Menu
9.9 h/s
Lade Planeten…
Sonnensystem-Planetarium
Links ziehen zum Drehen Rechts ziehen zum Verschieben Scrollen zum Zoomen Planet anklicken zum Folgen Space Zeit abspielen / pausieren Ansichten & Touren oben rechts Umlaufbahnen sind komprimiert — aktiviere „Wahrer Maßstab“ in den Einstellungen für echte Proportionen
Planet antippen für Details Ziehen zum Drehen Zusammenziehen zum Zoomen Mit zwei Fingern ziehen zum Verschieben
Planet anklicken für Details. Ziehen zum Drehen, Scrollen zum Zoomen. Planet antippen für Details. Zusammenziehen zum Zoomen.
  Richte dein Handy auf den Himmel!

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.