Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydra |
Right ascension | 08h 22m 49.95277s[2] |
Declination | +01° 51′ 33.5522″[2] |
Apparent magnitude (V) | 8.66-8.77[3] |
Characteristics | |
Evolutionary stage | main sequence |
Spectral type | G1/2V[4] |
B−V color index | 0.59[5] |
Variable type | BY Dra[3] |
Astrometry | |
Radial velocity (Rv) | 20.16±0.22[2] km/s |
Proper motion (μ) | RA: −51.362±0.017 mas/yr[2] Dec.: −49.047±0.013 mas/yr[2] |
Parallax (π) | 16.9267 ± 0.0168 mas[2] |
Distance | 192.7 ± 0.2 ly (59.08 ± 0.06 pc) |
Absolute magnitude (MV) | +0.4[6] |
Details | |
Mass | 1.0±0.1[6] M☉ |
Radius | 0.98+0.01 −0.03[7] R☉ |
Luminosity | 0.998±0.004[7] L☉ |
Surface gravity (log g) | 4.59±0.10[6] cgs |
Temperature | 5,837+80 −51[7] K |
Metallicity [Fe/H] | −0.18±0.20[6] dex |
Rotation | 3.296 days[6] |
Rotational velocity (v sin i) | 14.7±1.0[6] km/s |
Age | 2.3±2.1[8] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 70573 is a variable star in the equatorial constellation of Hydra. At a mean apparent visual magnitude of +8.7, this yellow-hued star is too dim to be visible to the naked eye. Based upon parallax measurements, it is located at a distance of 193 light years from the Sun, and is drifting further away with a radial velocity of 20.5 km/s. It is a candidate member of the proposed Hercules-Lyra Association of co-moving stars,[5] although this membership is disputed.[10]
This is a G-type main-sequence star with a stellar classification of G1/2V.[4] It is a BY Draconis variable that ranges in brightness from magnitude 8.66 down to 8.77 with a rotationally-modulated period of 3.296 days.[3] HD 70573 is generally considered to be a young star although estimates of its age vary from 60[11] million years to several billion years.[8] It has a projected rotational velocity of 15 km/s[6] and about the same mass, size, and luminosity as the Sun.
MAST
was invoked but never defined (see the help page).GaiaDR3
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