Astronomy:HR 4138
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Carina |
| Right ascension | 10h 30m 20.12710s[1] |
| Declination | −71° 59′ 34.0602″[1] |
| Apparent magnitude (V) | +4.72[2] |
| Characteristics | |
| Spectral type | A2IV[3][4] or A1V[5] or A2III[6] |
| B−V color index | +0.042±0.007[2] |
| Astrometry | |
| Radial velocity (Rv) | +7.5±0.4[2] km/s |
| Proper motion (μ) | RA: +27.59[1] mas/yr Dec.: −30.73[1] mas/yr |
| Parallax (π) | 12.52 ± 0.17[1] mas |
| Distance | 261 ± 4 ly (80 ± 1 pc) |
| Absolute magnitude (MV) | 0.21[2] |
| Details | |
| Mass | 2.10[7] M☉ |
| Radius | 3.45[8] R☉ |
| Luminosity | 75.06[2] L☉ |
| Surface gravity (log g) | 3.71[7] cgs |
| Temperature | 9,169±312[7] K |
| Metallicity [Fe/H] | +0.06[2] dex |
| Rotational velocity (v sin i) | 12[7] km/s |
| Age | 403[7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HR 4138 is a single[10] star in the constellation Carina. It has the Bayer designation K Carinae,[11] abbreviated K Car, while HR 4138 is the star's designation in the Bright Star Catalogue. It has a white hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.72.[2] This star is located at a distance of approximately 261 light years from the Sun based on parallax measurements,[1] and it is drifting further away with a radial velocity of +7.5 km/s.[2] Judging from its motion through space, it is a candidate member of the Sirius supercluster.[12]
This object is a superficially normal[4] A-type star. However, there is some disagreement over the evolutionary state of the star, as it has received luminosity classifications of a subgiant,[4] main sequence,[5] and a giant star.[6] Unexpectedly for an A-type star, a magnetic field has been detected.[4] It is around 400 million years old and has a low projected rotational velocity of 12 km/s.[7] The star displays an infrared excess,[10] indicating the presence of an orbiting debris disk with a black body temperature of 45 K at a separation of 314.2 astronomical unit|AU from the host star.[8]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ Gray, R. O.; Garrison, R. F. (1987), "The Early A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation", The Astrophysical Journal Supplement Series 65: 581, doi:10.1086/191237, Bibcode: 1987ApJS...65..581G.
- ↑ 4.0 4.1 4.2 4.3 Mathys, G.; Hubrig, S. (July 2006), "The diagnosis of the mean quadratic magnetic field of Ap stars", Astronomy and Astrophysics 453 (2): 699–715, doi:10.1051/0004-6361:20054353, Bibcode: 2006A&A...453..699M.
- ↑ 5.0 5.1 Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1975mcts.book.....H.
- ↑ 6.0 6.1 Levato, O. H. (August 1972), "Rotational Velocities and Spectral Types of Some A-Type Stars", Publications of the Astronomical Society of the Pacific 84 (500): 584, doi:10.1086/129336, Bibcode: 1972PASP...84..584L.
- ↑ 7.0 7.1 7.2 7.3 7.4 7.5 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, doi:10.1088/0004-637X/804/2/146, Bibcode: 2015ApJ...804..146D.
- ↑ 8.0 8.1 Cotten, Tara H.; Song, Inseok (July 2016), "A Comprehensive Census of Nearby Infrared Excess Stars", The Astrophysical Journal Supplement Series 225 (1): 24, doi:10.3847/0067-0049/225/1/15, 15, Bibcode: 2016ApJS..225...15C.
- ↑ "HD 91375". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+91375.
- ↑ 10.0 10.1 Rodriguez, David R.; Zuckerman, B. (February 2012), "Binaries among Debris Disk Stars", The Astrophysical Journal 745 (2): 147, doi:10.1088/0004-637X/745/2/147, Bibcode: 2012ApJ...745..147R.
- ↑ Kostjuk, N. D. (2004), "VizieR Online Data Catalog: HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index (Kostjuk, 2002)", VizieR On-line Data Catalog: IV/27A. Originally Published in: Institute of Astronomy of Russian Academy of Sciences (2002) 4027, Bibcode: 2004yCat.4027....0K.
- ↑ Palous, J.; Hauck, B. (July 1986), "The Sirius supercluster", Astronomy and Astrophysics 162: 54–61, Bibcode: 1986A&A...162...54P.
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