Statements (67)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:nebula
|
| gptkbp:bfsLayer |
4
|
| gptkbp:bfsParent |
gptkb:Supernova_1987_A
|
| gptkbp:age |
over 30 years
|
| gptkbp:analyzes |
elemental abundances
|
| gptkbp:associated_with |
gptkb:SN_1987_A
|
| gptkbp:composed_of |
hydrogen, helium, and heavier elements
|
| gptkbp:consists_of |
expanding shell
|
| gptkbp:contains |
gptkb:physicist
|
| gptkbp:depicted_in |
gptkb:physicist
southern hemisphere |
| gptkbp:diameter |
approximately 150 light-years
|
| gptkbp:discovered_by |
gptkb:1987
|
| gptkbp:distance |
approximately 168,000 light-years
|
| gptkbp:emissions_standard |
gptkb:X-rays
radio waves |
| gptkbp:examines |
light curve variations
shock wave interactions shock front dynamics |
| gptkbp:first_appearance |
gptkb:Ian_Shelton
|
| gptkbp:has_impact_on |
understanding of supernovae
|
| gptkbp:has_spectral_type |
Type II-P
|
| https://www.w3.org/2000/01/rdf-schema#label |
Supernova remnant 1987 A
|
| gptkbp:is_a |
cosmic event
|
| gptkbp:is_analyzed_in |
light echo phenomena
expansion rate |
| gptkbp:is_associated_with |
gptkb:supernova_1987_A
massive stars |
| gptkbp:is_connected_to |
galactic evolution
stellar nucleosynthesis massive star evolution |
| gptkbp:is_documented_in |
gptkb:literary_work
astronomical surveys astronomical catalogs |
| gptkbp:is_explored_in |
astrophysical simulations
|
| gptkbp:is_influential_in |
modern astronomy
supernova research |
| gptkbp:is_located_near |
gptkb:Tarazed
|
| gptkbp:is_monitored_by |
ground-based telescopes
|
| gptkbp:is_observed_in |
optical wavelengths
space telescopes infrared wavelengths |
| gptkbp:is_part_of |
gptkb:LMC_1987_A
gptkb:LMC_star_cluster gptkb:LMC_star_formation_region gptkb:LMC_supernova_remnants gptkb:LMC LMC astronomical phenomena LMC star formation events LMC star formation history |
| gptkbp:is_related_to |
cosmic rays
|
| gptkbp:is_studied_in |
gptkb:Hubble_Space_Telescope
astrophysics neutrino astronomy stellar explosions interstellar medium interactions neutrino emissions cosmic microwave background interactions |
| gptkbp:is_used_in |
cosmology research
|
| gptkbp:lighting |
monitored over time
|
| gptkbp:located_in |
gptkb:Large_Magellanic_Cloud
|
| gptkbp:notable_for |
its historical significance
its brightness its discovery by amateur astronomers. |
| gptkbp:resulted_in |
supernova explosion
|
| gptkbp:significance |
stellar evolution studies
|
| gptkbp:type |
gptkb:Type_II_supernova
|