Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Corona Australis |
Right ascension | 19h 03m 17.69619s[1] |
Declination | −38° 15′ 11.3335″[1] |
Apparent magnitude (V) | 5.69 to 5.73[2] |
Characteristics | |
Spectral type | F2 III/IV[3] or F0 IIIn[4] |
B−V color index | +0.32[5] |
Variable type | δ Scuti[2] |
Astrometry | |
Radial velocity (Rv) | 4±7.4[6] km/s |
Proper motion (μ) | RA: +12.794 mas/yr[1] Dec.: +14.271 mas/yr[1] |
Parallax (π) | 15.2952 ± 0.0559 mas[1] |
Distance | 213.2 ± 0.8 ly (65.4 ± 0.2 pc) |
Absolute magnitude (MV) | +1.55[7] |
Details | |
Mass | 1.83+0.07 −0.06[8] M☉ |
Radius | 2.85±0.14[9] R☉ |
Luminosity | 17.5+0.2 −0.1[1] L☉ |
Surface gravity (log g) | 3.75±0.12[10] cgs |
Temperature | 7,046±240[11] K |
Metallicity [Fe/H] | −0.21[12] dex |
Rotational velocity (v sin i) | 265[13] km/s |
Age | 1.25[11] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
V701 Coronae Australis (HD 176723; HR 7197; 40 G. Coronae Australis), or simply V701 CrA, is a solitary,[16] yellowish-white hued variable star located in the southern constellation Corona Australis. It has an average apparent magnitude of 5.72,[17] making it faintly visible to the naked eye under ideal conditions. The object is located relatively close at a distance of 213 light-years based on Gaia DR3 parallax measurements,[1] and it is currently receding with a poorly constrained heliocentric radial velocity of 4 km/s.[6] At its current distance, V701 CrA's brightness is diminished by a quarter of a magnitude due to extinction[18] and it has an absolute magnitude of +1.55.[7]
The object was first suspected to be variable in 1990. The variations matched that of δ Scuti variables.[20] Three years later, it was confirmed to be variable and was given the variable star designation V701 Coronae Australis.[21] It ranges from magnitude 5.69 to 5.73[2] within 3.25 hours.[22]
V701 CrA has a stellar classification of F2 III/IV,[3] indicating that it is an evolved F-type star with the blended luminosity class of a subgiant and giant star. It has also been given a class of F0 IIIn,[4] indicating broad or nebulous absorption lines due to rapid rotation. It has 1.83 times the mass of the Sun[8] and a slightly enlarged radius of 2.85 R☉.[9] It radiates 17.5 times the luminosity of the Sun[1] from its photosphere at an effective temperature of 7,046 K.[11] The star spins rapidly with a projected rotational velocity of 265 km/s,[13] which causes it to have an equatorial bulge that is 26% larger than the poles.[23] It is metal deficient with an iron abundance 62% that of the Sun ([Fe/H] = −0.21)[12] and it is estimated to be 1.25 billion years old.[11] V701 CrA was considered to be a chemically peculiar star and was given a class of FpSr. Its peculiarity is now considered to be doubtful.[24]
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