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About: DP Leonis

An Entity of Type: star, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org

DP Leonis (abbreviated DP Leo) is binary star system in the equatorial constellation of Leo. It is a variable star that ranges in apparent visual magnitude from 17.5 down to 19. The system is located at a distance of approximately 990 light-years from the Sun based on parallax. It is a cataclysmic variable star of the AM Herculis-type also known as polars. The system comprises an eclipsing white dwarf and red dwarf in tight orbit (nearly 1.5 hours) and an extrasolar planet. This eclipsing variable was discovered by and associates in 1982 as the optical counterpart to the EINSTEIN X-ray source E1114+182.

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dbo:abstract
  • DP del Lleó (DP Leonis) és un sistema binari eclipsant a aproximadament 1304 anys llum del Sol, probablement una estrella variable cataclísmica del tipus AM Herculis també coneguda com a polar. El sistema comprèn una nana blanca eclipsant i una nana vermella en òrbita estreta (gairebé 1,5 hores) i un planeta extrasolar. (ca)
  • DP Leonis (abbreviated DP Leo) is binary star system in the equatorial constellation of Leo. It is a variable star that ranges in apparent visual magnitude from 17.5 down to 19. The system is located at a distance of approximately 990 light-years from the Sun based on parallax. It is a cataclysmic variable star of the AM Herculis-type also known as polars. The system comprises an eclipsing white dwarf and red dwarf in tight orbit (nearly 1.5 hours) and an extrasolar planet. This eclipsing variable was discovered by and associates in 1982 as the optical counterpart to the EINSTEIN X-ray source E1114+182. (en)
  • DP Leonis (abbreviata DP Leo) è un sistema stellare binaria ad eclisse posto a circa 1304 anni-luce dal sistema Solare. Questo è un sistema a variabile cataclismica e più specificatamente del tipo AM Herculis, a partire dal nome della stella prototipo) comprendente una classe di stelle variabili intrinseche, consistenti di una stella binaria in cui una componente è una nana bianca, mentre l'altra è una stella normale che cede gas alla compagna. Il sistema DP Leonis comprende una stella nana bianca e una nana rossa in orbita stretta (circa 1,5 ore). (it)
  • しし座DP星(DP Leonis)は、太陽から約1304光年離れた位置にある食連星であり、恐らくポーラーとも呼ばれるヘルクレス座AM星型の激変星である。この系は、白色矮星と赤色矮星が軌道周期約1.5時間の非常に近い軌道を公転しており、さらに太陽系外惑星を持っている。 (ja)
  • DP Льва — затменная тесная двойная звёздная система, расположенная в созвездии Льва. Находится на расстоянии около 1304 световых лет (400 парсек) от Солнца. Вокруг этой двойной системы обращается, как минимум, одна экзопланета. (ru)
  • 獅子座DP(DP Leonis,DP Leo)是一個距離太陽約1304光年的食聯星,它可能是屬於武仙座AM型的激變變星,或稱為高偏振星。這個系統由相距甚近的一顆白矮星和一顆紅矮星(兩者互繞周期約1.5小時),以及一顆系外行星組成。 (zh)
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  • 25466851 (xsd:integer)
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  • 7412 (xsd:nonNegativeInteger)
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  • 1066500134 (xsd:integer)
dbo:wikiPageWikiLink
dbp:appmagV
  • 17.500000 (xsd:double)
dbp:colwidth
  • 30 (xsd:integer)
dbp:component
  • White dwarf (en)
  • Donor star (en)
dbp:constell
dbp:eccentricity
  • 0 (xsd:integer)
  • 0.390000 (xsd:double)
dbp:epe
  • DP+Leo (en)
dbp:epoch
dbp:exoplanet
dbp:inclination
  • 79.500000 (xsd:double)
dbp:mass
  • 0.090000 (xsd:double)
  • 0.600000 (xsd:double)
  • ≥6.1 ± 0.5 (en)
dbp:nsted
  • DP+Leo (en)
dbp:pError
  • 0.311000 (xsd:double)
dbp:parallax
  • 3.278100 (xsd:double)
dbp:period
  • 0.062363 (xsd:double)
  • 28 (xsd:integer)
dbp:periodUnit
  • year (en)
dbp:propMoDec
  • −1.444 (en)
dbp:propMoRa
  • −28.700 (en)
dbp:radialV
  • 0 (xsd:integer)
dbp:semimajor
  • 8.200000 (xsd:double)
dbp:simbad
  • DP+Leo (en)
dbp:temperature
  • 13500 (xsd:integer)
dbp:variable
dbp:wikiPageUsesTemplate
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gold:hypernym
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rdfs:comment
  • DP del Lleó (DP Leonis) és un sistema binari eclipsant a aproximadament 1304 anys llum del Sol, probablement una estrella variable cataclísmica del tipus AM Herculis també coneguda com a polar. El sistema comprèn una nana blanca eclipsant i una nana vermella en òrbita estreta (gairebé 1,5 hores) i un planeta extrasolar. (ca)
  • DP Leonis (abbreviated DP Leo) is binary star system in the equatorial constellation of Leo. It is a variable star that ranges in apparent visual magnitude from 17.5 down to 19. The system is located at a distance of approximately 990 light-years from the Sun based on parallax. It is a cataclysmic variable star of the AM Herculis-type also known as polars. The system comprises an eclipsing white dwarf and red dwarf in tight orbit (nearly 1.5 hours) and an extrasolar planet. This eclipsing variable was discovered by and associates in 1982 as the optical counterpart to the EINSTEIN X-ray source E1114+182. (en)
  • DP Leonis (abbreviata DP Leo) è un sistema stellare binaria ad eclisse posto a circa 1304 anni-luce dal sistema Solare. Questo è un sistema a variabile cataclismica e più specificatamente del tipo AM Herculis, a partire dal nome della stella prototipo) comprendente una classe di stelle variabili intrinseche, consistenti di una stella binaria in cui una componente è una nana bianca, mentre l'altra è una stella normale che cede gas alla compagna. Il sistema DP Leonis comprende una stella nana bianca e una nana rossa in orbita stretta (circa 1,5 ore). (it)
  • しし座DP星(DP Leonis)は、太陽から約1304光年離れた位置にある食連星であり、恐らくポーラーとも呼ばれるヘルクレス座AM星型の激変星である。この系は、白色矮星と赤色矮星が軌道周期約1.5時間の非常に近い軌道を公転しており、さらに太陽系外惑星を持っている。 (ja)
  • DP Льва — затменная тесная двойная звёздная система, расположенная в созвездии Льва. Находится на расстоянии около 1304 световых лет (400 парсек) от Солнца. Вокруг этой двойной системы обращается, как минимум, одна экзопланета. (ru)
  • 獅子座DP(DP Leonis,DP Leo)是一個距離太陽約1304光年的食聯星,它可能是屬於武仙座AM型的激變變星,或稱為高偏振星。這個系統由相距甚近的一顆白矮星和一顆紅矮星(兩者互繞周期約1.5小時),以及一顆系外行星組成。 (zh)
rdfs:label
  • DP del Lleó (ca)
  • DP Leonis (en)
  • DP Leonis (it)
  • しし座DP星 (ja)
  • DP Льва (ru)
  • 獅子座DP (zh)
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