
LHS 3844 b
Also written LHS 3844b
- Mass
- 2.37 × Earth
- Radius
- 1.29 × Earth
- Gravity
- 1.42 g
- Surface (est.)
- 648 K
- Year
- 11.1 hrs
- From Earth
- 48.6 ly
- Mass
- 2.37 × Earth
- Radius
- 1.29 × Earth
- Gravity
- 1.42 g
- Surface (est.)
- 648 K
- Year
- 11.1 hrs
- From Earth
- 48.6 ly
LHS 3844 system
- Type
- M-type (Red Dwarf)
- Spectral type
- M4.5-M5.0
- Temperature
- 3,080 K
- Radius
- 0.189 ☉
- Mass
- 0.151 ☉
- Planets
- 1
- Luminosity
- 2.72e-3 ☉
Published by the NASA Exoplanet Archive. This world’s temperature and habitability score are computed from this star’s measured luminosity, not from a stand-in for its class.
LHS 3844 b0.010 AUYou are here2.4 M⊕Star and planets drawn to scale: the star is 16 times as wide as LHS 3844 b, so only its edge is in view. Orbits spaced as in the star system view.
LHS 3844 b is one of the few rocky planets beyond the solar system whose surface astronomers have begun to read directly. NASA's Transiting Exoplanet Survey Satellite (TESS) found it, and the discovery was published in 2019 in a paper led by Roland Vanderspek. The planet is slightly larger than Earth and whips around a small, cool red dwarf star about 49 light-years away in roughly 11 hours.
Surface. Rocky surface with impact craters, possible volcanic features
Thin CO₂ and nitrogen atmosphere
Nitrogen atmosphere provides protection but not breathablePhysical Properties
Time Dilation
Clocks run 14.0 seconds per year slower than deep space — about 19 minutes over a lifetimeElemental Composition
How TerraForge built this world
LHS 3844 b, from the NASA Exoplanet Archive (found 2019). Measured: 2.37 Earth masses, 0.00624 AU, a 3080 K M-type star. Composition inferred from a measured bulk density of 1.10x Earth's, which is rock and iron, with a day locked to its 0.5-day year, as anything orbiting this close would be.



