T. Drant
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View article: Inferring the interior oxygen fugacity of rocky exoplanets from observations: Assessing biases by atmospheric chemistry
Inferring the interior oxygen fugacity of rocky exoplanets from observations: Assessing biases by atmospheric chemistry Open
In the era of the James Webb Space Telescope, inferring the presence and bulk composition of temperate rocky exoplanet atmospheres is now possible. The primary targets typically have equilibrium temperatures ranging from 400 to 1500 K, for…
View article: Optical constants of exoplanet haze analogs from 0.3 to 30 µm: Comparative sensitivity between spectrophotometry and ellipsometry
Optical constants of exoplanet haze analogs from 0.3 to 30 µm: Comparative sensitivity between spectrophotometry and ellipsometry Open
We report new optical constants (refractive index, n , and extinction coefficient, k ) for exoplanet haze analogs from 0.3 to 30 µm. The samples were produced in a simulated N 2 -dominated atmosphere with two different abundance ratios of …
View article: Organic detection in the near-infrared spectral Phobos regolith laboratory analogue in preparation for the Martian Moon eXploration mission
Organic detection in the near-infrared spectral Phobos regolith laboratory analogue in preparation for the Martian Moon eXploration mission Open
Context. The Martian Moon eXploration mission (MMX) of the Japanese space agency (JAXA) is scheduled to take off in September 2024 to explore Phobos and Deimos – the two martian moons – by in situ observations, but also by a sampling and r…