Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q2088855> ?p ?o }
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- Q2088855 subject Q7009834.
- Q2088855 subject Q7217188.
- Q2088855 subject Q7238065.
- Q2088855 subject Q7465898.
- Q2088855 subject Q7465903.
- Q2088855 abstract "HD 154672 is a yellow subgiant (spectral type G3 IV). It is about 65 parsecs away from the Sun that is larger than, but of a similar mass to, the Sun. However, HD 154672 is much older. The star is very metal-rich, which is one of the reasons why it was targeted for a planet search by the N2K Consortium, which discovered the gas giant planet HD 154672 b using Doppler Spectroscopy; the discovery was reported in October 2008. The N2K collaboration chose HD 154672 primarily because it aimed to discover the correlation between a star's metallicity and the mass of orbiting planets.HD 154672 was targeted by the Magellan Telescopes. It is the host of the first planet discovered from the telescopes by N2K.".
- Q2088855 thumbnail Magellan_Campanas.jpg?width=300.
- Q2088855 wikiPageExternalLink sim-id.pl?protocol=html&Ident=HD+154672&NbIdent=1&Radius=10&Radius.unit=arcmin&CooFrame=FK5&CooEpoch=2000&CooEqui=2000&output.max=all&o.catall=on&output.mesdisp=N&Bibyear1=1983&Bibyear2=2006&Frame1=FK5&Frame2=FK4&Frame3=G&Equi1=2000.0&Equi2=1950.0&Equi3=2000.0&Epoch1=2000.0&Epoch2=1950.0&Epoch3=2000.0.
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- Q2088855 wikiPageWikiLink Q525.
- Q2088855 wikiPageWikiLink Q531.
- Q2088855 wikiPageWikiLink Q555846.
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- Q2088855 wikiPageWikiLink Q661954.
- Q2088855 wikiPageWikiLink Q669166.
- Q2088855 wikiPageWikiLink Q7009834.
- Q2088855 wikiPageWikiLink Q7217188.
- Q2088855 wikiPageWikiLink Q7238065.
- Q2088855 wikiPageWikiLink Q7465898.
- Q2088855 wikiPageWikiLink Q7465903.
- Q2088855 wikiPageWikiLink Q854050.
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- Q2088855 type Place.
- Q2088855 type CelestialBody.
- Q2088855 type Location.
- Q2088855 type Place.
- Q2088855 type Star.
- Q2088855 type Thing.
- Q2088855 comment "HD 154672 is a yellow subgiant (spectral type G3 IV). It is about 65 parsecs away from the Sun that is larger than, but of a similar mass to, the Sun. However, HD 154672 is much older. The star is very metal-rich, which is one of the reasons why it was targeted for a planet search by the N2K Consortium, which discovered the gas giant planet HD 154672 b using Doppler Spectroscopy; the discovery was reported in October 2008.".
- Q2088855 label "HD 154672".
- Q2088855 depiction Magellan_Campanas.jpg.
- Q2088855 name "HD154672".