TOI-4379 is 2,104 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,020 K star; the first was found in 2024 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-4379 b goes round its star every 3.25 days, 27 times as often as Mercury goes round the Sun.
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.
| Surface temperature | 6,020 K |
| Mass | 1.372 solar masses |
| Radius | 1.976 solar radii |
| Luminosity | 4.34 times the Sun |
| Apparent magnitude | 12.661 |
| Age | about 4.51 billion years |
| Distance from the Sun | 2104.2 light-years (645.2 parsecs) |
| Position (J2000) | RA 252.0479°, Dec -32.4338° |
| Constellation | Scorpius |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-4379 b | 3.25 days | 0.0478 AU from Kepler’s law | 16.69 R⊕ | 353.74 M⊕ | Transit, 2024 |
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 6,020 K, 4.3 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.95 to 3.42 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 2,104 years ago, around 100 BC.