Mu Fornacis
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Fornax |
| Right ascension | 02h 12m 54.46962s[1] |
| Declination | −30° 43′ 25.7732″[1] |
| Apparent magnitude (V) | 5.27[2] |
| Characteristics | |
| Spectral type | A0 V[3] |
| U−B color index | −0.06[2] |
| B−V color index | −0.02[2] |
| Astrometry | |
| Radial velocity (Rv) | 10.0±3.7[4] km/s |
| Proper motion (μ) | RA: +14.10[1] mas/yr Dec.: +6.85[1] mas/yr |
| Parallax (π) | 10.18 ± 0.24[1] mas |
| Distance | 320 ± 8 ly (98 ± 2 pc) |
| Details | |
| Mass | 3.10[5] M☉ |
| Radius | 2.5[6] R☉ |
| Luminosity | 68.7[7] L☉ |
| Surface gravity (log g) | 3.71±0.14[5] cgs |
| Temperature | 11,745±399[5] K |
| Rotational velocity (v sin i) | 320[3] km/s |
| Age | 188[5] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
μ Fornacis (Latinised as Mu Fornacis) is the Bayer designation for a star in the southern constellation of Fornax. With an apparent visual magnitude of 5.27,[2] it is visible to the naked eye. The distance to this star, as determined by its annual parallax shift of 10.18 mas,[1] is around 320 light years.
This is an A-type main sequence star with a stellar classification of A0 V.[3] It is a Be star that displays "central quasi emission" (CQE) bumps in its spectrum due to a surrounding shell of material.[9] The star has an estimated 3.1[5] times the mass of the Sun and 2.5[6] times the Sun's radius. Mu Fornacis is spinning rapidly with a projected rotational velocity of 320 km/s[3] and is around 188 million years old.[5] It radiates 68.7[7] times the solar luminosity from its outer atmosphere at an effective temperature of 11,745 K.[5]
Mu Fornacis appears to be emitting an infrared excess at a wavelength of 22 μm, which could be due to an orbiting debris disk.[10]
References
- 1 2 3 4 5 6 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, Bibcode:2007A&A...474..653V, arXiv:0708.1752
, doi:10.1051/0004-6361:20078357. - 1 2 3 4 Cousins, A. W. J. (1973), "UBV photometry of some southern stars", Monthly Notes of the Astronomical Society of Southern Africa, 32: 11, Bibcode:1973MNSSA..32...11C.
- 1 2 3 4 Royer, F.; et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics, 463 (2): 671–682, Bibcode:2007A&A...463..671R, arXiv:astro-ph/0610785 , doi:10.1051/0004-6361:20065224.
- ↑ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, A61.
- 1 2 3 4 5 6 7 David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, Bibcode:2015ApJ...804..146D, arXiv:1501.03154 , doi:10.1088/0004-637X/804/2/146.
- 1 2 Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) – Third edition – Comments and statistics", Astronomy and Astrophysics, 367: 521–524, Bibcode:2001A&A...367..521P, arXiv:astro-ph/0012289 , doi:10.1051/0004-6361:20000451.
- 1 2 McDonald, I.; et al. (November 2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–357, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x.
- ↑ "mu. For – Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2017-01-24.
- ↑ Rivinius, Th.; et al. (November 2006), "Bright Be-shell stars", Astronomy and Astrophysics, 459 (1): 137–145, Bibcode:2006A&A...459..137R, doi:10.1051/0004-6361:20053008
- ↑ Wu, Chao-Jian; et al. (October 2013), "Bright 22 μm Excess Candidates from the Wise All-sky Catalog and the Hipparcos Main Catalog", The Astrophysical Journal Supplement, 208 (2): 12, Bibcode:2013ApJS..208...29W, arXiv:1308.3848 , doi:10.1088/0067-0049/208/2/29, 29.