HD 69830 is 41.0 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this K0V star; the first was found in 2006 by radial velocity (La Silla Observatory).
Fly there in 3DHD 69830 b goes round its star every 8.67 days, 10 times as often as Mercury goes round the Sun.
| Spectral type | K0V |
| Surface temperature | 5,385 K |
| Mass | 0.86 solar masses |
| Radius | 0.886947 solar radii |
| Luminosity | 0.6026 times the Sun |
| Apparent magnitude | 5.96004 |
| Age | about 7 billion years |
| Distance from the Sun | 41.0 light-years (12.6 parsecs) |
| Position (J2000) | RA 124.6010°, Dec -12.6364° |
| Constellation | Puppis |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 69830 b | 8.67 days | 0.0785 AU | 3.17 R⊕ estimated | 10.2 M⊕ minimum | Radial Velocity, 2006 |
| HD 69830 c | 31.6 days | 0.186 AU | 3.46 R⊕ estimated | 11.8 M⊕ minimum | Radial Velocity, 2006 |
| HD 69830 d | 197.0 days | 0.630 AU | 4.45 R⊕ estimated | 18.1 M⊕ minimum | Radial Velocity, 2006 |
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.