HD 219134 d

Planet· orbits HD 219134

HD 219134 d - a warm, more massive planet (~16 Earth masses) on a 47-day orbit. It does not transit, so its radius is a model estimate and no density is quoted; never imaged.

Open in 3D viewSee HD 219134 d in the live, interactive 3D map

Key facts

Mass
9.66 × 10²⁵ kg
16.2 M⊕
Year
46.74 Earth days
Distance from HD 219134
0.237 AU

Science

Physical

Mass
9.66 × 10²⁵ kg · 16.2 M⊕
Radius
Not measured
Does not transit — radius is a model estimate for a ~16-Earth-mass world, so no density is quoted.

Orbital

Semi-major axis
0.237 AU
From the NASA Exoplanet Archive (radial-velocity orbit)
Eccentricity
0.138
From the NASA Exoplanet Archive (radial-velocity orbit)
Inclination
0.00 °
From the NASA Exoplanet Archive (radial-velocity orbit)
Orbital period
46.7 days
From the NASA Exoplanet Archive (radial-velocity orbit)
Perihelion
0.204 AU
Computed from the orbital elements
Aphelion
0.27 AU
Computed from the orbital elements
Mean orbital velocity
55.2 km/s
Computed from the orbital elements

Composition

Bulk composition
A warm planet of ~16 Earth masses (a dynamical mass, shown plainly); it does not transit, so its size is a model estimate and it has never been 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
4.71 S⊕ · 4.71× the sunlight Earth receives
Computed from HD 219134's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
410 K (137 °C)
Computed model value for its 47-day orbit — not measured.

Discovery & history

Method
Radial-velocity detection (stellar wobble)
Name
Designated 'd' under the IAU convention that letters a star's planets 'b', 'c', 'd'... in the order they are discovered (the star itself is the unwritten 'a').

Part of the planet family announced in 2015 from radial-velocity data.

Images

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