The star
The star
UKIRT-2017-BLG-001L
- Type
- star
- Mass
- 0.81 × the Sun
The planets
UKIRT-2017-BLG-001L
UKIRT-2017-BLG-001L b
- Year
- 9.5 years
- Distance from star
- 4.18 AU
- Mass
- 1.3 Jupiters
- Size
- 14 × Earth
- Found
- 2018, microlensing (Mauna Kea Observatory)
Masses found by the wobble method are minimums, because the orbit's tilt is unknown. Temperatures are equilibrium estimates for a bare planet, before any atmosphere.
How we know
A lens in space
The system briefly magnified a more distant star; a planet left its own small blip in the brightening.
Sources
- Planet and star parameters: NASA Exoplanet Archive, Planetary Systems Composite Parameters, retrieved 1 Nov 2026. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with NASA under the Exoplanet Exploration Program.
- Position: HYG Database v4.1 (CC BY-SA 4.0).
- Habitable zone: a simple estimate from the star's brightness (√L × 0.95 to 1.67 AU), shown as a guide.