astro.wikisort.org - Meteorite

HD 48265 b is an extrasolar planet located approximately 293 light-years away in the constellation of Puppis, orbiting the 8th magnitude G-type main sequence star HD 48265. This planet has a minimum mass of 1.47 times that of Jupiter. Because the inclination is not known, the true mass is not known. This planet orbits at a distance of 1.81 AU with an orbital eccentricity of 0.08.[2][1]

HD 48265 b

Discovery
Discovered by	Minniti et al.
Discovery site	La Silla Observatory
Discovery date	October 29, 2008
Detection method	Doppler spectroscopy (CORALIE) m
Orbital characteristics
Semi-major axis	1.81±0.07 AU
Eccentricity	0.08±0.05[1]
Orbital period (sidereal)	780.3±4.6[1] d
Argument of periastron	344±138[1]
Semi-amplitude	27.7±1.2[1]
Star	HD 48265

As part of the NameExoWorlds project of the IAU, HD 48265 b has been named "Naqaỹa" ("brother") and HD 48265 "Nosaxa" ("springtime") in the Moqoit language, as voted by Argentine voters in an online poll.[3]

References

External links

• "HD 48265 b". Exoplanets. Archived from the original on 2012-03-04. Retrieved 2008-11-06.

На других языках

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- [en] HD 48265 b

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[es] HD 48265 b

HD 48265 b es un planeta extrasolar que se encuentra aproximadamente a 285 años luz en la constelación de Puppis, orbitando la estrella de tipo G HD 48265, de la secuencia principal. Este planeta orbita a una distancia de 0,45 UA y excentricidad, de 0,24. Su masa mínima equivale a 1,2 masas jovianas. Sin embargo solo se conoce su masa mínima, ya que la inclinación de la órbita no se conoce.

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