HD 5388
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Phoenix |
| Right ascension | 00h 55m 11.88995s[1] |
| Declination | –47° 24′ 21.4763″[1] |
| Apparent magnitude (V) | 6.73[2] |
| Characteristics | |
| Evolutionary stage | main sequence |
| Spectral type | F6V[2] |
| Apparent magnitude (B) | 7.73[3] |
| Apparent magnitude (J) | 5.795[4] |
| Apparent magnitude (H) | 5.524[4] |
| Apparent magnitude (K) | 5.441[4] |
| B−V color index | 0.500[2] |
| Astrometry | |
| Radial velocity (Rv) | +39.40±0.16[1] km/s |
| Proper motion (μ) | RA: −80.390[1] mas/yr Dec.: −178.132[1] mas/yr |
| Parallax (π) | 18.8155 ± 0.0268 mas[1] |
| Distance | 173.3 ± 0.2 ly (53.15 ± 0.08 pc) |
| Absolute magnitude (MV) | 3.10[2] |
| Details[2] | |
| Mass | 1.21 M☉ |
| Radius | 1.87+0.03 −0.04[1] R☉ |
| Luminosity | 4.770+0.012 −0.011[1] L☉ |
| Surface gravity (log g) | 4.28±0.06 cgs |
| Temperature | 6,297±32 K |
| Metallicity [Fe/H] | −0.27±0.02 dex |
| Rotation | 23 days |
| Rotational velocity (v sin i) | 4.2 km/s |
| Age | 5.5±0.5[5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
HD 5388 is a single[7] star in the southern constellation of Phoenix. It has the Gould designation 78 G. Phoenicis,[8] while HD 5388 is the star's Henry Draper Catalogue identifier. This object has a yellow-white hue and is too faint to be readily visible to average human eyesight, having an apparent visual magnitude of 6.73.[2] It is located at a separation of 173 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +39 km/s.[1]
This object is an ordinary F-type main-sequence star with a stellar classification of F6V,[2] indicating that it is generating energy through core hydrogen fusion. It is not chromospherically active and its metal content is half as much as the Sun. The star is larger and more massive than our Sun,[2] and radiates 4.8[1] times the Sun's luminosity from its photosphere at an effective temperature of 6297 K.[1]
In 2009, a gas giant planet was detected in orbit around the star using the HARPS instrument at La Silla Observatory.[2] This was later demonstrated to be a brown dwarf rather than a planet. It has an elliptical orbit with a period of 2.13 years.[9]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 69 MJ | 1.76 | 777±4 | 0.40±0.02 | — | — |
See also
References
- ^ a b c d e f g h i j k Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c d e f g h i j Santos, N. C.; et al. (2010). "The HARPS search for southern extrasolar planets XXI. Three new giant planets orbiting the metal-poor stars HD5388, HD181720, and HD190984". Astronomy and Astrophysics. 512. A47. arXiv:0912.3216. Bibcode:2010A&A...512A..47S. doi:10.1051/0004-6361/200913489.
- ^ Høg, E.; et al. (2000). The Tycho-2 catalogue of the 2.5 million brightest stars. Vol. 355. pp. L27. Bibcode:2000A&A...355L..27H. doi:10.1888/0333750888/2862. ISBN 978-0333750889.
{{cite book}}:|journal=ignored (help) - ^ a b c Cutri, R. M.; et al. (June 2003). "2MASS All Sky Catalog of point sources". NASA/IPAC. Bibcode:2003tmc..book.....C.
{{cite journal}}: Cite journal requires|journal=(help) - ^ Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951.
- ^ "HD 5388". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-11-06.
- ^ Tokovinin, Andrei (2014). "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs". The Astronomical Journal. 147 (4): 87. arXiv:1401.6827. Bibcode:2014AJ....147...87T. doi:10.1088/0004-6256/147/4/87.
- ^ Gould, Benjamin Apthorp. "Uranometria Argentina". Retrieved 2019-11-06.
- ^ a b Sahlmann, J.; et al. (2011). "HD 5388 b is a 69 MJup companion instead of a planet". Astronomy and Astrophysics Letters. 528. L8. arXiv:1102.3372. Bibcode:2011A&A...528L...8S. doi:10.1051/0004-6361/201116533.
