About: 60 Sagittarii

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

60 Sagittarii is a suspected binary star system in the southern constellation of Sagittarius. It has the Bayer designation A Sagittarii, while 60 Sagittarii is the Flamsteed designation. This naked-eye object forms the northwest corner of the asterism called the Terebellum and, with an apparent magnitude of approximately 4.84, it is the dimmest of the four stars in the Terebellum. It is located 379 light-years from the Sun, based on parallax, but is moving closer with a radial velocity of −51 km/s.

thumbnail
Property Value
dbo:abstract
  • 60 Sagittarii is a suspected binary star system in the southern constellation of Sagittarius. It has the Bayer designation A Sagittarii, while 60 Sagittarii is the Flamsteed designation. This naked-eye object forms the northwest corner of the asterism called the Terebellum and, with an apparent magnitude of approximately 4.84, it is the dimmest of the four stars in the Terebellum. It is located 379 light-years from the Sun, based on parallax, but is moving closer with a radial velocity of −51 km/s. The visible component is an aging G-type giant star with a stellar classification of G6 III, having exhausted the supply of hydrogen at its core and expanded to 17 the Sun's radius. In the Bright Star Catalogue it was listed with a class of G6 III Ba0.2, suggesting it is a mild barium star and thus might have a white dwarf companion. It is a red clump giant, indicating it is on the horizontal branch and is generating energy through the fusion of helium at its core. The star is radiating 170 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,997 K. (en)
  • 60 Sagittarii (A Sagittarii) é uma estrela na direção da Sagittarius. Possui uma ascensão reta de 19h 58m 57.18s e uma declinação de −26° 11′ 45.0″. Sua magnitude aparente é igual a 4.84. Considerando sua distância de 340 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.25. Pertence à classe espectral G8II/III. (pt)
  • 60 Sagittarii, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna, belägen i den västra delen av stjärnbilden Skytten och har även Bayer-beteckningen A Sagittarii. Den har en skenbar magnitud på 4,84 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 8,6 mas, beräknas den befinna sig på ett avstånd på ca 379 ljusår (ca 116 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -51 km/s. Den bildar det nordvästra hörnet av asterismen som kallas . (sv)
  • 人马座60 （60 Sagittarii），又称为人马座A，中文名狗国二，是一颗位于人马座的G-型巨星，距离地球约340光年。 它位于星群（中国古代星官称为狗国）的西北边，视星等为4.851，是飞弹螺星群最暗的一颗恒星。 (zh)
dbo:thumbnail
dbo:wikiPageID
  • 2651781 (xsd:integer)
dbo:wikiPageLength
  • 7594 (xsd:nonNegativeInteger)
dbo:wikiPageRevisionID
  • 1117759973 (xsd:integer)
dbo:wikiPageWikiLink
dbp:absmagV
  • −0.07 (en)
dbp:appmagV
  • 4.840000 (xsd:double)
dbp:caption
  • The four stars of the Terebellum (en)
dbp:class
  • G6 III (en)
dbp:constell
dbp:epoch
dbp:equinox
  • J2000.0 (en)
dbp:gravity
  • 2.780000 (xsd:double)
dbp:metalFe
  • −0.38 (en)
dbp:pError
  • 0.173200 (xsd:double)
dbp:parallax
  • 8.602500 (xsd:double)
dbp:propMoDec
  • +25.69 (en)
dbp:propMoRa
  • +35.31 (en)
dbp:rI
  • +0.47 (en)
dbp:type
  • horizontal branch (en)
dbp:uB
  • +0.55 (en)
dbp:wikiPageUsesTemplate
dcterms:subject
gold:hypernym
rdf:type
rdfs:comment
  • 60 Sagittarii (A Sagittarii) é uma estrela na direção da Sagittarius. Possui uma ascensão reta de 19h 58m 57.18s e uma declinação de −26° 11′ 45.0″. Sua magnitude aparente é igual a 4.84. Considerando sua distância de 340 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.25. Pertence à classe espectral G8II/III. (pt)
  • 60 Sagittarii, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna, belägen i den västra delen av stjärnbilden Skytten och har även Bayer-beteckningen A Sagittarii. Den har en skenbar magnitud på 4,84 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 8,6 mas, beräknas den befinna sig på ett avstånd på ca 379 ljusår (ca 116 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -51 km/s. Den bildar det nordvästra hörnet av asterismen som kallas . (sv)
  • 人马座60 （60 Sagittarii），又称为人马座A，中文名狗国二，是一颗位于人马座的G-型巨星，距离地球约340光年。 它位于星群（中国古代星官称为狗国）的西北边，视星等为4.851，是飞弹螺星群最暗的一颗恒星。 (zh)
  • 60 Sagittarii is a suspected binary star system in the southern constellation of Sagittarius. It has the Bayer designation A Sagittarii, while 60 Sagittarii is the Flamsteed designation. This naked-eye object forms the northwest corner of the asterism called the Terebellum and, with an apparent magnitude of approximately 4.84, it is the dimmest of the four stars in the Terebellum. It is located 379 light-years from the Sun, based on parallax, but is moving closer with a radial velocity of −51 km/s. (en)
rdfs:label
  • 60 Sagittarii (en)
  • 60 Sagittarii (pt)
  • 60 Sagittarii (sv)
  • 狗国二 (zh)
owl:sameAs
prov:wasDerivedFrom
foaf:depiction
foaf:isPrimaryTopicOf
is dbo:wikiPageRedirects of
is dbo:wikiPageWikiLink of
is foaf:primaryTopic of
Powered by OpenLink Virtuoso    This material is Open Knowledge     W3C Semantic Web Technology     This material is Open Knowledge    Valid XHTML + RDFa
This content was extracted from Wikipedia and is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License