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Epsilon Doradus

From Wikipedia, the free encyclopedia
Star in the constellation Dorado
Epsilon Doradus
Location of ε Doradus (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationDorado
Right ascension05h 49m 53.52107s[1]
Declination−66° 54′ 04.2787″[1]
Apparent magnitude (V)5.11[2]
Characteristics
Spectral typeB6 V[3]
U−Bcolor index−0.49[2]
B−Vcolor index−0.14[2]
Variable typeSPB[4]
Astrometry
Radial velocity (Rv)+15.5±1.6[5] km/s
Proper motion (μ)RA: −21.81[1]mas/yr
Dec.: +37.55[1]mas/yr
Parallax (π)5.68±0.15 mas[1]
Distance570 ± 20 ly
(176 ± 5 pc)
Absolute magnitude (MV)−0.20[6]
Details
Mass4.31±0.05[7] M
Radius3.8±0.6[4] R
Luminosity556[7] L
Surface gravity (log g)3.89±0.20[4] cgs
Temperature13,212[7] K
Rotational velocity (v sin i)17[7] km/s
Age210[6] Myr
Other designations
ε Dor,CD−66°351,Gaia DR2 4659664312127365632,HD 39844,HIP 27534,HR 2064,SAO 249368,2MASS J05495356-6654041[8]
Database references
SIMBADdata

Epsilon Doradus,Latinized from ε Doradus, is a solitary[9] star located in the southernconstellation ofDorado. It is visible to thenaked eye with anapparent visual magnitude of 5.11.[2] Based upon an annualparallax shift of 5.68 mas as measured from Earth, it is located roughly 570 light years from theSun. At that distance, the visual magnitude of the star is diminished by anextinction factor of 0.09 due tointerstellar dust.[6]

This is aB-type main sequence star with astellar classification of B6 V.[3] It is aslowly pulsating B-type star with a mean longitudinalmagnetic field strength of−64±26 G.[4] With 4.31[7] times themass of the Sun and 3.8[4] times theSun's radius, it is about 85% of the way through itsmain sequence lifetime.[7] The star is an estimated 210[6] million years old and is spinning with aprojected rotational velocity of 17 km/s.[7] Epsilon Doradus radiates 556 times thesolar luminosity from itsphotosphere at aneffective temperature of 13,212 K.[7]

References

[edit]
  1. ^abcdevan Leeuwen, F. (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.
  2. ^abcdJohnson, H. L. (1966), "UBVRIJKL Photometry of the Bright Stars",Communications of the Lunar and Planetary Laboratory,4: 99,Bibcode:1966CoLPL...4...99J.
  3. ^abHouk, Nancy (1979),Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,Bibcode:1978mcts.book.....H.
  4. ^abcdeHubrig, S.; et al. (April 2009), "New magnetic field measurements of β Cephei stars and slowly pulsating B stars",Astronomische Nachrichten,330 (4): 317,arXiv:0902.1314,Bibcode:2009AN....330..317H,doi:10.1002/asna.200811187,S2CID 17497112.
  5. ^de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  6. ^abcdGontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars",Astronomy Letters,38 (11):694–706,arXiv:1606.09028,Bibcode:2012AstL...38..694G,doi:10.1134/S1063773712110035,S2CID 119108982.
  7. ^abcdefghZorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  8. ^"eps Dor".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-04-14.
  9. ^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,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
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