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SELECTED WORLDWolf 1069 b
Wolf 1069 · M5.0 V host star · cool red dwarf · main sequence
Star temperature and orbital distance set incoming energy, but stellar size is also required. This calculation uses a typical radius for the listed spectral type, 30% reflectivity and even heat redistribution. It is not a ground-temperature forecast: air, clouds, oceans and surface reflectivity could move the result by tens to hundreds of degrees. A likely synchronous spin also means the permanent day and night sides would not share one ground temperature.
The marker above the bar is a typical temperature for this star’s class. The line below is Earth’s Sun.
Wolf 1069 is class M5.0 V. Its visible daylight would be dim and strongly red-orange; most of its energy is infrared.
Representative lit-side geometry only. On a locked world, the star’s real elevation would depend on where you stand.
Most plausible case. A single known planet around a 0.18-solar-radius star, 31 light-years away. It receives about 65% of Earth’s light, close to Proxima b’s energy, and the star spans about 1.4°. Dark rock, frost at the terminator, a possible small eyeball of slush. No sibling planet is known to share the sky.
Dry case. A dim red desert, dunes and dust, night-side cold trap for any ice.
Thick-air case. Clouds could hide the ground. The flux is temperate rather than inner-edge hot, so a steam sky is not required.
Walking. About 8% heavier than Earth, modelled from a minimum mass near 1.3 Earth masses. The sky has the red star and no known neighboring planet. The star is magnitude 14 from Earth.
Based on: Kossakowski et al. 2023; Teff 3158 K, R 0.18 Rsun, S 0.65, a 0.067 AU
Wolf 1069 b circles Wolf 1069. Use Higher and Lower to move your viewpoint above, through and below the orbital plane, and − / + to zoom. Orbit shapes and spacing are schematic.
Positions, distances, and system parameters come from the NASA Exoplanet Archive composite table, queried 25 Sep 2026. GJ 273 b uses the parallax in that row, 12.4 light-years. The 45 worlds follow Bohl, Lawrence, Lowry, and Kaltenegger.