Statements (140)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:open_cluster
gptkb:star |
| gptkbp:age |
about 1 million years
about 300,000 years around 2 million years |
| gptkbp:associated_with |
gptkb:star
star formation |
| gptkbp:availability |
data available for public access
|
| gptkbp:collaboration |
international collaboration in studies
|
| gptkbp:composed_by |
mostly hydrogen and helium
|
| gptkbp:contains |
young stars
massive stars |
| gptkbp:contains_star |
gptkb:HD_93129_B
gptkb:HD_93129_A gptkb:HD_93205 high star formation rate |
| gptkbp:coordinates |
located in the southern sky
|
| gptkbp:cultural_significance |
not significant in popular culture
|
| gptkbp:discovered_by |
gptkb:Robert_Trumpler
gptkb:Rudolf_Trumpler |
| gptkbp:discovery_year |
gptkb:1930
|
| gptkbp:distance_from_earth |
approximately 8,000 light years
about 8,000 light years |
| gptkbp:educational_value |
important for educational purposes
|
| gptkbp:future_prospects |
ongoing research planned
|
| gptkbp:has |
high stellar density
|
| gptkbp:has_color |
gptkb:blue
|
| gptkbp:has_luminosity |
frequent stellar interactions
rapid evolution of massive stars |
| gptkbp:has_spectral_type |
various types
O-type stars |
| https://www.w3.org/2000/01/rdf-schema#label |
Trumpler 14
|
| gptkbp:ingredients |
massive binary systems
|
| gptkbp:is_associated_with |
gptkb:NGC_3372
gptkb:interstellar_medium stellar formation massive star formation stellar winds massive star clusters star cluster dynamics |
| gptkbp:is_considered |
an important astronomical object
one of the most massive clusters |
| gptkbp:is_home_to |
O-type stars
multiple star systems young stellar objects blue supergiants massive binaries massive stars formation. multiple supernova progenitors |
| gptkbp:is_influential_in |
astrophysics research
stellar evolution studies stellar astrophysics |
| gptkbp:is_known_for |
high luminosity
stellar population studies stellar interactions star cluster formation high mass loss rates massive star population high concentration of young stars |
| gptkbp:is_located_at |
right ascension 10h 45m 3s
declination -59° 24' 0" |
| gptkbp:is_located_in |
southern hemisphere
Galactic plane |
| gptkbp:is_located_near |
gptkb:Carina_Nebula_core
gptkb:Eta_Carinae gptkb:NGC_3603 other star clusters |
| gptkbp:is_notable_for |
high luminosity
high stellar density high stellar activity high rate of stellar winds |
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
gptkb:Hubble_Space_Telescope optical wavelengths radio astronomy optical astronomy |
| gptkbp:is_part_of |
gptkb:Carina_star-forming_region
gptkb:Carina_constellation gptkb:NGC_3372 gptkb:star gptkb:Milky_Way_Galaxy stellar nursery Milky Way structure star cluster research open cluster family star cluster catalog star cluster formation theories |
| gptkbp:is_studied_for |
stellar dynamics
stellar evolution stellar population synthesis massive star clusters star cluster evolution stellar population characteristics |
| gptkbp:is_studied_in |
gptkb:spectroscopy
gptkb:astronomy astrophysics photometry |
| gptkbp:is_surrounded_by |
nebulae
|
| gptkbp:is_visible_from |
gptkb:Earth
Southern Hemisphere infrared spectrum visible light certain seasons infrared wavelengths |
| gptkbp:light_pollution_impact |
minimal impact due to location
|
| gptkbp:lighting |
very bright
apparent magnitude 6.0 light curve variability observed |
| gptkbp:located_in |
gptkb:Carina_Nebula
|
| gptkbp:losses |
significant mass loss from massive stars
|
| gptkbp:mass |
approximately 10,000 solar masses
about 100,000 solar masses contains hundreds of stars |
| gptkbp:nebula_interaction |
interacts with surrounding nebula
|
| gptkbp:notable_feature |
massive stars
|
| gptkbp:notable_person |
gptkb:HD_93129_B
gptkb:HD_93129_A WR 25 |
| gptkbp:notable_work |
studied for its massive star population
|
| gptkbp:part_of |
gptkb:Milky_Way_Galaxy
|
| gptkbp:population_density |
high density
|
| gptkbp:publications |
numerous scientific publications exist
|
| gptkbp:research |
observed since the 20th century
high extinction due to dust various observational techniques used |
| gptkbp:research_importance |
study of massive star formation
|
| gptkbp:research_institutes |
studied by multiple research institutions
|
| gptkbp:size |
about 30 light years across
|
| gptkbp:spectroscopic_studies |
spectroscopic studies of member stars
|
| gptkbp:stellar_age_range |
varied ages among stars
|
| gptkbp:stellar_cluster_dynamics |
dynamics influenced by massive stars
|
| gptkbp:stellar_mass_distribution |
varied mass distribution among stars
|
| gptkbp:stellar_wind_impact |
strong stellar winds from massive stars
|
| gptkbp:storage |
extensive photometric studies conducted
|
| gptkbp:supernova_potential |
potential for future supernovae
|
| gptkbp:surrounding_area |
Giant Molecular Cloud
|
| gptkbp:type |
gptkb:open_cluster
gptkb:star |
| gptkbp:bfsParent |
gptkb:Carina_Nebula
|
| gptkbp:bfsLayer |
4
|