OGLE-TR-10 is 4,387 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G2 V star; the first was found in 2004 by transit (OGLE).
Fly there in 3DOGLE-TR-10 b goes round its star every 3.10 days, 28 times as often as Mercury goes round the Sun.
| Spectral type | G2 V |
| Surface temperature | 5,950 K |
| Mass | 1.14 solar masses |
| Radius | 1.17 solar radii |
| Luminosity | 1.542 times the Sun |
| Apparent magnitude | 16.006 |
| Age | about 3.1 billion years |
| Distance from the Sun | 4386.7 light-years (1345.0 parsecs) |
| Position (J2000) | RA 267.8677°, Dec -29.8765° |
| Constellation | Sagittarius |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| OGLE-TR-10 b | 3.10 days | 0.0434 AU | 14.011 R⊕ | 197.05 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 5,950 K, 1.5 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.17 to 2.05 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 4,387 years ago, around 2400 BC.