About: HD 24160

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

HD 24160 is a single star in the equatorial constellation of Eridanus. It is visible to the naked eye with an apparent visual magnitude of 4.17. The distance to HD 24160 can be estimated from its annual parallax shift of 15.0 mas, yielding a separation of 217 light years. It is moving further from the Earth with a heliocentric radial velocity of +2 km/s. This object is a coronal member of the Ursa Major Moving Group of stars that share a common motion through space.

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  • HD 24160 is a single star in the equatorial constellation of Eridanus. It is visible to the naked eye with an apparent visual magnitude of 4.17. The distance to HD 24160 can be estimated from its annual parallax shift of 15.0 mas, yielding a separation of 217 light years. It is moving further from the Earth with a heliocentric radial velocity of +2 km/s. This object is a coronal member of the Ursa Major Moving Group of stars that share a common motion through space. At the age of 1.76 billion years old, HD 24160 is an evolved G-type giant star with a stellar classification of G7 III, having consumed the hydrogen at its core and tracked away from the main sequence. It has 2.33 times the mass of the Sun and has expanded to about 11 times the Sun's radius. The star is radiating 81.3 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,948 K. (en)
  • HD 24160 är en ensam stjärna i den mellersta delen av stjärnbilden Eridanus som också har Bayer-beteckningen g Eridani. Den har en skenbar magnitud av ca 4,17 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 15,0 mas, beräknas den befinna sig på ett avstånd på ca 217 ljusår (ca 67 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 2 km/s. Stjärnan ingår i Ursa Major rörelsegrupp av stjärnor med gemensam rörelse genom rymden. (sv)
  • HD 24160 (g Eridanus) é uma estrela na direção da Eridanus. Possui uma ascensão reta de 03h 49m 27.28s e uma declinação de −36° 12′ 00.4″. Sua magnitude aparente é igual a 4.17. Considerando sua distância de 210 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.13. Pertence à classe espectral G8III. (pt)
  • HD 24160，又名CD-36 1467，SAO 194559、HR 1195，是一颗恒星，视星等为4.17，位于銀經237.88，銀緯-51.4，其B1900.0坐标为赤經3h 45m 42.7s，赤緯-36° -51.4′ 11″。 (zh)
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dbp:absmagV
  • 0.130000 (xsd:double)
dbp:ageGyr
  • 1.760000 (xsd:double)
dbp:appmagV
  • 4.170000 (xsd:double)
dbp:class
  • G7 III (en)
dbp:constell
dbp:epoch
  • J2000 (en)
dbp:luminosity
  • 81.300000 (xsd:double)
dbp:mass
  • 2.330000 (xsd:double)
dbp:pError
  • 0.221100 (xsd:double)
dbp:parallax
  • 15.038900 (xsd:double)
dbp:propMoDec
  • −50.421 (en)
dbp:propMoRa
  • −44.841 (en)
dbp:radius
  • 11 (xsd:integer)
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  • HD 24160 är en ensam stjärna i den mellersta delen av stjärnbilden Eridanus som också har Bayer-beteckningen g Eridani. Den har en skenbar magnitud av ca 4,17 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 15,0 mas, beräknas den befinna sig på ett avstånd på ca 217 ljusår (ca 67 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 2 km/s. Stjärnan ingår i Ursa Major rörelsegrupp av stjärnor med gemensam rörelse genom rymden. (sv)
  • HD 24160 (g Eridanus) é uma estrela na direção da Eridanus. Possui uma ascensão reta de 03h 49m 27.28s e uma declinação de −36° 12′ 00.4″. Sua magnitude aparente é igual a 4.17. Considerando sua distância de 210 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.13. Pertence à classe espectral G8III. (pt)
  • HD 24160，又名CD-36 1467，SAO 194559、HR 1195，是一颗恒星，视星等为4.17，位于銀經237.88，銀緯-51.4，其B1900.0坐标为赤經3h 45m 42.7s，赤緯-36° -51.4′ 11″。 (zh)
  • HD 24160 is a single star in the equatorial constellation of Eridanus. It is visible to the naked eye with an apparent visual magnitude of 4.17. The distance to HD 24160 can be estimated from its annual parallax shift of 15.0 mas, yielding a separation of 217 light years. It is moving further from the Earth with a heliocentric radial velocity of +2 km/s. This object is a coronal member of the Ursa Major Moving Group of stars that share a common motion through space. (en)
rdfs:label
  • HD 24160 (en)
  • HD 24160 (pt)
  • HD 24160 (sv)
  • HD 24160 (zh)
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  • HD 24160 (en)
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