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TRAPPIST-1 e: Still No Answer On The Air

TRAPPIST-1 e: Still No Answer On The Air

The best rocky world we can actually check

Of every planet outside the solar system, this is the one best suited to the question people actually care about: does it have air? It is rocky, it sits in its star's habitable zone, and it crosses a very small, very dim star, which is what makes an atmosphere detectable at all. A planet passing a large bright star hides its thin shell of air in the glare. TRAPPIST-1 is barely bigger than Jupiter and cooler than a candle flame, so the contrast works in our favour. That combination is rare enough that JWST has spent significant time here.

Radius

0.920 Earth radii

Mass and density

0.692 Earth masses at 4.90 g/cm3

One year

6.101 Earth days

Host star

TRAPPIST-1 at 2566 K and 12% of the Sun's radius

Orbit radius

0.029 AU or about one thirteenth of Mercury's

Habitable zone

inside it, fourth of the seven planets

What four transits of JWST settled

0%

Cloudy hydrogen-dominated atmosphere above 80 percent by volume. Ruled out at better than three sigma.

A Venus-like atmosphere. Disfavoured by the data.

A Mars-like atmosphere. Disfavoured by the data.

A nitrogen-rich atmosphere with traces of methane and carbon dioxide. Still permitted.

No atmosphere at all. Still permitted.

🔭🪐📡01.05.2016 – 01.09.2025
01.05.2016Three transiting Earth-sized planets found around an obscure red dwarf, using a 60 cm telescope in Chile.
01.05.2016
01.02.2017Four more announced. Seven rocky worlds, three of them in the habitable zone, all orbiting closer than Mercury.
01.02.2017
01.01.2023JWST watches four transits of planet e with NIRSpec PRISM, hunting for starlight filtered through an atmosphere.
01.01.2023
01.09.2025Results published. A thick hydrogen atmosphere is ruled out. A nitrogen one is still allowed. No detection either way.
01.09.2025

The hardest problem is not the planet, it is the star. Red dwarfs are covered in spots and faculae, and starlight crossing those regions imprints a signal that looks very like an atmosphere. The published spectra show that contamination across 3 to 5 microns, which is exactly where the interesting molecules live.

The archive lists no measured equilibrium temperature for this planet. Derived from the star's output and distance, assuming a third of the light is reflected, it lands near 228 K, about minus 45 C. That is an estimate from two numbers, not a measurement, and the real surface depends on the air question above.

Two readings fit the same data: a thin nitrogen atmosphere, or bare rock with no \

air at all. Which would you bet on, and what observation would change your mind?

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