Gas giant · HD 94890
HD 94890 b
ExoplanetsDiscovered 2025
Scientific overview
HD 94890 b is a gas giant orbiting HD 94890, completing an orbit every 825 days, about 201 light-years from Earth. It was discovered in 2025 using the radial velocity method.
Host star
Planetary system — HD 94890 system
View the HD 94890 system (2 known planets).
| Planet | Class | Radius (R⊕) | Period (d) | Distance (ly) |
|---|---|---|---|---|
| HD 94890 bRadial Velocity · 2025 | Gas giant | 13.3 | 825 | 201 |
| HD 94890 cRadial Velocity · 2025 | Gas giant | 12.5 | 2492 | 201 |
Discovery and detection
Knowledge connections
- OrbitsIota Antliae
- Member of systemHD 94890 system
- Discovered by methodRadial Velocity Method
- Discovered atLa Silla Observatory
- Catalogued inNASA Exoplanet Archive