HD 94890 c · Asteria Star

Scientific overview

HD 94890 c is a gas giant orbiting HD 94890, completing an orbit every 2492 days, about 201 light-years from Earth. It was discovered in 2025 using the radial velocity method.

Host star

Iota Antliae

Spectral type

K0 III

Temperature

4,867 K

Mass

1.74 M☉

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

Detection method

Radial Velocity Method

Discovery year

2025

Discovered at

La Silla Observatory

Knowledge connections

OrbitsIota Antliae
Member of systemHD 94890 system
Discovered by methodRadial Velocity Method
Discovered atLa Silla Observatory
Catalogued inNASA Exoplanet Archive

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