Statements (52)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star cluster
|
| gptkbp:age |
approximately 2 million years
|
| gptkbp:associatedWith |
gptkb:Carina_star-forming_region
NGC 3372 |
| gptkbp:collaborations |
international astronomical community
|
| gptkbp:contains |
massive stars
|
| gptkbp:coordinates |
RA 10h 45m 0s, Dec -59° 40′ 0″
|
| gptkbp:established |
gptkb:Robert_Trumpler
|
| gptkbp:greatGrandfather |
potential for supernova events
|
| gptkbp:growthRate |
high star formation rate
|
| gptkbp:hasInternationalClassification |
classified as an open cluster
|
| gptkbp:hasPopulation |
age distribution analyzed
|
| gptkbp:historicalEvent |
first cataloged in 1930
|
| https://www.w3.org/2000/01/rdf-schema#label |
Trumpler 12
|
| gptkbp:image |
UBV_photometry_available
|
| gptkbp:internationalClassification |
spectroscopic studies conducted
|
| gptkbp:isFiledIn |
B-V = -0.33
|
| gptkbp:length |
approximately 8,000 light years
|
| gptkbp:lighting |
approximately 100,000 times that of the Sun
apparent magnitude 6.0 affected by light pollution in some regions |
| gptkbp:locatedIn |
gptkb:Carina_constellation
|
| gptkbp:model |
models applied to study evolution
|
| gptkbp:naturalResources |
solar metallicity
|
| gptkbp:nearbyAttractions |
trigonometric parallax used
|
| gptkbp:notableFeature |
HD 93129A
HD 93129B HD 93205 studies on stellar evolution |
| gptkbp:officialResidence |
high extinction due to dust
observed with ground-based telescopes |
| gptkbp:orbitalInclination |
mass function studied
stellar interactions observed |
| gptkbp:partOf |
gptkb:Carina_Nebula
|
| gptkbp:photography |
infrared imaging used
photometric variability studied |
| gptkbp:researchInterest |
numerous research papers published
studied for massive star formation |
| gptkbp:scientificName |
included in various astronomical catalogs
interactions with interstellar medium observed |
| gptkbp:servesGrade |
mass loss from stars observed
|
| gptkbp:size |
approximately 30 light years across
|
| gptkbp:termStart |
contains several variable stars
|
| gptkbp:type |
open cluster
O-type stars |
| gptkbp:universe |
dynamics of cluster studied
dynamics of stars analyzed |
| gptkbp:visibility |
best viewed in southern hemisphere
|
| gptkbp:vision |
young stellar population
strong stellar winds present |
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|
| gptkbp:weight |
approximately 10,000 solar masses
|