Teegarden's Star b

Planet· orbits Teegarden's Star

Teegarden's Star b - a temperate planet (minimum mass ~1.1 Earth) on a 4.9-day orbit; one of the most Earth-like worlds by mass and temperature yet found. Never imaged.

Open in 3D viewSee Teegarden's Star b in the live, interactive 3D map

Key facts

Minimum mass
6.93 × 10²⁴ kg
1.16 M⊕
Year
4.91 Earth days
Distance from Teegarden's Star
3,874,585 km

Science

Physical

Minimum mass (m·sin i)
6.93 × 10²⁴ kg · 1.16 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
3,874,585 km
From the NASA Exoplanet Archive (radial-velocity orbit)
Eccentricity
0.03
From the NASA Exoplanet Archive (radial-velocity orbit)
Inclination
0.00 °
From the NASA Exoplanet Archive (radial-velocity orbit)
Orbital period
4.9 days
From the NASA Exoplanet Archive (radial-velocity orbit)
Perihelion
3,758,347 km
Computed from the orbital elements
Aphelion
3,990,822 km
Computed from the orbital elements
Mean orbital velocity
57.4 km/s
Computed from the orbital elements

Composition

Bulk composition
Presumed rocky (minimum mass ~1.2 Earth), in the habitable zone; 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
1.09 S⊕ · 1.09× the sunlight Earth receives
Computed from Teegarden's Star's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
277 K (4 °C)
Computed model value — near Earth's, but 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'.

One of two planets announced in 2019 from CARMENES radial velocities - the inner, and among the highest-rated for potential habitability.

Images

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