About: HD 204313 b     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:Whole100003553, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FHD_204313_b&invfp=IFP_OFF&sas=SAME_AS_OFF&graph=http%3A%2F%2Fdbpedia.org&graph=http%3A%2F%2Fdbpedia.org

HD 204313 b is an extrasolar planet which orbits the G-type main sequence star HD 204313, located approximately 155 light years away in the constellation Capricorn. This planet orbits the star at a distance of 3.082 astronomical units and takes 1931 days or 5.29 years to revolve around the star. It has a minimum mass four times that of Jupiter. However the radius is not known since this planet was not detected by the transit method or direct imaging. Instead, this planet was detected by the radial velocity method using the CORALIE Echelle spectrograph mounted on the 1.2 meter located at La Silla Observatory in Atacama desert, Chile on August 11, 2009.

AttributesValues
rdf:type
rdfs:label
  • HD 204313 b (ar)
  • HD 204313 b (es)
  • HD 204313 b (en)
rdfs:comment
  • HD 204313 b (بالإنجليزية: HD 204313 b)‏ الذي يرمز له بالرمز HD 204313b، هو كوكب خارج المجموعة الشمسية، في كوكبة الجدي (كوكبة)، يتبع ‏. (ar)
  • HD 204313 b es un planeta extrasolar que orbita la estrella de tipo G HD 204313, localizado aproximadamente a 155 años luz, en la constelación de Capricornio. Este planeta tiene al menos 4 veces la masa de Júpiter y tarda 5,29 años en completar su periodo orbital, con un semieje mayor de 3,08 UA.​ Sin embargo, se desconoce su radio y su inclinación ya que no fue descubierto por el método de tránsito astronómico o . Este planeta fue detectado por el método de la velocidad radial usando el espectografo Echelle montado en el del observatorio de La Silla (Chile) el 11 de agosto de 2009. El astrónomo (2009) ha propuesto como el nombre común posible para HD 204313 b.​ (es)
  • HD 204313 b is an extrasolar planet which orbits the G-type main sequence star HD 204313, located approximately 155 light years away in the constellation Capricorn. This planet orbits the star at a distance of 3.082 astronomical units and takes 1931 days or 5.29 years to revolve around the star. It has a minimum mass four times that of Jupiter. However the radius is not known since this planet was not detected by the transit method or direct imaging. Instead, this planet was detected by the radial velocity method using the CORALIE Echelle spectrograph mounted on the 1.2 meter located at La Silla Observatory in Atacama desert, Chile on August 11, 2009. (en)
foaf:name
  • HD204313 b (en)
name
  • HD 204313 b (en)
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
sameAs
dbp:wikiPageUsesTemplate
apsis
  • astron (en)
discovered
discoverer
  • Segransan et al. (en)
discovery method
  • Radial velocity (en)
discovery site
star
has abstract
  • HD 204313 b (بالإنجليزية: HD 204313 b)‏ الذي يرمز له بالرمز HD 204313b، هو كوكب خارج المجموعة الشمسية، في كوكبة الجدي (كوكبة)، يتبع ‏. (ar)
  • HD 204313 b is an extrasolar planet which orbits the G-type main sequence star HD 204313, located approximately 155 light years away in the constellation Capricorn. This planet orbits the star at a distance of 3.082 astronomical units and takes 1931 days or 5.29 years to revolve around the star. It has a minimum mass four times that of Jupiter. However the radius is not known since this planet was not detected by the transit method or direct imaging. Instead, this planet was detected by the radial velocity method using the CORALIE Echelle spectrograph mounted on the 1.2 meter located at La Silla Observatory in Atacama desert, Chile on August 11, 2009. The planet's existence was independently confirmed in 2015, and in 2022 its inclination and true mass were measured via astrometry. (en)
  • HD 204313 b es un planeta extrasolar que orbita la estrella de tipo G HD 204313, localizado aproximadamente a 155 años luz, en la constelación de Capricornio. Este planeta tiene al menos 4 veces la masa de Júpiter y tarda 5,29 años en completar su periodo orbital, con un semieje mayor de 3,08 UA.​ Sin embargo, se desconoce su radio y su inclinación ya que no fue descubierto por el método de tránsito astronómico o . Este planeta fue detectado por el método de la velocidad radial usando el espectografo Echelle montado en el del observatorio de La Silla (Chile) el 11 de agosto de 2009. El astrónomo (2009) ha propuesto como el nombre común posible para HD 204313 b.​ (es)
gold:hypernym
prov:wasDerivedFrom
page length (characters) of wiki page
Method of discovery
  • Radial velocity(CORALIE)
discovery date
foaf:isPrimaryTopicOf
is Link from a Wikipage to another Wikipage of
is Wikipage redirect of
is exoplanet of
is foaf:primaryTopic of
Faceted Search & Find service v1.17_git139 as of Feb 29 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3330 as of Mar 19 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 59 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software