| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Draco |
| Right ascension | 16h 45m 17.88121s [1] |
| Declination | +56° 46′ 54.7985″ [1] |
| Apparent magnitude (V) | 4.84 [2] |
| Characteristics | |
| Spectral type | F2 V [3] |
| B−V color index | 0.375±0.013 [2] |
| Astrometry | |
| Radial velocity (Rv) | −2.0 [4] km/s |
| Proper motion (μ) |
RA: 24.85
mas/
yr Dec.: 67.07 mas/ yr |
| Parallax (π) | 39.2932 ± 0.3182 mas [1] |
| Distance | 83.0 ± 0.7
ly (25.4 ± 0.2 pc) |
| Absolute magnitude (MV) | 2.71 [2] |
| Orbit [5] | |
| Period (P) | 363.57 d |
| Eccentricity (e) | 0.35 |
| Periastron epoch (T) | 2415232.4 JD |
|
Argument of periastron (ω) (secondary) | 80.7° |
|
Semi-amplitude (K1) (primary) | 6.0 km/s |
| Details | |
| Mass | 1.43 [4] M☉ |
| Radius | 1.6 [6] R☉ |
| Luminosity | 6.91 [2] L☉ |
| Surface gravity (log g) | 4.05 [4] cgs |
| Temperature | 6,630 [7] K |
| Metallicity [Fe/H] | −0.23 [4] dex |
| Rotational velocity (v sin i) | 47.5±2.4 [7] km/s |
| Age | 2.30 [4] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 151613 is a binary star [5] system in the northern circumpolar constellation of Draco. It is visible to the naked eye with an apparent visual magnitude of 4.84. [2] The distance to this star, as estimated from its annual parallax shift of 39.3 mas, [1] is 83 light years. It is moving closer to the Earth with a heliocentric radial velocity of −2 km/s. [4]
This is a single-lined spectroscopic binary [3] system with an orbital period of 363.57 days and an eccentricity of 0.35. [5] The pair were resolved through speckle interferometry in 1977, showing an angular separation of 0.041 ″. They were later resolved in 1981 with a separation of 0.047″, but were unresolved during 20 other attempts between 1976–1991. [9] The system is a source of X-ray emission. [10] The visible component is an F-type main-sequence star with a stellar classification of F2 V. [3] It is around 2.3 [4] billion years old with a projected rotational velocity of 48 km/s. [7]
- ^ a b c d 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.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c Abt, Helmut A. (2009), "MK Classifications of Spectroscopic Binaries", The Astrophysical Journal Supplement, 180 (1): 117–18, Bibcode: 2009ApJS..180..117A, doi: 10.1088/0067-0049/180/1/117, S2CID 122811461.
- ^ a b c d e f g Casagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy and Astrophysics, 530: A138, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID 56118016.
- ^ a b c Pourbaix, D.; et al. (2004), "SB9: The Ninth Catalogue of Spectroscopic Binary Orbits", Astronomy & Astrophysics, 424: 727–732, arXiv: astro-ph/0406573, Bibcode: 2004A&A...424..727P, doi: 10.1051/0004-6361:20041213, S2CID 119387088.
- ^ Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition", Astronomy and Astrophysics, 367 (2): 521–524, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b c Reiners, Ansgar (January 2006), "Rotation- and temperature-dependence of stellar latitudinal differential rotation", Astronomy and Astrophysics, 446 (1): 267–277, arXiv: astro-ph/0509399, Bibcode: 2006A&A...446..267R, doi: 10.1051/0004-6361:20053911, S2CID 8642707
- ^ "HD 151613". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-18.
- ^ Hartkopf, William I.; Mason, Brian D. (September 2009), "Speckle Interferometry at Mount Wilson Observatory: Observations Obtained in 2006-2007 and 35 New Orbits", The Astronomical Journal, 138 (3): 813–826, Bibcode: 2009AJ....138..813H, doi: 10.1088/0004-6256/138/3/813.
- ^ Haakonsen, Christian Bernt; Rutledge, Robert E. (September 2009), "XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources", The Astrophysical Journal Supplement, 184 (1): 138–151, arXiv: 0910.3229, Bibcode: 2009ApJS..184..138H, doi: 10.1088/0067-0049/184/1/138, S2CID 119267456.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Draco |
| Right ascension | 16h 45m 17.88121s [1] |
| Declination | +56° 46′ 54.7985″ [1] |
| Apparent magnitude (V) | 4.84 [2] |
| Characteristics | |
| Spectral type | F2 V [3] |
| B−V color index | 0.375±0.013 [2] |
| Astrometry | |
| Radial velocity (Rv) | −2.0 [4] km/s |
| Proper motion (μ) |
RA: 24.85
mas/
yr Dec.: 67.07 mas/ yr |
| Parallax (π) | 39.2932 ± 0.3182 mas [1] |
| Distance | 83.0 ± 0.7
ly (25.4 ± 0.2 pc) |
| Absolute magnitude (MV) | 2.71 [2] |
| Orbit [5] | |
| Period (P) | 363.57 d |
| Eccentricity (e) | 0.35 |
| Periastron epoch (T) | 2415232.4 JD |
|
Argument of periastron (ω) (secondary) | 80.7° |
|
Semi-amplitude (K1) (primary) | 6.0 km/s |
| Details | |
| Mass | 1.43 [4] M☉ |
| Radius | 1.6 [6] R☉ |
| Luminosity | 6.91 [2] L☉ |
| Surface gravity (log g) | 4.05 [4] cgs |
| Temperature | 6,630 [7] K |
| Metallicity [Fe/H] | −0.23 [4] dex |
| Rotational velocity (v sin i) | 47.5±2.4 [7] km/s |
| Age | 2.30 [4] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 151613 is a binary star [5] system in the northern circumpolar constellation of Draco. It is visible to the naked eye with an apparent visual magnitude of 4.84. [2] The distance to this star, as estimated from its annual parallax shift of 39.3 mas, [1] is 83 light years. It is moving closer to the Earth with a heliocentric radial velocity of −2 km/s. [4]
This is a single-lined spectroscopic binary [3] system with an orbital period of 363.57 days and an eccentricity of 0.35. [5] The pair were resolved through speckle interferometry in 1977, showing an angular separation of 0.041 ″. They were later resolved in 1981 with a separation of 0.047″, but were unresolved during 20 other attempts between 1976–1991. [9] The system is a source of X-ray emission. [10] The visible component is an F-type main-sequence star with a stellar classification of F2 V. [3] It is around 2.3 [4] billion years old with a projected rotational velocity of 48 km/s. [7]
- ^ a b c d 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.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c Abt, Helmut A. (2009), "MK Classifications of Spectroscopic Binaries", The Astrophysical Journal Supplement, 180 (1): 117–18, Bibcode: 2009ApJS..180..117A, doi: 10.1088/0067-0049/180/1/117, S2CID 122811461.
- ^ a b c d e f g Casagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy and Astrophysics, 530: A138, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID 56118016.
- ^ a b c Pourbaix, D.; et al. (2004), "SB9: The Ninth Catalogue of Spectroscopic Binary Orbits", Astronomy & Astrophysics, 424: 727–732, arXiv: astro-ph/0406573, Bibcode: 2004A&A...424..727P, doi: 10.1051/0004-6361:20041213, S2CID 119387088.
- ^ Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition", Astronomy and Astrophysics, 367 (2): 521–524, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b c Reiners, Ansgar (January 2006), "Rotation- and temperature-dependence of stellar latitudinal differential rotation", Astronomy and Astrophysics, 446 (1): 267–277, arXiv: astro-ph/0509399, Bibcode: 2006A&A...446..267R, doi: 10.1051/0004-6361:20053911, S2CID 8642707
- ^ "HD 151613". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-18.
- ^ Hartkopf, William I.; Mason, Brian D. (September 2009), "Speckle Interferometry at Mount Wilson Observatory: Observations Obtained in 2006-2007 and 35 New Orbits", The Astronomical Journal, 138 (3): 813–826, Bibcode: 2009AJ....138..813H, doi: 10.1088/0004-6256/138/3/813.
- ^ Haakonsen, Christian Bernt; Rutledge, Robert E. (September 2009), "XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources", The Astrophysical Journal Supplement, 184 (1): 138–151, arXiv: 0910.3229, Bibcode: 2009ApJS..184..138H, doi: 10.1088/0067-0049/184/1/138, S2CID 119267456.