Alpha Doradus
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Dorado |
A | |
Right ascension | 04h 33m 59.778s |
Declination | −55° 02′ 41.91″[1] |
Apparent magnitude (V) | 3.27[2] |
B | |
Right ascension | 04h 33m 59.782s |
Declination | −55° 02′ 42.39″[3] |
Apparent magnitude (V) | 4.3[2] |
Characteristics | |
U−B color index | −0.35[2] |
B−V color index | −0.10[2] |
R−I color index | −0.09[2] |
A | |
Spectral type | A0IIIp[2] |
Variable type | ACV [4] |
B | |
Spectral type | B9IV[2] |
Astrometry | |
A | |
Radial velocity (Rv) | 25.6 ± 0.9[5] km/s |
Proper motion (μ) | RA: 58.06[1] mas/yr Dec.: 12.73[1] mas/yr |
Parallax (π) | 19.34±0.31 mas [6] |
Distance | 169 ± 3 ly (51.7 ± 0.8 pc) |
B | |
Proper motion (μ) | RA: 42.83[3] mas/yr Dec.: 12.94[3] mas/yr |
Orbit [7] | |
Period (P) | 12.1 y |
Semi-major axis (a) | 0.18′′ |
Eccentricity (e) | 0.80 |
Inclination (i) | 31° |
Longitude of the node (Ω) | 140° |
Periastron epoch (T) | B1986 |
Argument of periastron (ω) (secondary) | 193° |
Details | |
A | |
Mass | 3.33 ± 0.10[8] M☉ |
Radius | 3.5 ± 0.3[8] R☉ |
Luminosity (bolometric) | 195[8] L☉ |
Surface gravity (log g) | 4.02 ± 0.07[8] cgs |
Temperature | 11,588[8] K |
Rotation | 2.94 days[8] |
B | |
Mass | 2.7[9] M☉ |
Radius | 1.9[9] R☉ |
Luminosity (bolometric) | 70[9] L☉ |
Temperature | 12,200[9] K |
Other designations | |
α Dor, Alpha Doradus, Alpha Dor, CD−55 916, CPD−55 663, FK5 171, GC 5600, HD 29305, HIP 21281, HR 1465, SAO 233564, PPM 333592, CCDM J04340-5503AB, WDS 04340-5503AB[5] | |
Database references | |
SIMBAD | data |
Alpha Doradus, Latinized from α Doradus, is the brightest star in the southern constellation of Dorado. The distance to this system, as measured using the parallax method, is about 169 light-years (52 parsecs).[6]
This is a binary star system[9] with an overall apparent visual magnitude that varies between 3.26 and 3.30,[4] making this one of the brightest binary stars.[12] The system consists of a subgiant star of spectral type B revolving around a giant star with spectral type A in an eccentric orbit with a period of about 12 years.[2] [7] The orbital separation varies from 2 astronomical units at periastron to 17.5 astronomical units at apastron. The primary, α Doradus A, is a chemically peculiar star whose atmosphere displays an abnormally high abundance of silicon, making this an Si star.[8]
Alpha Doradus has an optical companion, CCDM J04340-5503C, located 77 arcseconds away along a position angle of 94°. It has no physical relation to the other two stars.[2] [13]
References
[edit ]- ^ a b c HIP 21281, record for component 1, Hipparcos catalogue; CDS ID I/239.
- ^ a b c d e f g h i HR 1465, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line September 3, 2008.
- ^ a b c HIP 21281, record for component 2, Hipparcos catalogue; CDS ID I/239.
- ^ a b alf Dor, database entry, The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars Archived 2017年06月20日 at the Wayback Machine, Sternberg Astronomical Institute, Moscow, Russia. Accessed on line September 3, 2008.
- ^ a b V* alf Dor -- Variable Star, database entry, SIMBAD. Accessed on line September 3, 2008.
- ^ a b van Leeuwen, F. (November 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. S2CID 18759600.
- ^ a b "Entry 04340-5503", Sixth Catalog of Orbits of Visual Binary Stars, United States Naval Observatory, archived from the original on 2005年04月24日, retrieved 2008年09月03日
- ^ a b c d e f g North, P. (June 1998), "Do SI stars undergo any rotational braking?", Astronomy and Astrophysics, 334: 181–187, arXiv:astro-ph/9802286 , Bibcode:1998A&A...334..181N
- ^ a b c d e Kaler, James B., Alpha Dor , retrieved 2012年03月04日
- ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
- ^ "alf Dor". The International Variable Star Index. AAVSO. Retrieved 2 July 2022.
- ^ Heintz, W. D. (April 1984), "Note on the orbit of alpha Doradus", The Observatory, 104: 88–89, Bibcode:1984Obs...104...88H
- ^ "Entry 04340-5503, discoverer code HJ3668, components AB-C", The Washington Double Star Catalog, United States Naval Observatory, archived from the original on 2008年04月12日, retrieved 2008年09月03日