About: HD 34266

An Entity of Type: star, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org:8891

HD 34266, also known as HR 1721 is a solitary, yellow hued star located in the southern constellation Columba, the dove. It has an apparent magnitude of 5.73, making it faintly visible to the naked eye under ideal conditions. Based on Gaia DR3 parallax measurements, the object is located 539 light years away. It appears to be drifting away from the Solar System, having a heliocentric radial velocity of 13.2 km/s.

Property	Value
dbo:abstract	HD 34266, also known as HR 1721 is a solitary, yellow hued star located in the southern constellation Columba, the dove. It has an apparent magnitude of 5.73, making it faintly visible to the naked eye under ideal conditions. Based on Gaia DR3 parallax measurements, the object is located 539 light years away. It appears to be drifting away from the Solar System, having a heliocentric radial velocity of 13.2 km/s. This is an evolved giant star that is currently on the red giant branch, fusing hydrogen in a shell around an inert helium core. It has a stellar classification of G8 III. HD 34266 is calculated to be 490 million years old, almost 10 times younger than our Sun. However, it already left the main sequence due to a mass of 3.42 M☉. HD 34266 has expanded to 16.2 times the Sun's girth and now radiates 144 times the luminosity of the Sun from its photosphere at an effective temperature of 4,970 K. HD 34266 has a near solar metallicity and spins modestly with a projected rotational velocity of 2.3 km/s. (en) HD 34266 är en ensam stjärna i den mellersta delen av stjärnbilden Duvan. Den har en skenbar magnitud av ca 5,73 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 6,0 mas, beräknas den befinna sig på ett avstånd på ca 548 ljusår (ca 168 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 13 km/s. (sv) HD 34266，又名CD-36 2127，SAO 195683、HR 1721，是一颗恒星，视星等为5.76，位于銀經239.65，銀緯-34.3，其B1900.0坐标为赤經5h 10m 56.5s，赤緯-36° -34.3′ 29″。 (zh)
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dbp:bV	+1.01 (en)
dbp:class	G8 III (en)
dbp:constell	dbr:Columba_(constellation)
dbp:epoch	J2000 (en)
dbp:gravity	2.680000 (xsd:double)
dbp:luminosity	144 (xsd:integer)
dbp:mass	3.420000 (xsd:double)
dbp:metalFe	+0.04 (en)
dbp:pError	0.031600 (xsd:double)
dbp:parallax	6.046000 (xsd:double)
dbp:propMoDec	+13.944 (en)
dbp:propMoRa	+11.005 (en)
dbp:radialV	13.200000 (xsd:double)
dbp:radius	16.200000 (xsd:double)
dbp:rotationalVelocity	2.300000 (xsd:double)
dbp:temperature	4970 (xsd:integer)
dbp:type	dbr:Red_giant_branch
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rdfs:comment	HD 34266 är en ensam stjärna i den mellersta delen av stjärnbilden Duvan. Den har en skenbar magnitud av ca 5,73 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 6,0 mas, beräknas den befinna sig på ett avstånd på ca 548 ljusår (ca 168 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 13 km/s. (sv) HD 34266，又名CD-36 2127，SAO 195683、HR 1721，是一颗恒星，视星等为5.76，位于銀經239.65，銀緯-34.3，其B1900.0坐标为赤經5h 10m 56.5s，赤緯-36° -34.3′ 29″。 (zh) HD 34266, also known as HR 1721 is a solitary, yellow hued star located in the southern constellation Columba, the dove. It has an apparent magnitude of 5.73, making it faintly visible to the naked eye under ideal conditions. Based on Gaia DR3 parallax measurements, the object is located 539 light years away. It appears to be drifting away from the Solar System, having a heliocentric radial velocity of 13.2 km/s. (en)
rdfs:label	HD 34266 (en) HD 34266 (sv) HD 34266 (zh)
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