TOI-2095 is 137 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this M2.5 V star; the first was found in 2023 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-2095 b goes round its star every 17.7 days, 5 times as often as Mercury goes round the Sun.
| Spectral type | M2.5 V |
| Surface temperature | 3,759 K |
| Mass | 0.44 solar masses |
| Radius | 0.44 solar radii |
| Luminosity | 0.03476 times the Sun |
| Apparent magnitude | 13.19 |
| Age | about 1 billion years |
| Distance from the Sun | 136.7 light-years (41.9 parsecs) |
| Position (J2000) | RA 285.6365°, Dec 75.4185° |
| Constellation | Draco |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-2095 b | 17.7 days | 0.101 AU | 1.25 R⊕ | 4.1 M⊕ | Transit, 2023 |
| TOI-2095 c | 28.2 days | 0.137 AU | 1.33 R⊕ | 7.4 M⊕ | Transit, 2023 |
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 3,759 K, 0.035 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.19 to 0.37 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 137 years ago, around 1890.