Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Corona Australis |
Right ascension | 18h 49m 34.99649s[1] |
Declination | −43° 26′ 02.7522″[1] |
Apparent magnitude (V) | 5.59±0.01[2] |
Characteristics | |
Evolutionary stage | main sequence star[3] |
Spectral type | B9 IV[4] |
B−V color index | −0.08[5] |
Astrometry | |
Radial velocity (Rv) | −23.0±4.3[6] km/s |
Proper motion (μ) | RA: −2.963 mas/yr[1] Dec.: −25.374 mas/yr[1] |
Parallax (π) | 4.25 ± 0.1158 mas[1] |
Distance | 770 ± 20 ly (235 ± 6 pc) |
Absolute magnitude (MV) | −0.24[7] |
Details | |
Mass | 3.23±0.08[3] M☉ |
Radius | 5.82±0.31[8] R☉ |
Luminosity | 171+20 −18[3] L☉ |
Surface gravity (log g) | 3.47[9] cgs |
Temperature | 10,940±255[3] K |
Metallicity [Fe/H] | +0.06[9] dex |
Rotational velocity (v sin i) | 30[10] km/s |
Age | 213[11] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Eta2 Coronae Australis (Eta2 CrA), Latinized from η2 Coronae Australis, is a solitary star[14] located in the southern constellation of Corona Australis. It is visible to the naked eye as a dim, blue-white hued star with an apparent visual magnitude of 5.59.[2] Gaia DR3 parallax measurements imply a distance of 770 light years from the Solar System,[1] but it is drifting closer with a radial velocity of −23 km/s.[6] At its current distance Eta2 CrA's brightness is diminished by 0.27 magnitudes due to stellar extinction from interstellar dust[15] and it has an absolute magnitude of −0.24.[7]
This object has a stellar classification of B9 IV,[4] indicating that is a slightly evolved a B-type subgiant star. However, Zorec & Royer (2012) model it to be a dwarf star that has completed 80.4% of its main sequence lifetime.[3] It is estimated to be 213 million years old[11] and it has a mass that is 3.23 times that of the Sun.[3] The star is radiating 171 times the luminosity of the Sun[3] from its photosphere 5.82 times the radius of the Sun[8] at an effective temperature of 10,940 K.[3] Eta2 CrA has a near-solar metallicity at [Fe/H] = +0.06[9] and spins modestly with a projected rotational velocity of 30 km/s.[10] Some earlier catalogues listed the object as a chemically peculiar star but that status is now considered to be doubtful.[16]
GaiaDR3
was invoked but never defined (see the help page).Tycho2000
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