Astronomy:AK Pictoris
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Pictor |
Right ascension | 06h 38m 00.36576s[1] |
Declination | −61° 32′ 00.1941″[1] |
Apparent magnitude (V) | 6.182[2] (6.32 / 8.77)[3] |
Characteristics | |
Spectral type | G2 + K5:[4] |
B−V color index | +0.62[5] |
Variable type | BY Dra[6] |
Astrometry | |
Radial velocity (Rv) | 32.10 ± 0.5[7] km/s |
Proper motion (μ) | RA: -47.84[1] mas/yr Dec.: 72.73[1] mas/yr |
Parallax (π) | 46.96 ± 0.81[1] mas |
Distance | 69 ± 1 ly (21.3 ± 0.4 pc) |
Absolute magnitude (MV) | 4.63[8] + ? |
Orbit[3] | |
Period (P) | 217.6 yr |
Semi-major axis (a) | 2.004″ |
Eccentricity (e) | 0.336 |
Inclination (i) | 93.9° |
Longitude of the node (Ω) | 91.6° |
Periastron epoch (T) | 2033.9 |
Argument of periastron (ω) (secondary) | 357.3° |
Details | |
AK Pic A | |
Mass | 1.03[9] M☉ |
Radius | 1.22[9] R☉ |
Luminosity | 1.45[9] L☉ |
Temperature | 5860[4] K |
Rotational velocity (v sin i) | 15.1 ± 0.8[8] km/s |
AK Pic B | |
Luminosity | 0.25[4] L☉ |
Temperature | 4400[4] K |
Rotational velocity (v sin i) | 15.5 ± 2.0[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
AK Pictoris is a star system in the constellation Pictor. Its combined apparent magnitude is 6.182.[2] Based on the system's parallax, it is located 69 light-years (21.3 parsecs) away.[1] AK Pictoris is a member of the AB Doradus moving group,[9] a group of stars with similar motions that are thought to be associated.
AK Pictoris is a binary star. Its two stars orbit each other every 217.6 years, separated by 2.004″.[3] The primary star is a G-type star[4] with similar properties to the Sun. The secondary star is a K-type star.[4] The primary star is a young BY Draconis variable,[6] a class of variable stars that derive their variability from stellar rotation. It is also known to host a debris disk, inferred from its infrared excess.[9]
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. http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A%2526A...474..653VFUL.
- ↑ 2.0 2.1 2.2 "V* AK Pic". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V%2A+AK+Pic.
- ↑ 3.0 3.1 3.2 "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 20 July 2017.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 McCarthy, Kyle; White, Russel J. (2012). "The Sizes of the Nearest Young Stars". The Astronomical Journal 143 (6): 134. doi:10.1088/0004-6256/143/6/134. Bibcode: 2012AJ....143..134M.
- ↑ Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory 4: 99. Bibcode: 1966CoLPL...4...99J.
- ↑ 6.0 6.1 Samus', N. N.; Goranskii, V. P.; Durlevich, O. V.; Zharova, A. V.; Kazarovets, E. V.; Kireeva, N. N.; Pastukhova, E. N.; Williams, D. B. et al. (2003). "An Electronic Version of the Second Volume of the General Catalogue of Variable Stars with Improved Coordinates". Astronomy Letters 29 (7): 468. doi:10.1134/1.1589864. Bibcode: 2003AstL...29..468S.
- ↑ 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.
- ↑ 8.0 8.1 8.2 Fuhrmann, K.; Chini, R. (2015). "Multiplicity Among F-Type Stars. II". The Astrophysical Journal 809 (1): 107. doi:10.1088/0004-637X/809/1/107. Bibcode: 2015ApJ...809..107F.
- ↑ 9.0 9.1 9.2 9.3 9.4 Plavchan, Peter; Werner, M. W.; Chen, C. H.; Stapelfeldt, K. R.; Su, K. Y. L.; Stauffer, J. R.; Song, I. (2009). "New Debris Disks Around Young, Low-Mass Stars Discovered with Thespitzer Space Telescope". The Astrophysical Journal 698 (2): 1068–1094. doi:10.1088/0004-637X/698/2/1068. Bibcode: 2009ApJ...698.1068P.
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