OGLE-2019-BLG-0468L is 14,351 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this G star; the first was found in 2022 by microlensing (OGLE).
Fly there in 3DOGLE-2019-BLG-0468L c was found by microlensing: its star briefly magnified the light of a more distant one. That alignment happens once, so the planet cannot be watched again this way.
Where the archive gives only a period or only an orbit size, the other is worked out from Kepler’s third law with the star’s mass.
| Spectral type | G |
| Mass | 0.92 solar masses |
| Distance from the Sun | 14351.0 light-years (4400.0 parsecs) |
| Position (J2000) | RA 266.4060°, Dec -24.4473° |
| Constellation | Sagittarius |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| OGLE-2019-BLG-0468L c | 4.8 years from Kepler’s law | 2.770 AU | 12.5 R⊕ estimated | 3248.2 M⊕ | Microlensing, 2022 |
| OGLE-2019-BLG-0468L b | 6.2 years from Kepler’s law | 3.290 AU | 13.1 R⊕ estimated | 1090.2 M⊕ | Microlensing, 2022 |
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.