TOI-4137 is 1,093 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,202 K star; the first was found in 2022 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-4137 b goes round its star every 3.80 days, 23 times as often as Mercury goes round the Sun.
| Surface temperature | 6,202 K |
| Mass | 1.313 solar masses |
| Radius | 1.438 solar radii |
| Luminosity | 2.75 times the Sun |
| Apparent magnitude | 11.31 |
| Age | about 2.1 billion years |
| Distance from the Sun | 1092.6 light-years (335.0 parsecs) |
| Position (J2000) | RA 77.6129°, Dec 70.3911° |
| Constellation | Camelopardalis |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-4137 b | 3.80 days | 0.0522 AU | 13.574 R⊕ | 457.67 M⊕ | Transit, 2022 |
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 6,202 K, 2.8 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.54 to 2.68 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 1,093 years ago, around AD 930.