Host star — Kepler-991
- Spectral type
- —
- Temperature
- 4,392 K
- Radius
- 0.61 R☉
- Mass
- 0.64 M☉
- Luminosity
- 0.148 L☉
- Distance
- 389.6 pc (1,271 ly)
Cooler than the Sun. Orange or red dwarf.
Orbits Kepler-991 · 1,271 light-years from Earth
Kepler-991 b orbits a cool, dimly glowing M-dwarf star at a distance of 0.31 AU, receiving enough stellar energy to maintain an equilibrium temperature of 260 Kelvin—roughly minus 13 degrees Celsius, or about as cold as Antarctica's interior. With a radius 2.54 times Earth's and a density of 2.34 g/cm³, this Neptune-like world likely retains a substantial atmosphere and possible water ice or even subsurface liquid water, though its exact composition remains unknown. Its circular 82.5-day orbit suggests orbital stability, a prerequisite for habitability. However, at 1,270 light-years away and discovered by the transit method in 2016, direct characterization of its atmosphere remains impossible with current technology, leaving critical questions unanswered: Is there a rocky surface beneath the atmosphere? Does liquid water exist? Could it be tidally locked to its star? The habitability score of 83 reflects these tantalizing but unresolved possibilities. This world's distance and faintness make it a long-term target for future space telescopes capable of atmospheric spectroscopy, but for now it remains a promising candidate whose true nature awaits discovery.
Kepler-991 b is a Neptune-like world — probably wrapped in thick layers of hydrogen, helium, and ices. There may be no solid surface at all, just clouds all the way down.
Surface gravity is about 1.1g — noticeably heavier what you're used to on Earth.
With an equilibrium temperature around -13°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.
An orbital period of 83 days makes the year 4.4× shorter than Earth's. You'd celebrate your birthday more often here.
Logarithmic bars so Jupiter-class planets fit the same scale as Earth-size worlds.
Cooler than the Sun. Orange or red dwarf.
Detected by measuring the tiny dip in starlight as the planet crosses in front of its star.
Nearly circular orbit.
Low density — probably icy or gas-rich.
A transit photometer watches a star nonstop and measures its brightness to ~0.01%. When a planet passes between us and the star, the star dims briefly — the deeper the dip, the bigger the planet. This is how Kepler and TESS found most known exoplanets.
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.