HIP 67522 is 415 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this G1 V star; the first was found in 2020 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DHIP 67522 b goes round its star every 6.96 days, 13 times as often as Mercury goes round the Sun.
| Spectral type | G1 V |
| Surface temperature | 5,675 K |
| Mass | 1.22 solar masses |
| Radius | 1.38 solar radii |
| Luminosity | 1.75 times the Sun |
| Apparent magnitude | 9.79 |
| Age | about 0.017 billion years |
| Distance from the Sun | 415.1 light-years (127.3 parsecs) |
| Position (J2000) | RA 207.5260°, Dec -40.8359° |
| Constellation | Centaurus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HIP 67522 b | 6.96 days | 0.0748 AU | 9.9872 R⊕ | 13.8 M⊕ | Transit, 2020 |
| HIP 67522 c | 14.3 days | 0.123 AU | 7.936 R⊕ | 22 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.