DMPP-2 is 450 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this F5 V star; the first was found in 2019 by radial velocity (Multiple Facilities).
Fly there in 3DDMPP-2 c goes round its star every 3.17 days, 28 times as often as Mercury goes round the Sun.
| Spectral type | F5 V |
| Surface temperature | 6,500 K |
| Mass | 1.41 solar masses |
| Radius | 1.78 solar radii |
| Luminosity | 1.27 times the Sun |
| Apparent magnitude | 8.57 |
| Age | about 2 billion years |
| Distance from the Sun | 449.9 light-years (137.9 parsecs) |
| Position (J2000) | RA 27.4077°, Dec -34.4591° |
| Constellation | Fornax |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| DMPP-2 c | 3.17 days | 0.0479 AU | 8.26 R⊕ estimated | 51.79 M⊕ minimum | Radial Velocity, 2026 |
| DMPP-2 b | 5.20 days | 0.0664 AU | 14.2 R⊕ estimated | 171.48 M⊕ minimum | Radial Velocity, 2019 |
| DMPP-2 d | 16.5 days | 0.143 AU | 11.6 R⊕ estimated | 91.79 M⊕ minimum | Radial Velocity, 2026 |
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 6,500 K, 1.3 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.03 to 1.78 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 450 years ago, around 1580.