HD 93385
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vela |
Right ascension | 10h 46m 15.1160s[1] |
Declination | –41° 27′ 51.7261″[1] |
Apparent magnitude (V) | 7.486[2] |
Characteristics | |
Spectral type | G2/G3 V[3] |
B−V color index | 0.595[4] |
Astrometry | |
Radial velocity (Rv) | +47.80 ± 0.61[5] km/s |
Proper motion (μ) | RA: −48.197±0.045[1] mas/yr Dec.: −54.727±0.043[1] mas/yr |
Parallax (π) | 23.0405 ± 0.0342[1] mas |
Distance | 141.6 ± 0.2 ly (43.40 ± 0.06 pc) |
Details | |
Mass | 1.07[4] M☉ |
Radius | 1.17[6] R☉ |
Luminosity | 1.42[6] L☉ |
Surface gravity (log g) | 4.08 ± 0.11[6] cgs |
Temperature | 5,823 ± 35[6] K |
Metallicity [Fe/H] | –0.05 ± 0.03[6] dex |
Age | 4.13[4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 93385 is a star in the southern constellation of Vela. At an apparent visual magnitude of 7.5,[2] it is too faint to be seen with the unaided eye. Parallax measurements made using the Gaia spacecraft show an annual shift of 23.04 milli-arcseconds. This is equivalent to a physical separation of around 142[1] light years from the Sun.
This is an ordinary main sequence star with a stellar classification of G2/G3 V.[3] The physical properties of HD 93385 are similar to those of the Sun; it is slightly larger with 107%[4] of the Sun's mass, 117% of the radius, and 142% of the luminosity. The abundance of elements, other than hydrogen and helium, is nearly the same as in the Sun.[6] It is currently at an unusual low level of surface activity and thus is a candidate Maunder minimum analog.[4]
A physical companion star with an apparent visual magnitude of 12.29 is located at an angular separation of 10.32 arcseconds (equivalent to projected separation of 448 AU) along a position angle of 288°. It is estimated to have 45% of the mass of the Sun.[8]
The survey in 2015 have ruled out the existence of any additional stellar companions at projected distances from 12 to 352 astronomical units.[9]
Planetary system[]
This star hosts two close-orbiting, super-Earth-like planets, suspected since 2011 and confirmed in 2021.[10][11] The first has 8.3 times the mass of the Earth and an orbital period of 13.186 days. The second is 10.1 times the Earth's mass with a period of 46.025 days.[12] The third planet candidate on innermost orbit was discovered in 2017[13] and confirmed in 2021.[11]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
≥4.2[11] M |