Gamma Doradus
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]
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 | |
Database references | |
SIMBAD | data |
References
- V* gam Dor -- Variable Star of gamma Dor type, database entry, SIMBAD. Accessed on line November 17, 2008.
- 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, Bibcode: 1999PASP..111..840K.
- 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.
- Gamma Dor Archived 2008-07-04 at the Wayback Machine, Jim Kaler, Stars. Accessed on line November 17, 2008.
- 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, Bibcode: 1994MNRAS.270..905B.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.