Beta Coronae Australis
Template:Location mark Location of β CrA (circled) | |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Corona Australis |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | 4.10±0.01[2] |
| Characteristics | |
| Spectral type | K0 II/III CN1.5[3] |
| U−B Template:Engvar | +1.07[4] |
| B−V Template:Engvar | +1.20[4] |
| R−I Template:Engvar | +0.61[4] |
| Astrometry | |
| Radial velocity (Rv) | 2.7±0.7[5] km/s |
| Proper motion (μ) | RA: +4.37 mas/yr[1] Dec.: −36.65 mas/yr[1] |
| Parallax (π) | 6.88±0.25 mas[1] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | −1.71[6] |
| Details | |
| Mass | 5.17±0.26[7] Template:Solar mass |
| Radius | 38.5±1.9[8] Template:Solar radius |
| Luminosity | 614±33[9] Template:Solar luminosity |
| Surface gravity (log g) | 1.26[10] cgs |
| Temperature | 4,575±55[11] K |
| Metallicity [Fe/H] | +0.24[10] dex |
| Rotational velocity (v sin i) | 6.2±2[12] km/s |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| Template:Odlist[13] | |
| Database references | |
| SIMBAD | data |
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Beta Coronae Australis (Beta CrA), Latinized from β Coronae Australis, is a solitary star[14] located in the southern constellation Corona Australis. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.10.[2] The star is located around 470 light years distant from the Sun based on parallax,[1] and is drifting further away with a radial velocity of Script error: No such module "val"..[5] At its current distance, Beta CrA's brightness is diminished by 0.29 magnitudes due to interstellar dust.[15]
Beta CrA has a stellar classification of K0 II/III CN1.5,[3] indicating that it is an evolved K-type star with the blended luminosity class of a bright giant and a regular giant star. The suffix CN1.5 indicates that the object has an anomalous overabundance of cyano radicals in its spectrum, making it a CN star. Having exhausted the supply of hydrogen at its core, the star has expanded to 39 times the Sun's girth.[9] It has 5.17 times the mass of the Sun shines with a luminosity 614 times that of the Sun[9] from its photosphere at a surface temperature of Script error: No such module "val"..[11] Beta CrA is metal enriched (174% solar iron abundance[10]) and spins modestly with a projected rotational velocity of Script error: No such module "val"..[12]
References
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- ↑ * bet CrA -- Star, database entry, SIMBAD. Accessed on line September 5, 2008.
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