:INFO Super-earth around KOI-351 It is 1.31 times Earth's radius, closest in size to Earth. A year there lasts 7.01 days, on an orbit 5 times closer to its star than Mercury is to the Sun. Its equilibrium temperature is 1080 K (derived from the star rather than measured), hot enough to melt lead. The host star KOI-351 runs at 6080 K with 1.20 times the Sun's mass. :JOURNEY KOI-351 from the inside out 1 0.074 AU 2 0.089 AU 3 0.320 AU 4 0.420 AU 5 0.480 AU :STATS [icon:TARGET] Radius | 1.31 Earth radii [icon:FIRE] Equilibrium temperature | 1080 K (derived) [icon:CLOCK] One year | 7.01 days [icon:BOLT] Orbit radius | 0.0740 AU [icon:STAR] Host star | KOI-351 at 6080 K [icon:USERS] Distance | 2767 light-years [icon:TRENDING_DOWN] Starlight blocked | 0.010% at each transit :PATH What you get from the shadow How deep the star dims fixes the planet's size relative to it. :TIMELINE 🔭🪐📅 2013-01-01 | KOI-351 b, KOI-351 c, KOI-351 d, KOI-351 e, KOI-351 f 2017-01-01 | Kepler-90 i :CHECKLIST The state of the record for this planet [ ] A radius from transit photometry. Yes. [ ] A measured mass. No. [ ] A density, the one clue to composition. No. [ ] A semi-major axis. Yes. [ ] A measured temperature rather than a derived one. No. [ ] An eccentricity, so the orbit shape is known. No. :NOTE The archive lists no measured equilibrium temperature for this planet. The 1080 K quoted here is derived from the star's output and the orbital distance, assuming a third of the light is reflected. It is an estimate from two numbers, not an observation. :NOTE.half The detection is a shadow crossing a disc. Shadows have no weight, which is the whole reason the mass column is empty. :NOTE.half KOI-351 has 8 known planets. A crowded system is worth more than the sum of its planets: the timing of each transit constrains the others. :NOTE Found by Kepler in 2013. Kepler's method needed repetition, not brightness. It could find small planets around faint stars, provided they came round quickly enough to be seen twice. :THREAD :LINK https://exoplanetarchive.ipac.caltech.edu/overview/KOI-351%20b Every parameter ever published for KOI-351 b, at the NASA Exoplanet Archive