TOI-6884 is 1,834 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,330 K star; the first was found in 2026 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-6884 b goes round its star every 4.81 days, 18 times as often as Mercury goes round the Sun.
| Surface temperature | 6,330 K |
| Mass | 1.41 solar masses |
| Radius | 1.84 solar radii |
| Luminosity | 4.91 times the Sun |
| Apparent magnitude | 11.985 |
| Age | about 2.61 billion years |
| Distance from the Sun | 1834.2 light-years (562.4 parsecs) |
| Position (J2000) | RA 193.0088°, Dec 26.6740° |
| Constellation | Coma Berenices |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-6884 b | 4.81 days | 0.0629 AU | 10.391 R⊕ | 8365.2 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 6,330 K, 4.9 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 2.04 to 3.55 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 1,834 years ago, around AD 190.