About: 13 Ceti

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13 Ceti is a triple star system in the equatorial constellation of Cetus. It is dimly visible to the naked eye with a combined apparent visual magnitude of 5.20. The system is located at a distance of approximately 69 light years from the Sun based on stellar parallax, and is drifting further away with a radial velocity of +10.4 km/s. It shares a common motion with the Hyades moving group, although it is too old to be a member.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body star
rdfs:label	13 Ceti (en) 13 Ceti (es) 13 Ceti (it) Gliese 23 (nl) 13 Ceti (sv) 13 Кита (ru) 天溷增二 (zh)
rdfs:comment	13 Ceti è una stella bianco-gialla nella sequenza principale di magnitudine 5,2 situata nella costellazione della Balena. Dista 69 anni luce dal sistema solare. (it) Gliese 23 is een dubbelster van het F7V en G4V, gelegen in het sterrenbeeld Walvis op 69,32 lichtjaar van de Zon. De ster heeft een relatieve snelheid ten opzichte van de zon van 43,2 km/s. (nl) 13 Ceti, eller BU Ceti, är en trippelstjärna och eruptiv variabel av RS Canum Venaticorum-typ (RS) i stjärnbilden Valfisken. 13 Ceti varierar mellan visuell magnitud +3,86 och 3,96 utan någon fastställd periodicitet. Den befinner sig på ett avstånd av ungefär 70 ljusår. (sv) 鯨魚座13，又名BD-04 62，HD 3196、SAO 128839、HR 142，是鯨魚座的一颗恒星，视星等为5.2，位于銀經112.89，銀緯-66.15，其B1900.0坐标为赤經0h 30m 6s，赤緯-4° -66.15′ 36″。 (zh) 13 Ceti is a triple star system in the equatorial constellation of Cetus. It is dimly visible to the naked eye with a combined apparent visual magnitude of 5.20. The system is located at a distance of approximately 69 light years from the Sun based on stellar parallax, and is drifting further away with a radial velocity of +10.4 km/s. It shares a common motion with the Hyades moving group, although it is too old to be a member. (en) 13 Ceti (13 Cet / HD 3196 / GJ 23) es un sistema estelar localizado en la constelación de Cetus. Situado a una distancia de 69 años luz del Sistema Solar, tiene magnitud aparente +5,20. La componente principal del sistema, 13 Ceti A, es una enana blanco-amarilla de tipo espectral F8V —semejante, por ejemplo, a γ Pavonis o a 111 Tauri— con una masa un 18% mayor que la masa solar.La componente secundaria, 13 Ceti B, es un análogo solar de tipo G0V o G2V cuya masa es comparable a la solar.El semieje mayor de la órbita entre las dos componentes es de 0,23 segundos de arco, equivalente a una separación proyectada de 4,9 UA. Emplean 6,92 años en completar una vuelta alrededor del centro de masas común. (es) 13 Кита (13 Ceti, сокращ. 13 Cet) — кратная звезда в экваториальном созвездии Кита. Звезда имеет видимую звёздную величину +5,2m, и, согласно шкале Бортля, звезда видна невооружённым глазом на засвеченном пригородном небе (англ. Bright suburban sky). Из измерений параллакса, полученных во время миссии Hipparcos известно, что звёзды удалены примерно на 69,3 св. лет (21,6 пк) от Солнца. Звезды наблюдается южнее , то есть видна практически на всей территории обитаемой Земли, за исключением полярных областей Антарктиды. Лучшее время для наблюдения — сентябрь. (ru)
name	B (en) Ab (en)
dcterms:subject	Bright Star Catalogue objects Cetus (constellation) Durchmusterung objects F-type main-sequence stars Flamsteed objects G-type main-sequence stars Gliese and GJ objects Henry Draper Catalogue objects Hipparcos objects K-type main-sequence stars Objects with variable star designations RS Canum Venaticorum variables Spectroscopic binaries Triple stars
Wikipage page ID	65820116 (xsd:integer)
Wikipage revision ID	1080006099 (xsd:integer)
Link from a Wikipage to another Wikipage	Stellar classification Bright Star Catalogue objects Cetus (constellation) Durchmusterung objects F-type main-sequence stars Flamsteed objects G-type main-sequence stars Gliese and GJ objects Henry Draper Catalogue objects Hipparcos objects K-type main-sequence stars Objects with variable star designations RS Canum Venaticorum variables Spectroscopic binaries Triple stars Constellation RS Canum Venaticorum variable Edwin Brant Frost George W. Hough Light year Main sequence Orbital period Stellar parallax Cetus G-type main-sequence star K-type main-sequence star EXOSAT Celestial equator Angular separation Hyades Stream Sun CHARA array Position angle Spectroscopic binary Apparent visual magnitude Orbital eccentricity Radial velocity Sherburne Wesley Burnham F-type main-sequence star X-ray astronomy Variable star designation Magnetic activity Triple star system
sameAs	13 Ceti 13 Ceti 13 Ceti 13 Ceti 13 Ceti 13 Ceti 13 Ceti 13 Ceti 13 Ceti
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