Gliese 163
Gliese 163 is an M3.5V red dwarf located 49 light years (15.0 pc) from the sun, in the constellation Dorado.[3] Its coordinates in the night sky are RA 04h 9m 16s and Dec. -53°22'. It has a visual magnitude of 11.8 and an absolute magnitude of 10.9.[3] Other stellar catalog names for it include HIP 19394 and LHS 188.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Dorado |
Right ascension | 04h 09m 15.663s |
Declination | −53° 22′ 25.31″ |
Apparent magnitude (V) | 11.8 |
Characteristics | |
Spectral type | M3.5V |
Astrometry | |
Absolute magnitude (MV) | 10.9 |
Details | |
Mass | 0.30[1] M☉ |
Luminosity | 0.01 L☉ |
Temperature | 3300[1] K |
Metallicity [Fe/H] | 0.1 ± 0.1[1] dex |
Rotation | 61.0±0.3 d[2] |
Age | 0.77 ± 0.03[1] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Planetary system
In September 2012, astronomers using the HARPS instrument announced the discovery of two planets orbiting Gliese 163.[4][5] One planet, Gliese 163 c, with an orbital period of 26 days, and a minimum mass of 6.9 Earth masses, was considered potentially in the habitable zone, although hotter than Earth, with a temperature of 60 deg. C (140 deg. F) It has an ecc. of 0.03 or 3 per.. A second planet, Gliese 163 b, was also announced, with an orbital period of 9 days. It would be way too hot to be considered habitable. Evidence was also found for a third planet orbiting further out than c and b.[4][5] In June 2013, it was concluded that at least 3 planets orbit around the star with a fourth planet being a possibility.[1] In a paper submitted to arXiv in June 2019, Gliese 163 was found to have five planets.[6]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥9.9±2.3 M⊕ | 0.060+0.005 −0.006 |
8.6312+0.0023 −0.0021 |
0.02+0.12 −0.02 |
— | — |
c | ≥7.6+2.9 −2.3 M⊕ |
0.124+0.010 −0.013 |
25.637±0.042 | 0.03+0.18 −0.03 |
— | — |
f | ≥6.8±4.4 M⊕ | 0.326+0.027 −0.034 |
109.5+1.6 −1.4 |
0.04+0.23 −0.04 |
— | — |
e | ≥13.6+8.2 −6.5 M⊕ |
0.700±0.066 | 349+12 −10 |
0.03+0.25 −0.03 |
— | — |
d | ≥20.2±7.6 M⊕ | 1.021+0.088 −0.118 |
604+29 −24 |
0.02+0.22 −0.02 |
— | — |
References
- Tuomi, M.; Anglada-Escudé, G. (2013). "Up to four planets around the M dwarf GJ 163". Astronomy & Astrophysics. 556: A111. arXiv:1306.1717. doi:10.1051/0004-6361/201321174. S2CID 16214668.
- Suárez Mascareño, A.; et al. (September 2015), "Rotation periods of late-type dwarf stars from time series high-resolution spectroscopy of chromospheric indicators", Monthly Notices of the Royal Astronomical Society, 452 (3): 2745–2756, arXiv:1506.08039, Bibcode:2015MNRAS.452.2745S, doi:10.1093/mnras/stv1441, S2CID 119181646.
- Staff (September 20, 2012). "LHS 188 -- High proper-motion Star". Centre de données astronomiques de Strasbourg (Strasbourg astronomical Data Center). Retrieved September 20, 2012.
- Méndez, Abel (August 29, 2012). "A Hot Potential Habitable Exoplanet around Gliese 163". University of Puerto Rico at Arecibo (Planetary Habitability Laboratory). Retrieved September 20, 2012.
- Redd, Nola Taylor (September 20, 2012). "Newfound Alien Planet a Top Contender to Host Life". Space.com. Retrieved September 20, 2012.
- Tuomi, M.; et al. (11 June 2019). "Frequency of planets orbiting M dwarfs in the Solar neighborhood". arXiv:1906.04644 [astro-ph.EP].
- Bonfils, X.; Lo Curto, G.; Correia, A. C. M.; Laskar, J.; Udry, S.; Delfosse, X.; Forveille, T.; Astudillo-Defru, N.; Benz, W.; Bouchy, F.; Gillon, M.; Hébrard, G.; Lovis, C.; Mayor, M.; Moutou, C.; Naef, D.; Neves, V.; Pepe, F.; Perrier, C.; Queloz, D.; Santos, N. C.; Ségransan, D. (5 August 2013). "The HARPS search for southern extra-solar planets". Astronomy & Astrophysics. 556: A110. arXiv:1306.0904. Bibcode:2013A&A...556A.110B. doi:10.1051/0004-6361/201220237. S2CID 118456453.