About: WASP-59

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

WASP-59 is a K-type main-sequence star about 379 light-years away. The star's age is essentially unconstrained by observations. WASP-59 is slightly depleted in heavy elements, having 70% of the solar abundance of iron. The star produces extremely low levels of ultraviolet light, indicating an absence of flare activity. A multiplicity survey in 2015 did not detect any stellar companions to WASP-59.

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dbo:abstract
  • WASP-59 is a K-type main-sequence star about 379 light-years away. The star's age is essentially unconstrained by observations. WASP-59 is slightly depleted in heavy elements, having 70% of the solar abundance of iron. The star produces extremely low levels of ultraviolet light, indicating an absence of flare activity. A multiplicity survey in 2015 did not detect any stellar companions to WASP-59. (en)
  • WASP-59 — звезда, которая находится в созвездии Пегас на расстоянии приблизительно 407 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
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  • WASP-59 (en)
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  • WASP-59 is a K-type main-sequence star about 379 light-years away. The star's age is essentially unconstrained by observations. WASP-59 is slightly depleted in heavy elements, having 70% of the solar abundance of iron. The star produces extremely low levels of ultraviolet light, indicating an absence of flare activity. A multiplicity survey in 2015 did not detect any stellar companions to WASP-59. (en)
  • WASP-59 — звезда, которая находится в созвездии Пегас на расстоянии приблизительно 407 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
rdfs:label
  • WASP-59 (en)
  • WASP-59 (ru)
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  • WASP-59 (en)
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