OGLE-TR-111 is 3,484 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this K2 V star; the first was found in 2004 by transit (OGLE).
Fly there in 3DOGLE-TR-111 b goes round its star every 4.01 days, 22 times as often as Mercury goes round the Sun.
| Spectral type | K2 V |
| Surface temperature | 5,040 K |
| Mass | 0.82 solar masses |
| Radius | 0.83 solar radii |
| Luminosity | 0.4585 times the Sun |
| Apparent magnitude | 16.707 |
| Age | about 8.8 billion years |
| Distance from the Sun | 3484.4 light-years (1068.3 parsecs) |
| Position (J2000) | RA 163.3241°, Dec -61.4057° |
| Constellation | Carina |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| OGLE-TR-111 b | 4.01 days | 0.0473 AU | 11.422 R⊕ | 174.8 M⊕ | Transit, 2004 |
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 5,040 K, 0.46 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.67 to 1.21 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 3,484 years ago, around 1500 BC.