We have spent decades looking for Earth 2.0 — a planet the right distance from its star, with the right atmosphere, where life could exist. JWST just made that search considerably more complicated.
In April 2026, the telescope released observations of TRAPPIST-1b and TRAPPIST-1c — two Earth-sized planets orbiting a dim red dwarf 40 light-years away. The data, from 60 hours of continuous observation covering each planet's full orbit, produced the first detailed climate maps of Earth-sized worlds around another star. What they showed: both planets are airless, their daysides running at roughly 217°C and 96°C respectively, their nightsides cold enough to freeze nitrogen. The temperature gap between day and night hemispheres exceeds 500 degrees on both worlds. No atmosphere means no heat redistribution, no buffer between the scorched and frozen sides. The findings were published in Nature Astronomy and the preprint is on arXiv.
Three siblings in the same system — TRAPPIST-1e, 1f, and 1g — sit in what astronomers call the habitable zone, the range of distances where liquid water could theoretically persist on a surface. Those planets were not part of this study. Whether any of them retained atmospheres is an open question the telescope is now designed to answer. But the broader pattern the data confirms is uncomfortable: the habitable zone framework was defined for planets that rotate the way Earth does. Three-quarters of the Milky Way's stars are red dwarfs. Planets in the habitable zone around them tend to be close enough for gravity to tidally lock their rotation — one face always cooked, one face always frozen. The universe, it turns out, built most of its potentially habitable planets differently than Earth.
The TRAPPIST-1 system, discovered in 2016, has become the reference case for this problem in exoplanet science. The telescope watched thermal radiation shift across each planet's day side as it rotated, revealing a temperature landscape unlike anything in our solar system. On Earth, atmospheric and oceanic circulation keeps the temperature gap between hottest and coldest surface at roughly 110 degrees. The gap on TRAPPIST-1b is about five times that. Whether these planets lost their atmospheres early in their histories — and whether any of the habitable-zone siblings still have theirs — are the questions JWST is built to answer. The climate map of two dead worlds is in. The answer for the others will take years of observation to arrive.
The habitable zone was always a guess at what life needs. The sample size of worlds where we can actually check is finally growing.