Lambda2 Fornacis
Appearance
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Fornax |
Right ascension | 02h 36m 58.61s[1] |
Declination | –34° 34′ 40.7″[1] |
Apparent magnitude (V) | 5.78 |
Characteristics | |
Spectral type | G1V |
B−V color index | 0.67 |
Astrometry | |
Radial velocity (Rv) | 10.3 ± 2 km/s |
Proper motion (μ) | RA: –18.35 ± 0.22[1] mas/yr Dec.: –259.35 ± 0.27[1] mas/yr |
Parallax (π) | 38.79 ± 0.40 mas[1] |
Distance | 84.1 ± 0.9 ly (25.8 ± 0.3 pc) |
Absolute magnitude (MV) | 3.74 ± 0.04[2] |
Details | |
Mass | 1.18 ± 0.04[2] M☉ |
Radius | 1.50 ± 0.05[2] R☉ |
Surface gravity (log g) | 4.12 ± 0.03[2] cgs |
Temperature | 5,936[2] K |
Metallicity [Fe/H] | +0.19[2] dex |
Age | 4.34 ± 0.82[2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
ARICNS | data |
Lambda2 Fornacis (also called HD 16417) is a 6th magnitude G-type main sequence star located approximately 84 light years away in the constellation of Fornax. It is more massive, hotter, and more metal-rich than our Sun and only 300 million years younger.
Planetary system
Precision Doppler spectroscopy from an intensive 48 night observing campaign on the Anglo-Australian Telescope has revealed the presence of a low-mass extrasolar planet orbiting the star.[3]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥0.069 ± 0.007 MJ | 0.14 ± 0.01 | 17.24 ± 0.01 | 0.2 ± 0.09 | — | — |
See also
References
- ^ a b c d e van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
- ^ a b c d e f g da Silva, L.; et al. (November 2006), "Basic physical parameters of a selected sample of evolved stars", Astronomy and Astrophysics, 458 (2): 609–623, arXiv:astro-ph/0608160, Bibcode:2006A&A...458..609D, doi:10.1051/0004-6361:20065105
- ^ a b O’Toole, Simon; et al. (2009). "A Neptune-mass Planet Orbiting the Nearby G Dwarf HD16417". The Astrophysical Journal. 697 (2): 1263–1268. arXiv:0902.4024. Bibcode:2009ApJ...697.1263O. doi:10.1088/0004-637X/697/2/1263.