NGC 2516

GPTKB entity

Statements (105)
Predicate Object
gptkbp:instance_of gptkb:open_cluster
gptkb:star
gptkbp:age approximately 135 million years
gptkbp:apparent_magnitude 4.5
used to study stellar populations
gptkbp:associated_with the Carina Nebula
gptkbp:astrophysical_importance important for studying stellar evolution
gptkbp:astrophysical_significance studied for stellar evolution
gptkbp:cluster_age age estimated through isochrone fitting.
gptkbp:cluster_formation formed from a star-forming region.
gptkbp:cluster_shape irregular shape observed.
gptkbp:collaborations collaborative studies with international teams.
gptkbp:contains_star gptkb:NGC_2547
gptkb:NGC_2451
gptkb:NGC_2546
approximately 100
approximately 100 stars
formed from the same molecular cloud
studied for its gravitational interactions.
gptkbp:coordinates RA 07h 58m, Dec -60° 53'.
l = 287.5°, b = -6.0°
gptkbp:cultural_references mentioned in astronomical literature.
gptkbp:declination -60° 53' 00"
gptkbp:discovered_by gptkb:James_Dunlop
gptkb:John_Frederick_William_Herschel
gptkbp:discovery_year 1826
1834
gptkbp:distance distance estimated using parallax.
gptkbp:distance_from_earth about 1,200 light years
gptkbp:educational_value used in educational astronomy programs.
gptkbp:exhibition gptkb:New_General_Catalogue
gptkbp:frequency observed throughout the year in southern hemisphere
gptkbp:future_prospects ongoing research planned.
gptkbp:has_color 0.5
B-V = 0.5
gptkbp:has_luminosity provides insights into stellar evolution processes
provides insights into stellar life cycles.
gptkbp:has_spectral_type various types
gptkbp:historical_significance one of the prominent clusters in the southern sky.
https://www.w3.org/2000/01/rdf-schema#label NGC 2516
gptkbp:image Hubble Space Telescope images available
gptkbp:is_visible_from best viewed in southern hemisphere
gptkbp:light_pollution_impact visibility affected by urban areas.
gptkbp:lighting moderately bright cluster
appears bright to the naked eye.
light curves of member stars analyzed
gptkbp:located_in gptkb:Carina_constellation
gptkbp:location southern celestial hemisphere
gptkbp:mass approximately 1,000 solar masses
mainly young stars
contains a mix of early and late-type stars.
mass estimated through dynamical studies.
gptkbp:membership includes both main sequence and giant stars
contains both binary and single stars
gptkbp:merchandise associated with the Carina Nebula.
gptkbp:metallicity solar metallicity
gptkbp:notable_person gptkb:HD_65750
gptkb:HD_65751
gptkb:HD_65752
gptkb:HD_65753
gptkb:HD_65754
HD 65802
HD 65803
HD 65804
HD 65805
HD 65806
HD 65807
HD 65808
HD 65809
HD 65810
gptkbp:population_density moderate density
moderate density cluster
gptkbp:previous_name C 0755-605
Collinder 228
Loden 100
Melotte 112
gptkbp:public_interest popular among amateur astronomers.
gptkbp:research observed by many astronomers
observed by various astronomers
observed with telescopes
available in various astronomical databases
best observed during winter months.
can be affected by light pollution.
data collected from various observatories.
subject of various astrophysical studies
light pollution affects visibility
best viewed with binoculars
gptkbp:research_focus studied for its stellar dynamics
used to study stellar dynamics.
gptkbp:research_importance important for understanding open clusters.
gptkbp:right_ascension 07h 58m 00s
gptkbp:scientific_classification classified as a young open cluster.
gptkbp:size approximately 20 arcminutes
gptkbp:spectroscopic_studies spectroscopic data collected.
gptkbp:star_count approximately 100 stars identified.
gptkbp:stellar_motion stars exhibit proper motion.
gptkbp:storage available
extensive photometric studies conducted.
extensively studied in photometry
gptkbp:type gptkb:open_cluster
Galactic open cluster
gptkbp:bfsParent gptkb:Carina
gptkb:Carina_constellation
gptkb:NGC_3293
gptkbp:bfsLayer 5