Statements (48)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:age |
a few million years
|
| gptkbp:apparent_magnitude |
approximately 3.5
|
| gptkbp:archaeological_findings |
observed by astronomers for centuries
|
| gptkbp:astrophysical_importance |
significant for understanding stellar evolution.
|
| gptkbp:average_temperature |
around 12,000 K
|
| gptkbp:brightness_fluctuation |
notable for brightness fluctuations
|
| gptkbp:constellation |
gptkb:Cygnus
|
| gptkbp:contains_star |
possible binary system
classified as a variable star |
| gptkbp:coordinates |
located in the Milky Way galaxy
|
| gptkbp:cultural_references |
mentioned in various astronomical texts
|
| gptkbp:discovery_year |
1600s
|
| gptkbp:distance |
approximately 5,000 light years
|
| gptkbp:emissions_standard |
strong hydrogen and helium lines
|
| gptkbp:explosion |
potential supernova candidate
|
| gptkbp:first_described_by |
as a nova-like star
|
| gptkbp:formulation |
gptkb:Luminous_Blue_Variable
|
| gptkbp:has_luminosity |
approximately 100,000 times that of the Sun
evolved from a massive main-sequence star influences dynamics in its surrounding region |
| gptkbp:has_spectral_type |
gptkb:B-type_supergiant
|
| gptkbp:historical_significance |
one of the first stars to be classified as a nova
|
| https://www.w3.org/2000/01/rdf-schema#label |
P Cygni
|
| gptkbp:hubble_space_telescope_observation |
observed in various wavelengths
|
| gptkbp:is_observed_in |
gptkb:Johannes_Kepler
|
| gptkbp:lighting |
irregular variability
affected by light pollution in urban areas analyzed for light curve patterns exhibits irregular light curve variability |
| gptkbp:losses |
high mass loss rate due to stellar winds
|
| gptkbp:mass |
approximately 20 times that of the Sun
part of the massive star population in Cygnus |
| gptkbp:mass_loss_mechanism |
driven by radiation pressure
|
| gptkbp:notable_for |
its strong emission lines
|
| gptkbp:research |
difficult to observe due to its brightness
extensively studied in the 20th century important for scientific research in astrophysics |
| gptkbp:research_importance |
important for understanding massive star evolution
|
| gptkbp:spectroscopic_studies |
extensively studied spectroscopically
|
| gptkbp:stellar_nucleosynthesis |
contributes to nucleosynthesis in the galaxy
|
| gptkbp:stellar_remnants |
potential remnant of a supernova explosion
|
| gptkbp:stellar_wind_speed |
high stellar wind speed
|
| gptkbp:storage |
subject of many photometric studies
|
| gptkbp:type |
gptkb:Supernova
|
| gptkbp:bfsParent |
gptkb:LBV
gptkb:Luminous_Blue_Variables |
| gptkbp:bfsLayer |
7
|