Properties (61)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star cluster
|
| gptkbp:age |
approximately 10 million years
|
| gptkbp:associatedWith |
none known
|
| gptkbp:beam |
impact on surrounding gas
|
| gptkbp:bestTimeToVisit |
summer months
|
| gptkbp:collaborations |
international research teams
|
| gptkbp:collectionSize |
monitored over time
|
| gptkbp:contains |
several hundred stars
|
| gptkbp:dataUsage |
accessible through databases
|
| gptkbp:diameter |
approximately 10 light years
higher than surrounding area |
| gptkbp:established |
gptkb:Robert_Trumpler
|
| gptkbp:exhibits |
included in various star catalogs
|
| gptkbp:format |
active region
|
| gptkbp:geographicalFeature |
l = 30.5°, b = -5.0°
|
| gptkbp:growthRate |
estimated from observations
|
| gptkbp:hasVariants |
-06° 24' 00"
|
| gptkbp:historicalEvent |
monitored for decades
|
| gptkbp:historicalResearch |
ongoing studies planned.
|
| gptkbp:historicalSignificance |
noted by early astronomers
|
| https://www.w3.org/2000/01/rdf-schema#label |
Trumpler 11
|
| gptkbp:image |
available in various catalogs
based_on_isochrone_fitting |
| gptkbp:internationalClassification |
used to analyze star composition
|
| gptkbp:is_a_hub_for |
studied for gravitational interactions
|
| gptkbp:isFiledIn |
B-V = 0.5
|
| gptkbp:legalStatus |
18h 53m 30s
|
| gptkbp:length |
approximately 4,000 light years
|
| gptkbp:lighting |
variable stars present
apparent magnitude 6.5 visible from urban areas |
| gptkbp:localHistory |
investigated through simulations
|
| gptkbp:locatedIn |
Milky Way
|
| gptkbp:membership |
part_of_the_Scutum_constellation
|
| gptkbp:missionCapabilities |
used for analysis
|
| gptkbp:naturalResources |
solar metallicity
|
| gptkbp:nearbyAttractions |
NGC 6705
|
| gptkbp:notableFeature |
HD 170740
HD 170741 HD 170742 |
| gptkbp:officialResidence |
crowded field
visible in binoculars |
| gptkbp:orbitalInclination |
analyzed for distribution
applied to understand composition studied for close encounters |
| gptkbp:photography |
used for distance estimation
captured in various wavelengths noted in some stars |
| gptkbp:publications |
numerous scientific papers
|
| gptkbp:relatedModel |
compared with theoretical predictions
|
| gptkbp:releaseYear |
1930
|
| gptkbp:researchInterest |
studied for stellar evolution
|
| gptkbp:scientificName |
important for cluster dynamics
influences cluster environment |
| gptkbp:serves |
observed in massive stars
|
| gptkbp:type |
open cluster
various types |
| gptkbp:universe |
part of larger galactic structure
|
| gptkbp:vision |
young stars
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|
| gptkbp:weight |
approximately 1,000 solar masses
|