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Statements

Subject Item
dbr:HD_143699
rdf:type
dbo:CelestialBody yago:WikicatHenryDraperCatalogueObjects yago:Object100002684 dbo:Star yago:PhysicalEntity100001930 owl:Thing dbo:Place schema:Place dbo:Location
rdfs:label
HD 143699 HD 143699 HD 143699 HD143699
rdfs:comment
HD 143699 is a single star in the southern constellation of Lupus. It is a dim star but visible to the naked eye with an apparent visual magnitude of 4.90. Based upon an annual parallax shift of 9.2 mas, it is located around 350 light years away. It is most likely (90% chance) a member of the Upper Centaurus–Lupus subgroup of the Sco OB2 moving group. HD 143699，又名CD-3810832，SAO 207276、HR 5967，是一颗恒星，视星等为4.89，位于銀經339.12，銀緯10.43，其B1900.0坐标为赤經15h 56m 45s，赤緯-38° 10.43′ 24″。 'HD 143699 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Vargen. Den har en skenbar magnitud av ca 4,90 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 9,2 mas, beräknas den befinna sig på ett avstånd på ca 350 ljusår (ca 108 parsek) från solen. Den ingår med 90 procent sannolikhet i övre Centaurus-Lupus, en undergrupp av rörelsegruppen Scorpii OB2. HD143699 — хімічно пекулярна зоря спектрального класу B6, що має видиму зоряну величину в смузі V приблизно 4,9.Вона розташована на відстані близько 526,9 світлових років від Сонця.
foaf:name
HD 143699
dcterms:subject
dbc:Hipparcos_objects dbc:B-type_subgiants dbc:Durchmusterung_objects dbc:Lupus_(constellation) dbc:Helium-weak_stars dbc:Henry_Draper_Catalogue_objects dbc:Bright_Star_Catalogue_objects
dbo:wikiPageID
37692074
dbo:wikiPageRevisionID
1086505607
dbo:wikiPageWikiLink
dbr:Sun's_radius dbr:Sun's_luminosity dbr:Stellar_magnetic_field dbr:Giant_star dbc:Hipparcos_objects dbc:B-type_subgiants dbr:Lupus_(constellation) dbr:Effective_temperature dbr:Projected_rotational_velocity dbr:Sco_OB2 dbr:Moving_group dbr:Magnetic_field dbc:Lupus_(constellation) dbc:Durchmusterung_objects dbr:Photosphere dbr:Chemically_peculiar_star dbr:Stellar_spectrum dbr:Main_sequence dbc:Helium-weak_stars dbr:Stellar_classification dbr:Light_year dbr:Stellar_evolution dbr:Star dbr:Constellation dbr:Radio dbc:Henry_Draper_Catalogue_objects dbr:Mass_of_the_Sun dbr:Apparent_visual_magnitude dbr:Stellar_parallax dbc:Bright_Star_Catalogue_objects
owl:sameAs
dbpedia-sv:HD_143699 dbpedia-uk:HD143699 freebase:m.0ndxp7t n14:HD143699 n15:HD143699 wikidata:Q5629292 yago-res:HD_143699 dbpedia-zh:HD_143699 n24:4kwb9
dbp:wikiPageUsesTemplate
dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_astrometry dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_character dbt:DEC dbt:Starbox_observe dbt:RA dbt:Stars_of_Lupus dbt:Val dbt:Odlist dbt:Reflist dbt:Starbox_reference
dbp:absmagV
−0.54
dbp:appmagV
4.9
dbp:class
B5/7 III/IV
dbp:constell
dbr:Lupus_(constellation)
dbp:epoch
J2000
dbp:pError
0.4693
dbp:parallax
9.226800000000001
dbp:propMoDec
−28.147
dbp:propMoRa
−18.488
dbp:radius
4.4
dbp:rotationalVelocity
123
dbo:abstract
'HD 143699 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Vargen. Den har en skenbar magnitud av ca 4,90 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 9,2 mas, beräknas den befinna sig på ett avstånd på ca 350 ljusår (ca 108 parsek) från solen. Den ingår med 90 procent sannolikhet i övre Centaurus-Lupus, en undergrupp av rörelsegruppen Scorpii OB2. HD 143699，又名CD-3810832，SAO 207276、HR 5967，是一颗恒星，视星等为4.89，位于銀經339.12，銀緯10.43，其B1900.0坐标为赤經15h 56m 45s，赤緯-38° 10.43′ 24″。 HD143699 — хімічно пекулярна зоря спектрального класу B6, що має видиму зоряну величину в смузі V приблизно 4,9.Вона розташована на відстані близько 526,9 світлових років від Сонця. HD 143699 is a single star in the southern constellation of Lupus. It is a dim star but visible to the naked eye with an apparent visual magnitude of 4.90. Based upon an annual parallax shift of 9.2 mas, it is located around 350 light years away. It is most likely (90% chance) a member of the Upper Centaurus–Lupus subgroup of the Sco OB2 moving group. This star has a stellar classification of B5/7 III/IV, suggesting it is an evolving star that is entering the giant stage. However, according to Zorec and Royer (2012) it is only 56% of the way through its main sequence lifespan. It is a chemically peculiar magnetic B star, showing an averaged quadratic field strength of (167.2±140.4)×10−3 T. Helium-weak, it displays an underabundance of helium in its spectrum. Radio emissions have been detected from this source. HD 143699 has 4.3 times the mass of the Sun and 4.4 times the Sun's radius. It has a high rate of spin with a projected rotational velocity of 123 km/s. The star is radiating 438 times the Sun's luminosity from its photosphere at an effective temperature of 14,521 K.
gold:hypernym
dbr:Star
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wikipedia-en:HD_143699?oldid=1086505607&ns=0
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7406
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dbr:List_of_stars_in_Lupus
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dbr:HD_143699