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Statements

Subject Item
dbr:Zeta_Scuti
rdf:type
yago:LivingThing100004258 schema:Place dbo:CelestialBody yago:GiantStar109288769 yago:Organism100004475 dbo:Place yago:Object100002684 dbo:Location yago:Animal100015388 yago:CelestialBody109239740 yago:WikicatGiantStars yago:Whole100003553 yago:WikicatK-typeGiants yago:PhysicalEntity100001930 dbo:Star owl:Thing yago:NaturalObject100019128 yago:Star109444100 yago:WikicatBayerObjects yago:Giant101323781
rdfs:label
Zeta Scuti Дзета Щита Zeta Scuti Zeta Scuti Zeta Scuti
rdfs:comment
Zeta Scuti (ζ Scuti, förkortad Zeta Sct, ζ Sct), som är stjärnans Bayer-beteckning, är en dubbelstjärna i västra delen av stjärnbilden Skölden. Den har en skenbar magnitud av 4,66 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 15,8 mas, beräknas den befinna sig på ett avstånd av ca 210 ljusår (63 parsek) från solen. Den rör sig närmare solen med en radiell hastighet på -5 km/s. ζ Щита (лат. ζ Scuti / ζ Sct) — спектрально-двойная звезда в созвездии Щита на расстоянии приблизительно 191 светового года от нас. Главный компонент, ζ Щита А, — холодный жёлтый гигант спектрального класса G. Zeta Scuti (ζ Sct) – trzecia co do jasności gwiazda w gwiazdozbiorze Tarczy. Oddalona jest o około 207 lat świetlnych od Słońca. Zeta Scuti jest pomarańczowym olbrzymem należącym do typu widmowego K o jasności obserwowanej równej 4,66m oraz układem podwójnym o okresie 6,5 roku. Zeta Scuti (3 Scuti) é uma estrela na direção da constelação de Scutum. Possui uma ascensão reta de 18h 23m 39.55s e uma declinação de −08° 56′ 04.2″. Sua magnitude aparente é igual a 4.66. Considerando sua distância de 191 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.82. Pertence à classe espectral K0III. Zeta Scuti, Latinized from ζ Scuti, is the Bayer designation for a star in the southern constellation of Scutum. It is a faint star but visible to the naked eye with an apparent magnitude of 4.66. The distance to this star, as determined via parallax measurement, is around 210 light years. It is moving closer to the Sun with a radial velocity of −5 km/s.
foaf:name
ζ Scuti
dbp:name
ζ Scuti B
foaf:depiction
n16:Scutum_constellation_map.svg n16:Red_circle.svg
dct:subject
dbc:Henry_Draper_Catalogue_objects dbc:TIC_objects dbc:G-type_giants dbc:Scutum_(constellation) dbc:Hipparcos_objects dbc:Bayer_objects dbc:Durchmusterung_objects dbc:Bright_Star_Catalogue_objects dbc:Astrometric_binaries
dbo:wikiPageID
2673970
dbo:wikiPageRevisionID
1079519742
dbo:wikiPageWikiLink
dbr:Sun's_luminosity dbr:Sun's_radius dbr:Stellar_parallax dbr:Photosphere dbr:G-type_star dbr:Radial_velocity dbc:TIC_objects dbc:Henry_Draper_Catalogue_objects dbr:Bayer_designation dbc:Scutum_(constellation) dbr:Effective_temperature dbr:Orbital_eccentricity dbc:G-type_giants dbr:Scutum_(constellation) dbc:Hipparcos_objects dbr:Stellar_classification dbc:Bayer_objects dbr:Mass_of_the_Sun dbr:Giant_star dbc:Durchmusterung_objects dbr:Latinisation_of_names dbr:Light_year dbr:Apparent_magnitude dbr:Astrometric_binary dbr:Constellation dbc:Astrometric_binaries dbr:Stellar_spectrum dbc:Bright_Star_Catalogue_objects dbr:Star
owl:sameAs
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dbp:wikiPageUsesTemplate
dbt:Odlist dbt:DEC dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_astrometry dbt:Starbox_orbit dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_character dbt:Stars_of_Scutum dbt:RA dbt:Location_mark dbt:Starbox_reference dbt:Reflist dbt:Short_description
dbo:thumbnail
n16:Scutum_constellation_map.svg?width=300
dbp:axisUnitless
21.6
dbp:absmagV
0.66
dbp:appmagV
4.66
dbp:bV
+0.94
dbp:class
G9 IIIb Fe-0.5
dbp:constell
dbr:Scutum_(constellation)
dbp:eccentricity
0.1
dbp:epoch
J2000
dbp:gravity
2.61
dbp:inclination
89
dbp:luminosity
62.04
dbp:mass
1.29
dbp:metalFe
−0.08
dbp:node
226
dbp:pError
1.02
dbp:parallax
15.78
dbp:periarg
242.1
dbp:periastron
2418278.3
dbp:periodUnitless
2.0508768E8
dbp:primary
ζ Scuti A
dbp:propMoDec
+51.24
dbp:propMoRa
+49.59
dbp:radialV
−5.02
dbp:radius
9.300000000000001
dbp:rotationalVelocity
1.5
dbp:temperature
4750
dbp:uB
+0.72
dbo:abstract
Zeta Scuti, Latinized from ζ Scuti, is the Bayer designation for a star in the southern constellation of Scutum. It is a faint star but visible to the naked eye with an apparent magnitude of 4.66. The distance to this star, as determined via parallax measurement, is around 210 light years. It is moving closer to the Sun with a radial velocity of −5 km/s. This is an astrometric binary system with a period of 6.5 years (2,374 days) and an orbital eccentricity of 0.10. The visible component is an aging giant star of type G with a stellar classification of G9 IIIb Fe−0.5. The suffix notation indicates the spectrum displays a mild underabundance of iron. It has 1.29 times the mass of the Sun and has expanded to 9.3 times the Sun's radius. The star is radiating 62 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,750 K. ζ Щита (лат. ζ Scuti / ζ Sct) — спектрально-двойная звезда в созвездии Щита на расстоянии приблизительно 191 светового года от нас. Главный компонент, ζ Щита А, — холодный жёлтый гигант спектрального класса G. Zeta Scuti (3 Scuti) é uma estrela na direção da constelação de Scutum. Possui uma ascensão reta de 18h 23m 39.55s e uma declinação de −08° 56′ 04.2″. Sua magnitude aparente é igual a 4.66. Considerando sua distância de 191 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.82. Pertence à classe espectral K0III. Zeta Scuti (ζ Sct) – trzecia co do jasności gwiazda w gwiazdozbiorze Tarczy. Oddalona jest o około 207 lat świetlnych od Słońca. Zeta Scuti jest pomarańczowym olbrzymem należącym do typu widmowego K o jasności obserwowanej równej 4,66m oraz układem podwójnym o okresie 6,5 roku. Zeta Scuti (ζ Scuti, förkortad Zeta Sct, ζ Sct), som är stjärnans Bayer-beteckning, är en dubbelstjärna i västra delen av stjärnbilden Skölden. Den har en skenbar magnitud av 4,66 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 15,8 mas, beräknas den befinna sig på ett avstånd av ca 210 ljusår (63 parsek) från solen. Den rör sig närmare solen med en radiell hastighet på -5 km/s.
gold:hypernym
dbr:Designation
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7114
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