Theta Circini
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Circinus |
Right ascension | 15h 04m 48.18600s[1] |
Declination | −64° 01′ 52.8611″[1] |
Apparent magnitude (V) | 5.110[2] (5.90 + 5.90)[3] |
Characteristics | |
Spectral type | B3 Ve[4] (B2 + B2)[3] |
B−V color index | +0.00[2] |
Variable type | GCAS[5] |
Astrometry | |
Proper motion (μ) | RA: +102.65[1] mas/yr Dec.: +9.35[1] mas/yr |
Parallax (π) | 11.82 ± 0.30[1] mas |
Distance | 276 ± 7 ly (85 ± 2 pc) |
Absolute magnitude (MV) | −2.43/−2.43[3] |
Orbit[4] | |
Period (P) | ±0.78 39.62yr |
Semi-major axis (a) | 64±0.00056″ 0.085 |
Eccentricity (e) | ±0.0081 0.3014 |
Inclination (i) | ±2.0 153.3° |
Longitude of the node (Ω) | ±5.2 228.0° |
Periastron epoch (T) | 993.81±0.12 1 |
Argument of periastron (ω) (secondary) | ±6.5 68.6° |
Details | |
θ Cir A | |
Mass | ±0.6 9.3[6] M☉ |
Surface gravity (log g) | 3.38[2] cgs |
Temperature | 19,099[2] K |
Rotational velocity (v sin i) | ±13 195[7] km/s |
Age | ±6.1 27.1[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Theta Circini (θ Cir), is a binary star located in the southern constellation of Circinus, to the northwest of Alpha Circini.[5] It is faintly visible to the naked eye with an apparent visual magnitude of 5.110.[2] Based upon an annual parallax shift of 11.82 mas,[1] it is located at a distance of about 276 light years from the Sun.
This is an astrometric binary[9] star system with an orbital period of about 39.6 years, an eccentricity of 0.3, and a semimajor axis of 85.64 mas.[4] The pair show a combined stellar classification of B3 Ve,[4] which matches a B-type main sequence star.[4] The 'e' suffix on the class indicates this is a Be star. Alternate classifications include B4 Vnp[6] and B4npe,[4] with the 'n' indicating broad ("nebulous") absorption lines due to rotation and the 'p' meaning a chemically peculiar star. The two components appear to have similar visual magnitude, mass, and classification.[4] The system behaves as a Gamma Cassiopeia variable[5] showing occasional outbursts of up to 0.27 in magnitude.[10]
References
- 1 2 3 4 5 6 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, Bibcode:2007A&A...474..653V, arXiv:0708.1752 , doi:10.1051/0004-6361:20078357.
- 1 2 3 4 5 Soubiran, C.; et al. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, Bibcode:2010A&A...515A.111S, arXiv:1004.1069 , doi:10.1051/0004-6361/201014247.
- 1 2 3 Cvetkovic, Z.; Ninkovic, S. (June 2010), "On the Component Masses of Visual Binaries", Serbian Astronomical Journal, 180: 71–80, Bibcode:2010SerAJ.180...71C, doi:10.2298/SAJ1080071C.
- 1 2 3 4 5 6 7 Mason, Brian D.; et al. (September 2010), "Binary Star Orbits. IV. Orbits of 18 Southern Interferometric Pairs", The Astronomical Journal, 140 (3): 735−743, Bibcode:2010AJ....140..735M, doi:10.1088/0004-6256/140/3/735.
- 1 2 3 Arnold, H. J. P.; et al. (1999), The Photographic Atlas of the Stars, CRC Press, p. 176, ISBN 0750306548.
- 1 2 3 Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, Bibcode:2011MNRAS.410..190T, arXiv:1007.4883 , doi:10.1111/j.1365-2966.2010.17434.x.
- ↑ Frémat, Y.; et al. (September 2005), "Effects of gravitational darkening on the determination of fundamental parameters in fast-rotating B-type stars", Astronomy and Astrophysics, 440 (1): 305–320, Bibcode:2005A&A...440..305F, arXiv:astro-ph/0503381 , doi:10.1051/0004-6361:20042229.
- ↑ "tet Cir -- Be Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2017-01-18.
- ↑ Mason, Brian D.; et al. (July 1997), "A Speckle Survey of Southern Be Stars", Be Star Newsletter, 32: 9−10, Bibcode:1997BeSN...32....9M.
- ↑ Adelman, S. J.; et al. (December 2000), "On the Variability of O4-B5 Luminosity Class III-V Stars", Information Bulletin on Variable Stars (5008): 1, Bibcode:2000IBVS.5008....1A.
External links
- http://server3.wikisky.org/starview?object_type=1&object_id=2046
- http://varsao.com.ar/Curva_theta_Cir.htm (light curve)