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WASP-66, also known as TYC 7193-1804-1, is an F-type star in the constellation Antlia. It has an apparent magnitude of 11.6, which is much too faint to be seen with the unaided eye and is located at a distance of 1,630 light years. According to a survey published in 2017, WASP-66 has one suspected companion - a red dwarf star with an effective temperature of 3,330±150 K and a projected separation of 6,800±700 AU.

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  • WASP-66 (fr)
  • WASP-66 (ru)
  • WASP-66 (en)
  • WASP-66 (zh)
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  • WASP-66 — звезда, которая находится в созвездии Насос на расстоянии приблизительно 1239 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
  • WASP-66，又名TYC 7193-1804-1，是一顆像太陽的恆星，其光譜型為F4，位於唧筒座。它的視星等為11.6，對肉眼來說太黯淡了，因此不能看見。它有一顆質量為木星2.3倍的行星，需要4天才能圍繞它一週，於2012年以凌日法發現。 (zh)
  • WASP-66, aussi connue sous la dénomination TYC 7193-1804-1, est une étoile de la constellation de la Machine pneumatique. Sa magnitude apparente est de 11,6, ce qui est bien trop faible pour être visible à l'œil nu. Elle est distante de 1 650±44 a.l. (∼506 pc) de la Terre et elle se rapproche de nous avec une vitesse radiale de −10,49 km/s. (fr)
  • WASP-66, also known as TYC 7193-1804-1, is an F-type star in the constellation Antlia. It has an apparent magnitude of 11.6, which is much too faint to be seen with the unaided eye and is located at a distance of 1,630 light years. According to a survey published in 2017, WASP-66 has one suspected companion - a red dwarf star with an effective temperature of 3,330±150 K and a projected separation of 6,800±700 AU. (en)
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  • WASP-66 (en)
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appmag v
constell
eccentricity
  • <0.046 (en)
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exoplanet
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  • −13.476 (en)
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  • WASP-66, aussi connue sous la dénomination TYC 7193-1804-1, est une étoile de la constellation de la Machine pneumatique. Sa magnitude apparente est de 11,6, ce qui est bien trop faible pour être visible à l'œil nu. Elle est distante de 1 650±44 a.l. (∼506 pc) de la Terre et elle se rapproche de nous avec une vitesse radiale de −10,49 km/s. Il s'agit d'une étoile type spectral F4. Elle est 1,30 fois plus massive que le Soleil et son rayon est 1,75 fois plus grand que celui du Soleil. Sa luminosité est un peu plus de 4 fois supérieure à celle du Soleil et sa température de surface est de 6 600 K. En 2012, une planète orbitant WASP-66 a été découverte. possède une masse d'environ 2,3 fois celle de Jupiter. Il lui faut 4 jours pour compléter son orbite autour de son étoile, faisant d'elle un Jupiter chaud. La planète a été découverte par la méthode des transits (lorsque la planète passe devant son étoile, elle bloque temporairement une partie de sa lumière). (fr)
  • WASP-66, also known as TYC 7193-1804-1, is an F-type star in the constellation Antlia. It has an apparent magnitude of 11.6, which is much too faint to be seen with the unaided eye and is located at a distance of 1,630 light years. WASP-66 has a classification of F4.5 V, which states that it is an ordinary F-type main sequence star that is fusing hydrogen at its core. At present it has 130% the mass of the Sun and 175 the radius of the Sun. It has an effective temperature of 6,600 K, which gives it a yellowish-white hue. The star is younger than Sun at 3.7+0.7−1.2 billion years, and may be either metal-poor or similar to Sun in concentration of heavy elements. Currently it is spinning moderately with a projected rotational velocity of 13.4 km/s. According to a survey published in 2017, WASP-66 has one suspected companion - a red dwarf star with an effective temperature of 3,330±150 K and a projected separation of 6,800±700 AU. (en)
  • WASP-66 — звезда, которая находится в созвездии Насос на расстоянии приблизительно 1239 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
  • WASP-66，又名TYC 7193-1804-1，是一顆像太陽的恆星，其光譜型為F4，位於唧筒座。它的視星等為11.6，對肉眼來說太黯淡了，因此不能看見。它有一顆質量為木星2.3倍的行星，需要4天才能圍繞它一週，於2012年以凌日法發現。 (zh)
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