GJ 3341 is 77.0 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this M2.5 star; the first was found in 2015 by radial velocity (La Silla Observatory).
Fly there in 3DGJ 3341 b goes round its star every 14.2 days, 6 times as often as Mercury goes round the Sun.
| Spectral type | M2.5 |
| Surface temperature | 3,526 K |
| Mass | 0.47 solar masses |
| Radius | 0.439 solar radii |
| Luminosity | 0.02897 times the Sun |
| Apparent magnitude | 12.062 |
| Distance from the Sun | 77.0 light-years (23.6 parsecs) |
| Position (J2000) | RA 78.9471°, Dec -31.2948° |
| Constellation | Columba |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| GJ 3341 b | 14.2 days | 0.0890 AU | 2.46 R⊕ estimated | 6.6 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 3,526 K, 0.029 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.18 to 0.34 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 77 years ago, within living memory.