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HD 48265 b 
Summary
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]
| Discovery | |
|---|---|
| Discovered by | Minniti et al. |
| Discovery site | La Silla Observatory |
| Discovery date | October 29, 2008 |
| Doppler spectroscopy (CORALIE) m | |
| Orbital characteristics | |
| 1.81±0.07 AU | |
| Eccentricity | 0.08±0.05[1] |
| 780.3±4.6[1] d | |
| 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 edit
- ^ a b c d e Jenkins, J. S.; et al. (2017). "New planetary systems from the Calan–Hertfordshire Extrasolar Planet Search". Monthly Notices of the Royal Astronomical Society. 466 (1): 443–473. arXiv:1603.09391. Bibcode:2017MNRAS.466..443J. doi:10.1093/mnras/stw2811.
- ^ Minniti, Dante; et al. (2009). "Low-Mass Companions for Five Solar-Type Stars From the Magellan Planet Search Program". The Astrophysical Journal. 693 (2): 1424–1430. arXiv:0810.5348. Bibcode:2009ApJ...693.1424M. doi:10.1088/0004-637X/693/2/1424. S2CID 119224845.
- ^ Salas, Javier (17 December 2019). "Rosalía de Castro ya tiene su estrella | Ciencia | EL PAÍS". El País.
External links edit
- "HD 48265 b". Exoplanets. Archived from the original on 2012-03-04. Retrieved 2008-11-06.