OGLE-TR-132 is 6,564 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this F5 V star; the first was found in 2004 by transit (OGLE).
Fly there in 3DOGLE-TR-132 b goes round its star every 40.6 hours, 52 times as often as Mercury goes round the Sun.
| Spectral type | F5 V |
| Surface temperature | 6,210 K |
| Mass | 1.305 solar masses |
| Radius | 1.32 solar radii |
| Luminosity | 2.35 times the Sun |
| Apparent magnitude | 16.536 |
| Age | about 1.2 billion years |
| Distance from the Sun | 6564.3 light-years (2012.6 parsecs) |
| Position (J2000) | RA 162.6441°, Dec -61.9572° |
| Constellation | Carina |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| OGLE-TR-132 b | 40.6 hours | 0.0303 AU | 13.45 R⊕ | 375.02 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 6,210 K, 2.4 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.42 to 2.48 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 6,564 years ago, around 4500 BC.