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    This artist’s concept shows what the ultra-hot super-Earth exoplanet TOI-561 b could look like based on observations from NASA’s James Webb Space Telescope and other observatories. Webb data suggests that the planet is surrounded by a thick atmosphere above a global magma ocean. Credit: NASA, ESA, CSA, Ralf Crawford (STScI)
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  • Oxidation of organics under hydrothermal conditions: Implications for the evolution of methane on Mars

Oxidation of organics under hydrothermal conditions: Implications for the evolution of methane on Mars

Foustoukos, D. I.; Stern, J. C.
2010
GEOCHIMICA ET COSMOCHIMICA ACTA

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