Statements (90)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:Puppis_constellation
gptkb:Puppis gptkb:Argo_Navis |
| gptkbp:age |
approximately 10 million years
approximately 5 million years |
| gptkbp:apparent_magnitude |
-0.5
2.2 -6.5 |
| gptkbp:area |
approximately 30 times that of the Sun
approximately 15 solar radii approximately 30 solar radii |
| gptkbp:average_temperature |
approximately 20,000 K
approximately 22,000 K |
| gptkbp:brand |
gptkb:HD_66811
|
| gptkbp:constellation |
gptkb:Puppis
|
| gptkbp:cultural_significance |
navigational star
|
| gptkbp:curated_by |
gptkb:HIP_39444
|
| gptkbp:depicted_in |
gptkb:physicist
visible to the naked eye southern hemisphere |
| gptkbp:distance |
approximately 63 light years
approximately 460 light years |
| gptkbp:exhibition |
the Henry Draper Catalogue
the Yale Bright Star Catalog |
| gptkbp:formulation |
not a variable star
|
| gptkbp:has_color |
-0.25
|
| gptkbp:has_friend |
gptkb:Zeta_Puppis_B
|
| gptkbp:has_luminosity |
approximately 100,000 times that of the Sun
approximately 60,000 times that of the Sun |
| gptkbp:has_setting |
gptkb:HIP_39402
|
| gptkbp:has_spectral_type |
B2 Iae
|
| gptkbp:has_team |
-0.12 arcseconds/year
0.01 arcseconds/year -0.05 arcseconds/year |
| https://www.w3.org/2000/01/rdf-schema#label |
Zeta Puppis
|
| gptkbp:includes |
star catalogs
|
| gptkbp:is_a |
gptkb:star
|
| gptkbp:is_associated_with |
massive star formation regions
the Puppis constellation |
| gptkbp:is_considered_as |
a potential supernova candidate
a benchmark for stellar models |
| gptkbp:is_involved_in |
stellar evolution
|
| gptkbp:is_known_for |
strong stellar winds
its brightness and size its role in understanding stellar evolution. its high mass loss rate |
| gptkbp:is_noted_for |
its rapid rotation
its significant brightness variation |
| gptkbp:is_observed_in |
amateur astronomers
telescopes various wavelengths |
| gptkbp:is_part_of |
gptkb:Milky_Way_galaxy
the southern celestial hemisphere the HR diagram the local stellar neighborhood the southern sky the galactic structure the Milky Way's stellar population the open cluster NGC 2451 the Puppis constellation group the brightest stars in its constellation |
| gptkbp:is_recognized_by |
its Bayer designation
|
| gptkbp:is_referenced_in |
various astronomical studies
|
| gptkbp:is_related_to |
other blue supergiants
|
| gptkbp:is_studied_in |
astrophysics
stellar atmospheres |
| gptkbp:is_used_in |
navigational astronomy
stellar classification systems |
| gptkbp:leadership |
gptkb:HD_66811
|
| gptkbp:located_in |
constellation Puppis
|
| gptkbp:marketed_as |
gptkb:Zeta_Puppis
|
| gptkbp:mass |
approximately 20 solar masses
approximately 20 times that of the Sun |
| gptkbp:measures |
photometry
|
| gptkbp:name |
gptkb:Zeta_Puppis
|
| gptkbp:named_after |
the Greek letter Zeta
|
| gptkbp:notable_feature |
high luminosity
massive size rapid rotation strong stellar winds part of the Milky Way part of the Argo Navis constellation |
| gptkbp:parallax |
0.051 arcseconds
|
| gptkbp:scientific_classification |
a luminous blue variable star
|
| gptkbp:type |
blue supergiant
|
| gptkbp:type_of |
blue supergiant
|
| gptkbp:year_created |
1834
ancient times |