Lacaille 9352 d

Planet· orbits Lacaille 9352

Lacaille 9352 d — the outermost of the four (minimum mass ~6.1 Earth) on a 50.8-day orbit, cool enough that it may lie near or beyond the temperate zone. Never imaged.

Open in 3D viewSee Lacaille 9352 d in the live, interactive 3D map

Key facts

Minimum mass
3.64 × 10²⁵ kg
6.1 M⊕
Year
50.77 Earth days
Distance from Lacaille 9352
0.212 AU

Science

Physical

Minimum mass (m·sin i)
3.64 × 10²⁵ kg · 6.1 M⊕
Radial-velocity detection measures m·sin i; the true mass depends on the unknown orbital inclination.
Radius
Not measured
No transit — the radius is a model estimate; true size unknown.

Orbital

Semi-major axis
0.212 AU
From the NASA Exoplanet Archive (radial-velocity orbit)
Eccentricity
0
From the NASA Exoplanet Archive (radial-velocity orbit)
Inclination
0.00 °
From the NASA Exoplanet Archive (radial-velocity orbit)
Orbital period
50.8 days
From the NASA Exoplanet Archive (radial-velocity orbit)
Perihelion
0.212 AU
Computed from the orbital elements
Aphelion
0.212 AU
Computed from the orbital elements
Mean orbital velocity
45.4 km/s
Computed from the orbital elements

Composition

Bulk composition
Cool sub-Neptune or super-Earth (minimum mass ~6.1 Earth); never imaged.
Cloud appearance
Appearance based on ESO/M. Kornmesser's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The banded clouds shown are a representation of its class, shown only in Visual mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
0.819 S⊕ · 82% of the sunlight Earth receives
Computed from Lacaille 9352's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
241 K (-32 °C)
Computed model value (no atmosphere assumed), the coolest of the four — not measured.

Discovery & history

Method
Radial-velocity detection (stellar wobble)
Name
Designated 'd' as the third planet found around its star, following the IAU convention of lettering planets in discovery order from 'b'.

Established in 2026 with planet e as the radial-velocity baseline lengthened, completing the four-planet family (Hartogh et al. 2026).

Images

No official imagery available — this object has never been visited and no officially-licensed depiction exists.