GSC 06214-00210 is 354 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this K7 star; the first was found in 2010 by imaging (Palomar Observatory).
Fly there in 3DGSC 06214-00210 b was photographed directly: it is one of the few exoplanets seen as its own point of light rather than inferred from its star.
Where the archive gives only a period or only an orbit size, the other is worked out from Kepler’s third law with the star’s mass.
| Spectral type | K7 |
| Surface temperature | 4,200 K |
| Mass | 0.9 solar masses |
| Radius | 0.90484 solar radii |
| Luminosity | 0.3802 times the Sun |
| Apparent magnitude | 12.416 |
| Age | about 0.005 billion years |
| Distance from the Sun | 353.9 light-years (108.5 parsecs) |
| Position (J2000) | RA 245.4777°, Dec -20.7193° |
| Constellation | Scorpius |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| GSC 06214-00210 b | 6034.2 years from Kepler’s law | 320.000 AU | 20.176 R⊕ | 5000 M⊕ | Imaging, 2010 |
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.