Lacaille 9352 b

Planet· orbits Lacaille 9352

Lacaille 9352 b — a hot super-Earth (minimum mass ~3.9 Earth) on a 9.3-day orbit, one of the first two planets found here. Too hot for liquid water; never imaged.

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

Key facts

Minimum mass
2.33 × 10²⁵ kg
3.9 M⊕
Year
9.26 Earth days
Distance from Lacaille 9352
10,217,535 km

Science

Physical

Minimum mass (m·sin i)
2.33 × 10²⁵ kg · 3.9 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
10,217,535 km
From the NASA Exoplanet Archive (radial-velocity orbit)
Eccentricity
0.14
From the NASA Exoplanet Archive (radial-velocity orbit)
Inclination
0.00 °
From the NASA Exoplanet Archive (radial-velocity orbit)
Orbital period
9.3 days
From the NASA Exoplanet Archive (radial-velocity orbit)
Perihelion
8,787,080 km
Computed from the orbital elements
Aphelion
11,647,989 km
Computed from the orbital elements
Mean orbital velocity
80.2 km/s
Computed from the orbital elements

Composition

Bulk composition
Presumed rocky/super-Earth (minimum mass ~3.9 Earth); never imaged.
Surface appearance
Appearance based on ESO/M. Kornmesser's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The surface shown is an artistic representation, shown only in Visual mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
7.89 S⊕ · 7.89× the sunlight Earth receives
Computed from Lacaille 9352's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
426 K (153 °C)
Computed model value (no atmosphere assumed) — not measured.

Discovery & history

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

Announced in 2020 by the RedDots team from HARPS radial velocities — one of the closest transiting-search targets, though it has not been seen to transit.

Images

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