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Exoplanet atmospheres

Retention, loss, and observational detection of atmospheres on planets outside the solar system.

Current stories

scienceOne report1 publisher

JWST data resolve a puffy hot Jupiter's atmosphere into a ring with raised 'gems'

Astronomers used JWST data and a technique called transmission strings to map WASP-17b's atmosphere as a ring with raised 'gems'. The temperature contrast they found matches theory, so the result is a test of the method.

Publishers:space.com

Reality

Evidence55
Adoption
Not scored
Hype gap+15
Incentives
Not scored
Confidence60
scienceOne report1 publisher

JWST transit data show WASP-17b's atmosphere is more extended on its evening side

Cornell and Bristol researchers applied transmission strings to JWST data and found WASP-17b's atmosphere more extended on one side. The shape matches theoretical predictions, so the study is a first test of the method on one planet.

Publishers:phys.org

Reality

Evidence62
Adoption
Not scored
Hype gap+20
Incentives
Not scored
Confidence55
scienceOne report1 publisher

Gemini South spectra put WASP-189b's magnesium-to-silicon ratio close to its star's

WASP-189b, nearly 320 light-years away, has a magnesium-to-silicon ratio that closely matches its host star's, astronomers report. Teams that predict rocky-planet makeup from stellar chemistry now have a check, made on a giant planet.

Publishers:sciencedaily.com

Reality

Evidence35
Adoption
Not scored
Hype gap+40
Incentives55
Confidence40
scienceOne report1 publisher

Webb finds evidence of an atmosphere on HD 3167 b, the coldest lava world yet to show one

University of Chicago researchers report Webb evidence of an atmosphere on HD 3167 b, a rocky planet with a 24-hour orbit. Planets that close to a star are expected to lose gas to stellar wind and high-energy light, so the result could help explain how rocky worlds keep their atmospheres.

Publishers:sciencedaily.com

Reality

Evidence50
Adoption
Not scored
Hype gap+20
Incentives45
Confidence50
scienceOne report1 publisher

Escaping helium hints at a long-lived atmosphere on LHS 1140b

Helium reported escaping LHS 1140b, a habitable-zone planet 1.7 times Earth's size, may signal a long-lived secondary atmosphere around a red dwarf. The result is tenuous and the planet could still be a mini-Neptune, so its use as a test of whether red-dwarf worlds keep their air depends on confirmation.

Publishers:phys.org

Reality

Evidence40
Adoption
Not scored
Hype gap+25
Incentives
Not scored
Confidence45
scienceOne report1 publisher

Early Webb analyses put giant planet HATS-6 b about 300 degrees Celsius below its standard estimate

University of Maryland astronomers using Webb found ammonia on HATS-6 b and early temperatures near 120 C, against the 425 C usually cited. Their leading suspect is reflective cloud, and the planet's chemistry readings depend on that temperature.

Publishers:phys.org

Reality

Evidence55
Adoption
Not scored
Hype gap+15
Incentives
Not scored
Confidence50
scienceOne report1 publisher

Webb eclipse measurements suggest HD 3167 b, the coolest known lava world, holds an atmosphere

University of Chicago astronomers report that HD 3167 b, a super-Earth with a one-day orbit, has a dayside cooler than bare rock should allow. That makes it the coolest atmosphere case so far for a ten-planet program looking for the temperature at which lava worlds start to keep their atmospheres.

Publishers:phys.org

Reality

Evidence45
Adoption
Not scored
Hype gap+15
Incentives
Not scored
Confidence50
scienceOne report1 publisher

Radiative cooling and a falling Bowen ratio nearly cancel in a new global wind theory

Malte Jansen and colleagues derive the work that drives Earth's winds from two atmospheric quantities and find that warming's effects on them almost cancel, while the same simulations push storm tracks poleward.

Publishers:eos.org phys.org

Reality

Evidence55
Adoption
Not scored
Hype gap+10
Incentives40
Confidence60
scienceOne report1 publisher

Principal component analysis reads a brown dwarf's weather from its JWST light curve

Astronomers at Trinity College Dublin report that two components account for most of what changes in SIMP 0136's rotating spectrum, a decomposition they hope to refine for fainter brown dwarfs.

Publishers:phys.org

Reality

Evidence55
Adoption15
Hype gap+25
Incentives60
Confidence55
scienceOne report1 publisher

Stanford's lava-world model puts a second atmosphere boundary inside the cosmic shoreline

A new model says molten surfaces meter outgassing slowly enough to match escape losses for billions of years, which reshuffles the target list for follow-up spectroscopy of hot rocky planets.

Publishers:phys.org

Reality

Evidence58
Adoption
Not scored
Hype gap+18
Incentives62
Confidence55