About: HD 163376

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http://dbpedia.org/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FHD_163376

HD 163376 is a single star in the southern constellation of Scorpius. It has a ruddy hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.88. The distance to this star, as determined using parallax measurements, is approximately 450 light years. It is drifting further from the Sun with a radial velocity of about 4 km/s. The absolute magnitude of this star is −0.82.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body yago:WikicatM-typeGiants yago:WikicatVariableStars yago:Animal100015388 yago:CelestialBody109239740 yago:Giant101323781 yago:LivingThing100004258 yago:NaturalObject100019128 yago:Object100002684 yago:Organism100004475 yago:PhysicalEntity100001930 yago:WikicatHenryDraperCatalogueObjects star yago:Star109444100 yago:VariableStar109469152 yago:Whole100003553
rdfs:label	HD 163376 (en) HD 163376 (sv) HD 163376 (zh)
rdfs:comment	HD 163376 är en ensam stjärna belägen i den södra delen av stjärnbilden Skorpionen. Den har en högsta skenbar magnitud av ca 4,88 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,2 mas, beräknas den befinna sig på ett avstånd på ca 450 ljusår (ca 139 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 4 km/s. (sv) HD 163376，又名CD-4112231，SAO 228578、HR 6682，是一颗恒星，视星等为4.88，位于銀經350.18，銀緯-8.59，其B1900.0坐标为赤經17h 50m 41.4s，赤緯-41° -8.59′ 7″。 (zh) HD 163376 is a single star in the southern constellation of Scorpius. It has a ruddy hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.88. The distance to this star, as determined using parallax measurements, is approximately 450 light years. It is drifting further from the Sun with a radial velocity of about 4 km/s. The absolute magnitude of this star is −0.82. (en)
dcterms:subject	Bright Star Catalogue objects Durchmusterung objects Henry Draper Catalogue objects Hipparcos objects M-type giants Scorpius (constellation) Suspected variables
Wikipage page ID	38559576 (xsd:integer)
Wikipage revision ID	1079519495 (xsd:integer)
Link from a Wikipage to another Wikipage	Stellar classification Bright Star Catalogue objects Durchmusterung objects Henry Draper Catalogue objects Hipparcos objects M-type giants Scorpius (constellation) Suspected variables Constellation Photosphere Effective temperature Light year Star Stellar parallax Absolute magnitude Stellar core Red giant Sun Apparent visual magnitude Radial velocity Variable star Scorpius (constellation) Radius of the Sun Sun's luminosity
sameAs	HD 163376 HD 163376 HD 163376 HD 163376 HD 163376 HD 163376 HD 163376 HD 163376
dbp:wikiPageUsesTemplate	dbt:End dbt:Reflist dbt:Starbox_astrometry dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_character dbt:Starbox_detail dbt:Starbox_observe dbt:Starbox_reference dbt:Stars_of_Scorpius dbt:Val dbt:DEC dbt:Odlist dbt:RA
absmag v	−0.82 (en)
appmag v	4.880000 (xsd:double)
class	M0 III (en)
constell	Scorpius (constellation)
epoch	J2000 (en)
gravity	0.790000 (xsd:double)
mass	1.120000 (xsd:double)
metal fe	+0.04 (en)
p error	0.270000 (xsd:double)
parallax	7.220000 (xsd:double)
variable	suspected (en)
has abstract	HD 163376 is a single star in the southern constellation of Scorpius. It has a ruddy hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.88. The distance to this star, as determined using parallax measurements, is approximately 450 light years. It is drifting further from the Sun with a radial velocity of about 4 km/s. The absolute magnitude of this star is −0.82. This object is an aging red giant star with a stellar classification of M0 III, having exhausted the supply of hydrogen at its core then cooled and expanded. At present it has a radius around 61 times the radius of the Sun. It is a suspected variable star of unknown type, with a brightness that has been measured ranging from 4.94 down to 4.98. The star is radiating 832 times the Sun's luminosity from its photosphere at an effective temperature of 3,972 K. (en) HD 163376 är en ensam stjärna belägen i den södra delen av stjärnbilden Skorpionen. Den har en högsta skenbar magnitud av ca 4,88 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,2 mas, beräknas den befinna sig på ett avstånd på ca 450 ljusår (ca 139 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 4 km/s. (sv) HD 163376，又名CD-4112231，SAO 228578、HR 6682，是一颗恒星，视星等为4.88，位于銀經350.18，銀緯-8.59，其B1900.0坐标为赤經17h 50m 41.4s，赤緯-41° -8.59′ 7″。 (zh)
gold:hypernym	Star
prov:wasDerivedFrom	wikipedia-en:HD_163376?oldid=1079519495&ns=0
page length (characters) of wiki page	5852 (xsd:nonNegativeInteger)
foaf:isPrimaryTopicOf	wikipedia-en:HD_163376
is Link from a Wikipage to another Wikipage of	HIP 87936

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