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HD 94890 planetary system

HD 94890 is an orange main-sequence star of spectral type K0 III approximately 201 light-years from Earth (61.70 parsecs). It hosts 2 confirmed exoplanets.

Host star

Name
HD 94890
Spectral type
K0 III
Effective temperature
4,867 K
Mass
1.74 M☉ (solar masses)
Radius
10.71 R☉ (solar radii)
Distance
61.70 pc (201 ly)
Hipparcos catalog
HIP 53502

Confirmed planets (2)

Planet Class Mass (M⊕) Radius (R⊕) Period (d) Distance (AU) Eq. temp (K) Discovered
HD 94890 b Neptune-like 676.97 13.30 824.61 2.0700 2025
HD 94890 c Neptune-like 2831.85 12.50 2492.19 4.3300 2025

The planets in detail

HD 94890 b is a Neptune-like world with about 13.30 Earth radii and 676.97 Earth masses. It orbits HD 94890 at 2.0700 AU with a 2.3-Earth-year orbit, and no published equilibrium temperature. Its orbit is notably eccentric (e = 0.22), meaning the distance to its star — and the irradiation it receives — varies substantially over each year. It was confirmed in 2025 via radial velocity (Doppler) measurements.

HD 94890 c is a Neptune-like world with about 12.50 Earth radii and 2831.85 Earth masses. It orbits HD 94890 at 4.3300 AU with a 6.8-Earth-year orbit, and no published equilibrium temperature. It was confirmed in 2025 via radial velocity (Doppler) measurements.

Discovery

All 2 planets in the HD 94890 system were detected in 2025 using radial velocity (Doppler) measurements. Detection facilities: La Silla Observatory.

Observing from Earth

Exoplanets cannot be resolved visually with amateur telescopes — the host star's glare is overwhelming and even space-based direct imaging requires sophisticated coronagraphs. What you can observe is the host star itself at right ascension 164.1798°, declination -37.1383°. Use the 3D orrery above to inspect orbital geometry, planetary scale, and the habitable-zone overlay — the orbits are computed from the published Keplerian elements and animate at user-controlled time rates.