About: Theta Pavonis

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θ Pavonis, Latinized as Theta Pavonis, is a single star in the southern constellation of Pavo. It is just visible to the naked eye as a dim, white-hued star, having an apparent visual magnitude of 5.71. This star is located 213 light years from the Sun based on parallax. It lies six arc-minutes north of the barred lenticular galaxy .

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body star
rdfs:label	Theta Pavonis (pt) Theta Pavonis (en) Theta Pavonis (sv) 孔雀座θ (zh)
rdfs:comment	Theta Pavonis (θ Pav, förkortat Theta Pav, θ Pav) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Påfågeln. Den har en skenbar magnitud på 5,73och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 14,8 mas, beräknas den befinna sig på ett avstånd på ca 221 ljusår (ca 68 parsek) från solen. (sv) Theta Pavonis (43 Pavonis) é uma estrela na direção da constelação de Pavo. Possui uma ascensão reta de 18h 48m 37.96s e uma declinação de −65° 04′ 39.0″. Sua magnitude aparente é igual a 5.71. Considerando sua distância de 226 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.54. Pertence à classe espectral A9V. (pt) 孔雀座θ，又名CP-65 3754，HD 173168、SAO 254374、HR 7036，是孔雀座的一颗恒星，视星等为5.73，位于銀經330.43，銀緯-24.14，其B1900.0坐标为赤經18h 38m 48s，赤緯-65° -24.14′ 52″。 (zh) θ Pavonis, Latinized as Theta Pavonis, is a single star in the southern constellation of Pavo. It is just visible to the naked eye as a dim, white-hued star, having an apparent visual magnitude of 5.71. This star is located 213 light years from the Sun based on parallax. It lies six arc-minutes north of the barred lenticular galaxy . (en)
foaf:name	θ Pavonis (en)
foaf:depiction
dct:subject	A-type main-sequence stars Bayer objects Bright Star Catalogue objects Durchmusterung objects Henry Draper Catalogue objects Hipparcos objects Pavo (constellation)
Wikipage page ID	45496549 (xsd:integer)
Wikipage revision ID	1118102271 (xsd:integer)
Link from a Wikipage to another Wikipage	Pavo (constellation) Stellar classification A-type main-sequence stars Bayer objects Bright Star Catalogue objects Durchmusterung objects Henry Draper Catalogue objects Hipparcos objects Constellation Photosphere Effective temperature Convection zone Barred lenticular galaxy Arc-minute Light year Star Stellar parallax A-type main-sequence star Pavo (constellation) Stellar core Apparent visual magnitude X-ray astronomy Romanization of Greek Mass of the Sun Hydrogen fusion Sun's radius Projected rotational velocity Luminosity of the Sun dbr:NGC_6684
sameAs	Theta Pavonis Theta Pavonis Theta Pavonis Theta Pavonis Theta Pavonis Theta Pavonis Theta Pavonis
dbp:wikiPageUsesTemplate	dbt:Cn dbt:Reflist dbt:Short_description dbt:Starbox_astrometry dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_character dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_reference dbt:Val dbt:DEC dbt:Location_mark dbt:Odlist dbt:RA dbt:Stars_of_Pavo
thumbnail	wiki-commons:Special:FilePath/Pavo_constellation_map.svg?width=300
absmag v	1.560000 (xsd:double)
age myr	425 (xsd:integer)
appmag v	5.710000 (xsd:double)
class	A8V (en)
constell	Pavo (constellation)
epoch	J2000 (en)
mass	1.560000 (xsd:double)
metal fe	+0.01 (en)
p error	0.074100 (xsd:double)
parallax	15.325200 (xsd:double)
prop mo dec	−78.246 (en)
prop mo ra	−38.266 (en)
rotational velocity	245 (xsd:integer)
type	main sequence (en)
has abstract	θ Pavonis, Latinized as Theta Pavonis, is a single star in the southern constellation of Pavo. It is just visible to the naked eye as a dim, white-hued star, having an apparent visual magnitude of 5.71. This star is located 213 light years from the Sun based on parallax. This object is an A-type main-sequence star with a stellar classification of A8V, which indicates it is generating energy through hydrogen fusion at its core. It displays little to no detectable X-ray emission, suggesting a weak corona and, at best, a shallow convection zone. Theta Pavonis is 425 million years old and is spinning rapidly with a projected rotational velocity of 245 km/s. The star has 1.56 times the mass of the Sun and 2.51 times the Sun's radius. It is radiating 17.4 times the luminosity of the Sun from its photosphere at an effective temperature of 7,453 K. It lies six arc-minutes north of the barred lenticular galaxy . (en) Theta Pavonis (θ Pav, förkortat Theta Pav, θ Pav) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Påfågeln. Den har en skenbar magnitud på 5,73och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 14,8 mas, beräknas den befinna sig på ett avstånd på ca 221 ljusår (ca 68 parsek) från solen. (sv) Theta Pavonis (43 Pavonis) é uma estrela na direção da constelação de Pavo. Possui uma ascensão reta de 18h 48m 37.96s e uma declinação de −65° 04′ 39.0″. Sua magnitude aparente é igual a 5.71. Considerando sua distância de 226 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.54. Pertence à classe espectral A9V. (pt) 孔雀座θ，又名CP-65 3754，HD 173168、SAO 254374、HR 7036，是孔雀座的一颗恒星，视星等为5.73，位于銀經330.43，銀緯-24.14，其B1900.0坐标为赤經18h 38m 48s，赤緯-65° -24.14′ 52″。 (zh)
gold:hypernym	Star

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