Host star — Teegarden's Star
- Spectral type
- M7.0 V
- Temperature
- 3,034 K
- Radius
- 0.12 R☉
- Mass
- 0.10 M☉
- Luminosity
- 0.001 L☉
- Distance
- 3.8 pc (12.5 ly)
Red dwarf — the most common type of star. Cool and small.
Very cool — a faint red dwarf.
Orbits Teegarden's Star · 12.5 light-years from Earth
Teegarden's Star b is a rocky world barely larger than Earth—just 1.05 Earth radii with a similar density—orbiting an ultracool red dwarf only 12.5 light-years away. Its equilibrium temperature of 277 Kelvin (4 degrees Celsius) places it near Earth's average, a genuinely promising sign for habitability. However, the planet circles its tiny host star every 4.91 days at just 0.0259 astronomical units, extremely close and likely causing tidal locking, where one hemisphere perpetually faces the star while the other freezes in darkness. The star itself is remarkably faint and dim, with a surface temperature of only 3,030 Kelvin. Whether liquid water could exist in a stable habitable zone on such a tidally locked world remains uncertain; models disagree on whether atmospheric circulation could redistribute heat from the day side to survival-enabling twilight zones or night side refugia. Despite these unknowns, Teegarden's Star b earned a habitability score of 88 out of 100, making it one of the most Earth-like exoplanets known. Its proximity and discovery via radial velocity—a method that reveals planetary mass directly—make it an exceptional target for future atmospheric studies that might constrain whether habitability is truly possible.
Teegarden's Star b is a rocky world, potentially similar in composition to Earth or Mars — a solid surface you could, in theory, stand on.
Surface gravity is about 1.1g — noticeably heavier what you're used to on Earth.
With an equilibrium temperature around 4°C, this planet sits in the temperature range where liquid water could potentially exist on the surface — a key ingredient for life as we know it.
A year here is only 4.9 Earth days. Seasons, if they exist, change in a matter of hours.
Logarithmic bars so Jupiter-class planets fit the same scale as Earth-size worlds.
Red dwarf — the most common type of star. Cool and small.
Very cool — a faint red dwarf.
Detected by the star's wobble — gravitational tug from the orbiting planet shifts spectral lines.
Mildly elliptical — similar to most Solar System planets.
Rocky composition likely. Earth is 5.51 g/cm³.
A planet orbiting a star pulls it slightly back and forth. That motion compresses the star's light when moving toward us (blueshift) and stretches it away (redshift). Precision spectrographs detect the wobble at metres-per-second — enough to infer a planet's mass and orbit.
Where this host star sits among … exoplanet host stars. The main sequence band runs diagonally — giants and supergiants sit above, white dwarfs below.
ESI combines radius similarity and equilibrium temperature similarity. Earth = 100. Mars ≈ 73. Venus ≈ 44. This score reflects two physical parameters only — not atmosphere, water, or magnetic field.