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Statements

Subject Item
dbr:HD_92788
rdf:type
dbo:CelestialBody yago:Object100002684 yago:Whole100003553 yago:WikicatHenryDraperCatalogueObjects yago:CelestialBody109239740 yago:WikicatSolar-typeStars yago:Star109444100 owl:Thing dbo:Place yago:PhysicalEntity100001930 yago:WikicatG-typeMain-sequenceStars dbo:Star yago:WikicatG-typeStars dbo:Location yago:NaturalObject100019128 yago:WikicatHipparcosObjects schema:Place
rdfs:label
HD 92788 HD 92788 HD 92788 HD 92788 HD 92788 HD 92788
rdfs:comment
HD 92788 is a star in the equatorial constellation of Sextans. It has a yellow hue but is too dim to be visible to the naked eye, having an apparent visual magnitude of 7.31. The star is located at a distance of 113 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −4.5 km/s. Two planets have been found in orbit around the star. HD 92788是一顆距離地球約107光年的黃矮星，位於六分儀座。該恆星質量和金屬量較太陽高，但體積稍低於太陽。 HD 92788 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Sextanten. Den har en skenbar magnitud av ca 7,31 och kräver åtminstone en handkikare eller ett mindre teleskop för att kunna observeras. Baserat på parallaxmätning inom Hipparcosuppdraget enligt Gaia Data Release 2 på ca 28,8 mas, beräknas den befinna sig på ett avstånd på ca 113 ljusår (ca 35 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -4,5 km/s. HD 92788 è una stella nella costellazione del Sestante, distante 107 anni luce dal sistema solare. Nel 2001 è stato scoperto un esopianeta che orbita attorno a questa stella, HD 92788 b. HD 92788 ist ein 107,06 Lichtjahre von der Erde entfernter Gelber Zwerg mit einer Rektaszension von 10h 42m 48s und einer Deklination von -02° 11' 01". Er besitzt eine scheinbare Helligkeit von 7,31 mag. Im Jahre 2000 entdeckte Debra Fischer einen extrasolaren Planeten, der diesen Stern umkreist. Dieser trägt den Namen HD 92788 b. HD 92788は、ろくぶんぎ座の方角に約113光年の距離にあるG型主系列星である。太陽より質量、半径は若干大きい。金属量は太陽よりも多い。
dcterms:subject
dbc:Henry_Draper_Catalogue_objects dbc:Durchmusterung_objects dbc:Hipparcos_objects dbc:Sextans_(constellation) dbc:G-type_main-sequence_stars dbc:2MASS_objects dbc:Planetary_systems_with_two_confirmed_planets
dbo:wikiPageID
14445033
dbo:wikiPageRevisionID
1121782716
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dbo:wikiPageExternalLink
n13:star.php%3Fst=HD+92788
owl:sameAs
dbpedia-he:HD_92788 wikidata:Q81193 dbpedia-fa:اچ‌دی_۹۲۷۸۸ dbpedia-de:HD_92788 n18:4yM26 dbpedia-it:HD_92788 dbpedia-sv:HD_92788 dbpedia-ja:HD_92788 yago-res:HD_92788 dbpedia-sk:HD_92788 freebase:m.03d3rg7 dbpedia-zh:HD_92788
dbp:wikiPageUsesTemplate
dbt:± dbt:Stars_of_Sextans dbt:RA dbt:OrbitboxPlanet dbt:Starbox_begin dbt:Starbox_catalog dbt:Orbitbox_end dbt:Starbox_astrometry dbt:Starbox_detail dbt:Starbox_end dbt:OrbitboxPlanet_begin dbt:Starbox_character dbt:DEC dbt:Starbox_observe dbt:Cite_encyclopedia dbt:Val dbt:Odlist dbt:Convert dbt:Reflist dbt:Sky dbt:Short_description dbt:Starbox_reference
dbp:absmagV
4.56
dbp:appmagV
7.31
dbp:class
G6V
dbp:constell
dbr:Sextans
dbp:epoch
J2000
dbp:exoplanet
dbr:HD_92788_b dbr:HD_92788_c
dbp:gravity
4.39
dbp:mass
1.032
dbp:nsted
HD+92788
dbp:pError
0.0493
dbp:parallax
28.8281
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2738880.0
dbp:simbad
HD+92788
dbo:abstract
HD 92788は、ろくぶんぎ座の方角に約113光年の距離にあるG型主系列星である。太陽より質量、半径は若干大きい。金属量は太陽よりも多い。 HD 92788 is a star in the equatorial constellation of Sextans. It has a yellow hue but is too dim to be visible to the naked eye, having an apparent visual magnitude of 7.31. The star is located at a distance of 113 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −4.5 km/s. Two planets have been found in orbit around the star. This is a G-type main-sequence star with a stellar classification of G6V. It is estimated to be around eight billion years old and is spinning with a rotation period of 31.7 days. The star has a similar mass to the Sun and is slightly larger in radius, with a high metallicity. It is radiating 1.25 times the luminosity of the Sun from its photosphere at an effective temperature of 5,722 K. HD 92788 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Sextanten. Den har en skenbar magnitud av ca 7,31 och kräver åtminstone en handkikare eller ett mindre teleskop för att kunna observeras. Baserat på parallaxmätning inom Hipparcosuppdraget enligt Gaia Data Release 2 på ca 28,8 mas, beräknas den befinna sig på ett avstånd på ca 113 ljusår (ca 35 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -4,5 km/s. HD 92788 è una stella nella costellazione del Sestante, distante 107 anni luce dal sistema solare. Nel 2001 è stato scoperto un esopianeta che orbita attorno a questa stella, HD 92788 b. HD 92788 ist ein 107,06 Lichtjahre von der Erde entfernter Gelber Zwerg mit einer Rektaszension von 10h 42m 48s und einer Deklination von -02° 11' 01". Er besitzt eine scheinbare Helligkeit von 7,31 mag. Im Jahre 2000 entdeckte Debra Fischer einen extrasolaren Planeten, der diesen Stern umkreist. Dieser trägt den Namen HD 92788 b. HD 92788是一顆距離地球約107光年的黃矮星，位於六分儀座。該恆星質量和金屬量較太陽高，但體積稍低於太陽。
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dbr:Star
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10343
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