TOI-1452 is 99.5 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this M4 +/- 0.5 V star; the first was found in 2022 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1452 b goes round its star every 11.1 days, 8 times as often as Mercury goes round the Sun.
TOI-1452 is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.
| Spectral type | M4 +/- 0.5 V |
| Surface temperature | 3,185 K |
| Mass | 0.249 solar masses |
| Radius | 0.275 solar radii |
| Luminosity | 0.007 times the Sun |
| Apparent magnitude | 14.354 |
| Distance from the Sun | 99.5 light-years (30.5 parsecs) |
| Position (J2000) | RA 290.1740°, Dec 73.1951° |
| Constellation | Draco |
TOI-1452 A is a M4 star of magnitude 12.3, moving through space with it. In 2020 it was 3.1″ from TOI-1452, at position angle 183° (Washington Double Star Catalog, 19207+7312 TOI1452): 94.6 AU on the sky at this distance. The true distance can only be larger.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1452 b | 11.1 days | 0.0610 AU | 1.672 R⊕ | 4.82 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.