1 Lacertae
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Lacerta |
| Right ascension | 22h 15m 58.17673s[1] |
| Declination | +37° 44′ 55.4385″[1] |
| Apparent magnitude (V) | 4.15[2] |
| Characteristics | |
| Spectral type | K3II-III[3] |
| U−B color index | +1.70[2] |
| B−V color index | +1.43[2] |
| Astrometry | |
| Radial velocity (Rv) | −8.58[4] km/s |
| Proper motion (μ) | RA: +8.85[1] mas/yr Dec.: –0.72[1] mas/yr |
| Parallax (π) | 5.25 ± 0.23[1] mas |
| Distance | 620 ± 30 ly (190 ± 8 pc) |
| Absolute magnitude (MV) | −2.61+0.27 −0.24[5] |
| Details | |
| Radius | 51[6] R☉ |
| Surface gravity (log g) | 1.75[7] cgs |
| Temperature | 4,350[7] K |
| Metallicity [Fe/H] | −0.12[7] dex |
| Rotational velocity (v sin i) | 10[8] km/s |
| Other designations | |
1 Lacertae (1 Lac) is a solitary[10] star in the northern constellation of Lacerta. It is visible to the naked eye with an apparent magnitude of 4.15.[2] Based upon measurements by the Hipparcos spacecraft, this star is located at a distance of roughly 420 light years.[1] A stellar classification of K3II-III[3] suggests this is an evolved giant star. It has expanded to an estimated 51[6] times the radius of the Sun. The effective temperature of 4,350[7] K for the stellar atmosphere gives it the orange-hued glow of a K-type star.[11]
References
- 1 2 3 4 5 6 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.
- 1 2 3 4 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data (SIMBAD), Bibcode:1986EgUBV........0M.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 Herbig, George H.; Spalding, John F., Jr. (January 1955), "Axial Rotation and Line Broadening in Stars of Spectral Types F0-K5", Astrophysical Journal 121: 118, Bibcode:1955ApJ...121..118H, doi:10.1086/145969.
- ↑ Famaey, B.; et al. (2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics 430: 165–186, arXiv:astro-ph/0409579, Bibcode:2005A&A...430..165F, doi:10.1051/0004-6361:20041272.
- ↑ Carney, Bruce W.; et al. (March 2008), "Rotation and Macroturbulence in Metal-Poor Field Red Giant and Red Horizontal Branch Stars", The Astronomical Journal 135 (3): 892–906, arXiv:0711.4984, Bibcode:2008AJ....135..892C, doi:10.1088/0004-6256/135/3/892.
- 1 2 Pasinetti-Fracassini, L. E.; et al. (February 2001), "Catalogue of Stellar Diameters (CADARS)", Astronomy and Astrophysics 367: 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451.
- 1 2 3 4 McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series 74: 1075–1128, Bibcode:1990ApJS...74.1075M, doi:10.1086/191527.
- ↑ Bernacca, P. L.; Perinotto, M. (1970). "A catalogue of stellar rotational velocities". Contributi Osservatorio Astronomico di Padova in Asiago 239. Bibcode:1970CoAsi.239....1B.
- ↑ "1 Lac -- Variable Star", SIMBAD Astronomical Database (Centre de Données astronomiques de Strasbourg), retrieved 2016-03-07.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.
- ↑ "The Colour of Stars", Australia Telescope, Outreach and Education (Commonwealth Scientific and Industrial Research Organisation), December 21, 2004, retrieved 2012-01-16.
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