OGLE-TR-182 is 8,160 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 5,924 K star; the first was found in 2007 by transit (OGLE).
Fly there in 3DOGLE-TR-182 b goes round its star every 3.98 days, 22 times as often as Mercury goes round the Sun.
| Surface temperature | 5,924 K |
| Mass | 1.14 solar masses |
| Radius | 1.14 solar radii |
| Luminosity | 1.74 times the Sun |
| Apparent magnitude | 16.9195 |
| Age | about 4.3 billion years |
| Distance from the Sun | 8159.6 light-years (2501.7 parsecs) |
| Position (J2000) | RA 167.3279°, Dec -61.0953° |
| Constellation | Carina |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| OGLE-TR-182 b | 3.98 days | 0.0510 AU | 12.666 R⊕ | 321 M⊕ | Transit, 2007 |
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 5,924 K, 1.7 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.24 to 2.18 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 8,160 years ago, around 6100 BC.