HR 6806
| Observation data Epoch 2000 Equinox 2000 | |
|---|---|
| Constellation | Hercules |
| Right ascension | 18h 09m 37.41626s[1] |
| Declination | +38° 27′ 27.9960″[1] |
| Apparent magnitude (V) | 6.40[2] |
| Characteristics | |
| Spectral type | K2 V[3] |
| U−B color index | +0.585[2] |
| B−V color index | +0.875[2] |
| Astrometry | |
| Radial velocity (Rv) | −19.473 ± 0.028[4] km/s |
| Proper motion (μ) | RA: −316.44[1] mas/yr Dec.: −468.47[1] mas/yr |
| Parallax (π) | 90.71 ± 0.30[1] mas |
| Distance | 36.0 ± 0.1 ly (11.02 ± 0.04 pc) |
| Details | |
| Surface gravity (log g) | 4.53[3] cgs |
| Temperature | 4,900[3] K |
| Metallicity [Fe/H] | −0.61[3] dex |
| Rotation | 42 d[5] |
| Rotational velocity (v sin i) | 4.82[6] km/s |
| Age | 5.8–7.1[7] Gyr |
| Other designations | |
HR 6806 is a solitary, orange, main sequence (K2 V) star located thirty-six light-years away, in the constellation Hercules. It appears to be rotating slowly with an estimated period of 42 days. The star has an inactive chromosphere, with a surface magnetic field strength of 1,500 G.[5]
There is a nearby brown dwarf, WISE J180901.07+383805.4, at an angular separation of 769″, which would correspond to a projected separation of 8460 AU at the distance of HR 6806. However, this is most likely a typical T7 dwarf, which would place it at a distance of 91 ly (28 pc)—ruling out a physical association. This is confirmed by the differing proper motion of the star and this object.[9]
References
- 1 2 3 4 5 van Leeuwen, F. (November 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.
- 1 2 3 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data (SIMBAD), Bibcode:1986EgUBV........0M.
- 1 2 3 4 Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637.
- ↑ Soubiran, C.; et al. (April 2013), "The catalogue of radial velocity standard stars for Gaia. I. Pre-launch release", Astronomy & Astrophysics 552: 11, Bibcode:2013A&A...552A..64S, doi:10.1051/0004-6361/201220927, A64.
- 1 2 Basri, Gibor; Marcy, Geoffrey W. (July 1988), "Physical realism in the analysis of stellar magnetic fields", Astrophysical Journal, Part 1 330: 274−285, Bibcode:1988ApJ...330..274B, doi:10.1086/166471.
- ↑ Martínez-Arnáiz, R.; et al. (September 2010), "Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter", Astronomy and Astrophysics 520: A79, arXiv:1002.4391, Bibcode:2010A&A...520A..79M, doi:10.1051/0004-6361/200913725.
- ↑ Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008), "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics", The Astrophysical Journal 687 (2): 1264–1293, arXiv:0807.1686, Bibcode:2008ApJ...687.1264M, doi:10.1086/591785.
- ↑ "HR 6806 -- Variable Star", SIMBAD (Centre de Données astronomiques de Strasbourg), retrieved 2015-11-02.
- ↑ Luhman, Kevin L.; et al. (December 2012), "New M, L, and T Dwarf Companions to Nearby Stars from the Wide-field Infrared Survey Explorer", The Astrophysical Journal 760 (2): 9, arXiv:1211.3977, Bibcode:2012ApJ...760..152L, doi:10.1088/0004-637X/760/2/152, 152.
External links
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