Researchers used JWST/MIRI to observe eclipses of the exoplanet GJ 3929 b — a warm Earth orbiting an M-dwarf. Analysis of four eclipse depth measurements (118±22 ppm) and dayside temperature (641 K) came in lower than previous estimates. This opens the possibility of a thin atmosphere, though a bare rock scenario cannot be ruled out. A thick CO₂ atmosphere without thermal inversion is ruled out at 3σ significance. Like a stone that doesn't get as hot as expected during the day, the planet hints at wearing an invisible gas 'blanket'.
In the depths of the constellation Hercules, around the dim M-dwarf GJ 3929, orbits a world one-and-a-half times Earth's size—like a billet on an anvil. A year here flashes by in 2.6 days, and the dayside hemisphere is heated to 640 Kelvin: metallurgists know that tin melts at that temperature. The JWST telescope caught moments when the planet hid behind the star, recording its faint thermal echo—like a glowing part cooling in the shade. Four such eclipses, processed with a new FN-PCA method, allowed measuring the flux with record precision: 118±22 parts per million of the star's brightness. This figure is the key to the puzzle: is the planet wrapped in a gas cloak or standing before us naked?
The blacksmith forge analogy here is not just poetry. The star's radiation acts like a hammer: each X-ray or ultraviolet photon can knock a molecule out of the upper atmosphere. If the planet's gravity isn't strong enough, the gases flee into interstellar space, leaving the rocky body a bare core. For GJ 3929 b, this process appears to be complete. Spectral analysis showed: if an ocean of carbon dioxide with pressure like Venus's were sloshing there, the thermal emission would be different—more uniform, smeared by winds from the dayside to the nightside. But the observations paint a different picture: the heat is concentrated in one spot, like the glowing heart of a forging that fades without bellows. A dense atmosphere is ruled out with three-sigma confidence.
Yet absolute emptiness is also not confirmed. From visit to visit, the eclipse depth varies at the 2.5σ level: perhaps the tidal locking is incomplete, and the planet still shows the star different "cheeks," or a ghostly atmosphere of volatile rocks briefly appears. Such a result is a boundary post on the cosmic shoreline that William Borucki, father of Kepler, spoke of. The work on GJ 3929 b is the first detailed analysis from the Rocky Worlds DDT program, and it already shows that even four JWST sessions may not yield a definite answer. To figure it out, we need statistics on dozens of worlds—like in a forge, where a single hammer blow doesn't reveal all the metal's properties.
The outlook is exciting. If most warm terrestrial planets around red dwarfs turn out to be airless, this will sharply narrow the search for life—but will also direct efforts toward ocean planets or worlds with thin envelopes elusive to photometry. Instruments are already being designed to directly see biosignatures: oxygen, methane, water vapor. Spectroscopy across a broad range, planned with the future Habitable Worlds telescope, will be able to peek into the gap between "atmosphere" and "no atmosphere," where the transit method barely reaches. And then the star's hammer will cease to be a destroyer—it will become an indicator, spotlighting the rare islands where a thin gas veil has sheltered life. GJ 3929 b is just the first nail driven into the foundation of this new worldview. Meanwhile, somewhere in Hercules, a rocky ball silently cools, its only atmosphere the infrared glow of its own interior.
🎯 The dayside of GJ 3929 b is heated to 640 Kelvin—about the melting point of tin—and its orbital period is just 2.6 Earth days: a year there flashes by faster than a week on Earth.