TOI-2374 is 439 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 5,002 K star; the first was found in 2024 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-2374 b goes round its star every 4.31 days, 20 times as often as Mercury goes round the Sun.
TOI-2374 is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.
| Surface temperature | 5,002 K |
| Mass | 0.802 solar masses |
| Radius | 0.711 solar radii |
| Luminosity | 0.285 times the Sun |
| Apparent magnitude | 12.095 |
| Age | about 4.5 billion years |
| Distance from the Sun | 439.2 light-years (134.7 parsecs) |
| Position (J2000) | RA 319.4982°, Dec -22.0498° |
| Constellation | Capricornus |
TOI-2374 A is a G1V star of magnitude 9.34, moving through space with it. In 2016 it was 22.3″ from TOI-2374, at position angle 47° (Washington Double Star Catalog, 21180-2203 RSS 558): 3,003 AU on the sky at this distance. The true distance can only be larger.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-2374 b | 4.31 days | 0.0482 AU | 7.4876 R⊕ | 61.659 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 5,002 K, 0.28 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.53 to 0.96 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 439 years ago, around 1590.