NGTS-39 is 908 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this F9 V star; the first was found in 2026 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DNGTS-39 b goes round its star every 58.2 days, 1.5 times as often as Mercury goes round the Sun.
| Spectral type | F9 V |
| Surface temperature | 6,053 K |
| Mass | 1.16 solar masses |
| Radius | 1.16 solar radii |
| Luminosity | 1.582 times the Sun |
| Apparent magnitude | 11.568 |
| Age | about 2.2 billion years |
| Distance from the Sun | 908.0 light-years (278.4 parsecs) |
| Position (J2000) | RA 109.9387°, Dec 9.9413° |
| Constellation | Canis Minor |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| NGTS-39 b | 58.2 days | 0.308 AU | 12.195 R⊕ | 466.25 M⊕ | Transit, 2026 |
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 6,053 K, 1.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.18 to 2.06 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 908 years ago, around 1120.