Statements (101)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:analysis |
involves complex algorithms
|
| gptkbp:apparent_magnitude |
magnitude 3.0 at peak
|
| gptkbp:associated_with |
the Tarantula Nebula
neutrino burst |
| gptkbp:bomb_load |
core collapse of a massive star
core-collapse 10^51 ergs |
| gptkbp:class |
held to discuss findings
|
| gptkbp:collaboration |
international astronomers
involved international research teams with global observatories |
| gptkbp:collaborations |
with physicists
|
| gptkbp:collaborative_projects |
with astrophysics departments
|
| gptkbp:community |
collaborative studies
|
| gptkbp:community_engagement |
outreach programs
|
| gptkbp:conference |
discussed in numerous meetings
|
| gptkbp:coordinates |
in the LMC
in the Large Magellanic Cloud |
| gptkbp:cosmic_distance_scale |
important for measurements
|
| gptkbp:cosmological_importance |
helps measure cosmic distances
|
| gptkbp:cultural_impact |
inspired art and literature
|
| gptkbp:discovered_by |
gptkb:Robert_Kirshner
gptkb:Henrietta_Leavitt |
| gptkbp:discovery_year |
gptkb:1987
|
| gptkbp:distance_from_earth |
approximately 168,000 light-years
|
| gptkbp:economic_impact |
advancements in imaging techniques
|
| gptkbp:educational_resources |
used in teaching
|
| gptkbp:educational_value |
used in astronomy education
|
| gptkbp:emissions_standard |
detected
|
| gptkbp:events |
conducted regularly
|
| gptkbp:followed_by |
X-ray emission
visible in multiple wavelengths |
| gptkbp:future_prospects |
continues to be a subject of study
expected to continue |
| gptkbp:has_spectral_type |
hydrogen-rich
hydrogen-rich spectrum |
| gptkbp:has_supernova |
gptkb:SN_1987_A_remnant
|
| gptkbp:historical_significance |
first supernova observed in the modern era
first supernova observed in real-time |
| https://www.w3.org/2000/01/rdf-schema#label |
LMC 1 supernova
|
| gptkbp:impact |
provided insights into stellar evolution
contributes to understanding of dark energy significant in astrophysics advances in supernova research first observed neutrinos from a supernova |
| gptkbp:impact_on_public_understanding |
increased interest in astronomy
|
| gptkbp:influence_on_cosmology |
calibration of distance scale
|
| gptkbp:is_a_fusion_of |
produced heavy elements
|
| gptkbp:is_a_phenomenon_that |
gamma-ray bursts
|
| gptkbp:is_a_source_of |
Kamiokande II
detected by Kamiokande II |
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:legacy |
pioneering study of supernovae
in supernova research |
| gptkbp:light_curve_duration |
several months
|
| gptkbp:lighting |
gptkb:plateau
plateau phase important for understanding supernovae plateau followed by a decline occurred in 1987 |
| gptkbp:located_in |
gptkb:Large_Magellanic_Cloud
|
| gptkbp:model |
tested against observations
supports models of stellar evolution |
| gptkbp:next_event |
planned for ongoing study
|
| gptkbp:notable_features |
ring structure
|
| gptkbp:notable_galaxies |
gptkb:Milky_Way
|
| gptkbp:observational_significance |
important for studying stellar evolution
|
| gptkbp:peak_magnitude |
-18.5
|
| gptkbp:photometric_observations |
conducted by various observatories
|
| gptkbp:preserved_by |
gptkb:SN_1987_A
heavy elements about 0.5 light-years across about 0.5 light-years consists of ejected material and neutron star |
| gptkbp:progenitor_star_type |
red supergiant
|
| gptkbp:provides_information_on |
among institutions
|
| gptkbp:public_interest |
widely covered in media
captured public attention |
| gptkbp:publications |
numerous papers published
|
| gptkbp:related_event |
neutrino burst detection
|
| gptkbp:remnant_evolution |
continues to evolve over time
monitored over decades |
| gptkbp:reproduction |
gptkb:Giant
|
| gptkbp:research |
photometry
ongoing research used for analysis distance and brightness light curve data 1987 to present monitored for decades used include telescopes extensively studied in various wavelengths utilized advanced telescopes |
| gptkbp:scientific_papers |
published on findings
|
| gptkbp:significance |
first observed in modern times
|
| gptkbp:spectroscopic_observations |
provided insights into explosion dynamics
|
| gptkbp:stellar_collapse |
result of core-collapse
|
| gptkbp:stellar_nucleosynthesis |
contributed to knowledge
|
| gptkbp:travel_time |
168,000 years
|
| gptkbp:type |
gptkb:Type_II_supernova
|