Kepler-186 c

Planet· orbits Kepler-186

Kepler-186 c — a super-Earth (1.25 Earth radii) on a 7-day orbit. Its size is measured; its mass is size-estimated, so no density is quoted. Warm and probably rocky. Never imaged.

Open in 3D viewSee Kepler-186 c in the live, interactive 3D map

Key facts

Radius
7,964 km
1.25× wider than Earth
Year
7.27 Earth days
Distance from Kepler-186
6,746,864 km

Science

Physical

Radius
7,964 km · 1.25× wider than Earth

Orbital

Semi-major axis
6,746,864 km
From the NASA Exoplanet Archive (transit + orbit fit)
Eccentricity
0
From the NASA Exoplanet Archive (transit + orbit fit)
Inclination
0.00 °
From the NASA Exoplanet Archive (transit + orbit fit)
Orbital period
7.3 days
From the NASA Exoplanet Archive (transit + orbit fit)
Perihelion
6,746,864 km
Computed from the orbital elements
Aphelion
6,746,864 km
Computed from the orbital elements
Mean orbital velocity
67.5 km/s
Computed from the orbital elements

Composition

Bulk composition
A super-Earth (1.25 Earth radii); its size is measured, its mass only size-estimated, so no density is quoted. Warm and probably rocky. Never imaged.
Surface appearance
Appearance based on NASA/JPL-Caltech'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
20.3 S⊕ · 20.3× the sunlight Earth receives
Computed from Kepler-186's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
464 K (191 °C)
Computed model value for its 7-day orbit — not measured.

Discovery & history

Method
Transit detection
Name
Designated 'c' under the IAU convention that letters a star's planets 'b', 'c', 'd'... in the order they are found (the star is the unwritten 'a'); no IAU proper name has been assigned.

One of the four confirmed inner planets of Kepler-186 (2014).

Images

No telescope has imaged this world — it is known only from the tiny dip it makes crossing its star. Only its host system has been pictured (see the system view); its true surface appearance is unknown.