HD 202772 A is 527 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,442 K star; the first was found in 2019 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DHD 202772 A b goes round its star every 3.31 days, 27 times as often as Mercury goes round the Sun.
HD 202772 A 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 | 6,442 K |
| Mass | 1.721 solar masses |
| Radius | 2.554 solar radii |
| Luminosity | 10.22 times the Sun |
| Apparent magnitude | 8.324 |
| Age | about 1.63 billion years |
| Distance from the Sun | 526.7 light-years (161.5 parsecs) |
| Position (J2000) | RA 319.6996°, Dec -26.6164° |
| Constellation | Capricornus |
HD 202772 B has no spectral type listed of magnitude 10.21, moving through space with it. In 2019 it was 1.3″ from HD 202772 A, at position angle 295° (Washington Double Star Catalog, 21188-2637 SEE 443): 210 AU on the sky at this distance. The true distance can only be larger. Its colour is estimated from its brightness.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 202772 A b | 3.31 days | 0.0521 AU | 18.237 R⊕ | 323.55 M⊕ | Transit, 2019 |
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.