Astronomy:12 Lyncis
From HandWiki
Short description: Star in the constellation Lynx
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Lynx |
Right ascension | 06h 46m 14.13019s[1] |
Declination | +59° 26′ 30.0227″[1] |
Apparent magnitude (V) | 4.86[2] (5.44 / 6.00)[3] |
Characteristics | |
Spectral type | A3V[2] (A1.5V + A2V)[4] |
U−B color index | +0.08[5] |
B−V color index | +0.084±0.012[2] |
Astrometry | |
Radial velocity (Rv) | −3.0±4.2[6] km/s |
Proper motion (μ) | RA: −19.63[1] mas/yr Dec.: −7.23[1] mas/yr |
Parallax (π) | 15.19 ± 0.78[1] mas |
Distance | 210 ± 10 ly (66 ± 3 pc) |
Absolute magnitude (MV) | 0.77[2] |
Orbit[3] | |
Period (P) | 907.6 yr |
Semi-major axis (a) | 2.30″ |
Eccentricity (e) | 0.3700 |
Inclination (i) | 134.7° |
Longitude of the node (Ω) | 166.5° |
Periastron epoch (T) | B 2677.4 |
Argument of periastron (ω) (secondary) | 322.6° |
Details | |
12 Lyn A | |
Radius | 2.52[4] R☉ |
Rotational velocity (v sin i) | 90±30[4] km/s |
12 Lyn B | |
Radius | 2.44[4] R☉ |
Rotational velocity (v sin i) | 100±30[4] km/s |
Other designations | |
Database references | |
SIMBAD | 12 Lyn |
12 Lyn A | |
12 Lyn B |
12 Lyncis, abbreviated 12 Lyn, is a triple star[8] system in the constellation Lynx. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.87. When seen through a telescope, it can be separated into three stars: two components with magnitudes 5.4 and 6.0 that lie at an angular separation by 1.8″ (as of 1992) and a yellow-hued star of magnitude 7.2 at a separation of 8.6″ (as of 1990).[9][10] The orbit of the two brighter stars is not known with certainty, but appears to have a period of somewhere around 700 to 900 years.[11] The pair have a projected separation of 128 astronomical unit|AU.[4] Parallax indicates the system is 210±10 light years distant from Earth.[1]
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. Archived from the original on 2016-04-02. https://web.archive.org/web/20160402233353/http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A&A...474..653VFUL.
- ↑ 2.0 2.1 2.2 2.3 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 "Sixth Catalog of Orbits of Visual Binary Stars". United States Naval Observatory. http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6. Retrieved 28 May 2017.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 Howe, K. S.; Clarke, C. J. (January 2009). "An analysis of v sin (i) correlations in early-type binaries". Monthly Notices of the Royal Astronomical Society 392 (1): 448–454. doi:10.1111/j.1365-2966.2008.14073.x. Bibcode: 2009MNRAS.392..448H.
- ↑ Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory 4: 99. Bibcode: 1966CoLPL...4...99J.
- ↑ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. Bibcode: 2006AstL...32..759G.
- ↑ "* 12 Lyn". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=%2A+12+Lyn.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society 389 (2): 869–879. doi:10.1111/j.1365-2966.2008.13596.x. Bibcode: 2008MNRAS.389..869E.
- ↑ Mason, Brian D. et al. (2001), "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog", The Astronomical Journal 122 (6): 3466, doi:10.1086/323920, Bibcode: 2001AJ....122.3466M.
- ↑ Monks, Neale (2010). Go-To Telescopes Under Suburban Skies. New York, New York: Springer Science & Business Media. p. 56. ISBN 9781441968517. https://books.google.com/books?id=waO6tUtfblsC&pg=PA56.
- ↑ Malkov, O. Yu.; Tamazian, V.S.; Docobo, J.A.; Chulkov, D.A. (2012). "Dynamical Masses of a Selected Sample of Orbital Binaries". Astronomy and Astrophysics 546: 5. doi:10.1051/0004-6361/201219774. A69. Bibcode: 2012A&A...546A..69M.
Original source: https://en.wikipedia.org/wiki/12 Lyncis.
Read more |