HD 48265 b

HD 48265 b / Naqaỹa
Discovery
Discovered byMinniti et al.
Discovery siteLa Silla Observatory
Discovery dateOctober 29, 2008
Doppler spectroscopy
(CORALIE)
Orbital characteristics
1.81±0.07 AU
Eccentricity0.08±0.05[1]
780.3±4.6[1] d
344±138[1]
Semi-amplitude27.7±1.2[1]
StarHD 48265

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. It has a minimum mass of 1.47 times that of Jupiter. Because its inclination is not known, its true mass is not known. It orbits at a distance of 1.81 AU with an orbital eccentricity of 0.08.[2][1]

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

  1. ^ a b c d e Cite error: The named reference Jenkins2017 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference Minniti2009 was invoked but never defined (see the help page).
  3. ^ Salas, Javier (17 December 2019). "Rosalía de Castro ya tiene su estrella | Ciencia | EL PAÍS". El País.