HD 93385 is 141 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this G2/G3 V star; the first was found in 2021 by radial velocity (La Silla Observatory).
Fly there in 3DHD 93385 b goes round its star every 7.34 days, 12 times as often as Mercury goes round the Sun.
| Spectral type | G2/G3 V |
| Surface temperature | 5,977 K |
| Mass | 1.04 solar masses |
| Radius | 1.18484 solar radii |
| Luminosity | 1.61 times the Sun |
| Apparent magnitude | 7.49 |
| Age | about 3.3 billion years |
| Distance from the Sun | 141.4 light-years (43.3 parsecs) |
| Position (J2000) | RA 161.5627°, Dec -41.4646° |
| Constellation | Vela |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 93385 b | 7.34 days | 0.0756 AU | 1.88 R⊕ estimated | 4.2 M⊕ minimum | Radial Velocity, 2021 |
| HD 93385 c | 13.2 days | 0.112 AU | 2.56 R⊕ estimated | 7.1 M⊕ minimum | Radial Velocity, 2021 |
| HD 93385 d | 45.9 days | 0.257 AU | 2.89 R⊕ estimated | 8.7 M⊕ minimum | Radial Velocity, 2021 |
Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.