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SELECTED WORLDKepler-1544 b
Kepler-1544 · K2V host star · orange star · 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.
The marker above the bar is a typical temperature for this star’s class. The line below is Earth’s Sun.
Kepler-1544 is class K2V. Its daylight would have a warmer orange-gold cast than sunlight on Earth.
Representative daytime geometry only; the star’s height in the sky changes through the day.
Most plausible case. A K star near 4900 K and 0.74 solar radii. From 0.55 AU it spans about 0.72°, and the planet receives about 83% of Earth’s light. Radius 1.78 Earth radii, large for bare rock. Orange daylight, temperate flux, a 169-day year so a fixed dayside is unlikely. If the surface is rock, it is ordinary warm ground. More often at this size the “surface” is under a volatile layer.
Dry case. Warm rock and dunes under an orange, Sun-sized star, if the envelope was lost.
Thick-air case. The better bet. Clouds, and no visible ground.
Walking. About 21% heavier than Earth only if it is rocky. No known neighbor. Magnitude 14, about 1,100 light-years away.
Based on: NASA composite; Teff 4886 K, R 0.74 Rsun, S 0.83, Rp 1.78, a 0.545 AU
Kepler-1544 b circles Kepler-1544. 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.