gptkbp:cosmological_importance |
helps measure cosmic distances
|
| gptkbp:cultural_impact |
inspired art and literature
|
| gptkbp:discovered_by |
gptkb:1987
gptkb:Ian_Shelton |
| gptkbp:distance_from_earth |
approximately 168,000 light-years
|
| gptkbp:educational_value |
used in educational materials
|
| gptkbp:expansion_plans |
about 5,000 km/s
|
| gptkbp:exploded_from |
gptkb:Supernova
|
| gptkbp:followed_by |
observed for years post-explosion
|
| gptkbp:future_prospects |
continues to be a subject of study
|
| gptkbp:has_luminosity |
related to massive stars' life cycles
|
| gptkbp:has_spectral_type |
hydrogen-rich
|
| gptkbp:has_supernova |
compared to other historical supernovae
|
| gptkbp:hosts |
gptkb:NGC_1987
|
| https://www.w3.org/2000/01/rdf-schema#label |
supernova 1987 A
|
| gptkbp:impact |
provided insights into supernova mechanisms
influenced cosmological models |
| gptkbp:influence_on_astrophysical_models |
influenced models of stellar evolution
|
| gptkbp:influence_on_star_formation |
affects nearby star formation
|
| gptkbp:initial_explosion_energy |
about 10^51 ergs
|
| gptkbp:interaction_with_surrounding_medium |
produced shock waves
|
| gptkbp:is_a_source_of |
detected by Kamiokande II
|
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:legacy |
pioneering study of supernovae
|
| gptkbp:legacy_in_astronomy |
remains a key event in astronomy history
|
| gptkbp:light_echoes |
observed in subsequent years
|
| gptkbp:lighting |
monitored over several years
|
| gptkbp:located_in |
gptkb:Large_Magellanic_Cloud
|
| gptkbp:mass_loss_before_explosion |
significant mass loss
|
| gptkbp:model |
influenced models of stellar explosions
|
| gptkbp:neutrino_event_date |
February 23, 1987
|
| gptkbp:observational_impact |
increased interest in supernova research
|
| gptkbp:observational_techniques_developed |
new techniques developed for analysis
|
| gptkbp:observed_wavelengths |
optical, infrared, and radio
|
| gptkbp:preserved_by |
gptkb:1987_A_remnant
complex structure observed |
| gptkbp:provides_information_on |
data shared among researchers
|
| gptkbp:public_interest |
captured public attention
|
| gptkbp:publications |
numerous papers published
extensive literature available featured in major scientific journals |
| gptkbp:research |
extensively studied by astronomers
advanced techniques developed for study difficulties in observing distant supernovae rich observational history |
| gptkbp:significance |
first naked-eye supernova since 1604
|
| gptkbp:type |
gptkb:Type_II_supernova
|
| gptkbp:bfsParent |
gptkb:SN_1994_I_remnant
gptkb:Supernova_remnant_1987_A |
| gptkbp:bfsLayer |
6
|