HIP 27435 is a yellow main-sequence star that is 49 light years away with one planet that is about twice the mass of Uranus and orbits in the star's habitable zone
| Observation data Epoch J2000.0 Equinox J2000.0 |
|
|---|---|
| Constellation | Orion |
| Right ascension | 05h 48m 34.93996s[1] |
| Declination | −04° 05′ 40.7153″[1] |
| Apparent magnitude (V) | +5.97[2] |
| Characteristics | |
| Spectral type | G4V[3] |
| U−B color index | +0.10[2] |
| B−V color index | +0.64[2] |
| Astrometry | |
| Radial velocity (Rv) | +31.2[4] km/s |
| Proper motion (μ) | RA: 60.84 ± 0.41[1] mas/yr Dec.: –228.35 ± 0.33[1] mas/yr |
| Parallax (π) | 65.89 ± 0.41[1] mas |
| Distance | 49.5 ± 0.3 ly (15.18 ± 0.09 pc) |
| Details | |
| Mass | 0.886[5] M☉ |
| Radius | 0.9331 ± 0.0162[5] R☉ |
| Luminosity | 0.7943 ± 0.0101[5] L☉ |
| Surface gravity (log g) | 4.36 ± 0.06[3] cgs |
| Temperature | 5,660 ± 20[3] K |
| Metallicity [Fe/H] | –0.27 ± 0.03[3] dex |
| Rotational velocity(v sin i) | 2.61[6] km/s |
| Age | 6.2[7] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
| Extrasolar Planets Encyclopaedia |
data |
Some Early scans
These were falsified quickly as local carriers. They contain SML for identification.
