HD 67087 is 250 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this F8 V star; the first was found in 2015 by radial velocity (Multiple Observatories).
Fly there in 3DHD 67087 c takes 6.5 years to go round its star once.
| Spectral type | F8 V |
| Surface temperature | 6,330 K |
| Mass | 1.36 solar masses |
| Radius | 1.55 solar radii |
| Luminosity | 3.467 times the Sun |
| Apparent magnitude | 8.05 |
| Age | about 1.45 billion years |
| Distance from the Sun | 249.6 light-years (76.5 parsecs) |
| Position (J2000) | RA 121.9156°, Dec 31.5512° |
| Constellation | Gemini |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 67087 b | 352.2 days | 1.080 AU | 13.1 R⊕ estimated | 973 M⊕ minimum | Radial Velocity, 2015 |
| HD 67087 c | 6.5 years | 3.860 AU | 12.9 R⊕ estimated | 1540 M⊕ minimum | Radial Velocity, 2015 |
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.
For a star of 6,330 K, 3.5 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.71 to 2.98 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.
The light you see left 250 years ago, around 1780.