YZ Ceti c

Planet· orbits YZ Ceti

YZ Ceti c - the middle planet of YZ Ceti (minimum mass ~1.1 Earth), on a 3-day orbit. Never imaged.

Open in 3D viewSee YZ Ceti c in the live, interactive 3D map

Key facts

Minimum mass
6.81 × 10²⁴ kg
1.14 M⊕
Year
3.06 Earth days
Distance from YZ Ceti
3,231,314 km

Science

Physical

Minimum mass (m·sin i)
6.81 × 10²⁴ kg · 1.14 M⊕
Radial-velocity detection measures m·sin i; the true mass depends on the unknown orbital inclination.
Radius
Not measured
No transit — radius is a model estimate; true size unknown.

Orbital

Semi-major axis
3,231,314 km
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
3.1 days
From the NASA Exoplanet Archive (radial-velocity orbit)
Perihelion
3,231,314 km
Computed from the orbital elements
Aphelion
3,231,314 km
Computed from the orbital elements
Mean orbital velocity
76.8 km/s
Computed from the orbital elements

Composition

Bulk composition
Presumed rocky (minimum mass ~1.1 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
4.72 S⊕ · 4.72× the sunlight Earth receives
Computed from YZ Ceti's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
410 K (137 °C)
Computed model value — not measured.

Discovery & history

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

The second of three planets found by HARPS in 2017.

Images

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