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Statements

Subject Item
dbr:HD_63922
rdf:type
dbo:Star yago:Whole100003553 owl:Thing yago:CelestialBody109239740 dbo:Place yago:Organism100004475 yago:PhysicalEntity100001930 schema:Place dbo:Location yago:NaturalObject100019128 dbo:CelestialBody yago:Animal100015388 yago:WikicatB-typeStars yago:WikicatBinaryStars yago:WikicatB-typeGiants yago:BinaryStar109221070 yago:Giant101323781 yago:Star109444100 yago:WikicatHenryDraperCatalogueObjects yago:Object100002684 yago:LivingThing100004258
rdfs:label
HD 63922 HD 63922 HD 63922 HD 63922 HD 63922 199 Puppis
rdfs:comment
HD 63922 is a class B0III (blue giant) star in the constellation Puppis. Its apparent magnitude is 4.11 and it is approximately 1600 light years away based on parallax. It is a multiple star; the primary has one close companion, Ab, at 0.3" separation and magnitude 7.19, and a more distant one, B, at 59.1" and 8.79 magnitude. P Puppis( Ne doit pas être confondu avec (= HD 60863), ni avec ρ (Rho) Puppis. ) P PuppisHD 63922 Autres désignations P Pup, HR 3055, HD 63922, HIP 38164, CD-46 3458, CPD-46 1795, SAO 219035, WDS J07492 -4622 Aa,Ab P Puppis (en abrégé P Pup), également désignée HD 63922 ou HR 3055, est une étoile binaire de la constellation australe de la Poupe. Sa magnitude apparente est de 4,11. D'après la mesure de sa parallaxe par le satellite Hipparcos, le système est distant d'environ 510 pc (∼1 660 a.l.) de la Terre. Il se rapproche du système solaire à une vitesse radiale héliocentrique de −24 km/s. HD 63922 (nota anche come P Puppis) è una stella gigante azzurra di magnitudine 4,09 situata nella costellazione della Poppa. Dista 1608 anni luce dal sistema solare. 199 Puppis (P Puppis) é uma estrela na direção da Puppis. Possui uma ascensão reta de 07h 49m 14.30s e uma declinação de −46° 22′ 23.6″. Sua magnitude aparente é igual a 4.10. Considerando sua distância de 1964 anos-luz em relação à Terra, sua magnitude absoluta é igual a −4.80. Pertence à classe espectral B0III. HD 63922 är en trippelstjärna belägen i den södra delen av stjärnbilden Akterskeppet, som också har Bayer-beteckningen P Puppis. Den har en skenbar magnitud av ca 4,11 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 2,0 mas, beräknas den befinna sig på ett avstånd på ca 1 600 ljusår (ca 510 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 24 km/s. HD 63922，又名CD-46 3458，SAO 219035、HR 3055，是一颗恒星，视星等为4.11，位于銀經260.18，銀緯-10.19，其B1900.0坐标为赤經7h 46m 11.4s，赤緯-46° -10.19′ 16″。
foaf:name
HD 63922
foaf:depiction
n9:Puppis_constellation_map.svg n9:Red_circle.svg
dcterms:subject
dbc:Puppis dbc:Bayer_objects dbc:Henry_Draper_Catalogue_objects dbc:Bright_Star_Catalogue_objects dbc:Binary_stars dbc:Hipparcos_objects dbc:B-type_giants dbc:Durchmusterung_objects
dbo:wikiPageID
38324388
dbo:wikiPageRevisionID
1079514939
dbo:wikiPageWikiLink
dbr:Harvard_Revised_catalogue dbr:Rho_Puppis dbr:Constellation dbr:Boss_General_catalogue dbr:Star dbc:Puppis dbc:Henry_Draper_Catalogue_objects dbc:Bayer_objects dbr:Smithsonian_Astrophysical_Observatory_catalogue dbr:Durchmusterung dbr:Hipparcos_catalogue dbr:Guide_Star_Catalogue dbc:Bright_Star_Catalogue_objects dbr:Henry_Draper_Catalogue dbc:Durchmusterung_objects dbr:Catalog_of_Components_of_Double_and_Multiple_Stars dbc:Binary_stars dbr:Washington_Double_Star_Catalog dbc:Hipparcos_objects dbc:B-type_giants dbr:Puppis_(constellation)
owl:sameAs
wikidata:Q3781481 dbpedia-fr:HD_63922 n10:3VXGj freebase:m.0q40qtn yago-res:HD_63922 dbpedia-zh:HD_63922 dbpedia-pt:199_Puppis dbpedia-sv:HD_63922 dbpedia-it:HD_63922
dbp:wikiPageUsesTemplate
dbt:About dbt:Distinguish dbt:Short_description dbt:Stars_of_Puppis dbt:Location_mark dbt:Giant-star-stub dbt:Multi-star-stub dbt:Starbox_reference dbt:DEC dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_character dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_astrometry dbt:Reflist dbt:RA
dbo:thumbnail
n9:Puppis_constellation_map.svg?width=300
dbp:absmagV
-4.37
dbp:appmagV
4.11
dbp:bV
−0.18
dbp:class
B0III
dbp:constell
dbr:Puppis_(constellation)
dbp:epoch
J2000
dbp:gravity
3.95
dbp:luminosity
3209
dbp:mass
19.3
dbp:metalFe
+0.16
dbp:pError
0.28
dbp:parallax
1.98
dbp:propMoDec
+8.66
dbp:propMoRa
-4.37
dbp:radialV
+24.00
dbp:rotationalVelocity
49
dbp:temperature
31200
dbp:uB
−1.01
dbo:abstract
P Puppis( Ne doit pas être confondu avec (= HD 60863), ni avec ρ (Rho) Puppis. ) P PuppisHD 63922 Autres désignations P Pup, HR 3055, HD 63922, HIP 38164, CD-46 3458, CPD-46 1795, SAO 219035, WDS J07492 -4622 Aa,Ab P Puppis (en abrégé P Pup), également désignée HD 63922 ou HR 3055, est une étoile binaire de la constellation australe de la Poupe. Sa magnitude apparente est de 4,11. D'après la mesure de sa parallaxe par le satellite Hipparcos, le système est distant d'environ 510 pc (∼1 660 a.l.) de la Terre. Il se rapproche du système solaire à une vitesse radiale héliocentrique de −24 km/s. HD 63922，又名CD-46 3458，SAO 219035、HR 3055，是一颗恒星，视星等为4.11，位于銀經260.18，銀緯-10.19，其B1900.0坐标为赤經7h 46m 11.4s，赤緯-46° -10.19′ 16″。 199 Puppis (P Puppis) é uma estrela na direção da Puppis. Possui uma ascensão reta de 07h 49m 14.30s e uma declinação de −46° 22′ 23.6″. Sua magnitude aparente é igual a 4.10. Considerando sua distância de 1964 anos-luz em relação à Terra, sua magnitude absoluta é igual a −4.80. Pertence à classe espectral B0III. HD 63922 is a class B0III (blue giant) star in the constellation Puppis. Its apparent magnitude is 4.11 and it is approximately 1600 light years away based on parallax. It is a multiple star; the primary has one close companion, Ab, at 0.3" separation and magnitude 7.19, and a more distant one, B, at 59.1" and 8.79 magnitude. HD 63922 (nota anche come P Puppis) è una stella gigante azzurra di magnitudine 4,09 situata nella costellazione della Poppa. Dista 1608 anni luce dal sistema solare. HD 63922 är en trippelstjärna belägen i den södra delen av stjärnbilden Akterskeppet, som också har Bayer-beteckningen P Puppis. Den har en skenbar magnitud av ca 4,11 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 2,0 mas, beräknas den befinna sig på ett avstånd på ca 1 600 ljusår (ca 510 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 24 km/s.
gold:hypernym
dbr:Star
prov:wasDerivedFrom
wikipedia-en:HD_63922?oldid=1079514939&ns=0
dbo:wikiPageLength
5657
foaf:isPrimaryTopicOf
wikipedia-en:HD_63922