Gamma Doradus

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γ Doradus
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Dorado
Right ascension 04h 16m 01.5857s[1]
Declination −51° 29′ 11.933″[1]
Apparent magnitude (V) 4.25[2]
Characteristics
Spectral type F0V[2]
U−B color index +0.03[3]
B−V color index +0.30[3]
R−I color index +0.16[3]
Variable type Gamma Doradus variable[1]
Astrometry
Radial velocity (Rv) 25.2 ± 2[1] km/s
Proper motion (μ) RA: 100.57[1] mas/yr
Dec.: 184.23[1] mas/yr
Parallax (π) 49.26 ± 0.50[1] mas
Distance 66.2 ± 0.7 ly
(20.3 ± 0.2 pc)
Absolute magnitude (MV) 2.72[2]
Details
Mass 1.57[2] M
Radius 1.70[2] R
Luminosity (bolometric) 7.0[2] L
Temperature 7200[2] K
Metallicity [M/H] = −0.02[2]
Rotational velocity (v sin i) 62[2] km/s
Other designations
γ Dor, Gamma Doradus, Gamma Dor, CD−51 1066, CPD−51 524, FK5 157, GC 5179, GJ 167.1, GJ 9150, HD 27290, HIP 19893, HR 1338, PPM 333343, SAO 233457.[1]
Database references
SIMBAD data

Gamma Doradus (Gamma Dor, γ Doradus, γ Dor) is the third brightest star in the constellation of Dorado.[4] It has an apparent visual magnitude of approximately 4.25 and is a variable star, the type star of the class of Gamma Doradus variables. These stars, like γ Doradus, are pulsating variables which vary in brightness by less than a tenth of a magnitude owing to nonradial gravity wave oscillations.[2] The magnitude of γ Doradus itself has been observed to have two sinusoidal variations with periods of approximately 17.6 and 18.2 hours. There is also some additional unexplained, apparently random fluctuation.[5]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 V* gam Dor -- Variable Star of gamma Dor type, database entry, SIMBAD. Accessed on line November 17, 2008.
  2. 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 2.8 2.9 Gamma Doradus Stars: Defining a New Class of Pulsating Variables, Anthony B. Kaye et al., Publications of the Astronomical Society of the Pacific 111, #761 (July 1999), pp. 840–844, Bibcode1999PASP..111..840K.
  3. 3.0 3.1 3.2 HR 1338, 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 November 17, 2008.
  4. Gamma Dor, Jim Kaler, Stars. Accessed on line November 17, 2008.
  5. γ Doradus: evidence for a new class of pulsating star, L. A. Balona, K. Krisciunas, and A. W. J. Cousins, Monthly Notices of the Royal Astronomical Society 270, #4 (October 15, 1994), pp. 905–913, Bibcode1994MNRAS.270..905B.


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